Obama Will Retire Shuttle in 2010, US Will Go Back to the Moon in 2020

This could still happen in 2020 (NASA)

[/caption]In a budget blueprint released by the White House on Thursday, President Barack Obama has confirmed his intent to carry out the planned retirement of the ageing Space Shuttle next year. Additionally, the the blueprint affirms Obama’s stance on a return trip to the Moon. The US will return to the lunar surface by the year 2020, following the time scale set out by George W. Bush’s 2004 Vision for Space Exploration. However, there is no mention that the next manned lunar mission will be carried out by the Constellation Program, a project plagued by criticism about its design and technology.

Although the blueprint may differ from the final budget submitted to Congress in April, it looks like there is some certainty about the future of the shuttle and the direction NASA will be taking over the next decade. And now the space agency has a little bit more money to do something about that troublesome 5-year gap in US manned access to space

So, any hope to extend the life of the Shuttle looks to have been dashed. Although there could still be a chance for a shuttle extension when the final budget is submitted, it seems as if President Obama has made his intent very clear; the 25 year-old space launch system will be mothballed, as planned, in 2010. This may come as a relief to many as extending the operational lifetime of the shuttle could be a safety risk, however, many on Florida’s Space Coast won’t be so happy as they could be looking at losing their jobs sooner than they would have hoped.

Generally, these decisions have been welcomed, including the extra $2.4 billion NASA will receive for the 2010 fiscal year (when compared with 2008):

Combined with $1 billion provided to NASA in the $787 billion stimulus package signed into law Feb. 17, the agency would receive $2 billion more than in the $17.7 billion 2009 NASA budget that was passed by the House – an increase that equals an Obama campaign promise. — Florida Today

It remains uncertain how the gap between shuttle retirement and Constellation launch could be shortened from the minimum of five years, but the extra cash is bound to boost confidence. But where does the blueprint say Constellation is even part of the plan? It doesn’t, sparking some media sources to point out that it remains a possibility that the Ares rocket system could be abandoned in favour of making the existing Atlas V or Delta IV rockets human rated. However, space policy specialists are advising not to read too much into the omission.

The budget doesn’t say a whole lot about any specific system,” said John Logsdon, a space policy analyst at the National Air and Space Museum in Washington, DC. “I wouldn’t interpret the absence of the words ‘Constellation’, ‘Ares’, and ‘Orion’ one way or another. That’s really up to the the new management team, when it gets there.”

After all, since the departure of Michael Griffin as NASA Administrator, the space agency has been without a leader. Acting NASA Administrator Christopher Scolese is currently at the helm, saying that the new budget “is fiscally responsible and reflects the administration’s desire for a robust and innovative agency.” Unfortunately the details about the use of Constellation may remain sketchy until the final budget is submitted.

This may be the case, but President Obama has obviously seen the merit in the original plans to get man back to the Moon by the year 2020, despite criticism from a guy who has actually stood on the Moon, Buzz Aldrin. In an “alternative” proposal for the future of NASA, Aldrin and two co-authors posted a draft of the “Unified Space Vision” on the National Space Society’s website this week (Update: the draft has now been “Removed At Request of the Authors”), urging the administration not to mount an unnecessary lunar mission (been there, done that) and go straight for manned exploration of the asteroids and Mars. The Unified Space Vision, unfortunately, was probably too hard on NASA’s accomplishments, saying that “post-Apollo NASA” has become a “visionless jobs-providing enterprise that achieves little or nothing,” in developing a viable space transportation system. Many of the points raised are valid (and occasionally very tough), but would require a complete change in NASA’s structure to accomplish. I doubt we’ll see any radical changes being enacted any time soon.

So, we now have a pretty good idea as to what’s going to happen to the shuttle next year; it looks like the plan to get the US back to the Moon by 2020 is still on and NASA has been given an extra $2 billion to play with. I hope they spend it wisely, perhaps on private space launch contracts?

Sources: Florida Today, New Scientist

Introducing NASA’s Virtual Universe “Astronaut: Moon, Mars and Beyond”

A scene from Astronaut: Moon, Mars and Beyond

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If, like me, you are a fan of first-person computer games and space exploration, you may be more than a little excited to hear about this news. A group of companies are currently working with NASA to create a Massively Multiplayer Online Role Playing Game (MMORPG) based around the space agency’s endeavours. They will use a game engine more familiar driving first-person shooters than online roleplay adventures; the tried and tested Unreal Engine 3 technology.

The Internet has a growing number of vast space-based MMORPGs, but NASA is hoping to use one of the most advanced gaming engines to develop an engrossing first-person online adventure, where players can choose their own mission to explore space, interact with other players and build settlements on other worlds. All this will take place in a scientifically accurate vision of a near-future Universe in 2035…

ammb_feb20Players will pick a profession like a roboticist, space geologist, astrobiologist or mechanical engineer and work together as a team as they explore space and complete missions, establishing bases and outposts and traveling to the farthest reaches of the solar system,” explained Jerry Heneghan, founder and CEO of Virtual Heroes, one of the companies involved with developing the NASA MMORPG Astronaut: Moon, Mars and Beyond. “The game will offer both individual challenges and team-based objectives to encourage players to use real-life applications of science, math and engineering to unlock new in-game vehicles, spacesuits, robotics and mining apparatus that will propel them further into space.”

MMORPGs are increasingly popular gaming platforms, where players can participate in seemingly boundless virtual universes. Popular examples of MMORPGs are World of Warcraft (which dominates with a monthly subscriber base of 11.5 million people), Second Life, EverQuest and space-based rollplayer games such as EVE Online and Star Trek Online.

Ever wanted to take a spin on the Moon?
Ever wanted to take a spin on the Moon?

Now NASA is hoping to create a very popular online gaming/educational experience that will not only entertain, but get young people interested in a career in science and engineering. What’s more, it is hoped the game will incorporate the Unreal Engine 3 Editor so that players can design their own content, from spaceships and stations to mission profiles. The developers will also include scenarios, such as the threat of near-Earth asteroid impacts and other reality-based events as the online community develops. This will provide a problem-solving/adventure element, while keeping the science grounded in science fact.

See more screenshots from the game »

There are concerns that a NASA space reality platform may not be very popular, as other in-space universes offer space fantasy, with epic spaceship battles and alien encounters. Also, the technical detail in carrying out “mundane” astronaut tasks may be a turn-off; virtual universes depend on exploration rather than educational tasks. Hopefully NASA and MMORPG developers will strike a healthy balance between education and entertainment.

Exploring Mars with NASAs MMORPG
Exploring Mars with NASAs MMORPG

However, I’m very excited to see Astronaut appear online sometime next year.

Sources: Big Download, Softpedia

Orbiting Carbon Observatory Launch Failure

The OCO launches on board a Taurus booster from Vandenberg Air Force Base (NASA TV)

[/caption]This morning (Tuesday), shortly after 2am PST (10am GMT), the launch of Orbiting Carbon Observatory (OCO) mission resulted in failure. According to reports from NASA, a “launch contingency” was declared shortly after the Taurus rocket upper stage finished firing T+12 minutes, 30 seconds into the flight. The rocket nose cone fairing failed to separate as expected, therefore the satellite could not be released. Further news is pending, but it appears that the failed Taurus XL upper stage plus OCO satellite remains in orbit. The OCO mission is declared lost…

The Orbiting Carbon Observatory (OCO) was launched by a Taurus XL rocket at 1:55:30 am PST from California’s Vandenberg Air Force Base, set for a polar orbit at an altitude of 438 miles (704 km) to begin an important and detailed study into the carbon dioxide content of our atmosphere. The satellite was designed to provide NASA with an insight to the sources of human and natural carbon emissions, as well as pin-pointing our planet’s carbon “sinks”. Unfortunately, the opportunity to gather valuable data with this about the global impact of carbon emissions with the advanced OCO mission has been lost.

At 2:16 am (PST), NASA launch commentator George Diller confirmed that a launch contingency had been implemented:

This is Taurus launch control. It appears that we have had a launch contingency. We don’t have the exact nature of the loss of mission, but NASA launch director Chuck Dovale has directed that the launch contingency plan be implemented. We will try to bring you any additional information as soon as we have it.” — Chuck Dovale (courtesy of Spaceflight Now)

The Orbiting Carbon Observatory (NASA)
The Orbiting Carbon Observatory (NASA)
A few minutes later, Diller went into some more detail about the failure to get the OCO into orbit. The casing (or fairing) failed to separated successfully, trapping the satellite inside the Taurus XL upper stage. NASA scientists continued to ascertain what condition the spacecraft was in, but any hopes of a successful outcome to the contingency were dashed when Diller said, “Right now, we do know that we have not had a successful launch tonight and will not be able to have a successful OCO mission.”

A terribly sad night for NASA and a terrible set-back to efforts to understand the full impact of human activity on the Earth’s atmosphere.

Special thanks to @govertschilling and @Zurack for their help with notifying me of the situation and forwarding me links via Twitter.

Source: Spaceflight Now

NASA Delays Discovery Launch Fourth Time

The space shuttle Discovery moved to the Kennedy Space Center Launch Pad on Jan. 14, but launch has been postponed until further notice. Credit: NASA/Troy Cryder

 

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NASA announced yet another delay for the launch of the Discovery STS-119 mission to the International Space Station Friday, marking the fourth time the mission has been postponed.

An all-day review of the craft’s readiness for launch left managers still under-confident about the operations of three hydrogen control valves that channel gaseous hydrogen from the main engines to the external fuel tank. Engineering teams have been working to identify what caused damage to a flow control valve on shuttle Endeavour during its November 2008 flight. NASA managers decided Friday more data and possible testing are required before launch can proceed.

“We need to complete more work to have a better understanding before flying,” said Bill Gerstenmaier, associate administrator for Space Operations at NASA Headquarters in Washington. Gerstenmaier chaired Friday’s Flight Readiness Review. 

“We were not driven by schedule pressure and did the right thing. When we fly, we want to do so with full confidence.”

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The STS-119 crew members gather in front of the hatch into space shuttle Discovery to place the mission plaque. Standing from left are Mission Specialists Joseph Acaba, Koichi Wakata, Steve Swanson, John Phillips and Richard Arnold and Pilot Tony Antonelli. Kneeling in front is Commander Lee Archambault. Photo credit: NASA/Kim Shiflett January 20, 2009

 

Besides understanding what happened with Endeavor’s valves last fall, teams also have tried to determine the consequences if a valve piece were to break off and strike part of the shuttle and external fuel tank.

Meanwhile, the Discovery launch date has shifted from Feb. 12, to Feb. 19, to Feb. 22, Feb. 27 and now — as of last night’s briefing — is postponed until further notice. The Space Shuttle Program has been asked to develop a plan for further inspections. The plan will be reviewed during a meeting on Wednesday, Feb. 25 and a new target launch date may be considered then.

The STS-119 mission is supposed to enhance the solar gathering power of the International Space Station so it might support a larger crew. When it does fly,  STS-119 will tote two solar array wings, each of which has two 115-foot-long arrays, for a total wing span of 240 feet, including the equipment that connects the two halves and allows them to twist as they track the sun. Altogether, the four sets of arrays can generate 84 to 120 kilowatts of electricity – enough to provide power for more than 40 average homes.

The mission astronauts arrived at the Kennedy Space Center Jan. 19 and have more or less been in standby mode ever since, shuttling back and forth between Florida and the Johnson Space Center in Houston. On Wednesday of this week, STS-119 mission specialists Richard Arnold and Joseph Acaba were in the Neutral Buoyancy Laboratory at Johnson, brushing up on spacewalk procedures. As of Thursday, the astronauts were in launch-countdown mode which included preflight quarantine.

Sweet Potatoes Flew into Space Aboard Columbia

Sweet potato cuttings grown in an Alabama laboratory were flown aboard Columbia to test root growth in microgravity. Courtesy of NASA.

 

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A team of researchers from the Deep South sent sweet potato plants into space, as part of an experiment aimed at providing food for long-term space missions.

Desmond G. Mortley, from the G.W. Carver Agricultural Experiment Station at Alabama’s Tuskegee University, and his colleagues launched the sweet potato cuttings on a five-day mission aboard the space shuttle Columbia, and compared their success to ground-based cuttings at Kennedy Space Center in Florida.

“The intent of the experiment was to study if stem cuttings would be a successful means of propagating plants in space, just as they are on Earth,” said Raymond Wheeler, a study co-author from NASA’s Biological Science Office at the Kennedy Space Center. “The results showed that the cuttings did indeed produce adventitious roots in microgravity, suggesting that cuttings should work well in space settings.”

The sweet potato experiment was flown on Columbia’s July 1999 mission to the Chandra X-Ray Observatory. The study findings were published in the May 2008 issue of the Journal of American Society for Horticultural Science, although a public press release was issued just this week.

Seeds of several crops have been grown in microgravity, but this was the first test for plants grown from cuttings. Cuttings grow roots faster than seeds do, and sweet potato cuttings regenerate very easily. This made them ideal for the study.

According to the study authors, all of the cuttings produced roots and growth was “quite vigorous in both ground-based and flight samples.” Except for a slight browning of some root tips in the flight samples, all of the stem cuttings appeared normal, they added. The roots on the flight cuttings tended to grow in random directions, sometimes perpendicular to the stems. Also, stem cuttings grown in microgravity had more roots and longer roots than ground-based controls.

The next step, Mortley and his colleagues say, will be to experiment over longer space missions to test root cuttings’ ability to grow plants.

Source: Eurekalert and Journal of American Society for Horticultural Science.

NASA’s Kepler Mission Ready for Launch

Technicians working inside the Astrotech Space Operations facility near NASA's Kennedy Space Center look over the Kepler spacecraft soon after it arrived in Florida in preparation for launch. Image credit: NASA/Tim Jacobs

 

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NASA’s Kepler spacecraft is ready to be moved to the launch pad today and will blast off within weeks, with a mission to address an age-old question: Are we alone?

Kepler is scheduled to blast into space from Florida’s Cape Canaveral Air Force Station aboard a Delta II rocket on March 5 at 10:48 p.m. eastern time (7:48 p.m. Pacific). It is the first mission with the ability to find planets like Earth — rocky planets that orbit sun-like stars in a warm zone where liquid water could be maintained on the surface. If Earth-sized and slightly larger planets are as common around other stars as some astronomers suspect, Kepler could spy hundreds of them within the next few years.

If so, “life may well be common throughout our universe,” said William Borucki, NASA’s principal investigator for Kepler science, who spoke about the mission Thursday afternoon at a NASA press conference. “If on the other hand we don’t find any, that will be another profound discovery. In fact it will mean there will be no Star Trek.”

 

The Kepler mission will spend three and a half years surveying more than 100,000 sun-like stars in the Cygnus-Lyra region of our Milky Way galaxy.  Its telescope is specially designed to detect the periodic dimming of stars that planets cause as they pass by. Some star systems are oriented in such a way that their planets cross in front of their stars, as seen from our Earthly point of view. As the planets pass by, they cause their stars’ light to slightly dim, or wink.

The telescope can detect even the faintest of these winks, registering changes in brightness of only 20 parts per million. To achieve this resolution, Kepler will use the largest camera ever launched into space, a 95-megapixel array of charged couple devices, known as CCDs.

“If Kepler were to look down at a small town on Earth at night from space, it would be able to detect the dimming of a porch light as somebody passed in front,” James Fanson, Kepler project manager at NASA’s Jet Propulsion Laboratory in Pasadena, California, said in a press release. During the briefing he added that the resolution is “akin to measuring a flea as it creeps across the headlight of an automobile at night. That’s the level of precision we have to achieve.”

Fanson added that Kepler, at a cost of about $500 million, is “the most complex piece of space flight hardware ever built” by the Boulder, Colorado-based Ball Aerospace & Technologies Corp.

The exoplanet research field has already proven exciting, Borucki said. Just over three hundred exoplanets have been detected so far, most of them gas giants like Jupiter and Saturn because those are the easiest to spot with pre-Kepler instruments. Already, the known exoplanets are an eclectic bunch.

“We’re finding planets that [would] float like foam on water,” Borucki said. “We’re finding planets with the density of lead.” And whereas researchers were expecting planet with orderly, circular orbits and sizes that increased with distances from stars, they’re finding a chaotic mix of behaviors — eccentric orbits, and giant, gaseous worlds so close to their parent stars that they complete full orbits within days.

By staring at one large patch of sky for the duration of its lifetime, Kepler will be able to watch planets periodically transit their stars over multiple cycles, allowing astronomers to confirm the presence of planets and use the Hubble and Spitzer space telescopes, along with ground-based telescopes, to characterize their atmospheres and orbits. Earth-size planets in habitable zones would theoretically take about a year to complete one orbit, so Kepler will monitor those stars for at least three years to confirm the planets’ presence.

The first objects likely to be reported will be the Jupiter- and Saturn-sized planets, and gradually — as confirmations roll in and detections get more focused — Neptune and then Earth-sized detections will be more likely to emerge, said exoplanet hunter Debra Fischer of San Francisco State University in California, who is not directly involved with the mission.

“We have a good chance of finding Mars-size planets, and a possibility of finding Mercury-sized planets” with Kepler, she said. “We don’t think we can do better than that.”

The scientists are in no rush to announce new discoveries until they’re “bulletproof,” they said — which could translate into years of suspense for the world’s Trekkies.

“We don’t want to have false discoveries,” Borucki said. “We want to be sure when we say it’s an earth, its an earth.”

Source: NASA teleconference and press release.

New Recipe for Dwarf Galaxies: Start with Leftover Gas

NASA's Galaxy Evolution Explorer reveals, for the first time, dwarf galaxies forming out of nothing more than pristine gas likely leftover from the early universe. Credit: NASA/JPL-Caltech/DSS

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Apparently, dwarf galaxies can spring out of thin air.

Astronomers using NASA’s Galaxy Evolution Explorer have spotted unexpected new galaxies in the constellation Leo that appear to be forming out of nothing more than pristine gas, probably leftover from the early universe.  The gas lacks both dark matter and metals — previously thought to be building blocks for galaxy formation.

Dwarf galaxies are relatively small collections of stars that often orbit around larger galaxies like our Milky Way. Though never seen before, the researchers say this new type of dwarf galaxy may be common throughout the more distant and early universe, when pristine gas was more pervasive. Their discovery appears in this week’s issue of the journal Nature.

The newly described dwarf galaxies are in the Leo Ring, a huge cloud of hydrogen and helium that traces a ragged path around two massive galaxies in the constellation Leo. The cloud is thought likely to be a primordial object, an ancient remnant of material that has remained relatively unchanged since the very earliest days of the universe. Identified about 25 years ago by radio waves, the ring cannot be seen in visible light.

“This intriguing object has been studied for decades with world-class telescopes operating at radio and optical wavelengths,” said lead study author David Thilker of Johns Hopkins University in Baltimore. He added that no stars were ever seen in the gaseous regions before. 

“But when we looked at the ring with the Galaxy Evolution Explorer, which is remarkably sensitive to ultraviolet light, we saw telltale evidence of recent massive star formation. It was really unexpected. We are witnessing galaxies forming out of a cloud of primordial gas.”

Our local universe contains two large galaxies, the Milky Way and the Andromeda galaxy, each with hundreds of billions of stars, and the Triangulum galaxy, with several tens of billions of stars. It also holds more than 40 much smaller dwarf galaxies, which have only a few billion stars. Invisible dark matter, detected by its gravitational influence, is a major component of both giant and dwarf galaxies with one exception — tidal dwarf galaxies.

Tidal dwarf galaxies condense out of gas recycled from other galaxies and have been separated from most of the dark matter with which they were originally associated. They are produced when galaxies collide and their gravitational masses interact. In the violence of the encounter, streamers of galactic material are pulled out away from the parent galaxies and the halos of dark matter that surround them.

Because they lack dark matter, the new galaxies observed in the Leo Ring resemble tidal dwarf galaxies, but they differ in a fundamental way. The gaseous material making up tidal dwarfs has already been cycled through a galaxy. It has been enriched with metals — elements heavier than helium — produced as stars evolve. “Leo Ring dwarfs are made of much more pristine material without metals,” Thilker said. “This discovery allows us to study the star formation process in gas that has not yet been enriched.”

Large, pristine clouds similar to the Leo Ring may have been more common throughout the early universe, Thilker said, and consequently may have produced many dwarf galaxies yet to be discovered that also lack dark matter.

Source: Caltech

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The forming dwarf galaxies shine in the far ultraviolet spectrum, rendered as blue in the call-out on the right hand side of this image. Near ultraviolet light, also obtained by the Galaxy Evolution Explorer, is displayed in green, and visible light from the blue part of the spectrum here is represented by red. The clumps (in circles) are distinctively blue, indicating they are primarily detected in far ultraviolet light. The faint blue overlay traces the outline of the Leo Ring, a huge cloud of hydrogen and helium that orbits around two massive galaxies in the constellation Leo (left panel). Credit: NASA/JPL-Caltech/DSS

NASA Study Predicted Outbreak of Deadly Virus

Scientists have long suspected that climatic variables like sea surface temperature and precipitation could foreshadow outbreaks of disease. Now, they have confirmation.

Responding to a deadly 1997 outbreak of the mosquito-borne disease Rift Valley fever, researchers had developed a “risk map,” pictured above, using NASA and National Oceanic and Atmospheric Administration measurements of sea surface temperatures, precipitation, and vegetation cover. As reported in a recent NASA-led study, the map gave public health officials in East Africa up to six weeks of warning for the 2006-2007 outbreak of the deadly Rift Valley fever in northeast Africa — enough time to lessen human impact.

On the map above, pink areas depict increased disease risk, while pale green areas reflect normal risk. Yellow dots represent reported Rift Valley fever cases in high-risk areas, while blue dots represent occurrences in non-risk areas. The researchers have detailed the map’s effectiveness in the Proceedings of the National Academy of Sciences.

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Scientists study a typical dambo habitat at Sukari Farm, a long-term Rift Valley Fever study site just outside Nairobi, Kenya. Dambos are natural breeding grounds for disease-carrying mosquitoes and can be observed from space with the aid of satellites. Credit: Assaf Anyamba

During an intense El Niño event in 1997, the largest known outbreak of Rift Valley fever spread across the Horn of Africa. About 90,000 people were infected with the virus, which is carried by mosquitoes and transmitted to humans by mosquito bites or through contact with infected livestock. That outbreak prompted the formation of a working group — funded by the U.S. Department of Defense Global Emerging Infections Surveillance and Response System — to try to predict future outbreaks.

The working group didn’t start from scratch. The link between the mosquito life cycle and vegetation growth was first described in a 1987 Science paper by co-authors Kenneth Linthicum of the U.S. Department of Agriculture and Compton Tucker of NASA’s Goddard Space Flight Center. Later, a 1999 Science paper described a link between Rift Valley fever and the El Niño-Southern Oscillation, a cyclical, global phenomenon of sea surface temperature changes that can contribute to extreme climate events around the world.

Building on that research, Assaf Anyamba of NASA Goddard and the University of Maryland, and his colleagues, set out to predict when conditions were ripe for excessive rainfall — and thus an outbreak. They started by examining satellite measurements of sea surface temperatures. One of the first indicators that El Niño will boost rainfall is a rise in the surface temperature of the eastern equatorial Pacific Ocean and the western equatorial Indian Ocean. Perhaps the most telling clue is a measure of the mosquito habitat itself. The researchers used a satellite-derived vegetation data set that measures the landscape’s “greenness.” Greener regions have more than the average amount of vegetation, which means more water and more potential habitat for infected mosquitoes. The resulting risk map for Rift Valley fever, showing areas of anomalous rainfall and vegetation growth over a three-month period, is updated and issued monthly as a means to guide ground-based mosquito and virus surveillance.

As early as September 2006, the monthly advisory from Anyamba and colleagues indicated an elevated risk of Rift Valley fever activity in East Africa. By November, Kenya’s government had begun collaborating with non-governmental organizations to implement disease mitigation measures—restricting animal movement, distributing mosquito bed nets, informing the public, and enacting programs to control mosquitoes and vaccinate animals. Between two and six weeks later—depending on the location—the disease was detected in humans.

After the 2006-2007 outbreak, Anyamba and colleagues assessed the effectiveness of the warning maps. They compared locations that had been identified as “at risk” with the locations where Rift Valley fever was reported. Of the 1,088 cases reported in Kenya, Somalia, and Tanzania, 64 percent fell within areas delineated on the risk map. The other 36 percent of cases did not occur within “at risk” areas, but none were more than 30 miles away, leading the researchers believe that they had identified most of the initial infection sites.

The potential for mapping the risk of disease outbreaks is not limited to Africa. Previous research has shown that risk maps are possible whenever the abundance of a virus can be linked to extremes in climate conditions. Chikungunya in east Africa and Hantavirus and West Nile virus in the United States, for example, have been linked to conditions of rainfall extremes.

“We are coming up on almost 30 years of vegetation data from satellites, which provides us with a good basis for predicting,” said Linthicum, co-author on the 1987 paper, upon his return from a Rift Valley fever workshop in Cairo, Egypt last month. “At this meeting, it was clear that using this tool as a basis for predictions has become accepted as the norm.”

Sources: NASA and the Proceedings of the National Academy of Sciences

New Theory: Bizarre Martian Deposits from Vast Ice at Equator

Ice core from Mars? Not quite. But this aggregation of soil grains, from Antarctica ice, derived from the same process now proposed for the Red Planet (Credit: Hans Paerl, University of North Carolina at Chapel Hill).

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Ice core from Mars? Not quite. But this aggregation of soil grains, from Antarctica ice, derived from the same process now proposed for the Red Planet (Credit: Hans Paerl, University of North Carolina at Chapel Hill)

The puzzling Meridiani Planum deposits on Mars — discovered by NASA’s Opportunity rover — could be remnants of a massive ancient ice field, according to a new study online in Nature Geoscience.

Paul Niles of NASA’s Johnson Space Center and Joseph Michalski, of Université Paris-Sud, analysed the chemistry, sedimentology and geology of the Meridiani Planum deposits using data from Opportunity. They suggest that sulphate formation and chemical weathering occurred within an ice deposit as massive as today’s polar ice caps on Mars. Once the ice sublimed away in a warmer climate, the remaining sediments kept their chemical signature, the authors suggest.

The new theory gets around a weakness in the previous belief, that the deposits were formed in a wet, shallow basin — because no evidence of such a basin has been found yet. But it comes with its own baggage: there’s not much evidence of massive ice in the region, either.

The Meridiani represent one of the flattest areas on the Martian surface, with long, rolling smooth plains, linear dunes and ridges. Based on the number of craters, scientists have speculated that it formed early in the Hesperian Era, roughly 3.8 billion years ago.

The intriguing place — right at the crosshairs of zero degrees longitude and zero degrees latitude — was initially spotted by the Mars Thermal Emission Spectrometer aboard NASA’s Mars Global Surveyor (1996-2006). It was then chosen as the landing site for NASA’s rover Opportunity, in 2004.

“Immediately upon touchdown, when we turned on the cameras for the first time and looked out on the plains, it became obvious that it was a different kind of place on Mars than we’d ever been before,” Michalski said.

Since then, the place has been the object of numerous chemistry studies which have generated a handful of competing theories about how its odd sulfate deposits might have formed. The prevailing theory, fronted by scientists on the Mars Exploration Rovers team, has it that the Meridiani Planum was once a shallow evaporation basin which was periodically wet, where wind helped drive away the moisture and left the deposits behind. Other scientists have proposed a catastrophic event like a volcano or major impact, perhaps with volcanic aerosols altering layered rocks at the surface.

Microscopic image of Meridiani Planum sediments. Image of outcrop of sediments at Meridiani Planum inside Endurance crater taken by the microscopic imager on sol 145 (Credit: NASA/JPL/Cornell/USGS).
Microscopic image of Meridiani Planum sediments. Image of outcrop of sediments at Meridiani Planum inside Endurance crater taken by the microscopic imager on sol 145 (Credit: NASA/JPL/Cornell/USGS).

But Michalski and Niles say the deposits formed when the area was covered with thick ice. Dust trapped within the ice would have warmed in the presence of sunlight, causing minor melting nearby. And because the ice also contained volcanic aerosols, the water that formed would have been highly acidic, and reacted with the dust, yielding the perplexing products in pockets within the ice that became the deposits when the ice sublimed. The same process happens to a limited extent in the Earth’s polar regions, Michalski said. The Meridiani Planum is near the equator, where large ice fields are lacking today. The authors propose that the ice could have formed in ancient times, when the poles were in a different place or when the Martian axis of rotation was at a different angle.

Michalski said the new theory gets around a lot of the sticking points in the older ones.

“It doesn’t require a basin to be present; it doesn’t require the groundwater,” he said. “We like a lot of aspects of the MER team’s hypothesis. One of the big problems is that you have to have a lot of acidic water in that situation.”

Brian Hynek, an atmospheric and space physicist at the University of Colorado in Boulder, had proposed a volcanic origin for the deposits in the past, but he said there are strengths to the new theory as well. For starters, he said, the ice pocket hypothesis could explain why salts of varying water solubility co-exist so closely in the Meridiani Planum deposits.

“The volume of the Meridiani deposits is similar to the amount of sediment contained within the layered ice-rich deposits at Mars’s south pole,” he added. “And sublimation of a sufficiently large dusty ice deposit would provide a convincing source for all the sediment, which other models have failed to provide.”

But he said there are shortfalls to the new theory too: No model has allowed for the necessarily massive ice deposits at the Martian equator, for example, and it’s curious how the dust and aerosols “could aggregate into consistent sand-sized particles” in the examined bedrock.

Hynek said of all the theories that could explain the strange deposits in the Meridiani Planum, none has emerged yet as a clear winner: “All have their strengths and all have significant weaknesses. I don’t think we’ve solved this mystery yet.”

Michalski is less cautious about the implications of the new work.

“We’re able to propose this process for the Meridiani deposits because there are a lot of data,” he said. “We think that it’s likely that the other sulfate deposits on Mars could have been formed by the same mechanism.”

Sources: Joseph Michalski and Brian Hynek

Fermi, Swift spy outburst from gamma-ray star

Gamma-rays flares from SGR J1550-5418 may arise when the magnetar's surface suddenly cracks, releasing energy stored within its powerful magnetic field. Credit:NASA/Goddard Space Flight Center Conceptual Image Lab

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NASA’s Swift satellite and Fermi Gamma-ray Space Telescope have keyed in on a rowdy stellar remnant 30,000 light-years away. The object, already known as a source of pulsing radio and X-ray signals, lies in the southern constellation Norma. It kicked out some moderate eruptions in October, but then it settled down again. Late last month, it roared to life.

“At times, this remarkable object has erupted with more than a hundred flares in as little as 20 minutes,” said Loredana Vetere, who is coordinating the Swift observations at Pennsylvania State University. “The most intense flares emitted more total energy than the sun does in 20 years.”

The new object has been cataloged as SGR J1550-5418. Because of the recent outbursts, astronomers will classify it as a soft-gamma-ray repeater. Only six such objects are known to science, and they share the trait that they unpredictably send out a series of X-ray and gamma-ray flares. In 2004, a giant flare from another soft-gamma-ray repeater was so intense it measurably affected Earth’s upper atmosphere from 50,000 light-years away.

The source of the wild emissions is probably a spinning neutron star — the superdense, city-sized remains of an exploded star. Measuring only about 12 miles (19 kilometers) across, a neutron star is more massive than the sun.

While neutron stars typically possess intense magnetic fields, a subgroup displays fields 1,000 times stronger. These so-called magnetars have the strongest magnetic fields of any known objects in the universe. SGR J1550-5418, which rotates once every 2.07 seconds, holds the record for the fastest-spinning magnetar. Astronomers think magnetars power their flares by tapping into the tremendous energy of their magnetic fields.

Fermi’s gamma-ray burst monitor is designed to investigate magnetar flares, and SGR J1550-5418 has already triggered the instrument more than 95 times since Jan. 22. Swift’s X-ray telescope captured the first “light echoes” ever seen from a oft-gamma-ray repeater when SGR J1550-5418 started exploding. Both the halo-like rings and their apparent expansion are an illusion caused by the finite speed of light and the longer path the scattered light must travel. NASA’s Wind satellite, the joint NASA-Japan Suzaku mission, and the European Space Agency’s INTEGRAL satellite also have detected flares from SGR J1550-5418.

Swift's X-Ray Telescope (XRT) captured an apparent expanding halo around the flaring neutron star SGR J1550-5418. The halo formed as X-rays from the brightest flares scattered off of intervening dust clouds. Credit: NASA/Swift/Jules Halpern (Columbia Univ.)
Swift's X-Ray Telescope (XRT) captured an apparent expanding halo around the flaring neutron star SGR J1550-5418. The halo formed as X-rays from the brightest flares scattered off of intervening dust clouds. Credit: NASA/Swift/Jules Halpern (Columbia Univ.)
Source: NASA