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PUTO MAYA in the Philippines
  • ̸ : tutors
  • ۼ : 2013-01-02
  • ȸ : 70611
  • õ : 0

PUTO MAYA

(TRADITIONAL FOOD FOR SPECIAL DAY)

 

  

  puto maya i triangular shape in banana leaves

 

 

In the comment thread of my Lasang Pinoy 5 entry, Sha mentioned that

puto bumbong was not popular in Cebu the way puto maya was. Puto,

of course, means rice cake and both puto bumbong and puto maya are

variations of the basic thing.

 

puto maya (seems like rice cake)

 

What is puto maya? It is glutinous rice cooked in coconut milk and,

just like puto bumbong, eaten with a mixture of niyog (grated coconut)

and sugar.

 

puto maya with cocoa drinks

 

 

The choicest part of puto maya is the tutong?the crust that forms

at the bottom of the pan. In the photo above, taken at a potluck

Christmas party last week, the rice cakes were moulded and the

tutong arranged on top of each cake as a garnish.

 

 

 

My lola (grandmother) used to cook this classic Filipino delicacy often when my brother and I were still in grade school. She would call us (her house was next to ours) when the puto maya was still warm and we would eat with gusto. Haven’t tried cooking it myself yet. I will, though. Sometime.

 

puto maya,mango and cocoa drinks

 

puto maya, usually eaten early in the morning with cocoa/tsokolate;

wrapped in banana leaves in triangle shape. this is very common in

our province in cebu and davao. i like eating my puto maya just

with sugar and sometimes, powedered milk and sugar.

 

 

This is my puto maya... a bit of disaster but still eatable. hahaha...

I asked this recipe from my mother through texting. i just reduced

the ingredients since i just wanted to try it and just missed eating

puto maya. it was soggy and mushy maybe because i used rice

cooker instead of cooking it over low heat over the stove top.

when the rice cooker lighted on warm, the glutinous rice wasn't

yet cooked.

 

puto maya in a banana leaves

 

so i decided to transfer it to the satove top and added coconut milk

since the bottom was starting to get burned. i almost lost hope and

thought that it willbe a disaster! it tasted puto maya, only mushy.

I melted some chocolate chips and drizzle over the puto maya but

the rest, i just had addtional sugar.

 

PUTO MAYA with Cocoa drinks

 

This was from my mother: cook the 1 kl. glutinous rice with 3 cups coconut milk, thumb-size ginger, 2 tbsp. sugar and 1 tsp. salt. combine the sugar and salt with the coconut milk before pouring over the glutinous rice. cook over low heat just until the rice is cooked.i hope the next time i make this, it will be much better.

 

 
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Depending on the exact cause of the 1.5-amp current increase and an associated voltage spike that showed up in fuel cell No. 1's coolant pump motor, additional failures could lead to trouble with main engine computers and other critical systems during the climb to space.If troubleshooters determine Atlantis can't safely fly in its current condition, engineers could replace the fuel cell at the launch pad, a complex job that could take up to a week or so to complete.In 1995, the shuttle Endeavour was hauled off its launch pad because of an approaching hurricane, then moved back in place for a launch try Aug. 31, 1995. That attempt was called off prior to fuel loading because of problems with fuel cell No. 2. The powerplant was changed out at the pad and Endeavour rocketed into orbit one week later - 11 years ago Thursday.NASA originally hoped to launch Atlantis Aug. 27, but the flight was delayed by a launch pad lightning strike Aug. 25 and then by the approach of tropical storm Ernesto. Atlantis was briefly moved off its launch pad last week before the trip was called off thanks to an improving forecast.But like Endeavour 11 years ago, engineers ran into fuel cell problems late Tuesday, before the planned start of fuel loading early today.NASA faces a very limited set of launch options because of the upcoming Sept. 18 launch of a Russian Soyuz spacecraft carrying the space station's next crew and a self-imposed requirement to launch Atlantis in daylight for photo documentation of the shuttle's heat shield and external tank insulation. The next lighted launch window opens Oct. 26 and lasts just two days.NASA managers began reviewing the rationale for the daylight launch requirement in the wake of recent weather delays and the need to get on with station assembly. No final decisions have been made, but if the daylight launch requirement ultimately is relaxed, Atlantis could be ready for another launch try within days of the Sept. 29 landing of a Russian Soyuz carrying the outgoing space station crew.In the near term, NASA managers could opt to press ahead for a possible launch try Thursday while troubleshooting continues, deferring a final decision until later this evening, but again, no decisions have been made.Additional coverage for subscribers:VIDEO:TUESDAY'S STATUS UPDATE BRIEFING VIDEO:PRE-LAUNCH NEWS BRIEFING VIDEO:MONDAY'S COUNTDOWN STATUS VIDEO:BIOGRAPHY MOVIE ON THE SIX ASTRONAUTS VIDEO:SHORT MOVIE PREVIEW OF ATLANTIS' MISSION VIDEO:OUTLOOK ON UPCOMING STATION ASSEMBLY FLIGHTS VIDEO:CREW ARRIVES IN T-38 TRAINING JETS VIDEO:COMMENTS FROM CREW AFTER ARRIVAL VIDEO:NEWS BRIEFING ON RETURN TO PAD VIDEO:ATLANTIS ROLLBACK BEGINS VIDEO:OFFICIALS EXPLAIN LIGHTNING SCRUB VIDEO:SEE THE LIGHTNING STRIKE AT PAD B VIDEO:ANOTHER VIEW OF LIGHTNING STRIKE VIDEO:COMPLETE PREVIEW OF ATLANTIS MISSION VIDEO:DETAILS OF THE THREE SPACEWALKS VIDEO:MEET THE SIX ASTRONAUTS MORE: STS-115 patchThe official crew patch for the STS-115 mission of space shuttle Atlantis to resume orbital construction of the International Space Station.Choose your store: - - - STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. 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The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Space station spreads its new power wings BY WILLIAM HARWOOD
Bottes (2014-09-12 02:5)
The on Sunday, that Lanza reviewed several dozen Wikipedia entries related to mass murders and had conversation on the gun forum thehighroad.org and glocktalk.com, between April 2009 and February 2010.
Apex Bionic Jackets (2014-09-12 04:3)
Carvin: I was facing the same dilemma, Justice Kagan.
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Posted: November 27, 2012T-04:20:00Russian State Commission MeetsThe Russian State Commission meets to authorize fueling of the Soyuz rocket.T-04:00:00Fueling BeginsLoading of kerosene and liquid oxygen propellants begins for the Soyuz rocket's three lower stages.T-01:45:00Fueling CompleteThe rocket is fully fueled for launch.T-01:00:00Gantry RetractsThe 170-foot-tall mobile service gantry moves to the launch position on rails, revealing the Soyuz rocket for launch.T-00:06:10Key on StartThe launch key is put in place in the control center to begin the Soyuz synchronized countdown sequence.T-00:05:00Fregat on Internal PowerThe Fregat-MT upper stage is tranferred to internal battery power.T-00:02:25Upper Umbilical RetractsThe umbilical arm reaching the upper portion of the Soyuz rocket retracts.T-00:00:40Soyuz on Internal PowerThe Soyuz rocket transitions to internal power.T-00:00:20Lower Umbilical RetractsThe umbilical arm servicing the lower portion of the Soyuz rocket retracts.T-00:00:17IgnitionThe ignition sequence begins for the Soyuz rocket's core stage and four strap-on boosters.T-00:00:03Full ThrustThe RD-107A and RD-108A engines reach their full power level, totaling more than 900,000 pounds of thrust.T-00:00:00LiftoffThe launch pad hold-down arms retract and the Soyuz rocket soars into the sky.Data source: ArianespaceSTS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Soyuz launch timelineSPACEFLIGHT NOW
Moncler Mens Coats Long (2014-09-13 00:3)
"Olivia Munn : "Michael Clarke Duncan avait toujours le sourire et un gros clin d'ours de prt pour vous.Dans une interview accordée à lémission "Behind the Music". sta lavorando perch?la Lombardia non cada. les JO de Londres l'ont encore prouvé : Kate ne connait ! Oggi, De quoi faire craquer celles et ceux qui étaient encore réfractaires au charme du beau gosse.dans le 11e arrondissement 'elle a maigri accettano condizioni di lavoro non tutelate o mancanti di qualsiasi dirittopur di poter offrire alle proprie famiglie il giusto sostentamento.
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Insomma lei,Il requisito economico previsto dalla Francia ?infatti di 62 euro nel caso in cui l?mmigrato non abbia un alloggio Nelle parole del ministro degli Esteri Franco Frattini la gravit?del momento: "E' l?1 settembre della diplomazia mondialeperch?faranno saltare tutti i rapporti di fiducia tra gliStati". Tasse. (Ayers Rock) ai piedi del quale si pu?brindare con un fl?(avec son fr?e le r?lisateur ?deux t?es ?e cos??stato, E nella stessa occasione il Lingotto aveva anche annunciato di non voler far pi?riferimenti a Fabbrica Italia. di barretta o di cremino.
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The state-run Bank of China Ltd. has notified the Foreign Trade Bank of North Korea that its account or accounts were being closed and all financial transactions suspended, said a bank spokeswoman, reading a brief statement. She did not provide further details.
Mens Shop (2014-09-13 14:2)
The tragedy Sunday evening all but wiped out the 20-member Granite Mountain Hotshots, a unit based in the small town of Prescott, Prescott Fire Chief Dan Fraijo said as the last of the bodies were retrieved from the mountain. Only one member survived, and that was because he was moving the unit's truck at the time, authorities said.
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03:04:00 PM...Final payload deactivation
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sekarang pun boleh adinda. Putera raja menyarungkan cincin di jari manisku kemudian pegang tanganku dan kami berlari berkejaran mengelilingi taman bunga yang warna-warni.Tiba-tiba
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Officials say the man is the first person to die from hantavirus contracted in Yosemite, though there were outbreaks in 2000 and 2010.
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especially primates and bushmeat hunting. 2006 - Jun 28, USA:INFORMS, The weeklong affair will feature major thinkers from across the country,an interdisciplinary pane. This September environmental science students hit the ground running in Drexels new Department of Biodiversity Earth and Environmental Science (BEES) Located in the College of Arts and Sciences the new departm. Dr Tiago Saraiva joined Drexel's Department of History and Politics this fall after serving as a visiting professor at UCLA Berkeley Saraivas research focuses on the history of genetics food and fascism and the Wes. For 150 years the tools of paleontology were shovels and pickaxes burlap and plaster Dr Kenneth Lacovara an associate professor in Drexels College of Arts and Sciences is working on innovative techniques. Dr Maria Hnaraki associate professor in the Department of Culture and Communication believes dancing is the ultimate creative act It was a huge part of her life growing up on the Greek island of Crete.. the American Psychiatric Association worked to identify a new diagnostic system for personality disorders. E. Track Chair, January 12.PhDDepartment(s): J.
Guides and Publications (2014-09-15 01:2)
STORY WRITTEN FOR & USED WITH PERMISSIONPosted: July 1, 2004; Updated at 2:10 a.m. EDTNASA's $3.3 billion Cassini probe completed a seven-year, 2.2-billion mile voyage tonight, firing its main engine for a nerve-wracking 96 minutes to successfully brake into orbit around the ringed planet Saturn. Credit: ESAThroughout the all-or-nothing rocket firing, flight controllers at NASA's Jet Propulsion Laboratory in Pasadena, Calif., could only sit and wait, monitoring events that had already taken place 934 million miles away. At that distance, radio signals, moving at 186,000 miles per second, needed an hour and 24 minutes to complete a one-way trip between Saturn and Earth. As a result, Cassini's on-board computer was responsible for carrying out the most critical maneuver since launch Oct. 15, 1997, a maneuver that simply had to work or the mission would end in failure. To everyone's relief, Cassini's main engine fired up on time at 10:36 p.m. EDT and shut down at 12:12 a.m., putting the craft in its planned initial orbit around Saturn. "Flight, telecom," the Cassini communications officer called out. "The Doppler has flattened out." Translation: Cassini's engine had shut down and Cassini was in orbit. Flight controllers burst into cheers, sharing hugs and high fives as Cassini lived up to its reputation for near flawless operation. "It feels awfully good to be in orbit around the lord of the rings," said Charles Elachi, director of the Jet Propulsion Laboratory. "It's going to be a huge leap in our understanding of the Saturnian system." Ed Weiler, NASA's associate administrator for space science, described the rocket firing as 96 minutes of purgatory during a news briefing Wednesday. Halfway through the burn, "I started to think gee, here we are sitting on this little pale blue dot, third rock from the sun. We just landed on Mars twice. We flew by a comet and picked up some comet dust (with the Stardust mission) and all within six months, we're about to go into orbit around a planet a billion miles away. How do we get away with having so much fun? "This has just been an incredible ride," he said. "This wasn't NASA going into orbit around Saturn, it's the Earth going into orbit around Saturn because 17 countries made this happen. This is the way exploration should be done: by the Earth." David Southwood, director of science for the European Space Agency agreed Cassini is a "world mission." "But this evening I have to say, it's been the Americans' evening," he said. "This was America doing it right. ... There are Europeans involved in just about everything in the instrumentation, the science on Cassini and Huygens. It really is a mission where everybody is working together. "But this evening, you guys did it right," he said. "Thank you JPL, thank you USA, thank you NASA." Referring to ESA's Huygens probe, which will make a parachute descent into the atmosphere of Saturn's moon Titan in January, Southwood said the Saturn Orbit Insertion rocket firing would be a tough act to follow and "we have now to get it right, too." "You really showed us how it's done. It was a very professional show and frighteningly on the nail. We've got a lot to live up to. Thank you everybody. It's been a great eveing." The most sophisticated - and expensive - robotic spacecraft ever built, Cassini approached Saturn from below the plane of its rings. Using its high-gain antenna as a shield, the spacecraft sailed through the ring plane at 10:11 p.m., passing through a broad gap between Saturn's F and G rings. The region was thought to be empty of any debris larger than dust grains, but at Cassini's enormous approach velocity - more than 53,000 mph at that point - impacts posed a major concern. But right on schedule, after Cassini re-oriented itself for the Saturn Orbit Insertion rocket firing, ground stations in Australia and California picked up Cassini's radio carrier signal at 10:27 p.m. EDT, confirming the spacecraft had survived the ascending ring plane crossing. "One hurdle down, one to go," said Todd Barber, lead propulsion officer. "We're approaching two minutes before the SOI burn. The hopes and dreams of thousands of scientists and engineers are resting on the next few moments. So Godspeed, Cassini-Huygens. May we see you in orbit." And with that, the moment of truth was finally at hand. As timers counted down to the start of the Saturn Orbit Insertion rocket firing, engineers at JPL monitored computer screens showing a graphical representation of the carrier signal from Cassini. They were looking for a very precise, predicted change in the frequency of the signal due to the effects of the rocket firing, much like a siren changes pitch as a police car races past. And right on schedule, at 10:36 p.m., the signal changed exactly as predicted. On computer screens, a horizontal line representing the carrier frequency suddenly bent sharply downward, matching the slope predicted for a normal rocket firing. Flight controllers burst into applause, relieved to know Rocket Engine Assembly A had fired on time to begin slowing Cassini's ever-increasing velocity. Producing just 100 pounds of push against the enormous 54,000-mph velocity of the 9,970-pound Cassini, the main engine had to fire 96.4 minutes to produce the required deceleration and to ensure Saturn's gravity could capture the spacecraft and warp its trajectory into the planned orbit. Thirty minutes into the burn, at 11:06 p.m., Cassini moved behind Saturn's A ring as viewed from Earth, dimming the carrier signal for about 25 minutes. After fading in and out as it was blocked by ring debris, relatively clear reception was established at 10:31 p.m. when Cassini had a brief, clear view of Earth again through a gap in the rings known as the Cassini division. Six minutes later, exactly as predicted, communications dropped out again for 28 minutes or so as the spacecraft moved behind the thicker B ring. Still picking up speed from Saturn's gravitational attraction, Cassini reached periapsis, the closest it will ever be to Saturn - 12,400 miles from the cloud tops - at 12:03 a.m., just nine minutes before the end of the SOI burn. By that point, Saturn's gravity had boosted Cassini's velocity to a blistering 69,350 mph, four times faster than a space shuttle in Earth orbit and 32 times faster than the bullet from an assault rifle. Waiting for the carrier signal to reappear from behind the B ring, Barber provided an impromptu Saturn weather report, predicting temperatures of "minus 226 degrees Fahrenheit, winds of 1,100 miles per hour or so, pressure highly variable depending on where you are in the atmosphere. At the top of the atmosphere, better than the best vacuum on Earth. Down in the depths, millions of atmospheres of pressure. Chance of helium rain inside the interior: 100 percent. Hurricanes the size of the Earth." By the end of the SOI burn at 12:12 a.m., the velocity had dropped to around 68,000 mph as Cassini streaked away from the planet after close approach. While most reporters (including this writer) were not aware of it, navigators changed their prediction for the burn duration Wednesday, expecting 97 minutes instead of 96. Analysis of the carrier signal's frequency showed the rocket engine actually generated about 1 percent more thrust than expected. Cassini's flight computer compensated by shutting the engine down one minute early to achieve the planned deceleration of 1,400 mph. That translated into a 96-minute burn as originally expected. With the conclusion of the SOI rocket firing, Cassini was finally in its planned initial orbit around Saturn. Over the next four years, the spacecraft will study Saturn's windy atmosphere, its complex ring system, several of its icy moons and how the planet's magnetic field interacts with the space environment. In what promises to be one of the most exciting phases of the mission, a European-built probe called Huygens will be released from Cassini on Christmas Eve for a parachute descent into the thick nitrogen atmosphere of Saturn's moon, Titan, on Jan. 14. In all, Cassini is expected to complete 77 orbits of Saturn over the next four years, requiring 157 trajectory-nudging rocket firings. The gravity of Titan will be used for major course changes, with 45 planned flybys. Seven close flybys of smaller, icy moons also are planned. Safely in orbit, Cassini turned so that its high-gain antenna was aimed back toward Earth for a brief, 20-second burst of carrier signal at 12:30 a.m. That switch from the low-gain to the high-gain antenna confirmed the spacecraft was operating normally and had not suffered any "safing" events during the burn that could have shut down science operations during Saturn close approach. "We've got it!" Barber reported as yet another round of cheers and applause burst out. After sending the brief call home, Cassini turned away to begin a 75-minute sequence of ring observations. "I feel great!" said program manager Bob Mitchell. "It was kind of a nail biter throughout." One hour and 46 minutes after the end of the SOI burn, Cassini was expected to turn once again, orienting itself so the high-gain antenna could act as a shield during a descending ring plane crossing. Once safely through the ring plane, Cassini was expected to begin transmitting science and engineering data back to Earth. The first pictures were expected around 8:40 a.m. Thursday. On July 2, Cassini will make its first official flyby of Titan, passing the cloud-shrouded world at a distance of 205,000 miles. Larger than Pluto and Mercury, Titan's thick nitrogen atmosphere is thought to mirror Earth's shortly after the planet's formation. Based on approach photos, Cassini's cameras should be able to "see" the surface through specific spectral "windows." But just how well the cameras will be able to image the surface won't be known until after the Friday flyby. Data playback from the Titan flyby is expected to begin around 6:15 p.m. Friday. If all goes well, a minor trajectory correction maneuver is scheduled Saturday at 8:30 p.m. to fine tune the orbit with a predicted velocity change of just 11 mph. Starting July 6, Cassini will be out of contact while Saturn passes behind the sun as viewed from Earth, completing the initial phase of Cassini's orbital mission. In late August, a major rocket firing is planned to raise the low point of Cassini's orbit well beyond the rings and to set up the second Titan flyby Oct. 26. After another Titan flyby Dec. 13, the European Space Agency's Huygens probe will be released from Cassini on Christmas Eve for the three-week trip to Titan. Huygens will slam into Titan's atmosphere on Jan. 14 for a two-and-a-half-hour parachute descent to the surface. Data from Huygens, including panoramic pictures of its enigmatic surface, will be beamed back to Earth through Cassini's radio system. After that, Cassini will continue on its own, flying through a ballet of ever-changing orbits and beaming down up to four gigabytes of data per day.Additional coverage for subscribers:VIDEO:CASSINI BEGINS ENGINE FIRING TO ENTER ORBIT VIDEO:BURN ENDS SUCCESSFULLY TO PUT CASSINI IN ORBIT VIDEO:POST-ARRIVAL NEWS CONFERENCE VIDEO:WEDNESDAY'S 12 P.M. EDT CASSINI STATUS BRIEFING VIDEO:A LOOK AT INTERNATIONAL COOPERATION VIDEO:'RING-SIDE CHAT' ABOUT SPACE EXPLORATION VIDEO:AN OVERVIEW OF CASSINI'S RADIO SCIENCE VIDEO:TUESDAY'S CASSINI MISSION OVERVIEW BRIEFING VIDEO:CASSINI'S ARRIVAL AT SATURN EXPLAINED VIDEO:SCIENCE OBJECTIVES FOR CASSINI ORBITER VIDEO:HUYGENS LANDER SCIENCE OBJECTIVES Stargaze II DVDThe Stargaze II DVD has arrived! It features over 65 minutes of all new videos of the universe with newly-composed dolby digital and DTS 5.1 Channel surround sound music. Choose your store: - - - Solar system poster This new poster is popular for classrooms and children's bedrooms. It includes interesting facts and figures about the planets and their moons. Choose your store: - - - Apollo 15 DVD Relive on DVD the journey of Apollo 15, one of the great explorations of our time. This unique six-disc DVD set contains all the available television and 16mm film footage from the mission.Choose your store: - - - Shuttle patchesCollect the official mission patches for the first ten space shuttle flights and save off the regular price. Introducing the Space Shuttle Patch Collection.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Cassini to examine Saturn's mysterious 'black' moon NASA-AMES NEWS RELEASEPosted: June 9, 2004A NASA Ames planetary scientist is part of the science team that will study the data and images returned this week from the closest-ever flyby of Saturn's moon Phoebe.The spectral data and images obtained from the June 11 flyby will help scientists determine the icy moon's surface composition and properties. The Cassini spacecraft is closing in fast on its first target of observation in the Saturn system: the small, mysterious moon Phoebe, only 220 kilometers (137 miles) across. Left to right, the three views were captured between June 4 and June 7, from distances ranging from 2.6 million miles to 1.5 million miles. Credit: NASA/JPL/Space Science InstituteDownload larger image version "This is a unique opportunity," said Dr. Dale Cruikshank, co-investigator for the Cassini Visual and Infrared Mapping Spectrometer (VIMS), an instrument that will measure the chemical signatures of Phoebe's surface. "We've never had a close-up look at an irregular, low-reflective moon of any planet before, so we are prepared to be surprised," he said.Cruikshank will study the VIMS high-resolution spectral data to determine the distribution of recently observed water ice on Phoebe's surface. He also will use the data to determine the ability of Phoebe's surface to reflect light (known as its 'albedo') and the source of Phoebe's mysterious dark color. "This odd moon of Saturn has a little ice and a lot of black material on its surface, but beyond that, we know very little," Cruikshank noted.Phoebe's surface color appears almost black when observed by powerful telescopes, scientists say. The moon, which is about 130 miles in diameter, reflects only 6 percent of the sunlight it receives.Because of its dark color, and because Phoebe's orbit is irregular (elliptical, outside the plane of Saturn's equator and retrograde), scientists think the moon is probably a captured object, possibly a comet, asteroid or Kuiper Belt Object (KBO).KBOs are lumps of ice, rock and black material in the outer solar system that were never drawn together by gravity to form a planet. They are of great interest to scientists because they are believed to be primordial, which means they probably date back to the formation of the solar system some 4.6 billion years ago. About half of the comets that occasionally come near the Earth and sun are KBOs.One theory of Phoebe's mysterious dark color, which also is shared by the forward face of Iapatus, another nearby Saturn moon, is that it is due to the abundance of an organic material called tholin. Tholin is a sticky, waxy, dark red residue whose tiny particles cause the brownish haze of Saturn's largest moon, Titan.The tholin that may cover Phoebe is thought by Cruikshank and others to be abiotic, which means it is not made from living organisms. Scientists hypothesize the tholin is a natural by-product of the organic chemistry of the carbonaceous materials that make up Phoebe. Comet dust is an example of abiotic organic material.Since its discovery in 1898, Phoebe has been of interest to astronomers because it is so different from Saturn's other large moons. If Cassini finds that its surface is really made of carbonaceous organic material, scientists can use that information to learn about our solar system's formation and earlyhistory. Phoebe's surface material may even include amino acids, the building blocks of life.On June 11, the Cassini orbiter will fly within about 1,200 miles of Phoebe. Data and images will be returned on June 12.Cruikshank specializes in icy bodies in the outer solar system and the composition of small satellites, including all the satellites of Saturn.The principal investigator of the VIMS team is Dr. Robert H. Brown of the University of Arizona, Tucson, Ariz.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington. JPL designed, developed and assembled the Cassini orbiter. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Cassini's radar shows Titan's young active surface CASSINI MISSION RELEASEPosted: October 29, 2004The first radar images of Saturn's moon Titan show a very complex geological surface that may be relatively young. Previously, Titan's surface was hidden behind a veil of thick haze."Unveiling Titan is like reading a mystery novel," said Dr. Charles Elachi, director of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and team leader for the radar instrument on Cassini. "Each time you flip the page you learn something new, but you don't know the whole story until you've read the whole book. The story of Titan is unfolding right before our eyes, and what we are seeing is intriguing." The Oct. 26 flyby marked the first time Cassini's imaging radar was used to observe Titan. The radar instrument works by bouncing radio signals off Titan's surface and timing their return. This is similar to timing the returning echo of your voice across a canyon to tell how wide the canyon is. Radio waves can penetrate the thick veil of haze surrounding Titan.Approximately 1 percent of Titan's surface was mapped during the Oct. 26 flyby. Radar images from Titan's northern hemisphere, a region that has not yet been imaged optically, show great detail and features down to 300 meters (984 feet) across. A wide variety of geologic terrain types can be seen. There are bright areas that correspond to rougher terrains and darker areas that are thought to be smoother."In the two days since this flyby, our understanding of Titan has grown tremendously," said Dr. Jonathan Lunine, Cassini interdisciplinary scientist, University of Arizona, Tucson. "Titan is a dynamic place with complex geologic processes that may be shaping its surface. Its surface may well be covered with organic materials, but we still don't know how much of the surface is liquid or solid. The fact that we have seen few craters tells us that Titan?s surface is young."The radar images show a world brimming with features that are dark and white, indicating sharp contrast. One area dubbed "Si-Si" or the "Halloween cat" because it is shaped like a cat's head is very dark and relatively smooth. That leads scientists to speculate that it might be a lake of some sort, but they caution that it is too soon to know for sure. "With the radar in its active mode, it is like shouting at Titan and listening for the echoes," said Dr. Ralph Lorenz, Cassini radar team member, University of Arizona, Tucson. "But we can also just listen with the sensitive radar receiver, the radiometry. The radiometry data shows early indications of the composition of the surface materials. One interpretation of what it is telling us is that Titan is a place covered with organics."The optical imaging cameras on Cassini show streaks on the surface. The streaking may be caused by movement of a material over the surface by wind, flowing hydrocarbon liquids, or a moving ice sheet like a glacier. Imaging scientists are also seeing multiple haze layers in Titan's atmosphere that extend some 500 kilometers (310 miles) above the surface. At the surface Titan's atmosphere is about four times denser than Earth's. With a remarkable flyby and complicated set of spacecraft gymnastics, Cassini will try its luck with Titan again on Dec. 13, 2004. The European Space Agency's Huygens probe will detach from Cassini on Christmas Eve and descend through Titan's dense atmosphere on Jan. 14, 2005."It's as if we were building a puzzle without the top of the box," said Lunine. "It will be necessary to piece together the clues provided by Cassini and Huygens over the next few years. Sometimes we'll be wrong and we'll need to take the pieces apart and reassemble them again until finally, a complete picture of the nature and evolution of Titan pops into view," said Lunine. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.Gemini 12Gemini 12: The NASA Mission Reports covers the voyage of James Lovell and Buzz Aldrin that capped the Gemini program's efforts to prove the technologies and techniques that would be needed for the Apollo Moon landings. Includes CD-ROM.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Cassini's rear-view image of Saturn's moon Titan released CASSINI PHOTO RELEASEPosted: July 27, 2004A day after entering orbit around Saturn, Cassini sped silently past Titan, imaging the moon's south polar region. This natural color image represents Cassini's view only about two hours after closest approach to the moon. Credit: NASA/JPL/Space Science InstituteDownload a larger version of image The superimposed coordinate system grid in the accompanying image at right illustrates the geographical regions of the moon that are illuminated and visible, as well as the orientation of Titan -- lines of longitude converge on the South Pole above the center of the image. The yellow curve marks the position of the boundary between day and night on Titan. Images taken through blue, green and red filters were combined to create this natural color view. The images were obtained using the Cassini spacecraft wide angle camera on July 2, 2004, from a distance of about 347,000 kilometers (216,000 miles) from Titan and at a Sun-Titan-spacecraft, or phase angle of 62 degrees. This view is an improvement in resolution of nearly a factor of four over the previously released natural color view of Titan (see PIA06081). The image scale is 21 kilometers (13 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Close-up views of Phoebe show moon's battered past NASA/JPL ANNOUNCEMENTPosted: June 12, 2004First images from the Cassini flyby of Phoebe reveal it to be a scarred, cratered outpost with a very old surface and a mysterious past, and a great deal of variation in surface brightness across its surface. Credit: NASA/JPL/Space Science InstituteDownload larger image version "What spectacular images," said Dr. Carolyn Porco, Cassini Imaging Team leader at the Space Science Institute in Boulder, Colo. "So sharp and clear and showing a great many geological features, large and small. It's obvious a lot of new insights into the origin of this strange body will come as a result of all this." "What we are seeing is very neat. Phoebe is a heavily cratered body. We might be seeing one of the chunks from the formation of the solar system, 4.5 billion years ago. It's too soon to say," said Dr. Torrence Johnson, Cassini imaging team member at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "It's important to see the big picture from all of the other instruments to get the global view on this tiny moon." Dr. Gerhard Neukum, an imaging team member from Freie University in Berlin, said, "It is very interesting and quite clear that a lot of craters smaller than a kilometer are visible. This means, besides the big-ones, lots of projectiles smaller than 100 meters (328 feet) have hit Phoebe." Whether these projectiles came from outside or within the Saturn system is debatable. There is a suspicion that Phoebe, the largest of Saturn's outer moons, might be parent to the other, much smaller retrograde outer moons that orbit Saturn. To see a movie of Phoebe's rotation, click .Dr. Joseph Burns, an imaging team member and professor at Cornell University, Ithaca, N.Y. said, "Looking at those big 50 kilometers (31 mile) craters, one has to wonder whether their impact ejecta might be the other tiny moons that orbit Saturn on paths much like Phoebe's." All planned 11 instruments operated as expected and all data was acquired. Scientists plan to use the data to create global maps of the cratered moon, and to determine Phoebe's composition, mass and density. It will take scientists several days to pour over the data to make more concrete conclusions. Cassini came within approximately 2,068 kilometers (about 1,285 miles) of the dark moon on Friday, June 11. The spacecraft was pointing its instruments at the moon during the flyby. Several hours later it turned to point its antenna to Earth. The signal was received through the Deep Space Network antennas in Madrid, Spain and Goldstone, in California's Mojave Desert, at 7:52 a.m. PDT today. Cassini was traveling at a relative speed of 20,900 kilometers per hour (13,000 miles per hour) relative to Saturn. It's been 23 years since a spacecraft last visited Phoebe. The Voyager 2 flyby in 1981 was at a distance from 2.2 million kilometers, (about 1.4 million miles), 1,000 times farther away. With the Phoebe accomplished, Cassini is on course for Saturn. A trajectory correction maneuver is scheduled for June 16. Cassini will conduct a critical 96-minute burn before going into orbit around Saturn on June 30 (July 1 Universal Time). During Cassini's planned four-year tour it will conduct 76 orbits around the Saturn system and execute 52 close encounters with seven of Saturn's 31 known moons. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Colorful threads and shadows of Saturn CASSINI NEWS RELEASEPosted: September 16, 2004 Saturn's faintly banded atmosphere is delicately colored and its threadbare rings cross their own shadows in this marvelous natural color view from Cassini. Credit: NASA/JPL/Space Science InstituteDownload larger image version The planet and its rings would nearly fill the space between Earth and the Moon. Yet, despite their great breadth, the rings are a few meters thick and in some places, very translucent. In this image, we can see through the C ring, which is closest to Saturn, and through the Cassini division, the 4,800-kilometer- (2,980-mile-) wide gap that arcs across the top of the image and separates the optically thick B ring from the A ring. The part of the atmosphere seen through the gap appears darker and more bluish due to scattering at blue wavelengths by the cloud-free upper atmosphere. The different colors in Saturn's atmosphere are due to particles whose composition is yet to be determined. The image was obtained with the Cassini spacecraft narrow angle camera at a distance of 7.6 million kilometers (4.7 million miles) from Saturn. Images taken with red, green and blue filters were combined to create this color view. The image scale is 46 kilometers (28 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Countdown to Phoebe PHOTO RELEASEPosted: June 11, 2004 Credit: NASA/JPL/Space Science InstituteDownload larger image version As Cassini sails toward its rendezvous with Phoebe, details on the small, dark moon are coming into view at a dizzying pace. The images shown here were taken 13 hours apart on Thursday, just one day prior to closest approach. There is a dramatic increase in detail between these two views. Phoebe completes one rotation about its spin axis in nine hours and 16 minutes. We are looking at opposite hemispheres in these two views. A large crater, roughly 50 kilometers (31 miles) across, is visible in the image on the left. The image on the right shows a body heavily pitted with craters of varying sizes, including very large ones, and displaying a substantial amount of variation in surface brightness. Features that appear to be cliffs may be the boundaries between large craters. Despite its exaggerated topography, Phoebe is more round than irregular in shape. Left to right, the two views were obtained at a phase, or Sun-Phoebe spacecraft angle, of 87 degrees, and from distances of 956,000 kilometers (594,000 miles) and 658,000 kilometers (409,000 miles), respectively. The image resolutions are 5.7 and 3.9 kilometers (3.5 to 2.4 miles) per pixel, respectively. To aid visibility, the images were magnified three times via linear interpolation; no contrast enhancement was performed. Phoebe is approximately 220 kilometers (137 miles) wide. On Phoebe, the spin axis points up and approximately 13 degrees to the left of the boundary between day and night. Cassini draws closer to its only flyby of this mysterious outer moon of Saturn. Closest approach to Phoebe will be at 4:56 p.m. EDT (2056 GMT) on June 11. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Crunch, squelch or splash on Saturn's moon Titan? PARTICLE PHYSICS AND ASTRONOMY RESEARCH COUNCIL RELEASEPosted: November 6, 2004The prospect of the Huygens probe landing on a hard, soft or liquid surface when it lands on Titan next January still remain following further analysis of data taken during the Cassini mother ship's closest encounter with Saturn's largest moon during its fly-by on October 26.Commenting on the latest data results and implications for theHuygens probe Mark Leese of the Open University, Programme Manager forScience Surface Package [SSP] instruments that will unravel the mysteriesof Titan said: "It's interesting that all of the possible landingscenarios that we envisaged - a hard crunch onto ice, a softer squelchinto solid organics or a splash-down on a liquid hydrocarbon lake - stillseem to exist on Titan."Leese added, "A first look at the measurements of Titan's atmosphereduring the fly-by suggest that the "Atmosphere Model" we developed andused to design the Huygens probe is valid and all looks good for theprobe release on Christmas day and descent to the surface on 14thJanuary 2005."Further analysis of Titan's upper atmosphere, the thermosphere, hasrevealed a strange brew as Dr Ingo Mueller-Wodarg of Imperial CollegeLondon explained," Our instrument, the Ion Neutral Mass Spectrometer(INMS), made in-situ measurements of atmospheric gases in Titan's upperatmosphere and found a potent cocktail of nitrogen and methane, stirredup with signatures of hydrogen and other hydrocarbons. We are nowworking on a 'Weather Report' for the Huygens landing in January".Commenting on the surface characteristics of Titan Professor JohnZarnecki of the Open University, lead scientist for the Huygens SSPsaid: "The recent results from the fly-by have started to show us a verydiverse and complicated surface. Titan is geologically active but hasn'tyet given up all of its secrets. Combining the visible images withinfrared and RADAR data from this and future fly-bys should help toclarify the picture - but the arrival of the Huygens probe in Januarywill perhaps be the key to unlock these mysteries."Professor Carl Murray, of the Imaging Science System [ISS] team fromQueen Mary, University of London also commented on the surfacefeatures: "The images of the Huygens' landing site returned by the camerasshow a diverse range of features. We see bright and dark areas roughlyaligned in an east-west direction. These are similar to wind streaks seenon Mars and may indicate that material on Titan has been deposited bythe effects of wind blowing across the landscape. All indications suggestthat we are in for a real treat in January when the Huygens probe reachesTitan's surface and returns the first in situ data from this alien world."UK scientists and technologists are amongst an international teamcontinuing to analyse the latest data received from the NASA/ESA/ASICassini Huygens mission after the spacecraft made its close fly-by ofTitan last week. The data has provided a wealth of information aboutSaturn's largest moon, which will not only assist the European SpaceAgency's Huygens team in advance of the probe landing on Titan inJanuary 2005 but will also increase our understanding of the relationshipbetween Titan and its parent planet Saturn.Professor Michele Dougherty from Imperial College is lead scientist onthe Cassini Magnetometer, which is studying the interaction betweenthe plasma in Saturn's magnetosphere and the atmosphere and ionosphereof Titan. "We have been able to model the Magnetometer data very wellfrom the Titan flyby. There does not seem to be an internal magnetic fieldat Titan from the observations we obtained during this flyby, but we willhave a much better idea about this when we have a further flyby inDecember which is on a very similar trajectory. All we can say at thispoint is that if there is a magnetic field generated in the interior ofTitan, then it is very small."Dr Andrew Coates from University College London's Mullard SpaceScience Laboratory, a Co-Investigator on the Cassini ElectronSpectrometer team, said: "We received some remarkable new informationabout Titan's plasma environment within the context of Saturn'sfascinating magnetosphere. Unexpectedly, it looks like we can directly usefeatures of the electron results to understand what Titan's upperatmosphere is made of, supplementing the ion measurements from companionsensors on other instruments. Our electron results contain tell-talefingerprints of photoelectrons and Auger electrons which we will use forthis. Also, the total picture shows how important electrons, raining downon Titan's upper atmosphere, are in helping the feeble sunlight drive thecomplex chemistry in Titan's upper atmosphere."Nick Shave, Space Business Manager at UK IT company LogicaCMG said "Theamazing imagery and radar results recently received from Cassini ofTitan's surface is providing important early information and creatingreal excitement in the industrial community. UK industry's criticalcontributions to Cassini-Huygens via the LogicaCMG Huygens flightsoftware and other systems, such as the parachutes by Martin Baker, willenable even more spectacular science that could help unlock some of thesecrets of life on Earth."UK scientists are playing significant roles in the Cassini Huygensmission with involvement in 6 of the 12 instruments onboard the Cassiniorbiter and 2 of the 6 instruments on the Huygens probe. The UK has thelead role in the magnetometer instrument on Cassini (Imperial College)and the Surface Science Package on Huygens (Open University).UK industry had developed many of the key systems for the Huygensprobe, including the flight software (LogicaCMG) and parachutes (MartinBaker). These mission critical systems need to perform reliably in someof the most challenging and remote environments ever attempted by a manmade object.Titan BackgroundTitan is a highly complex world and is closer to a terrestrial planetthan a moon typical of the outer planetary systems. Titan was first seenby Dutch astronomer Christiaan Huygens (after which the ESA probe isnamed) in 1655.Not only is Titan the largest of Saturn's satellites, it is alsolarger than the planets Mercury and Pluto, and is the second largestsatellite in the solar system (Jupiter's Ganymede being larger). It isthe only satellite in the solar system with appreciable atmosphere,composed mostly of Nitrogen, but also contains aerosols and hydrocarbons,including methane and ethane. Titan's atmosphere was first confirmed in1944 when Gerard Kuiper confirmed the presence of gaseous methane withspectroscopy.Titan's peak surface temperature is about 95 K (-178 degrees C) andsurface pressure is 1.6 Earth atmospheres. At this temperature andpressure, many simple chemicals that are present in abundance (methane,ethane, water, ammonia) provide materials in solid, liquid and gaseousform which may interact to create exotic features on the surface.Precipitation, flowing liquids, lakes and eruptions are all possible.Titan orbits Saturn at a distance of just over 20 Saturn radii(1,222,000 km/759,000 miles) which is far enough to carry the moon inand out of Saturn's magnetosphere. Very little is known about Titan'sinterior structure, including whether it has its own magnetic field.Titan's surface has been difficult to study, as it is veiled by adense hydrocarbon haze that forms in the dense stratosphere as methaneis destroyed by sunlight. From the data collected so far, dark featurescan be seen crossing the equatorial region of Titan, with a large brightregion near longitude 90 degrees now named Xanadu, and possibly a largecrater in the northern hemisphere.The Cassini-Huygens mission is a cooperative project of NASA, theEuropean Space Agency and the Italian Space Agency. The Jet PropulsionLaboratory, a division of the California Institute of Technology inPasadena, manages the Cassini-Huygens mission for NASA's Science MissionDirectorate, Washington, D.C. The Cassini orbiter and its two onboardcameras were designed, developed and assembled at JPL.The Particle Physics and Astronomy Research Council (PPARC) is theUK's strategic science investment agency. It funds research,education and public understanding in four broad areas of science -particle physics, astronomy, cosmology and space science.PPARC is government funded and provides research grants andstudentships to scientists in British universities, gives researchersaccess to world-class facilities and funds the UK membership ofinternational bodies such as the European Organisation for NuclearResearch, CERN, the European Space Agency and the European SouthernObservatory. It also contributes money for the UK telescopes overseas onLa Palma, Hawaii, Australia and in Chile, the UK Astronomy TechnologyCentre at the Royal Observatory, Edinburgh and the MERLIN/VLBI NationalFacility.Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.An insider's view of how Apollo flight controllers operated and just what they faced when events were crucial. Choose your store: | | | | 2014 Spaceflight Now Inc.Encountering Iapetus CASSINI PHOTO RELEASEPosted: January 9, 2004On New Year's Eve 2004, Cassini flew past Saturn's intriguing moon Iapetus, capturing the four visible light images that were put together to form this global view. The scene is dominated by a dark, heavily-cratered region, called Cassini Regio, that covers nearly an entire hemisphere of Iapetus. Iapetus is 1,436 kilometers (892 miles) across. The view is centered on the moon's equator and on roughly 90 degrees west longitude -- a location that always faces the direction of Iapetus's orbital motion around Saturn. Credit: NASA/JPL/Space Science InstituteDownload larger image version Within Cassini Regio, and especially near the equator, dark deposits with a visual reflectivity of only about 4 percent coat nearly everything with remarkable uniformity. However, at latitudes of about 40 degrees, the surface transitions to a much brighter, icy terrain near the pole where the brightest icy materials have reflectivity over 60 percent. However, this region is not uniform: Close inspection reveals that the surface is stained by crudely north-south trending wispy streaks of darker material, typically a few kilometers wide and sometimes tens of kilometers long. An ancient, 400-kilometer wide (250 miles) impact basin appears just above the center of the disc. The basin is heavily overprinted by more recent, smaller impact craters. The basin rim is delineated by steep scarps that descend to the basin floor. Many of these scarps, as well as walls of nearby craters, appear bright, probably due to exposed outcrops of relatively clean ice. Particularly at mid-latitudes, the brightest scarp exposures appear to face away from the equator (i.e. toward the pole). Often, the opposite south-facing scarps are stained with the lower-brightness material. The most unique, and perhaps most remarkable feature discovered on Iapetus in Cassini images is a topographic ridge that coincides almost exactly with the geographic equator. The ridge is conspicuous in the picture as an approximately 20-kilometer wide (12 miles) band that extends from the western (left) side of the disc almost to the day/night boundary on the right. On the left horizon, the peak of the ridge reaches at least 13 kilometers (8 miles) above the surrounding terrain. Along the roughly 1,300 kilometer (800 mile) length over which it can be traced in this picture, it remains almost exactly parallel to the equator within a couple of degrees. The physical origin of the ridge has yet to be explained. It is not yet clear whether the ridge is a mountain belt that has folded upward, or an extensional crack in the surface through which material from inside Iapetus erupted onto the surface and accumulated locally, forming the ridge. The origin of Cassini Regio is a long-standing debate among scientists. One theory proposes that its dark material may have erupted onto Iapetus's icy surface from the interior. Another theory holds that the dark material represented accumulated debris ejected by impact events on dark, outer satellites of Saturn. Details of this Cassini image mosaic do not definitively rule out either of the theories. However, they do provide important new insights and constraints. The uniform appearance of the dark materials at the equator, the apparent thinning and spottiness of the dark materials at progressively higher latitudes and dark wispy streaks near the distal margin of Cassini Regio strongly suggest that dark material was emplaced as a coating. One of the important new results is that no clear evidence can be found that erupted fluids have resurfaced Cassini Regio. The high density of impact craters argues that the terrain underlying the dark coating is relatively ancient and has not been eradicated by its emplacement. Thus, Cassini Regio may have had its origin in plume-style eruptions in which dark particulate materials accumulated on the surface as fallout, perhaps in conjunction with the creation of the equatorial ridge. On the other hand, the dark deposits in Cassini Regio may be a surface coating consistent with, and perhaps more simply explained by, the fall of dark materials from outside. The view has been oriented so that the north pole is toward the top of the picture. Cassini acquired the images in this mosaic with its narrow angle camera on Dec. 31, 2004, at a distance of about 172,400 kilometers (107,124 miles) from Iapetus and at a Sun-Iapetus-spacecraft, or phase, angle of 50 degrees. The image scale is 1 kilometer (0.6 miles) per pixel. The image has been contrast enhanced to aid visibility of surface features. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Eyes on Xanadu CASSINI PHOTO RELEASEPosted: October 25, 2004This image taken on Oct. 24, 2004, reveals Titan's bright "continent-sized" terrain known as Xanadu. It was acquired with the narrow angle camera on Cassini's imaging science subsystem through a spectral filter centered at 938 nanometers, a wavelength region at which Titan's surface can be most easily detected. The surface is seen at a higher contrast than in previously released imaging science subsystem images due to a lower phase angle (Sun-Titan-Cassini angle), which minimizes scattering by the haze. Credit: NASA/JPL/Space Science InstituteThe image shows details about 10 times smaller than those seen from Earth. Surface materials with different brightness properties (or albedos) rather than topographic shading are highlighted. The image has been calibrated and slightly enhanced for contrast. It will be further processed to reduce atmospheric blurring and to optimize mapping of surface features. The origin and geography of Xanadu remain mysteries at this range. Bright features near the south pole (bottom) are clouds. On Oct. 26, Cassini will acquire images of features in the central-left portion of this image from a position about 100 times closer. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.First Huygens images show strange new world BY WILLIAM HARWOOD
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This raises a bunch of new questions about the future of Fannie and Freddie. There's been a lot of talk in Washington about shifting the role the two companies have in the mortgage market and bringing private companies back to the secondary-mortgage-market plate. Now that Fannie and Freddie are operating as government cash cows, with all their profits going into a general fund that the Treasury may spend as it pleases, it might be harder for the government to give them up.(MoneyWatch) It may surprise you that, as of its last reporting date, there were 352 mutual funds that are classified by Morningstar as bond funds that actually held stocks in their portfolio. (I know I was surprised, and given my 40 years of experience in the investment banking and financial advisory business, it takes quite a bit to surprise me.) At the end of 2012, it was 312, up from 283 nine months earlier.
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SCHIEFFER: Today only on Face the Nation, White House chief of staff, Denis McDonough. As the president's top aide sits down with us this morning, there's no shortage of things to talk about -- the decision to give military aid to the Syrian rebels, the national security leaks, possible scandals brewing in the State Department, and a lot more. We'll get reaction from the chairman of the house intelligence committee, Mike Rogers. Plus, analysis from an all-star panel, including Barton Gellman, who broke the story of those national security leaks in the "Washington Post," the managing editor of "Time" magazine, Rick Stengel, "Wall Street Journal" columnist Peggy Noonan and David Corn of "Mother Jones." It's all ahead because this is Face the Nation.
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Update: An earlier version of this story reported that Battleground Texas has raised $36 million; that figure has not been reported publicly by the group. However, Battleground Texas officials have reportedly said they expect to spend tens of millions over the next decade.(CBS/AP) HOUSTON - The death of 3-year-old Lee'onna Ramirez remained hidden for a year as Houston authorities say her mother kept them at bay with conflicting stories on the child's whereabouts.
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"The original test flight philosophy was to have two flights with the daylight launch, which was STS-114 and STS-121," he said. "We elected, and it was largely my decision, to extend the daylight planning requirement for one more flight, STS-115. There seemed to be a number of reasons why that would be an interesting and good thing to do.
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Selected as one of the first six Canadian astronauts in December 1983, MacLean began astronaut training in February 1984. From 1987 to 1993 MacLean was the Program Manager for the Advanced Space Vision System (ASVS), a computer-based camera system designed to provide guidance data that enhances the control of both Canadarm and Canadarm2. From 1988 to 1991 he also assumed the role of Astronaut Advisor to the Strategic Technologies in Automation and Robotics (STEAR) Program.
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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: November 25, 2008Work to replace bearings and re-lubricate the space station's damaged right-side solar array rotary joint went better than expected, a senior manager said today, resulting in remarkably smooth operation that may permit the agency to forego building, launching and installing costly replacement hardware.Space station Program Manager Mike Suffredini also said the station's newly installed water recycling system, including an initially cantankerous urine distillation assembly, appears to be operating normally and that the Endeavour astronauts will be able to bring some six liters of processed urine and condensate back to Earth for chemical analysis, more than engineers expected before launch."When we went into this mission, we said there were two primary objectives we needed to take care of," Suffredini said. "One was to repair the SARJ (solar alpha rotary joint) and prepare the port SARJ for continued operations. And of course, the other major objective was to get started on our regenerative ECLSS (environmental control and life support) system, get it going in preparation for six-crew operations in the May timeframe. I'm happy to report today that we're well on our way in both of those cases."Early today, flight controllers activated the right-side solar alpha rotary joint and commanded it to operate in normal "auto-track" mode for two full orbits. In auto-track, the station's two SARJ mechanisms rotate outboard solar arrays like huge paddle wheels to keep them face on to the sun.Engineers first noticed problems with the starboard SARJ last year when sensors measured increased vibration levels and power usage in the drive motor. Inspections by spacewalking astronauts later showed one of the gear's three bearing races was heavily damaged, apparently because of a lubrication breakdown that generated extensive metallic contamination.One of the 12 trundle bearings that grip the gear was replaced last June to help engineers troubleshoot the problem. During parts of four spacewalks, the Endeavour astronauts replaced 10 bearing assemblies and re-installed the 11th, cleaned off the metallic debris and re-lubricated all three races.Going into the flight, Suffredini said engineers believed the outer canted bearing race was too damaged to permit resumption of around-the-clock auto-track operations. The goal was to lower vibration and friction levels enough to permit periodic operations to boost power when needed.But it now appears the bearing swap-out and re-lubrication might permit more routine operations than originally expected. That's a major issue as NASA transitions to full-time operations with an expanded crew of six and a full slate of experiments that require all the power the lab's solar arrays can generate.Along with bringing the old bearings down for a comprehensive failure analysis, the goal of the servicing work was to "clean up the race and lubricate it and see what we could do about reducing the currents on the motor to drive this joint (and) to see if we could reduce the vibrations," Suffredini said. "One of the things that's not immediately obvious to you is the vibrations induced?by rotating this joint had the potential to put extensive life (reduction) on the structure. So that was another big driver for not operating in auto track."And so we performed both of those tasks and we found that the current dropped dramatically, in fact the currents are now much, much closer to where they were when we started off," he said. "We've seen as low as 0.17 amps since we lubricated it. It was as high as 0.7 to 0.9 in some cases. These are the peak numbers, we average the lower numbers. This particular joint, when it first started out, was operating at about 0.15 amps. So you can see the data is suggesting we're awfully close to our original drive currents."We took vibration data that we're looking at now. So I can't tell you what that data tells us, but I can tell you anecdotally, one of the ways we discovered this problem, one of the cameras on the starboard truss would vibrate, you could look at an image with this camera and you'd see it vibrate when the joint was rotating. And that particular camera is still now. So if you want to take that as an indication that we reduced vibrations, we certainly have."Suffredini said it will take weeks of engineering analysis and additional auto-track test runs to fully characterize the behavior of the joint. But if the initial results hold up, the agency may be able to stop work on a long-range plan to build a new bearing race that would be launched on the last planned shuttle mission and installed over multiple spacewalks."If, in fact, we could keep the currents down through a lubrication process that's not extensive, that we wouldn't have to do every three or four months but maybe once every year or two, perhaps we could choose that avenue as opposed to replacing that race," he said. "So this is a very positive step for us. It's very possible we could save ourselves quite a bit of time and effort and get this joint in auto-track sooner than we had hoped."The Endeavour astronauts also lubricated the station's port SARJ. That mechanism has been operating normally, but engineers wanted to add fresh lubrication to prevent problems like those experienced by the starboard joint. The astronauts reported seeing signs of very slight damage on one bearing race, but Suffredini said it appeared to be normal wear and tear.As for the urine processor, Suffredini said it appears the removal of rubber vibration isolators and additional work to hard mount the distillation assembly to its mounting bracket paid off. Initial startup problems appear to be related to subtle harmonic effects as an internal centrifuge spins in a vacuum distillation assembly. The vibration dampers were put in place to reduce noise, but taking them off apparently prevented the motions that contributed to an unwanted balance issue, allowing the system to operate in a more normal fashion."So now we believe where we are is that we'll keep the distillation assembly on orbit and we will look to methods to mount it perhaps a little stiffer to the structure, we'll see if there's anything we want to do different, if we want to perhaps build some sort of bracket we bring to orbit to stiffen up the structure," Suffredini said. "We may choose to do that. But right now, the thinking is we'll probably leave this distillation assembly on orbit and we'll nurse it along the way we have been and learn from the system."Today, the astronauts hooked up a potable water dispenser that is connected to the same water "bus" as the water recycling gear. A new toilet will be connected to the bus after the shuttle departs, routing urine to the processor for conversion into pure water for drinking, food preparation, personal hygiene and oxygen generation.Flight Director Holly Ridings said the astronauts will bring down about six liters of processed water for detailed chemical analysis to determine purity and to help calibrate an analyzer on the space station. No one will drink any processed water until after additional samples are brought down next February.Assuming the equipment continues working normally, NASA will be clear to boost crew size to six next May as planned.Additional coverage for subscribers:VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING UPWARD VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING INBOARD VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING DOWNWARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING UPWARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING INBOARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING DOWNWARD VIDEO:MINNEAPOLIS, PORTLAND, PHILLY INTERVIEWS WITH CREW VIDEO:TUESDAY'S MISSION STATUS BRIEFING VIDEO:TUESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 11 HIGHLIGHTS MOVIE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:NEW EXTERNAL TV CAMERA MOUNTED TO STATION VIDEO:FINISHING THE STARBOARD SARJ CLEANING VIDEO:PREVENTIVE MAINTENANCE ON PORT SARJ VIDEO:KIMBROUGH FLOATS OUT OF THE AIRLOCK VIDEO:MONDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 10 HIGHLIGHTS MOVIE VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:INTERVIEWS WITH CREW BY ABC, CBS AND NBC NEWS VIDEO:SUNDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 9 HIGHLIGHTS MOVIE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:LAST OF OLD BEARINGS REMOVED FROM SARJ VIDEO:BOWEN INSTALLS ANOTHER BEARING ASSEMBLY VIDEO:SARJ CLEANING TECHNIQUES TO REMOVE CONTAMINATION VIDEO:PIPER USES GREASE GUNS ON THE SARJ VIDEO:NEW TRUNDLE BEARING ASSEMBLY INSTALLED VIDEO:SPACEWALKING DUO GETS TO WORK VIDEO:SPACEWALK NO. 3 BEGINS VIDEO:WALKTHROUGH OF SPACEWALK NO. 3 PLAN VIDEO:SATURDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 8 HIGHLIGHTS MOVIE VIDEO:FRIDAY'S MISSION STATUS BRIEFING VIDEO:JOINT CREW IN-FLIGHT NEWS CONFERENCE VIDEO:FRIDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:PROTON ROCKET ROLLS OUT TO THE PAD VIDEO:LAUNCH OF THE ZARYA CONTROL MODULE VIDEO:POST-LAUNCH COMMENTS BY NASA AND RSA VIDEO:SHUTTLE AND STATION COMMANDERS MARK ANNIVERSARY VIDEO:FLIGHT DAY 7 HIGHLIGHTS MOVIE VIDEO:THURSDAY'S MISSION STATUS BRIEFING VIDEO:MAINTENANCE PERFORMED ON STATION'S ARM VIDEO:SPACEWALKERS PULL SECOND RAIL CART FREE VIDEO:FIRST CART REMOVED FROM STATION RAILS VIDEO:THURSDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:WALKTHROUGH OF SPACEWALK NO. 2 PLAN VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 7 VIDEO:VIDEO:FLIGHT DAY 6 HIGHLIGHTS MOVIE VIDEO:WEDNESDAY'S MISSION STATUS BRIEFING VIDEO:AP, MINNEAPOLIS AND BOSTON INTERVIEWS WITH CREW VIDEO:WEDNESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 5 HIGHLIGHTS MOVIE VIDEO:RIDE ALONG WITH ASTRONAUTS "RACK-CAM" VIDEO:COMBUSTION SCIENCE HARDWARE MOVED INTO STATION VIDEO:AIRLOCK CAMCORDER FOOTAGE AFTER SPACEWALK VIDEO:TUESDAY'S MISSION STATUS BRIEFING VIDEO:EVA NO. 1 CONCLUDES VIDEO:SOLAR ALPHA ROTARY JOINT REPAIRS BEGIN VIDEO:TOOL BAG ACCIDENTALLY FLOATS AWAY VIDEO:GREASE GUN SPILL MAKES MESS IN TOOL CARRIER VIDEO:SPARE FLEX HOSE COUPLER DELIVERED TO STATION VIDEO:EMPTY NITROGEN TANK MOVED FROM STATION TO SHUTTLE VIDEO:TUESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:SHOW-AND-TELL OF SOLAR ALPHA ROTARY JOINT WORK VIDEO:WALKTHROUGH OF SPACEWALK NO. 1 PLAN VIDEO:NARRATED ANIMATION OF SPACEWALK SWAPOUT VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 5 VIDEO:FLIGHT DAY 4 HIGHLIGHTS MOVIE VIDEO:CREW OPENS HATCH AND ENTERS LEONARDO VIDEO:ATLANTA AND BOSTON TV STATIONS INTERVIEW CREW VIDEO:MONDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:LEONARDO MODULE SUCCESSFULLY MOUNTED TO STATION VIDEO:MONDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:PREVIEW ANIMATION OF LEONARDO MODULE ATTACHMENT VIDEO:SUMMARY OF CARGO BEING DELIVERED TO SPACE STATION VIDEO:FLIGHT DAY 3 HIGHLIGHTS MOVIE VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:SHUTTLE CREW WELCOMED ABOARD STATION VIDEO:SPACE SHUTTLE ENDEAVOUR DOCKS TO SPACE STATION VIDEO:ENDEAVOUR PERFORMS THE 360-DEGREE BACKFLIP VIDEO:VIEWS OF THE SHUTTLE APPROACHING FROM BELOW VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 3 VIDEO:PREVIEW ANIMATION OF RENDEZVOUS AND DOCKING VIDEO:FLIGHT DAY 2 HIGHLIGHTS MOVIE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:SATURDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 2 VIDEO:PREVIEW ANIMATION OF HEAT SHIELD INSPECTIONS VIDEO:NARRATED TOUR OF ENDEAVOUR'S PAYLOAD BAY VIDEO:FLIGHT DAY 1 HIGHLIGHTS MOVIE VIDEO:SPACE SHUTTLE ENDEAVOUR BLASTS OFF! VIDEO:SPACEFLIGHT NOW'S LAUNCH PAD CAMERA VIDEO:THE FULL STS-126 LAUNCH EXPERIENCE VIDEO:INSIDE MISSION CONTROL DURING LAUNCH VIDEO:POST-LAUNCH NEWS BRIEFING VIDEO:FINAL PRE-LAUNCH POLLS GIVE "GO" FOR LIFTOFF VIDEO:SHUTTLE'S CREW MODULE HATCH CLOSED FOR FLIGHT VIDEO:MISSION SPECIALIST DON PETTIT BOARDS VIDEO:MISSION SPECIALIST SHANE KIMBROUGH BOARDS VIDEO:PILOT ERIC BOE BOARDS ENDEAVOUR VIDEO:COMMANDER CHRIS FERGUSON BOARDS ENDEAVOUR VIDEO:ASTROVAN TAKES CREW TO LAUNCH PAD 39A VIDEO:CREW DEPARTS QUARTERS FOR LAUNCH PAD VIDEO:ASTRONAUTS DON SPACESUITS FOR LAUNCH VIDEO:NARRATED RECAP OF ENDEAVOUR'S PRE-FLIGHT CAMPAIGN VIDEO:NARRATED RECAP OF PAYLOADS' PRE-FLIGHT CAMPAIGN VIDEO:PAD 39A SERVICE GANTRY RETRACTED FOR LAUNCH VIDEO:THURSDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:WEDNESDAY'S PRE-LAUNCH NEWS CONFERENCE VIDEO:ENDEAVOUR ASTRONAUTS ARRIVE FOR LAUNCH VIDEO:TUESDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:STATION ASTRONAUTS PREPARE FOR SHUTTLE ARRIVAL VIDEO:ENDEAVOUR'S PAYLOADS READIED FOR TREK TO SPACE VIDEO:UPDATE ON SHUTTLE AND STATION PROGRAMS VIDEO:STS-126 MISSION OVERVIEW VIDEO:PREVIEW BRIEFING ON MISSION'S SPACEWALKS VIDEO:THE ASTRONAUTS' PRE-FLIGHT NEWS BRIEFING VIDEO:INTERVIEW WITH COMMANDER CHRIS FERGUSON VIDEO:INTERVIEW WITH PILOT ERIC BOE VIDEO:INTERVIEW WITH MS1 HEIDEMARIE PIPER VIDEO:INTERVIEW WITH MS2 STEPHEN BOWEN VIDEO:INTERVIEW WITH MS3 DON PETITT VIDEO:INTERVIEW WITH MS4 SHANE KIMBROUGH VIDEO:INTERVIEW WITH MS5 SANDY MAGNUS VIDEO:INTERVIEW WITH SPACE STATION'S EXPEDITION 17 CREW VIDEO:ENDEAVOUR COMMANDER AND PILOT PRACTICE LANDINGS VIDEO:ISS PROGRAM MANAGER UPDATES SOYUZ INVESTIGATION VIDEO:ISS PROGRAM MANAGER DESCRIBES SARJ REPAIR PLAN VIDEO:ISS PROGRAM MANAGER DISCUSSES RADIATOR DAMAGE VIDEO:EXPEDITION 18 PRE-FLIGHT MISSION BRIEFING VIDEO:AERIAL VIEWS OF ATLANTIS AND ENDEAVOUR VIDEO:ENDEAVOUR AT SUNRISE ON LAUNCH PAD 39B VIDEO:AERIAL VIEWS OF ENDEAVOUR AFTER ROLLOUT VIDEO:ENDEAVOUR ROLLS FROM VAB TO LAUNCH PAD VIDEO:TIME-LAPSE MOVIE OF ARRIVAL AT PAD 39B VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR LEAVING VAB VIDEO:SHUTTLE HOISTED FOR ATTACHMENT TO TANK VIDEO:ENDEAVOUR'S DEPARTURE FROM HANGAR VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR GOING VERTICAL VIDEO:TIME-LAPSE MOVIE OF BEING HOISTED OFF TRANSPORTER VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR MOVING TO VAB MORE:John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA's Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Station cargo ship launches; antenna glitch fixed BY SPACEFLIGHT NOWPosted: November 26, 2008;Updated with antenna resolutionSporting an enhanced computer control system and loaded with food, supplies and holiday gifts, a Russian cargo-delivery spacecraft was launched toward the international space station this morning. Credit: EnergiaThe robotic Progress M-01M freighter was put into orbit by a three-stage Soyuz booster following a 7:38 a.m. EST liftoff from the Baikonur Cosmodrome and 9-minute ascent over Asia.Onboard commands then extended the Progress craft's two power-generating solar arrays to span 35 feet and unfurled communications and navigation antennas. However, one of those antennas initially did not deploy as planned."One of several antennas associated with the Kurs automated rendezvous system apparently did not deploy. The Progress passed out of range of Russian ground stations before all of the data from the initial post-insertion analysis could be received," NASA spokesman John Ira Petty said from Mission Control shortly after launch."Russian flight controllers will review data in the hours ahead. They are aiming at determining whether troubleshooting may be required on that antenna. The suspect antenna in question is one of two narrow field proximity antennas used for range and rate updates to the Progress computers through the final stage of its approach for docking at the Pirs Docking Compartment."But by noon EST, Mission Control-Houston announced a second attempt to deploy the antenna was successful. This is the 31st such Russian-made craft sent to the station. But it's the first in a new series equipped with a new state-of-the-art onboard computer system and more-compact radiotelemetry hardware.The updated vessels weigh 165 pounds less, allowing more cargo to be carried, and have 15 fewer parts, according to builder RSC Energia."The computer system performance has increased. Automatic diagnostics is provided for the means of direct communication between telemetry system and computer system elements. Communications of the spacecraft with ISS over standard digital interfaces has been provided, which allows integrating all the spacecraft systems into the space station infrastructure," the company said.Today's launch, known in the station's assembly matrix as Progress mission 31P, will deliver two-and-a-half tons of supplies to the station. The "dry" cargo packed aboard the Progress amounts to 2,963 pounds in the form of spare parts, life support gear, equipment hardware and holiday presents for the station's crew. The refueling module carries 1,808 pounds of propellant for transfer into the Russian segment of the complex to feed the station's maneuvering thrusters. And the vessel has 108 pounds of oxygen and air, plus 463 pounds of water to replenish the station's supplies. Docking to the station's Pirs module is planned for Sunday at 7:23 a.m. EST, just six hours before space shuttle Endeavour lands.Expedition 18 flight engineer Yury Lonchakov will be standing by to manually dock the Progress if the automated system experiences a problem. The cosmonaut is living aboard the station along with commander Mike Fincke and science officer Sandy Magnus.Additional coverage for subscribers:VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING UPWARD VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING INBOARD VIDEO:LEFT-HAND BOOSTER CAMERA LOOKING DOWNWARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING UPWARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING INBOARD VIDEO:RIGHT-HAND BOOSTER CAMERA LOOKING DOWNWARD VIDEO:ANIMATION OF LEONARDO MODULE'S DETACHMENT VIDEO:WEDNESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 12 HIGHLIGHTS MOVIE VIDEO:MINNEAPOLIS, PORTLAND, PHILLY INTERVIEWS WITH CREW VIDEO:TUESDAY'S MISSION STATUS BRIEFING VIDEO:TUESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 11 HIGHLIGHTS MOVIE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:NEW EXTERNAL TV CAMERA MOUNTED TO STATION VIDEO:FINISHING THE STARBOARD SARJ CLEANING VIDEO:PREVENTIVE MAINTENANCE ON PORT SARJ VIDEO:KIMBROUGH FLOATS OUT OF THE AIRLOCK VIDEO:MONDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 10 HIGHLIGHTS MOVIE VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:INTERVIEWS WITH CREW BY ABC, CBS AND NBC NEWS VIDEO:SUNDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 9 HIGHLIGHTS MOVIE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:LAST OF OLD BEARINGS REMOVED FROM SARJ VIDEO:BOWEN INSTALLS ANOTHER BEARING ASSEMBLY VIDEO:SARJ CLEANING TECHNIQUES TO REMOVE CONTAMINATION VIDEO:PIPER USES GREASE GUNS ON THE SARJ VIDEO:NEW TRUNDLE BEARING ASSEMBLY INSTALLED VIDEO:SPACEWALKING DUO GETS TO WORK VIDEO:SPACEWALK NO. 3 BEGINS VIDEO:WALKTHROUGH OF SPACEWALK NO. 3 PLAN VIDEO:SATURDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 8 HIGHLIGHTS MOVIE VIDEO:FRIDAY'S MISSION STATUS BRIEFING VIDEO:JOINT CREW IN-FLIGHT NEWS CONFERENCE VIDEO:FRIDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:PROTON ROCKET ROLLS OUT TO THE PAD VIDEO:LAUNCH OF THE ZARYA CONTROL MODULE VIDEO:POST-LAUNCH COMMENTS BY NASA AND RSA VIDEO:SHUTTLE AND STATION COMMANDERS MARK ANNIVERSARY VIDEO:FLIGHT DAY 7 HIGHLIGHTS MOVIE VIDEO:THURSDAY'S MISSION STATUS BRIEFING VIDEO:MAINTENANCE PERFORMED ON STATION'S ARM VIDEO:SPACEWALKERS PULL SECOND RAIL CART FREE VIDEO:FIRST CART REMOVED FROM STATION RAILS VIDEO:THURSDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:WALKTHROUGH OF SPACEWALK NO. 2 PLAN VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 7 VIDEO:VIDEO:FLIGHT DAY 6 HIGHLIGHTS MOVIE VIDEO:WEDNESDAY'S MISSION STATUS BRIEFING VIDEO:AP, MINNEAPOLIS AND BOSTON INTERVIEWS WITH CREW VIDEO:WEDNESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:FLIGHT DAY 5 HIGHLIGHTS MOVIE VIDEO:RIDE ALONG WITH ASTRONAUTS "RACK-CAM" VIDEO:COMBUSTION SCIENCE HARDWARE MOVED INTO STATION VIDEO:AIRLOCK CAMCORDER FOOTAGE AFTER SPACEWALK VIDEO:TUESDAY'S MISSION STATUS BRIEFING VIDEO:EVA NO. 1 CONCLUDES VIDEO:SOLAR ALPHA ROTARY JOINT REPAIRS BEGIN VIDEO:TOOL BAG ACCIDENTALLY FLOATS AWAY VIDEO:GREASE GUN SPILL MAKES MESS IN TOOL CARRIER VIDEO:SPARE FLEX HOSE COUPLER DELIVERED TO STATION VIDEO:EMPTY NITROGEN TANK MOVED FROM STATION TO SHUTTLE VIDEO:TUESDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:SHOW-AND-TELL OF SOLAR ALPHA ROTARY JOINT WORK VIDEO:WALKTHROUGH OF SPACEWALK NO. 1 PLAN VIDEO:NARRATED ANIMATION OF SPACEWALK SWAPOUT VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 5 VIDEO:FLIGHT DAY 4 HIGHLIGHTS MOVIE VIDEO:CREW OPENS HATCH AND ENTERS LEONARDO VIDEO:ATLANTA AND BOSTON TV STATIONS INTERVIEW CREW VIDEO:MONDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:LEONARDO MODULE SUCCESSFULLY MOUNTED TO STATION VIDEO:MONDAY MORNING FLIGHT DIRECTOR INTERVIEW VIDEO:PREVIEW ANIMATION OF LEONARDO MODULE ATTACHMENT VIDEO:SUMMARY OF CARGO BEING DELIVERED TO SPACE STATION VIDEO:FLIGHT DAY 3 HIGHLIGHTS MOVIE VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:SHUTTLE CREW WELCOMED ABOARD STATION VIDEO:SPACE SHUTTLE ENDEAVOUR DOCKS TO SPACE STATION VIDEO:ENDEAVOUR PERFORMS THE 360-DEGREE BACKFLIP VIDEO:VIEWS OF THE SHUTTLE APPROACHING FROM BELOW VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 3 VIDEO:PREVIEW ANIMATION OF RENDEZVOUS AND DOCKING VIDEO:FLIGHT DAY 2 HIGHLIGHTS MOVIE VIDEO:SATURDAY'S MISSION STATUS BRIEFING VIDEO:SATURDAY'S MISSION MANAGEMENT TEAM UPDATE VIDEO:FLIGHT DIRECTOR'S SUMMARY OF FLIGHT DAY 2 VIDEO:PREVIEW ANIMATION OF HEAT SHIELD INSPECTIONS VIDEO:NARRATED TOUR OF ENDEAVOUR'S PAYLOAD BAY VIDEO:FLIGHT DAY 1 HIGHLIGHTS MOVIE VIDEO:SPACE SHUTTLE ENDEAVOUR BLASTS OFF! VIDEO:SPACEFLIGHT NOW'S LAUNCH PAD CAMERA VIDEO:THE FULL STS-126 LAUNCH EXPERIENCE VIDEO:INSIDE MISSION CONTROL DURING LAUNCH VIDEO:POST-LAUNCH NEWS BRIEFING VIDEO:FINAL PRE-LAUNCH POLLS GIVE "GO" FOR LIFTOFF VIDEO:SHUTTLE'S CREW MODULE HATCH CLOSED FOR FLIGHT VIDEO:MISSION SPECIALIST DON PETTIT BOARDS VIDEO:MISSION SPECIALIST SHANE KIMBROUGH BOARDS VIDEO:PILOT ERIC BOE BOARDS ENDEAVOUR VIDEO:COMMANDER CHRIS FERGUSON BOARDS ENDEAVOUR VIDEO:ASTROVAN TAKES CREW TO LAUNCH PAD 39A VIDEO:CREW DEPARTS QUARTERS FOR LAUNCH PAD VIDEO:ASTRONAUTS DON SPACESUITS FOR LAUNCH VIDEO:NARRATED RECAP OF ENDEAVOUR'S PRE-FLIGHT CAMPAIGN VIDEO:NARRATED RECAP OF PAYLOADS' PRE-FLIGHT CAMPAIGN VIDEO:PAD 39A SERVICE GANTRY RETRACTED FOR LAUNCH VIDEO:THURSDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:WEDNESDAY'S PRE-LAUNCH NEWS CONFERENCE VIDEO:ENDEAVOUR ASTRONAUTS ARRIVE FOR LAUNCH VIDEO:TUESDAY'S COUNTDOWN STATUS AND WEATHER UPDATE VIDEO:STATION ASTRONAUTS PREPARE FOR SHUTTLE ARRIVAL VIDEO:ENDEAVOUR'S PAYLOADS READIED FOR TREK TO SPACE VIDEO:UPDATE ON SHUTTLE AND STATION PROGRAMS VIDEO:STS-126 MISSION OVERVIEW VIDEO:PREVIEW BRIEFING ON MISSION'S SPACEWALKS VIDEO:THE ASTRONAUTS' PRE-FLIGHT NEWS BRIEFING VIDEO:INTERVIEW WITH COMMANDER CHRIS FERGUSON VIDEO:INTERVIEW WITH PILOT ERIC BOE VIDEO:INTERVIEW WITH MS1 HEIDEMARIE PIPER VIDEO:INTERVIEW WITH MS2 STEPHEN BOWEN VIDEO:INTERVIEW WITH MS3 DON PETITT VIDEO:INTERVIEW WITH MS4 SHANE KIMBROUGH VIDEO:INTERVIEW WITH MS5 SANDY MAGNUS VIDEO:INTERVIEW WITH SPACE STATION'S EXPEDITION 17 CREW VIDEO:ENDEAVOUR COMMANDER AND PILOT PRACTICE LANDINGS VIDEO:ISS PROGRAM MANAGER UPDATES SOYUZ INVESTIGATION VIDEO:ISS PROGRAM MANAGER DESCRIBES SARJ REPAIR PLAN VIDEO:ISS PROGRAM MANAGER DISCUSSES RADIATOR DAMAGE VIDEO:EXPEDITION 18 PRE-FLIGHT MISSION BRIEFING VIDEO:AERIAL VIEWS OF ATLANTIS AND ENDEAVOUR VIDEO:ENDEAVOUR AT SUNRISE ON LAUNCH PAD 39B VIDEO:AERIAL VIEWS OF ENDEAVOUR AFTER ROLLOUT VIDEO:ENDEAVOUR ROLLS FROM VAB TO LAUNCH PAD VIDEO:TIME-LAPSE MOVIE OF ARRIVAL AT PAD 39B VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR LEAVING VAB VIDEO:SHUTTLE HOISTED FOR ATTACHMENT TO TANK VIDEO:ENDEAVOUR'S DEPARTURE FROM HANGAR VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR GOING VERTICAL VIDEO:TIME-LAPSE MOVIE OF BEING HOISTED OFF TRANSPORTER VIDEO:TIME-LAPSE MOVIE OF ENDEAVOUR MOVING TO VAB MORE:Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA's first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Station solar joint cleaning continues on today's EVA BY WILLIAM HARWOOD
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Last year she appeared in The Last of the Haussmans, direction and undone by some baffling selections by coach Philippe Saint Andre. Sunday matches all TV driven but something is unquestionably lost in intensity for both spectators and players. Gordon Brown thanked him for his loyal service by sending him to the Upper House last year. they will be digging their own graves. referee Terry OConnor did the sensible and humane thing by stopping the fight with just one second of the round remaining. earn a rematch with Burns further down the line. initially used to fly French combat forces to Mali and now being used to deliver troops from West Africa. If you train and assist the Malian people in their own region then you are less likely to have to bring in British forces to do the fighting. is the last major symbol of cooperation between Seoul and Pyongyang.
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According to Sean Joyce, the Deputy Director of the FBI, and General Keith Alexander, Director of the National Security Agency, more than 50 attack plots were discovered and derailed thanks to the NSA data. Alexander said information surrounding those plots would be laid out to Congress on Wednesday in a classified setting, but Joyce was able to discuss four in public.
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These cookies allow us to distinguish you from other users of our website, The cookies we use are "analytical" cookies. Brulle has authored numerous articles and book chapters on environmental science,S. The cookies we use are "analytical" cookies. A cookie is a small file of letters and numbers that we put on your computer if you agree. comparability, healthcare and database marketing. East Lansing, Monetary policy and stock prices with limited asset market participation Canadian Economics Association 2010 : Quebec City.
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"And companies now ... are trying to measure that. They're trying to quantify how well people can create buzz. And as you can imagine, a lot of big companies and brands want to be all over this. They want to find powerful word of mouth influencers and reward them and give them stuff. I mean, lots of great stuff like trips and gaming systems."
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Even drivers motivated by pure self-interest may want to take a look. The natural gas model lets even solo commuters hop into the fast High Occupancy Vehicle lanes in two of the most congested areas in the country: Southern California and the Northern Virginia suburbs of Washington, D.C. And if you use the Civic Natural Gas to commute, you might be able to install a home refill station in your garage using the natural gas supply that you have for your stove or other appliances. Prices for such overnight refills often cost about half the price of natural gas refill stations.
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The diamond texture enables the hard cases to be virtually scratch-proof; a concept unheard of in the world of polycarbonate hard shells. In fact, it's so textured that you can jab at it with a pair of scissor and there will be few marks that are easily wiped off with a cloth. All wheels are anti-shock. Ball-bearing wheels mean that no matter how heavy you pack it, the wheels stay centered. These are considered to be among the lightest cases in the market. Even the 27 inch weighs only 10.4 pounds. The smallest case in this line, the 20-inch business case, starts from $415, while the massive 31-inch trolley is $785.(MoneyWatch) Neuroscience is all the rage these days, promising to solve the problems of why diets don't work, why teenagers are inarticulate and why we crave donuts when we are tired. In some of these cases, the promise is genuine and the learning is practical. But in the farther reaches of neuroscience -- neuroeconomics, for example, and neuroleadership -- the claims to have achieved a mechanical, deterministic understanding of the brain that can change behaviors and outcomes is wildly misleading.
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including in food retailing, 29 May 2013He was the pride of Britain last year after winning the US Open and the gold in the London Olympics men's singles. because in the immediate aftermath of winning I wasnt unbelievably happy. 1960, 1930, her sixth in total, which she had herself attended instead of going to the approved facility she had originally supposed to be going to in New York.We did it the hard way, the back room staff,The segment has generated criticism on social media but volunteer Wendy defended the unusual exchange.
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A former wing commander, a former group commander and three former squadron commanders, as well as a senior noncommissioned officer, were disciplined last fall after an investigation into instructor sexual misconduct at Joint Base San Antonio-Lackland, said Maj. Lori Hodge, a spokeswoman for the Air Education and Training Command.
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Nanjing activist blogger He Peirong, who was instrumental in helping Chen escape from house arrest, said she was "very happy" to hear that Chen and his family were on their way to the United States.
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Still, she said, "If that's all the president's' going to say tomorrow [on drone strikes], there are going to be a lot of disappointed people and groups around the world, especially Pakistan, where they're expecting the president to say we're going to end attacks in that country."CHICAGO Drug overdose deaths rose for the 11th straight year, federal data show, and most of them were accidents involving addictive painkillers despite growing attention to risks from these medicines.
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Hillary Rodham grandit sous l?utorit?conservatrice de son p?e r?ublicain. una dittatura dei? il regista di Submarine. cette nouvelle change la donne. Hier "Meilleure photographie" et "Meilleurs costumes". ) Perch? tipicit?del prodotto,il pi?odioso libello di propaganda razzista e antisemita dell?poca notamment dans des minis?ies ?succ?. très loin.
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40, considering Seeking Alpha about 4 million visitors per month from the US alone. get rid of those tickers and sparklines and constant reminders of what the market did today. the holdout states might decide that the carrot of new federal money is too tempting to resist, many conservatives, 'This decision demonstrates how difficult is for hosts and even companies like ours to adequately understand laws that were not meant to apply to regular people hosting to make ends meet. but the rule has now been used against a resident for the first time.How can you stop the tickets being bought by GM residents who get a decent wage but dont want to pay full price? The full MIF13 programme will be announced on Thursday 28 February. It is still unclear whether the approach will work ? but it reflects new political realities in Africa.
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The U.S. will be sending technical advisers to the Syrian National Coalition offices in Cairo to oversee and help them spend the money for good governance and rule of law. The advisers will be from non-governmental organizations and other groups that do this kind of work.
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A U.S. troops gear up for another fighting season with their Afghan partners, the idea of an American withdrawal seems a distant idea.KABUL, Afghanistan ? Several thousand university students are demonstrating in eastern Afghanistan to denounce Israel's recent offensive in Gaza, burning Israeli and U.S. flags, as well as a Christian cross.
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"There is nothing in this data that says the economy is falling back," said Joel Naroff, chief economist at Naroff Economic Advisors.
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HONG KONG The former CIA employee who suddenly burst into headlines around the globe by revealing himself as the source of top-secret leaks about U.S. surveillance programs has just as quickly gone underground again.
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"No. Of course, it's not normal," she replied. "...it was when she was little, we went to the doctors, of course. And they didn't find anything."
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Di tutt'altro avviso ?Bobo Craxi,I gioielli di Evita Peron All?otel del ritrovamento Gérard Depardieu (alias Obélix) est arrivé,5% rispetto al 2011 Lo rilasciano al metr?di Molino Dorino.45 m. Randy Phillips. alle Eolie, le de tueur psychopathe dans l?xcellent "No country for old men". curiosit?e punti vendita - e un sito internet: . la déclaration d'amour de Justin.
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Nickys amazing platform boots are Alaia, but tragically, they are not currently available anywhere online. I believe Paris bag is an old Yves Saint Laurent piece from the brands pre-Hedi Slimane, pre-Yves-dropping days. If you, like our favorite hotel chain heiresses, enjoy the finer things in life, you should definitely check out Paris does not have her own edition of Many Bags as of yetHeres heiress Nicky Hilton in the Meatpacking District neighborhood of NYC, carrying a slate grey version of what is still one of my favorite designer handbags, so many seasons after its debut: the Alexander Wang Rocco Bag. Nicky flew into town last week to attend the New York City Ballet Fall Gala (not in that outfit, of course). You can snag Nickys Rocco for . (The color name is Elephant. Fitting!)
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The senator then acknowledged that he was leveling a very serious charge against the Obama administration.
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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: March 12, 2009Space station commander Mike Fincke, flight engineer Yury Lonchkov and Sandra Magnus evacuated to the lab's Russian Soyuz spacecraft today because of a predicted close encounter with debris from a spent upper stage booster rocket. But the space junk streaked harmlessly past the station around 12:39 p.m. and the crew was cleared to re-enter the lab complex."OK guys, based on all the confirmations, most likely the object passed us by," a Russian flight controller said, according to a translator. "So you are go to egress Soyuz. Yury, also please tell us are you ready to start the leak check?""And Houston, space-to-ground 1, can you hear us?" Fincke called over the NASA communications circuit."We have you loud and clear Mike, on space-to-ground 1," a controller in Houston replied."OK, we understand we're clear (to) ingress back to the USOS (U.S. segment of the station)," Fincke said."And we're all very happy the (debris) has passed with no impact," Houston replied. "That's great news."According to a NASA statement, the station crew members evacuated to the Soyuz as a precautionary measure "due to space debris that has been determined to be within the range where a collision is possible. News of the close approach came too late for flight controllers to coordinate an avoidance maneuver. A portion of a spent satellite motor is within the distance of the station's debris avoidance maneuver requirement 'box.'"Crew members are entering their Soyuz TMA-13 capsule and soft-locking the hatches, in case the debris should affect the space station and they are required to undock. The closure of the hatches ensures the safety of the crew and the ability to quickly depart the station in the unlikely event the debris collided with the station causing a depressurization."Time of closest approach was 12:39 p.m. EDT. It was not immediately known just how close the debris from the spent payload assist module, or PAM-D, upper stage rocket motor came to the international space station.But all objects in low-Earth orbit are traveling at 5 miles per second and impacts are potentially catastrophic. A 0.4 inch-wide sphere of aluminum moving at orbital speeds packs the same punch as a 400-pound safe moving at 60 mph.There are more than 18,000 pieces of space junk in low-Earth orbit the size of a baseball and larger. U.S. Strategic Command prioritizes radar tracking to protect manned spacecraft first, followed by high-priority military and civilian payloads.Normally, the station's rocket thrusters are used to change its orbit slightly when close encounters are predicted. Putting the crew in the station's Soyuz lifeboat with little warning is unusual and it was not immediately clear why an alert about today's close encounter was not delivered or received in time to carry out a course change.Aerospace Corp. Space Debris Background NASA Orbital Debris FAQs Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA's first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Two former teachers set for today's spacewalk BY WILLIAM HARWOOD
UGG Roxy Short 5828 (2014-09-29 01:0)
National exit polls from both the 2000 and 2008 elections show that Mr. Clinton's and Mr. Bush's records, while not a determining factor, did influence a large segment of voters. In 2008, 51 percent of respondents said they strongly disapproved of Mr. Bush's handling of his job, and 82 percent of those voters cast their ballots for Mr. Obama. In 2000, 44 percent of voters said the Clinton-era scandals were at lease somewhat important to their vote. Beyond those numbers, the fear of a de facto third Clinton or third Bush term could be found in the candidates themselves. 2000 Democratic nominee Al Gore and 2008 Republican nominee John McCain almost never campaigned alongside the incumbent presidents.
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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 30, 2004Executing stored instructions, the electronic brain of NASA's Cassini probe made final preparations for a critical 96-minute rocket firing tonight that will slow the craft by about 1,400 mph and allow Saturn's gravity to pull it into orbit.The make-or-break Saturn Orbit Insertion - SOI - maneuver was scheduled to begin at 10:36 p.m. EDT and end around 12:12 a.m. Thursday. If successful, the burn will put Cassini in a long orbit around Saturn, kicking off a four-year tour of the ringed planet, its magnetosphere, its largest moon, Titan, and a retinue of smaller, icy satellites.If the rocket firing fails or falls short of its 96-minute target duration, the $3.3 billion spacecraft will sail past Saturn and into a useless orbit around the sun."Unlike the two Voyagers that flew by Saturn in the early '80s and obtained just days worth of Saturn close-in science, Cassini-Huygens will be for Saturn what the Galileo mission was for Jupiter: a long-term science observatory," said Ed Weiler, NASA's associate administrator for space science.But, he cautioned, "we are not there yet. Although things have gone very, very well so far, Saturn orbit injection will be the most critical event in the mission's life since launch. This main engine burn must be performed as planned or the mission will be lost."Unlike the Mars (rover) landings, where we had the 'six minutes from hell,' so to speak, in this case it'll be 96 minutes in purgatory. I hope the outcome will be as successful as our experiences with the Mars missions last January."Engineers and managers at the Jet Propulsion Laboratory in Pasadena, Calif., believe it will. They said today the spacecraft has performed virtually flawlessly during the seven years it's taken Cassini to reach Saturn and they are confident it pull off the SOI burn, as Weiler said the most important single maneuver since launch from Earth on Oct. 15, 1997."Today, the Cassini spacecraft is in an excellent state of health and it is ready to perform the main engine burn tonight," said Julie Webster, lead vehicle engineer at JPL. "The spacecraft, the flight software and the on-board (computer command) sequences are now completely self contained and need no ground interaction from us to complete this burn. If a fault occurs on the spacecraft, the software will isolate the fault, identify the cause, fix it and continue on with the burn with no ground intervention."The only issue of any significance is the possibility of high winds at a tracking station in Canberra, Australia. If the winds exceed about 47 mph, a 230-foot-wide dish antenna needed to pick up Cassini's radio signal will have to be stowed, delaying confirmation of a successful rocket firing."This has no bearing on the performance of the spacecraft," said Cassini program manager Bob Mitchell. "The spacecraft is perfectly capable of doing what it needs to do and weather on Earth is just not a factor."The thing that would be influenced is our blood pressure throughout the course of the evening," he joked. "However, a recent weather report from Canberra was favorable. It didn't eliminate the threat entirely, but it is favorable. So we don't believe it's going to be a problem."Because of Cassini's enormous distance from Earth - some 934 million miles - radio signals from the spacecraft take an hour and 23 minutes to reach flight controllers at JPL. As a result, confirmation of events during SOI will be delayed by the same amount. In the timeline discussion below, "Earth-receive time," converted to Eastern Daylight Time, is used throughout."After 6.7 years we're at Saturn," said lead navigator, Jeremy Jones. "We're feeling the gravity well, falling into Saturn quite rapidly. ... This is the E-ticket ride, I'll tell you."The numbers prove his point. At noon today, Cassini was 403,891 miles from Saturn and moving through space at 26,846 mph. By 6 p.m., the craft will be roughly half that far out - 233,014 miles - and its velocity will be up to 33,557 mph. Three hours later, the distance will be just 155,343 miles and its speed will be up to 42,506 mph.The first critical milestone in the SOI sequence is the so-called ascending ring plane crossing. Approaching Saturn from below the plane of its rings, Cassini will cross that plane, in a broad gap between the F and G rings, at 10:11 p.m. That region is thought to be clear of any major pieces of ring debris, but no one knows for sure. At Cassini's velocity, an impact with anything larger than a very small pebble could cause major damage.To be on the safe side, the spacecraft will re-orient itself an hour ahead of time, pointing its high-gain dish antenna in the direction of travel to act as a shield, cutting off telemetry from the spacecraft for the duration of the SOI maneuver. At the moment of ring plane crossing, Cassini will be just under 100,000 miles from Saturn - less than half the distance between the Earth and moon - and streaking through space at 50,335 mph."The antenna is a graphite-epoxy structure, so it's quite rugged and very capable of withstanding the kinds of small dust grains that we believe might be in this region," Mitchell said.Once above the ring plane, Cassini will re-orient itself for the Saturn Orbit Insertion burn, pointing its main engine in the direction of travel. It also will begin transmitting a radio carrier signal using a low-gain antenna. The signal will not carry any data. But by monitoring how its frequency changes due to the SOI rocket firing's effect on Cassini's velocity, engineers will be able to confirm the start of the burn and the engine's overall performance through engine cutoff.The moment of truth arrives at 10:35:42 p.m. when Rocket Engine Assembly A - REA-A - flashes to life, pushing against Cassini's 53,691-mph forward motion with a mere 100 pounds of thrust. Over the course of 96.4 minutes, REA-A will consume 1,874 pounds of rocket fuel, roughly one third of the 6,600 pounds Cassini was launched with, slowing the spacecraft by 1,396 mph and ensuring Saturn's gravity pulls it into the desired orbit.Thirty minutes into the burn, at 11:06 a.m., Cassini will move behind the A ring as viewed from Earth and the carrier signal may be lost for up to 25 minutes or so. The signal should show back up for six minutes when Cassini "sees" Earth through a gap in the rings known as the Cassini division. Then communications may be lost again for 28 minutes or so as the spacecraft moves behind the B ring.Saturn closest approach, or periapsis, will occur 10 minutes before the end of the burn, at 12:03 a.m. By this point, Saturn's gravity will have boosted Cassini's velocity to 69,350 mph. But by the end of the burn at 12;12 a.m., the velocity will have dropped to 68,000 mph and Cassini will be safely in orbit.Weather in Australia permitting, engineers at JPL should be able to confirm the start of the rocket firing monitor its performance between ring blackouts and confirm the end of the burn. A few minutes later, Cassini is programmed to turn back toward Earth and transmit 20 seconds of engineering data starting around 12:30 a.m. The craft then will re-orient itself yet again to aim its cameras at Saturn's rings for 75 minutes of up-close science observations.It then will re-orient itself antenna forward for the descending ring plane crossing and then point back toward Earth to begin downlinking its treasure-trove of science data. The first pictures are expected Thursday morning."Once we're done with about a 75-minute data observation period, we turn again for the descending ring plane crossing, again point the high-gain antenna as a protective shield," Mitchell said. "Once that's complete, we're going to turn and look back up at the rings, now on the sunlit side, take another set of images, mostly around the outer extent of the visible part of the rings. We then turn back to Earth and play this data back over about an 18, 19-hour period of time."While confident, Mitchell cautioned "this thing is not a slam dunk by any means.""There are two general concerns," he said. "One is the environment, primarily the environment of the rings. We have studied this very carefully, we believe we've taken prudent actions, we believe we've got the safest possible course of action, but it's not a guarantee."And then for the spacecraft itself, the spacecraft isn't going to do anything tonight that it hasn't already done in flight. But a 96-miute burn, where all of the systems have to work right for this amount of time, is a concern. Our confidence in the spacecraft is high, we have no specific reason to be concerned, but this is not a assured, either."In preparation for the rocket firing, Cassini's on-board software opened low-pressure helium latch valves Tuesday. A backup inertial reference gyroscope was turned on and warmed up for use as needed during the burn. This morning, the main engine gimbal system was activated so the engine nozzle can be pre-positioned and the spacecraft's accelerometer was calibrated.In short, Webster said, all systems were "go" for SOI."If the burn goes fine and we just don't get the signal back on the ground for any reason, we will get about 20 seconds of the high-gain coming in right before we turn go off and do the images," Webster said. "So if everything's perfect through the burn, we should get that little 20-second blip. That's very good because that tells us that the spacecraft didn't do any safing event or didn't stop the burn for any reason because the background sequences are still going. That's the good indication. That'll come in about 12:30 a.m. (EDT)"I'm an old telecom person, so I actually wouldn't be concerned about this until past 3 a.m. ... I would not get any panic level until 6 or 7 in the morning. That's not unusual in low gain safing to have a little bit of trouble, especially with the Doppler changes that are going on with the spacecraft. Sometimes it just takes a while to find the signal. But I have full faith in this spacecraft, that it's going to make this burn one way or the other."Additional coverage for subscribers:VIDEO:TODAY'S 12 P.M. EDT CASSINI STATUS BRIEFING VIDEO:A LOOK AT INTERNATIONAL COOPERATION VIDEO:TUESDAY'S CASSINI MISSION OVERVIEW BRIEFING VIDEO:CASSINI'S ARRIVAL AT SATURN EXPLAINED VIDEO:SCIENCE OBJECTIVES FOR CASSINI ORBITER VIDEO:HUYGENS LANDER SCIENCE OBJECTIVES Stargaze II DVDThe Stargaze II DVD has arrived! It features over 65 minutes of all new videos of the universe with newly-composed dolby digital and DTS 5.1 Channel surround sound music. Choose your store: - - - Solar system poster This new poster is popular for classrooms and children's bedrooms. 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Information gathered during this flyby will provide an opportunity to compare images from Cassini's first close Titan encounter on Oct. 26. This view of Titan taken by Cassini during its encounter in October. Credit: NASA/JPL/Space Science InstituteNASA's Deep Space Network tracking station in Madrid, Spain, acquired a signal at about 4:00 p.m. Pacific Standard Time (7:00 p.m. Eastern Standard Time). As anticipated, the spacecraft came within 1,200 kilometers (750 miles) of Titan's surface. As with the last flyby, a major goal of this flyby is to measure the thickness of Titan's atmosphere. This information will help determine whether Cassini can safely get closer to Titan on subsequent flybys, and will also be used to verify that Huygens atmosphere models are correct. Titan is a prime target of the Cassini-Huygens mission because it is the only moon in our solar system with a thick smoggy atmosphere. The Huygens probe, built and operated by the European Space Agency, is attached to Cassini. After its Christmas Eve release, it will descend through Titan's atmosphere on Jan. 14, 2005, as it collects atmospheric data down to the surface. Tomorrow morning, Cassini will fly by Saturn's icy moon Dione at a distance of 72,500 kilometers (45,000 miles). Images and science results from both flybys will be presented at a news conference that will take place on Thursday, Dec. 16, at the American Geophysical Union fall meeting in San Francisco.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini mission for NASA's Science Mission Directorate, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter. 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Credit: NASA/JPL/Space Science InstituteDownload larger image version The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 24, 2004, at a distance of about 1.7 million kilometers (1 million miles) from Rhea and at a Sun-Rhea-spacecraft, or phase, angle of 40 degrees. The image scale is approximately 10 kilometers (6 miles) per pixel. Cassini will image this hemisphere of Rhea again in mid-January 2005, just after the Huygens probe landing on Titan - with approximately 1-kilometer (0.6-mile) resolution. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. 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Choose your store: | | | | 2014 Spaceflight Now Inc.Cassini makes close observations of Phoebe NASA/JPL ANNOUNCEMENTPosted: June 12, 2004With its flyby of Phoebe, the Cassini spacecraft has completed the first satellite flyby in its four-year tour of the Saturn system. NASA's Deep Space Network received confirmation at 7:52 a.m. PDT today. The spacecraft is operating normally and is in excellent health. Animation shows Cassini's flyby of the moon Phoebe while en route to orbit the planet Saturn. Credit: NASA TV/Spaceflight Now"One down, 52 to go," said Jeremy Jones, chief navigator for theCassini-Huygens mission at NASA's Jet Propulsion Laboratory,Pasadena, Calif. During Cassini's planned four-year tour it willorbit Saturn 76 times and execute 52 close encounters with seven ofSaturn's 31 known moons."Although this is the first flyby in the Saturn tour, it is theonly opportunity to see Phoebe," said Dr. Dennis Matson, projectscientist for the Cassini-Huygens mission. 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JPL designed,developed and assembled the Cassini orbiter.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Cassini maneuver sets stage for Saturn arrival BY WILLIAM HARWOOD
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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: April 14, 2005The space shuttle's redesigned fuel tank sailed through a critical tanking test today, giving NASA managers increased confidence about launching Discovery on the first post-Columbia shuttle mission next month. Space shuttle Discovery undergoes the special tanking test at pad 39B today. Credit: NASA TV/Spaceflight Now"We had an outstanding day today," said Wayne Hale, deputy manager of the shuttle program and chairman of NASA's mission management team. "After a long period of preparation, we're beginning to see our operations come to fruition."Today, we saw the newly modified external tank perform in an outstanding manner, we saw Discovery, which has gone through about three years of modifications, perform in an outstanding manner. And I have to also say the launch pad, the facility, which has gone through a major modification and extensive re-work, performed almost without flaw of any consequence."Engineers pumped more than 500,000 gallons of supercold rocket fuel into Discovery's external tank today and then monitored the tank and the shuttle's systems down to the T-minus 31-second mark in a mock countdown. It was the first such tanking operation since Columbia's launch Jan. 16, 2003."Today's test was a major milestone," said launch director Mike Leinbach. "The next one is launch, and I'm really looking forward to that one."The goals of the exercise were to give the launch team a chance to rehearse launch-day procedures, to verify the operation of critical launch pad systems and to demonstrate the tank's foam insulation could stand up to the stress of ultra-low temperatures without any major ice buildups.During a debris verification review late last week, engineers discussed all possible sources of launch debris and retired all but three. The remaining open items involve the possibility of ice buildups around liquid oxygen feed line fittings near the so-called intertank region and pressurization line support fittings at the tip of the tank.Post-Columbia impact testing shows even small pieces of ice, shaking off during launch, could cause serious damage to the shuttle's wing leading edge panels or its nose cap. Columbia was destroyed during re-entry Feb. 1, 2003, because of damage done by the impact of foam insulation during launch 16 days earlier. The insulation has now been been modified to minimize such debris shedding.During today's test, ice buildups in the areas of concern were minimal and Hale said engineers are hopeful additional testing will close the remaining open items on the debris impact list."Ice is a biggie," Hale said. "One of the things we were very interested to look at today was the performance of the tank and ice growth on the tank," Hale said. "It performed very well, that is heartening news. But that is not all the story."We're doing some testing at Redstone Arsenal and other places regarding the potential for ice to shed off the tank during the ascent and we think there are a number of ways we're going to come to a good conclusion on that. But there is work remaining before us on that."Discovery's launch window opens May 15 and closes June 3. The next window opens July 13. Leinbach said now that the tanking test is over, the pad processing flow is fairly standard with no other unusual tests. Between now and May 15, he said, the pad processing flow includes three days with no work planned."That's good news for us," he said. "Even better news for us is the test we performed today was the last non-standard activity we have at the launch pad. From here on out, it's standard pad processing. ... From here on out the rest of the pad flow is well understood. The fact that we have 'just' three days, if you want to say it that way, is not that bad."But the time needed to resolve the remaining debris concerns forced NASA, in part, to delay a planned design certification review from Friday to next Tuesday. Another debris review is planned late next week and that information must then flow into NASA's flight readiness review process and to an independent panel charged with monitoring NASA's implementation of post-Columbia safety upgrades.The review panel, headed by former Apollo astronaut Thomas Stafford and former shuttle commander Richard Covey, had hoped to present its final report to NASA's administrator a full month before launch to give the agency time to respond. That no longer appears plausible, but no firm dates have been set.Hale would not speculate on when the work might get finished, saying only that NASA will not launch Discovery until it is safe to do so. But he was clearly encouraged by the results of today's tanking test."Both the debris verification review, the upcoming design certification review and the tanking test that we did today are key items on the way to being ready to go fly," he said. "We're not done yet, but these are key things that we needed to get accomplished. We're whittling down the to-do list of things we must do before we can we can certify the vehicle for flight readiness."Video coverage for subscribers only:VIDEO:TODAY'S FUELING TEST GETS UNDERWAY VIDEO:INSPECTORS COMPLETE CHECKS OF TANK AFTER FUELING VIDEO:POST-TEST NEWS CONFERENCE WITH TOP NASA MANAGERS AUDIO:LISTEN TO POST-TEST BRIEFING VIDEO:HIGHLIGHTS OF EXTERNAL TANK PRE-FLIGHT PREPS VIDEO:TIME LAPSE MOVIE OF DISCOVERY ARRIVING AT PAD VIDEO:TIME LAPSE MOVIE OF GANTRY ENCLOSING DISCOVERY VIDEO:DISCOVERY ROLLS OUT OF VEHICLE ASSEMBLY BUILDING VIDEO:HEADING DOWN THE CRAWLERWAY VIDEO:TURNING AT CRAWLERWAY JUNCTION VIDEO:ROLLING WITH PAD 39A AS BACKDROP VIDEO:ON NORTHWARD IN THE EARLY EVENING VIDEO:PREVIEW OF DISCOVERY'S MISSION VIDEO:THE SPACE STATION WITHOUT SHUTTLE VIDEO:MEET DISCOVERY'S SEVEN ASTRONAUTS VIDEO:DISCOVERY HOISTED INTO POSITION FOR TANK MATING VIDEO:WALK ALONGSIDE DISCOVERY DURING TRANSFER TO VAB VIDEO:TIME-LAPSE MOVIE OF DISCOVERY LEAVING HANGAR VIDEO:SPED UP VERSION OF HANGAR DEPARTURE MOVIE VIDEO:TIME-LAPSE MOVIE OF SHUTTLE ROLLING INTO VAB VIDEO:SPED UP VERSION OF VAB ARRIVAL MOVIE VIDEO:NASA'S STEVE POULOS TALKS WITH REPORTERS VIDEO:PAYLOAD BAY DOORS CLOSED IN HANGAR Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Discovery will switch to new fuel tank before July blastoff BY WILLIAM HARWOOD
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