Monday, November 5, 2007

FlashbacK : 50 Years Ago: The First Dog in Orbit


It's today :Research on space is showing the unlimited fortune of creation ,



Just a month after the Soviet Union stunned the world by putting the first artificial satellite into orbit, it boasted a new victory - a much bigger satellite carrying a mongrel dog called Laika.


The mission, 50 years ago Saturday, ended sadly for Laika but helped pave the way for human flight.


As with other episodes of the Soviet space program, Laika's mission was hidden under a veil of secrecy, and only after the collapse of the Soviet Union could the participants tell the real story behind it.


The satellite that carried Laika into orbit was built in less than a month in what was perhaps the world's fastest-prepared space mission ever.


Excited by the international uproar over the launch of Sputnik on Oct. 4, 1957, Soviet leader Nikita Khrushchev summoned Sergei Korolyov, the father of the Soviet space program, and ordered him to come up with "something new" to celebrate the Nov. 7 anniversary of the 1917 Bolshevik Revolution.


Khrushchev's demand was a shock even for Korolyov, whose team had managed to put together the first Sputnik in less than three months, said Georgy Grechko, a cosmonaut who started his career as a space engineer.


"We didn't believe that you would outpace the Americans with your satellite, but you did it. Now you should launch something new by Nov. 7," Korolyov quoted Khrushchev telling him, according to Grechko.


Boris Chertok, Korolyov's right-hand man, said the short notice made it impossible to design a principally new spacecraft, but there was also little sense in simply repeating the Sputnik launch.


"Korolyov rightly feared that this holiday gift could end up in an accident that would spoil a hard-won victory," Chertok wrote in his memoirs. But they couldn't argue with Khrushchev, and the decision to conduct the launch was made on Oct. 12.


When someone on Korolyov's team suggested putting a dog into orbit, he jumped at the idea.


Little was known about the impact of space flight on living things, and some believed they would be unable to survive the launch or the conditions of outer space.


The Soviet Union had experimented with launching dogs on short suborbital missions during ballistic missile tests, and some of them survived several such missions. All of them were stray mongrel dogs - doctors believed they were able to adapt quicker to harsh conditions - and all were small so they could fit into the tiny capsules.


Just nine days before the launch, Doctor Vladimir Yazdovsky chose one of them - 2-year-old Laika - for the mission.


Stories about how she was chosen vary. Some say Laika was chosen for her good looks - a Soviet space pioneer had to be photogenic. Others say space doctors simply had a soft spot for Laika's main rival and didn't want to see her die: Since there was no way to design a re-entry vehicle in time for the launch, the glory of making space history also meant a certain death.


"Laika was quiet and charming," Yazdovsky wrote in his book chronicling the story of Soviet space medicine. He recalled that before heading to the launchpad, he took the dog home to play with his children.


"I wanted to do something nice for her: She had so little time left to live," Yazdovsky said.


Working round-the-clock, Korolyov and his team combined a capsule that would carry the dog with basic life-support systems and elements of the first Sputnik. To simplify the design, they decided not to separate the satellite from the booster's second stage.


They worked without blueprints at a pace that was breathtaking even at the time of the space race and seems utterly impossible by today's standards.


"Now when we have computers, sophisticated industrial equipment, lasers and other things, no one is capable of making a new satellite in just one month," Grechko said in an interview. "Now it would take a month just to start doing the paperwork. Korolyov told us later that it was the happiest month of his life."


As a result of some last-minute technical problems, Laika had to wait for the launch in the cabin for three days. The temperatures were low, and workers put a hose connected to a heater into the cockpit to keep her warm.


On Nov. 3, Laika blasted off into space in Sputnik 2, which weighed 1,118 pounds - a show of Soviet ability to take big payloads into space.


Sputnik 1 weighed just 184 pounds. The first U.S. satellite, Explorer 1, launched on Jan. 31, 1958, weighed about 31 pounds.


When Laika reached orbit, doctors found with relief that her pulse, which had risen on launch, and her blood pressure were normal. She ate specially prepared food from a container.


According to official Soviet reports, the dog was euthanized after a week. Laika's mission drew a wave of protests from animal protection activists in the West.


It wasn't until after the Soviet collapse, that some participants in the project told the true story: Laika indeed was to be euthanized with a programmed injection, but she apparently died of overheating after only a few hours in orbit. There was no information to indicate when exactly she died.


"It was impossible to build reliable life-support and thermal-control systems in such a short time," Chertok said in his memoirs.


Several other dogs died in failed launches before the successful space flight - and safe return to Earth - of Belka and Strelka in August 1960. After a few other flights with dogs, the Soviet Union put the world's first human - Yuri Gagarin - into space on April 12, 1961.


Gagarin is said to have joked: "I still don't understand who I am: the first human or the last dog in space."




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Sunday, November 4, 2007

Space : One Collective Soul in Outer Space


A reality check on dreams for space: the repairsThe crews from the shuttle Discovery and the International Space Station had a farewell ceremony today and closed the hatch between the two craft. Discovery will undock tomorrow and prepare for its return to Earth on Wednesday.
It was a blubberfest.
This has been an intense mission - the planned tasks involved some of the toughest technical challenges in the history of the space station's construction process, and included adding a new room to the station, the Harmony module, and moving an enormous solar array and truss from its temporary position on top of the station to its far left side.
Astronaut Scott Parazynski worked along the truss assembly of the International Space Station on Saturday, preparing equipment for mounting on the boom extension.
NASA/Reuters





But beyond those efforts, problems made the mission even tougher. The solar array tore as it was being re-deployed, setting off a scramble to come up with a spacewalk that could repair the tear and get the array functional before the shuttle left. Without that array fully extended and able to be rotated on its own rotary joint, space station construction would have been stalled and upcoming missions delayed.
And on top of that, spacewalkers detected damage to the rotary joint on the right side of the station, one that keeps the right-side solar arrays facing the sun - a problem that will have to be addressed down the road. In a high-risk, high-stakes spacewalk Dr. Scott E. Parazynski fixed the array on Saturday.
So it's no surprise that the farewells are more than a little emotional. Clayton Anderson, who spent 137 days as a space-station crew member and will be coming home on Discovery, kept turning off his microphone as he was overcome with emotion as he thanked the "folks on the ground" - flight-control engineering and training teams in Houston, Huntsville and Moscow. "I say thank you," he said, his voice breaking. "You are indeed the best and the brightest that our world has to offer."
Over the communications loop, there was loud applause from the "folks on the ground."
Mr. Anderson then played the song "Reunion," by Collective Soul. His crewmates swayed to the music (which in zero gravity has to be seen to be believed) as it played, tinny over the orbit-to-ground transmission:
Change will come
Change is here
Love fades out
Then love appears
Now my water's turned to wine
And these thoughts I have
I now claim as mine
I'm coming home
Change has been
Change will be
Time will tell
Then time will ease
Now my curtain has been drawn
And my heart can go
Where my heart does belong
I'm going home
Discovery's commander for this mission, Pamela A. Melroy, also teared up as she thanked the the station commander, Peggy A. Whitson, and the Russian cosmonaut on board the station, Yuri Malenchenko, and said goodbye to crew member Daniel M. Tani, who will stay aboard the station. "We promise we'll send somebody to come pick you up and bring you home," she joked.
"We're family now," she said.
Mr. Tani wiped his eyes repeatedly as well.
Col. Malenchenko made headlines in 2003 during his last stint aboard the station, when he got married from orbit: his bride, Ekaterina Dmitriev, was on earth in the Villa Capri restaurant near the Johnson Space Center. A justice of the peace did the honors; Col. Malenchenko wore a bowtie with his flight suit and was represented on the ground by a paper cut-out.
One can only wonder what the stoic Col. Malenchenko thought of the waterworks from his American crewmates, but when it came time to say goodbye, he gave Mr. Anderson what looked like a real rib-crusher of a hug.
Anyone who wants to see the emotional session can tune in to NASA television, where the farewell ceremonies are replayed as part of the highlights reel that runs on the hour.



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Saturday, November 3, 2007

Analysis Of Solar Wind Helps Illuminate solar System Evolved


Analyzing the mix of hydrogen, oxygen and noble gases found in the sun can answer one of the biggest questions of the universe: How did our solar system evolve? (Credit: iStockphoto/Alexander Hafemann)




As reservoirs of valuable information go, nothing beats the sun. This sphere of heat and energy holds 99.9 percent of the solar system, saved in all original proportions after planets and meteorites formed. Analyzing the mix of hydrogen, oxygen and noble gases found in the sun can answer one of the biggest questions of the universe: How did our solar system evolve?
Scientists at Washington University in St. Louis and a large team of colleagues marked the beginnings of that odyssey by examining samples of solar wind for neon and argon, two abundant noble gases.

These samples came from NASA's Genesis mission, which launched in 2001, and orbited the sun for more than two years, collecting samples of solar wind. In 2004, the soft landing planned for the craft went wrong and Genesis smashed into the Utah mud, splintering into more than 10,000 pieces. Fortunately, these fragments were large enough to yield highly precise data for neon and argon.


Alex Meshik, Ph.D., lead author and research professor of physics in Arts & Sciences at Washington University, credits mission planners for preparing for every outcome long before launch. At the time, decisions to craft solar wind collection arrays in different thickness in case they were broken on landing likely saved all data.


"The arrays are made of super-pure metals and diamonds deposited on sapphire," Meshik says. "There was no way to mark them otherwise. Now we can take a piece and know which array it came from."


Genesis collected samples by deploying different arrays during three types, or flow regimes, of solar wind: low-speed, high-speed and the spectacular coronal mass ejections. Because solar wind streams at different velocities in different regimes, on-board instruments move the arrays to collect separate data for the different regimes.


The abundances and isotopic composition of the noble gas from the regimes could in turn be used to understand how well the solar wind truly represents solar composition.


Data presented in the Science paper made one thing clear: The isotopic composition of neon and argon in all three regimes were the same. So measuring solar wind means that you are sampling the solar corona, the place at which ions stream out of the sun.


"This is good for future measurements of nitrogen and oxygen and other elements because if it's true for noble gases, it's true for other elements as well," says Meshik.


This work gives scientists who design models of how the solar system formed the actual ground truth, explains Charles Hohenberg, Ph.D., WUSTL professor of physics. Differences in isotopic composition between the planets and the sun tell us about their evolutions. Also, the team's ability to measure neon and argon with high precision helps other Genesis scientists calibrate their data.


Although Washington University scientists won't be measuring oxygen -- a critical element for planetary studies -- their Genesis findings will help scientists make their measurements more accurate.


"There are so many elements that other scientists would like to measure that are very, very difficult to measure because of their low abundance and high potential for contamination," says Hohenberg.


Refining the equipment


Even though WUSTL scientists were able to extract valuable data from Genesis' broken pieces, the work required the design of new equipment and refinement of existing measuring devices. Both Meshik and Hohenberg stressed the team aspect that made and continues to make this project possible.


Five of eight authors on the current Science paper come from Washington University. In addition to Meshik and Hohenberg, fourth-year graduate student Jennifer Mabry, whose Ph.D. research is based on this work; senior research scientist Olga Pravdivtseva, Ph.D.; and Yves Marrocchi, who is now at Nancy-Université in France, worked on all aspects of the project. Also among the co-authors is a former student of Hohenberg's, Chad Olinger, Ph.D., who is at Los Alamos.


Next, WUSTL scientists will measure heavy noble gases from the solar wind samples -- they've already redesigned two new mass spectrometers specially made for this effort. Unlike argon and neon, which are abundant enough for multiple measurements, the rarity of heavy nobles like xenon allow for perhaps only one or two attempts.


The Genesis mission was the first since the Apollo era to bring extraterrestrial material back to Earth, so the team wants the best measurement of the sun's xenon and krypton possible. Therefore, these measurements have been delayed while measurement techniques are optimized.


"If you look at meteorites, the argon that you measure is very close to what you see in the sun. That's not the case for xenon and krypton and that's not the case for the atmosphere. Understanding how those things all fit together is important. Nobody really knows yet," says Hohenberg.





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