The finding adds to accumulating evidence that at some times and in some places, Mars hosted favourable climate for microbial life.This image provided by NASA's Hubble Space Telescope shows a close-up of the red planet.


AP The finding adds to accumulating evidence that at some times and in some places, Mars hosted favourable climate for microbial life.This image provided by NASA's Hubble Space Telescope shows a close-up of the red planet.

American scientists claim to have found evidence that suggests Mars had a warm and wet climate which could have supported life some 3.5 billion years ago.

A team, led by planetary geologists at Brown University, found mounds of a mineral deposited on a volcanic cone less than 3.5 billion years ago that speak of a warm and wet past, and may preserve evidence of one of the most recent habitable microenvironments on the red planet.

Observations by the National Aeronautics and Space Administration's Mars Reconnaissance Orbiter enabled the researchers to identify the mineral as hydrated silica which can be dissolved, transported and concentrated by hot water or steam - a dead ringer that water was present at some time.

Best evidence yet

The mineral and the mounds' location on the flanks of a volcanic cone provide the best evidence yet on Mars for an intact deposit from a hydrothermal environment — a steam fumarole or a hot spring, said the researchers.

Such environments might have provided habitats for some of Earth's earliest life forms, they hoped.

“The heat and water required to create this deposit probably made this a habitable zone,” said J. R. Skok, lead author of the study, published in journal Nature Geoscience.

“If life did exist there, this would be a promising spot where it would have been entombed - a microbial mortuary, so to speak.”

Favourable climate

No studies have determined whether Mars has ever supported life, but this finding adds to accumulating evidence that at some times and in some places, Mars hosted favourable climate for microbial life.

The deposit is located in the sprawling, flat, volcanic zone known as Syrtis Major and was believed to have been left during the early Hesperian period, when most of Mars was already turning chilly and arid.

“Mars is just drying out,” Skok said, “and this is one last hospitable spot in a cooling, drying Mars.”

Concentrations of hydrated silica have been identified on Mars previously, including a nearly pure patch found by NASA's Mars Exploration Rover Spirit in 2007. However, this is the first found in an intact setting that clearly signals the mineral's origin.

“You have spectacular context for this deposit,” Skok said. “It's right on the flank of a volcano. The setting remains essentially the same as it was when the silica was deposited.”

Bright deposits

Observations by cameras on the Mars Reconnaissance Orbiter revealed patches of bright deposits near the summit of the cone, fanning down its flank, and on flatter ground in the vicinity.

The Brown researchers partnered with Scott Murchie, of Johns Hopkins University Applied Physics Laboratory, to analyse the bright exposures with the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) instrument on the orbiter.

Hydrated silica identified by the spectrometer in uphill locations, confirmed by stereo imaging, indicates that hot springs or fumaroles fed by underground heating created these deposits. Silica deposits around hydrothermal vents in Iceland are among the best parallels on Earth.

“The habitable zone would have been within and alongside the conduits carrying the heated water,” Murchie said.



The International Space Station -- which is coming up on a decade of continuous human habitation -- is a celebrated success in our species' quest to learn to live in space. Yet life in orbit has its serious trials, and mishaps along the way have proven just how much we still have to learn about being a spacefaring civilization.

In honor of Halloween, here are 10 ways space station living can become a little horror story:

10. Fingernails fall off

The spacesuit gloves astronauts wear while working outside the station during spacewalks have proven to be hazardous to their health.

A recent study found that about 10 percent of astronauts are victims of "fingernail trauma" from gloves, with a number of them losing a fingernail entirely because the glove pinched their fingers and reduced circulation.

Typically, the damage is worse the larger an astronaut's hand is. Maybe NASA should look for petite spaceflyers.

9. Weightless worries

Weightless living can have some pretty odd consequences without even going outside. Take, for example, the attack of the flying wasabi.

In March 2007 astronaut Sunita Williams was trying to squeeze some of the spicy green condiment onto her makeshift space sushi, when a squirt got loose, ultimately splattering the walls with wasabi and hiding stray droplets around the module.

It took a while to get the wasabi smell out after it had flown all over the place, Williams said at the time. And she had to forgo wasabi on future space meals, saying it was just "too dangerous."

8. Rough ride

While floating on the space station can be fun, getting to and from it can be a rough ride. Trips on the Russian Soyuz spacecraft, in particular, reportedly pack quite a punch of G forces.

"I've heard it described as a train wreck followed by a car crash followed by falling off your bike," NASA astronaut Tracy Caldwell Dyson said recently before she flew home from the station on one herself.

After she had experienced the trip, she said the rumors were dead on.

"It certainly didn't disappoint," Caldwell Dyson told SPACE.com after her return. "All the bangs, bells, whistles and sensations were there. The magnitudes of some things were a little surprising, but for the most part it was a pretty exciting ride."

7. Space diet of baby food

Though it's not just Tang and freeze-dried ice cream these days, food in space still leaves something to be desired.

Fresh fruit and vegetables are scarce, for example, and ground staples like bread are impractical because they leave crumbs, which in microgravity fly around everywhere instead of settling on the floor, and become a disaster to clean up. (Instead astronauts favor tortillas, which create fewer crumbs).

And astronauts tend to get sick of the same roster of re-heatable meals rotated on an eight-day schedule.

In the winter of 2004, however, an unmanned cargo ship due to deliver fresh food and supplies to the space station was delayed. In response, the crewmembers onboard – Expedition 10 commander Leroy Chiao of NASA and flight engineer Salizhan Sharipov of Russia – had to ration their meals.

The two ended up cutting their regular food consumption in half to conserve supplies, then making up for the lost calories by eating abundant desserts and candies. "It wasn't an unhealthy diet, but it wasn't an ideal diet either," Chiao said at the time.

6. Cramped quarters

While the station has grown considerably over the 10 years it's been permanently inhabited, many spaces are still a tight squeeze. And for the last year and a half, the normal crew size aboard the orbiting lab have been six, meaning what space there is has been shared by more bodies.

Sleeping can be particularly cramped inside an astronaut's "crew quarters" – essentially an alcove the size of a phone booth – and there are other hazards of catching some Zzz's in a free floating sleeping bag.

"During the night while you're sleeping, you might start drifting and end up somewhere you didn't intend to be in the first place," Canadian astronaut Julie Payette said in 2009.

Yet overall, the coziness of slumbering without gravity's incessant pull makes sleeping in space rather comfy, Payette said.

5. Hygiene hiccups

The lack of showers in space often puts a serious damper on the experience.

Microgravity makes it impossible to have a normal shower where water falls from a stream and falls docilely into a drain. Instead, astronauts on the International Space Station use a squirt gun that shoots out water and a wash cloth. They also have a special rinse-less shampoo to keep their hair clean.

"We wash like we would if we were on an expedition or a camping trip or something," Payette explained. "It works."

Still, who wants to keep that up for six months? Especially with the aforementioned tight living quarters!

4. Toilet troubles

One of the peskiest recurring problems on the station is the toilet situation.

There are two toilets on the space station – one in the Russian segment, and one in the United States modules. But both have been balky, breaking and requiring on-orbit plumbing jobs to get them working again.

Then there's the issue of what happens to the waste water – as of May 2009, urine is recycled into clean drinking water, and is also recycled into water for bathing and food preparation.

"It's sort of one of those horrible and fascinating kind of things. It's like, 'You're going to drink urine?'" said astronaut Sandra Magnus, who was living on the station when the urine recycling system was installed. "We're not, we're drinking processed water that started as urine."

3. Creaky bones

Beyond the daily nuisances, astronauts have to deal with serious health consequences from their time in orbit. One of the most significant of these is the effect on their bones.

A recent study found that astronauts' bone strength dips by at least 14 percent during a half-year stay in space. Other research indicates that an astronaut's bone mineral density can decrease by between 0.4 percent and 1.8 percent each month they are on the station, leading to greater risks of fractures and osteoporosis later in life.

While there is no complete fix for this problem, astronauts are diligent about bone-strengthening exercises while they're on the station, and undergo extensive rehabilitation once they're back on the ground to try to avoid possessing the bones of a 90-year-old.

2. Losing your lunch

Space sickness, too, can affect the best of 'em.

Acclimatizing to life in zero gravity, especially since no simulator can reproduce microgravity on the ground, takes time. It's not uncommon for astronauts to lose their lunch after liftoff before they even reach the space station.

And, to make matters worse, spewing chunks in space creates rather more of a mess than it would on Earth, since projectile vomit doesn't project toward the ground.

1. The loneliest number

Perhaps the hardest part of life in space is the feeling of isolation astronauts can get when they spend half a year removed from the whole planet, especially their friends and family. While astronauts can combat the loneliness by bonding with crewmates and making frequent calls home, they sometimes have to miss major life events back on Earth.

In December 2007, NASA astronaut Daniel Tani's mother died in a car accident while he was living on the space station. Tani had to grieve from more than 200 miles away in orbit, until he came back to Earth about two months later.

And in 2004, NASA astronaut Michael Fincke was forced to miss the birth of his second child, when his wife gave birth to daughter Tarali while he was serving a long-duration mission during the station's Expedition 9. He was able to meet his daughter four months later when he finally landed.

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NASA space station marks 10th year

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The views from this five-bedroom, two-bathroom home are, well, out of this world.


And for the past decade, not a day has passed when someone hasn't been able to gaze out at Earth streaming by 220 miles below.

Tuesday marks 10 years of humans permanently living and working aboard the International Space Station.

That will break the record of uninterrupted human presence in Earth orbit, eight days short of 10 years, by Mir, a Russian complex in orbit from 1986 to 2001.

"Once you realize what you're doing, then you're astonished by the fact that here you are, one of six people in space," said astronaut Tracy Caldwell Dyson, who lived for 188 days on the ISS. "It can make you emotional at times."

The station's first resident crew -- two Russians and an American -- opened the outpost for business Nov. 2, 2000, beginning human operations that continued despite system failures, the post-Columbia grounding of NASA's shuttle fleet and an old-fashioned malady, homesickness.

Three months into Expedition 1's four-month mission, NASA realized they had to make some adjustments: More time was allowed for speaking to loved ones back home, and the crew was encouraged to watch movies and listen to music they liked.

"That's what it's really like to live in space," said KSC Director Robert Cabana, who has flown into space four times on the shuttle but admits he regrets never having completed a long-duration flight aboard the station. "The shuttle is phenomenal, but those space station crews . . . ."

Sixty-four people have boarded the outpost for long-duration stays. In total, 196 explorers have visited -- not including seven space tourists, all buying seats onboard the Russian Soyuz.

Crews conduct scientific research -- the main purpose of the station -- but also have to be handy enough to repair everything from a malfunctioning toilet to a broken solar panel.

"Just like your house, we have issues we need to fix," said Dan Hartman, chairman of the space station mission management team. "We don't have the hardware store down the street. We sometimes use the MacGyver technique."

Earth is currently in a period of warming. Over the last century, Earth's average temperature rose about 1.1°F (0.6°C). In the last two decades, the rate of our world's warming accelerated and scientists predict that the globe will continue to warm over the course of the 21st century. Is this warming trend a reason for concern? After all, our world has witnessed extreme warm periods before, such as during the time of the dinosaurs. Earth has also seen numerous ice ages on roughly 11,000-year cycles for at least the last million years. So, change is perhaps the only constant in Earth's 4.5-billion-year history.

Scientists note that there are two new and different twists to today's changing climate: (1) The globe is warming at a faster rate than it ever has before; and (2) Humans are the main reason Earth is warming. Since the industrial revolution, which began in the mid-1800s, humans have attained the magnitude of a geological force in terms of our ability change Earth's environment and impact its climate system.

Since 1900, human population doubled and then double again. Today more than 6.5 billion people inhabit our world. By burning increasing amounts of coal and oil, we drove up carbon dioxide levels in the atmosphere by 30 percent. Carbon dioxide is a "greenhouse gas" that traps warmth near the surface.

Humans are also affecting Earth's climate system in other ways. For example, we transformed roughly 40 percent of Earth's habitable land surface to make way for our crop fields, cities, roads, livestock pastures, etc. We also released particulate pollution (called "aerosols") into the atmosphere. Changing the surface and introducing aerosols into the atmosphere can both increase and reduce cloud cover. Thus, in addition to driving up average global temperature, humans are also influencing rainfall and drought patterns around the world. While scientists have solid evidence of such human influence, more data and research are needed to better understand and quantify our impact on our world's climate system.

John Yembrick
Headquarters, Washington
202-358-1100
john.yembrick-1@nasa.gov

Kylie Clem
Johnson Space Center, Houston
281-483-5111
kylie.s.clem@nasa.gov


Oct. 28, 2010

MEDIA ADVISORY : M10-153


NASA Celebrates 10th Anniversary Of Space Station With Crew News Conference And New Web Content


WASHINGTON -- The International Space Station partner agencies will mark a major milestone on Nov. 2 with the 10-year anniversary of people living permanently aboard the space station. NASA will commemorate the event with a news conference featuring the six crew members currently in orbit.

NASA Administrator Charles Bolden will begin the event, speaking live to the station crew at 9:15 a.m. EDT from the Kennedy Space Center in Florida. His remarks and the following news conference will be broadcast live on NASA Television.

The news conference will begin immediately after the administrator's conversation with the crew and be open to participation from accredited media representatives at participating NASA or international partner locations. U.S. media planning to attend should contact their respective NASA newsroom by 4 p.m. Monday, Nov. 1.

Expedition 25, the 25th crew to live and work aboard the station, consists of Commander Doug Wheelock; his fellow NASA astronauts Scott Kelly and Shannon Walker; and Russian cosmonauts Fyodor Yurchikhin, Alexander Kaleri and Oleg Skripochka.

The crew is awaiting the launch of space shuttle Discovery's six astronauts on the STS-133 mission to deliver supplies, spare parts and a permanent cargo module to the station. STS-133 is scheduled to lift off at 4:40 p.m. EDT on Nov. 1 from Kennedy.

"As we look forward to the next 10 years, taking us through 2020, the space station will serve many roles," said Mike Suffredini, International Space Station program manager. "With its permanent human presence, it will serve as a foothold for long-term exploration into space, being an integral part of testing human endurance, equipment reliability and processes essential for space exploration."

Since the Expedition 1 crew arrived at the station, humans have continuously occupied the orbiting laboratory. More than 196 people have visited the complex, and by the exact time of the anniversary (5:21 a.m., Nov. 2, 2000), the station will have completed 57,361 orbits of the Earth, traveling some 1.5 billion miles.

Representatives of the five international agencies that built and operate the station have agreed in principle to continuing its use for another decade. The governments of the 15 participating nations in the station partnership are in the process of formally endorsing that plan. More than 600 different research and technology development experiments have been conducted on the station, many of which are producing advances in medicine, recycling systems and a fundamental understanding of the universe.

In addition to the crew news conference, NASA is updating the content of the International Space Station section of its website in recognition of the 10th anniversary. The update supports the on-going transition from station assembly to utilization. The website now will focus on the research in the unique microgravity environment of low-Earth orbit.

The updated section of the NASA website incorporates an improved organization system to help visitors find what they are looking for with regard to research and technology development, crews and expeditions, international cooperation and the new capabilities of the station as a U.S. national laboratory.

The new space station section also provides better linkages with social media applications, including a new International Space Station Program scientist blog, and Twitter accounts for astronauts aboard the station and the National Laboratory. For more information, visit:

http://www.nasa.gov/station

For a Flash feature and Web story on the first 10 years of human life aboard the station, visit:

http://www.nasa.gov/externalflash/expedition_10_years

http://www.nasa.gov/mission_pages/station/living/10years.html

Julie Robinson, space station program scientist, is sponsoring an inside look at how research is conducted on the station through a new blog. The blog will bring to the public the stories of the researchers and their discoveries as they unfold.

For the new program scientist blog, visit:

http://go.usa.gov/atI

weddell-sea-radar

The first flight of the mission will be flying over a previous path over the Weddell Sea. Credit: Seelye Martin, University of Washington

After five days of weather delays, the NASA's IceBridge mission flew its first flight over the Antarctic polar caps yesterday.

The 12-hour flight was a great success, according to a report from Michael Studinger, one of the scientists on board the plane.

IceBridge is a six-year campaign to survey and monitor areas of Earth's polar ice sheets, glaciers and sea ice and how they are responding to climate change. The goal of this first flight of the winter Antarctic mission was to sample the conditions of sea ice in the Weddell Sea off the Antarctic Peninsula.

IceBridge's DC-8 plane, packed with scientists and equipments, traveled along a pair of lines from last year's mission that extend across the sea ice from the tip of the Antarctic Peninsula to south of Cape Norvegia, and back again. The flight path crossed the tip of the peninsula, proceeded to the eastern Weddell Coast, moved down the coast about 200 nautical miles (370 kilometers), and then transited back, where the sea ice is 1,500 feet (457 meters) thick.

One of the ways in which the plane measures the sea ice below is by Lidar (Light Detection And Ranging), an optical remote-sensing technology that measures properties of scattered light to find range and/or other information of a distant target.

"Lidars were successfully used to record the surface elevation of the sea ice floes, which are largely overlain by snow at this time of year. Wide-band radars were successfully used to estimate the thickness of the snow cover," Kenneth Jezek, the mission's science definition team co-leader from Ohio State University, told OurAmazingPlanet. "Knowledge about the snow thickness and also the surface elevation of the combined sea ice/snow cover column ultimately can be used to estimate the sea ice thickness."

dc8-icebridge-2010

A window view of Weddell Sea ice. Credit: NASA

Researchers who are part of the project but not on board the flights are also able to watch the progress of the flight in real time. Beyond the reports of the first mission's instruments working, there hasn't been much available to the researchers on the ground, but possibly in future missions sample data can accompany the feed.

"Right now, the flight and instrument crews have their hands full and are doing a great job!" Jezek said.

In a far-reaching restatement of goals for the nation’s space agency, NASA administrator Charles Bolden says President Obama has ordered him to pursue three new objectives: to “re-inspire children” to study science and math, to “expand our international relationships,” and to “reach out to the Muslim world.” Of those three goals, Bolden said in a recent interview with al-Jazeera, the mission to reach out to Muslims is “perhaps foremost,” because it will help Islamic nations “feel good” about their scientific accomplishments.

In the same interview, Bolden also said the United States, which first sent men to the moon in 1969, is no longer capable of reaching beyond low earth orbit without help from other nations.

Bolden made the statements during a recent trip to the Middle East. He told al-Jazeera that in the wake of the president’s speech in Cairo last year, the American space agency is now pursuing “a new beginning of the relationship between the United States and the Muslim world.” Then:

When I became the NASA Administrator — before I became the NASA Administrator — [Obama] charged me with three things: One was he wanted me to help re-inspire children to want to get into science and math, he wanted me to expand our international relationships, and third, and perhaps foremost, he wanted me to find a way to reach out to the Muslim world and engage much more with dominantly Muslim nations to help them feel good about their historic contribution to science, math, and engineering.

Later in the interview, Bolden discussed NASA’s goal of greater international cooperation in space exploration. He said the United States, more than 40 years after the first moon mission, cannot reach beyond earth’s orbit today without assistance from abroad:

In his message in Cairo, [Obama] talked about expanding our international outreach, expanding our international involvement. We’re not going to go anywhere beyond low earth orbit as a single entity. The United States can’t do it, China can’t do it — no single nation is going to go to a place like Mars alone.

Bolden’s trip included a June 15 speech at the American University in Cairo. In that speech, he said in the past NASA worked mostly with countries that are capable of space exploration. But that, too, has changed in light of Obama’s Cairo initiative. “He asked NASA to change…by reaching out to ‘non-traditional’ partners and strengthening our cooperation in the Middle East, North Africa, Southeast Asia and in particular in Muslim-majority nations,” Bolden said. “NASA has embraced this charge.”

NASA is not only a space exploration agency,” Bolden concluded, “but also an earth improvement agency.”

Technicians at NASA's Kennedy Space Center in Florida have begun preparations to replace two seals for a fuel line, which had been leaking, for shuttle Discovery’s orbital maneuvering system engines. Crews will pump out propellants already inside the tanks and will replace the primary and secondary seals at a flange located at the interface where two propellant lines meet in the shuttle’s aft compartment.


Replacing the seals allows NASA managers to have the highest confidence in the system and will allow the seals and flange to be inspected.

Work to replace the seals and reload propellants into the orbital maneuvering and reaction control systems should be completed on Oct. 25 and is expected to still support Discovery’s targeted Nov. 1 launch date

Technicians completed a checkout of the Extra-vehicular Mobility Unit (EMU) for the STS-133 mission yesterday. Preparations for the upcoming launch countdown are under way.

The STS-133 astronauts will practice procedures for the mission's first spacewalk in the Neutral Buoyancy Laboratory.

Space Shuttle Mission: STS-133

Flange location in doghouse door
Image above: The connecting point in a fuel line, which had been leaking, for space shuttle Discovery’s right-side orbiter maneuvering system engine. Two seals will be replaced in the flange. Photo credit: NASA/KSC

During space shuttle Discovery's final spaceflight, the STS-133 crew members will take important spare parts to the International Space Station along with the Express Logistics Carrier-4. Discovery has been moved to Launch Pad 39A at NASA's Kennedy Space Center in Florida. STS-133 is slated to launch Nov. 1.


One of the clear features visible in the IBEX maps is an apparent knot in the ribbon. Scientists were anxious to see how this structure would change with time. The second map showed that the knot in the ribbon somehow spread out. It is as if the knot in the ribbon was literally untangled over only 6 months! Credit: IBEX Science Team/Goddard Scientific Visualization Studio/ESA

When NASA launched the Interstellar Boundary Explorer (IBEX) on October 19, 2008, space physicists held their collective breath for never-before-seen views of a collision zone far beyond the planets, roughly 10 billion miles away. That’s where the solar wind, an outward rush of charged particles and magnetic fields continuously spewed by the Sun, runs into the flow of particles and fields that permeates interstellar space in our neighborhood of the Milky Way galaxy.

No spacecraft had ever imaged the collision zone, which occurs in a region known as the heliosheath, because it emits no light. But the two detectors on IBEX are designed to “see” what the human eye cannot. The interaction of the solar wind and interstellar medium creates energetic neutral atoms of hydrogen, called ENAs, that zip away from the heliosheath in all directions. Some of these atoms pass near Earth, where IBEX records their arrival direction and energy. As the spacecraft slowly spins, the detectors gradually build up pictures of the ENAs as they arrive from all over the sky.

Mission scientists got their first surprise six months after launch, once the spacecraft had scanned enough overlapping strips of sky to create a complete 360° map. Instead of recording a relatively even distribution all the way around, as expected, IBEX found that the counts of ENAs — and thus the strength of the interaction in the heliosheath — varied dramatically from place to place. The detectors even discovered a long, enhanced “ribbon,” accentuated by an especially intense hotspot or “knot,” arcing across the sky.


Now scientists have finished assembling a second complete sweep around the sky, and IBEX has again delivered an unexpected result: the map has changed significantly. Overall, the intensity of ENAs has dropped 10% to 15%, and the hotspot has diminished and spread out along the ribbon. Details of these findings appear in the September 27th issue of Journal of Geophysical Research (Space Physics).

“We thought we might detect small changes occurring gradually throughout the Sun’s 11-year-long activity cycle, but not over just 6 months,” notes David McComas (Southwest Research Institute), principal investigator for the IBEX mission and the paper’s lead author. “These observations show that the interaction of the Sun with the interstellar medium is far more dynamic and variable than anyone envisioned.”

In the past, space physicists had little notion of what to expect along the boundary where the Sun’s own magnetic bubble, the heliosphere, meets interstellar space. Even though the solar wind travels outward at roughly a million miles per hour, it still takes about a year to reach the heliosphere’s edge. Also, the encounter zone within the heliosheath is believed to be several billion miles thick (roughly Pluto’s distance from the Sun). Finally, the ENAs take another six months to many years to complete the return trip back to Earth, depending on their direction and energy.

With ENAs starting out from such a wide range of distances and traveling back toward Earth at different speeds, IBEX mission scientists had expected that any highs and lows in intensity arising within the heliosheath would be hopelessly smeared out in the spacecraft’s all-sky maps. So they’re elated by the variations and changes seen so far by IBEX. These early results hint that the solar wind and the interstellar flow might be interacting in a thinner layer than many researchers had imagined possible.

McComas says the dropoff in intensity between the two all-sky maps perhaps makes sense, because the Sun is only now emerging from an unusually long period of very low activity and a correspondingly weak solar wind. The fewer the solar-wind particles that reached the heliosheath in recent years, the fewer the ENAs that got created. “We didn’t plan it this way,” says McComas, “but it’s an almost perfect situation, in that we’re seeing the interaction in its simplest state — before trying to interpret what turns out to be a much more complicated interaction than anticipated.”

Artist's concept of the Interstellar Boundary Explorer

Roughly the size of a card table, the Interstellar Boundary Explorer is the latest in NASA’s series of low-cost, rapidly developed Small Explorers spacecraft. Credit: NASA/Goddard Space Flight Center Conceptual Image Lab If IBEX remains healthy, and if the team gets approval to continue well past its planned two-year mission, then the changes it’s seeing in the distant heliosheath should become more dramatic as solar activity ramps up later in this decade.

“The surprising results from IBEX show that there is still exciting science that can be done with small missions,” comments Eric Christian, a member of the spacecraft’s research team and the program’s Deputy Mission Scientist at the Goddard Space Flight Center. “This is clearly a huge success for the Explorer program.” IBEX is one of a dozen Explorer-class missions operated by NASA’s Science Mission Directorate.

“The public might think that scientists make measurements and instantly know what’s going on, but that is not how science really works,” McComas observes. “We thought the outer heliosphere would be stable over time — and IBEX is showing us that it’s not. This is changing the game completely.”


Image of Polar Mesospheric Clouds taken July 14, 2009 by the AIM satellite.

This image of Polar Mesospheric Clouds (PMC) from the Aeronomy of Ice in the Mesosphere Cloud Imaging and Particle Size (AIM-CIPS) instrument on July 14, 2009 in the northern polar region. The North Pole (90N) is in the center. Latitude bands of 80N, 70N, and 60N are also indicated by the light blue circles.
Credit: NASA

GREENBELT, Md. -- NASA's Aeronomy of Ice in the Mesosphere (AIM) satellite has captured five complete polar seasons of noctilucent (NLC) or "night-shining" clouds with an unprecedented horizontal resolution of 3 miles by 3 miles. Results show that the cloud season turns on and off like a "geophysical light bulb" and they reveal evidence that high altitude mesospheric "weather" may follow similar patterns as our ever-changing weather near the Earth's surface. These findings were unveiled today at the Fall Meeting of the American Geophysical Union today in San Francisco.

The AIM measurements have provided the first comprehensive global-scale view of the complex life cycle of these clouds, also called Polar Mesospheric Clouds (PMCs), over three entire Northern Hemisphere and two Southern Hemisphere seasons revealing more about their formation, frequency and brightness and why they appear to be occurring at lower latitudes than ever before.

"The AIM findings have altered our previous understanding of why PMCs form and vary," stated AIM principal investigator Dr. James Russell III of Hampton University in Hampton, Va. "We have captured the brightest clouds ever observed and they display large variations in size and structure signifying a great sensitivity to the environment in which the clouds form. The cloud season abruptly turns on and off going from no clouds to near complete coverage in a matter of days with the reverse pattern occurring at the season end."

These bright "night-shining" clouds, which form 50 miles above Earth's surface, are seen by the spacecraft's instruments, starting in late May and lasting until late August in the north and from late November to late February in the south. The AIM satellite reports daily observations of the clouds at all longitudes and over a broad latitude range extending from 60 to 85 degrees in both hemispheres.

The clouds usually form at high latitudes during the summer of each hemisphere. They are made of ice crystals formed when water vapor condenses onto dust particles in the brutal cold of this region, at temperatures around minus 210 to minus 235 degrees Fahrenheit. They are called "night shining" clouds by observers on the ground because their high altitude allows them to continue reflecting sunlight after the sun has set below the horizon. They form a spectacular silvery blue display visible well into the night time.

Sophisticated multidimensional models have also advanced significantly in the last few years and together with AIM and other space and ground-based data have led to important advances in understanding these unusual and provocative clouds. The satellite data has shown that:

1. Temperature appears to control season onset, variability during the season, and season end. Water vapor is surely important but the role it plays in NLC variability is only now becoming more understood,

2. Large scale planetary waves in the Earth's upper atmosphere cause NLCs to vary globally, while shorter scale gravity waves cause the clouds to disappear regionally;

3. There is coupling between the summer and winter hemispheres: when temperature changes in the winter hemisphere, NLCs change correspondingly in the opposite hemisphere.

Computer models that include detailed physics of the clouds and couple the upper atmosphere environment where they occur with the lower regions of the atmosphere are being used to study the reasons the NLCs form and the causes for their variability. These models are able to reproduce many of the features found by AIM. Validation of the results using AIM and other data will help determine the underlying causes of the observed changes in NLCs.

The AIM results were produced by Mr. Larry Gordley and Dr. Mark Hervig and the Solar Occultation for Ice Experiment (SOFIE) team, Gats, Inc., Newport News, Va. and Dr. Cora Randall and the Cloud Imaging and Particle Size (CIPS) experiment team, University of Colorado, Laboratory for Atmospheric and Space Physics in Boulder and Dr. Scott Bailey, Va. Tech, Blacksburg, Va.; Modeling results were developed by Dr. Daniel Marsh of the National Center for Atmospheric Research in Boulder, Colorado and Professor Franz-Josef Lübken of the Leibniz-Institute of Atmospheric Physics, Kühlungsborn, Germany.

AIM is a NASA-funded SMall EXplorers (SMEX) mission. NASA's Goddard Space Flight Center manages the program for the agency's Science Mission Directorate at NASA Headquarters in Washington. The mission is led by the Principal Investigator from the Center for Atmospheric Sciences at Hampton University in VA. Instruments were built by the Laboratory for Atmospheric and Space Physics (LASP), University of Colorado, Boulder, and the Space Dynamics Laboratory, Utah State University. LASP also manages the AIM mission and controls the satellite. Orbital Sciences Corporation, Dulles, Va., designed, manufactured, and tested the AIM spacecraft, and provided the Pegasus launch vehicle.

For more information about the AIM mission, visit:http://www.nasa.gov/mission_pages/aim/news/nlc-secrets.html

It looks a bit like someone has accidentally got their thumb caught in front of lens as they take a picture of the Sun.

But this remarkable image shows the moon as it passes between a spacecraft and the sun - causing a partial eclipse.

In a first for NASA's SDO (Solar Dynamics Observatory), the camera was watching the Sun in a wavelength of extreme ultraviolet light just as the dark Moon began to pass in front.




The moon passing between the SDO and the sun on October 7th, 2010 in an image taken by Nasa's Solar Dynamics Observatory

Tendrils of super-heated plasma - known as solar flares - can be seen reaching far out into space.

Plasma loops like these can heat up to a blistering 20 million degrees Celsius.

The bright plasma loop streaking out on the far left of the image is around 860,000 miles across.
These images are not just nice to look at, however. Scientists who monitor the SDO say the partial eclipse will prove useful to them in improving how the equipment on board works.
The very sharp edge of the lunar limb allows us to measure the in-orbit characteristics of the telescope e.g., light diffraction on optics and filter support grids.

'Once these are characterized , we can use that information to correct our data for instrumental effects and sharpen up the images to even more detail.'

SDO provides better-than-HD quality views of the Sun at a variety of wavelengths and has been responsible for some of the spectacular solar flare images which have emerged in recent months as the Sun begins a period of heightened activity.


The SDO blasted off from Cape Canaveral, Florida in February 2010 and is on a five year mission which is expected to cost £550million.

The spacecraft, orbiting 22,000 miles above Earth, is 7.2ft by 14.8ft. The solar panels are 21ft across and produce 1450W of power.

Instruments on board have additional shielding because this is in the outer reaches of the Earth's radiation belt where levels can be quite high.
The spacecraft carries three instruments that take ultra-high resolution images of the Sun every minute. It is also able to study solar pressure waves generated on its surface.

Partners in the International Space Station programme have agreed on a new standard for docking systems, which will be capable also of implementing berthing. The agreement allows a range of compatible, but not necessarily identical,mechanisms for spacecraft docking. A first agreed version of the Interface Definition Document will be released on 25 October.



The International Docking System Standard (IDSS) provides the guidelines for a common interface to link spacecraft together.
It builds on the heritage of the Russian developed APAS system (Androgynous Peripheral Attachment System) used for the Space Shuttle for the ‘hard docking’ and the innovative soft-capture features of the new NASA and ESA systems. Other agencies will be free to choose specific features behind the interface.

“The IDSS is an outstanding example of international collaboration. We have developed a common language for docking systems to use the same 'words' in space when it comes to work together,”

“The Docking Standard sweeps away the boundaries for a truly global exploration endeavour. It will also make joint Spacecraft docking operations more routine and eliminate critical obstacles to joint space exploration undertakings,” she continued.

"Today, our future in space is more open-minded than ever. ESA has been committed to the development of this standard since the inception of the working group and has contributed to the document defining this standard interface. We have been working for a number of years on the development of the IBDM (International Berthing Docking Mechanism) and we are willing to make the IBDM compatible with this new international docking standard,”







Open and flexible standard

The initial IDSS definition document will be released into the public domain on 25 October. It will contain a preliminary description of the physical features and design loads of the standard docking interface.

The technical teams from the five ISS partner agencies will continue to work on additional refinements and additions to the initial standard. ESA, NASA, Roscosmos, the Japan Aerospace Exploration Agency and the Canadian Space Agency are represented on the Multilateral Coordination Board, which coordinates Station activities among the partners.

The space shuttle Discovery is leaking on the launch pad.
If it isn't fixed soon, the small fuel leak could delay Discovery's planned launch on Nov. 1. The flight to the International Space Station is be Discovery's last.

Shuttle engineers to put together a repair plan. Technicians will tighten the bolts on the leaking fuel line. If that resolves the problem, Discovery could still launch on time.

But if that doesn't help, they may have to replace four seals or even part of the line. The leak involves seepage of toxic hydrazine thruster fuel from the plumbing in one of the shuttle's orbital maneuvering system pods, or OMS pods. The OMS thrusters are used during flight for on-orbit course changes.

Last week, NASA replaced a cap in the system, but it did not stop the leak.


The worst-case scenario would involve bringing Discovery back to the Vehicle Assembly Building for more extensive and time-consuming repairs. If the shuttle does not lift off during the first week of November, the mission could be delayed until as late as next February, due to a combination of launch-pad conflicts and orbital constraints.


During its STS-133 mission, Discovery is to deliver a module to orbit for permanent attachment to the space station as an extra storage room. Next Monday, launch managers are due to set the shuttle's official launch date at a flight readiness review.


The shuttle Endeavour is due to take the flight after Discovery's, and one last mission is expected to be flown next summer, using the shuttle Atlantis. Then all three shuttles are to be retired and put in museums. The Smithsonian Institution's National Air and Space Museum has already called dibs on Discovery.

Space Shuttle Mission Simulator

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