NASA Finds Warmer Ocean Speeding Greenland Glacier Melt

Glaciers in west Greenland are melting 100 times faster at their end points beneath the ocean than they are at their surfaces, according to a new NASA/university study published online Feb. 14 in Nature Geoscience. The results suggest this undersea melting caused by warmer ocean waters is playing an important, if not dominant, role in the current evolution of Greenland's glaciers, a factor that had previously been overlooked.

Researchers Eric Rignot and Isabella Velicogna, both of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and the University of California, Irvine; along with colleague Michele Koppes of the University of British Columbia, Vancouver, Canada, measured the undersea melting rates of four glaciers in central west Greenland in the summer of 2008. They deployed oceanographic equipment in the glacier fjords, sampling the water at various depths to measure ocean currents, temperature and salinity, along with the depth of the fjords. The researchers found the melt rates of the glaciers studied was 100 times larger under the ocean at their terminus points than that observed at the glacial surfaces.

Rignot said the new study complements other recent research on the effects of ocean conditions in Greenland fjords. A study in the same online issue of Nature Geoscience by researcher Fiammetta Straneo of the Woods Hole Oceanographic Institution, Woods Hole, Mass., and colleagues looked at changes in oceanographic conditions in fjords that may be conducive to changes in undersea melting. Another 2008 Nature Geoscience study by researcher David Holland of New York University, New York, found that Greenland glaciers sped up as warm waters intruded into their fjords.

"Our study fills the gap by actually looking at these submarine melt rates, something that had never been done before in Greenland," Rignot said. "The results indicate rather large values that have vast implications for the evolution of the glaciers if ocean waters within these fjords continue to warm."

In recent years, scientists have observed a widespread acceleration of Greenland's glaciers, associated with thinning of their lower reaches as they reach the sea. In the past decade, surface melting of glaciers around Greenland due to warm air temperatures has increased in both magnitude and area, while snowfall has increased just slightly. The result is a tripling in the amount of ice mass lost in Greenland between 1996 and 2007. Of this loss, between 50 and 60 percent is attributable to a speedup in the flow of outlet glaciers, with the remainder due to increased surface melting.

But the glaciers also melt along their submerged faces, where they come into contact with warm ocean waters. A warmer ocean erodes a glacier's submerged, grounded ice and causes its grounding line -- the point at which a tidewater glacier floats free of its bed -- to retreat. Little is known about these rates of undersea melting and how they may influence the glaciers. The only previous measurements of undersea glacier melting were in Alaska.

The melting of glaciers beneath the ocean surface causes deep, warm, salty water to be drawn up toward the glacier's face, where it mixes turbulently with the glacier's cold, fresh water. The water then rises along the glacier face, melting its ice along the way, then reaches the ocean surface and flows away from the glacier in a plume. An ocean temperature of 3 degrees Celsius (37.4 degrees Fahrenheit) can melt glacial ice at a rate of several meters per day, or hundreds of meters over the course of a summer.

Rignot said the study points to the need to include the ocean factor if scientists are to increase the reliability of models used to predict how Greenland will be affected by climate change.

"All major Greenland glaciers end up in the ocean, and tidewater glaciers control 90 percent of the ice discharged by Greenland into the sea," Rignot said. "Submarine melting may therefore have a large indirect impact on the ice mass budget of the entire Greenland Ice Sheet. If we are to determine the future of the Greenland Ice Sheet more reliably in a changing climate, more complete and detailed studies of the interactions between ice and ocean at the ice sheet's margins are essential."

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Solar Dynamics Observatory Begins Mission to Study Our Sun

Solar Dynamics Observatory

The Atlas V roared to life Thursday morning to send the Solar Dynamics Observatory into space on its mission to evaluate the complex mechanisms of the sun. Liftoff came on-time at 10:23 a.m. EST from Launch Complex 41 at Cape Canaveral Air Force Station on Florida's Atlantic Coast.

The SDO spacecraft is in good shape midway through the launch phase that will eventually place it in an elongated orbit reaching more than 21,000 miles high. Eventually, SDO's orbit will be circularized and will reach about 22,300 miles in what is called geosynchronous orbit. From that altitude, the spacecraft will point its instruments at the sun and relay the readings instantly to a ground station in New Mexico.

The research is expected to reveal the sun's inner workings by constantly taking high resolution images of the sun, collecting readings from inside the sun and measuring its magnetic field activity. This data is expected to give researchers the insight they need to eventually predict solar storms and other activity on the sun that can affect spacecraft in orbit, astronauts on the International Space Station and electronic and other systems on Earth.Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Tranquility Node Up and Running on Station

Tranquility Node Up and Running on Station

Computers and other systems have been activated on the space station's new Tranquility node. Mission managers have extended Endeavour's stay by a day.

The crew relocated the cupola at 1:25 a.m. EST from the Tranquility node’s forward side to Tranquility’s nadir (Earth-facing) port. The second stage capture of the cupola was at 1:31 a.m. EST, signifying the completion of the module’s relocation. It is securely latched and all Common Berthing Mechanism bolts have been driven in.

Astronauts Move Cupola, Activate Tranquility

Astronauts on space shuttle Endeavour relocated one of the new modules they just delivered to the International Space Station, and pressed ahead with activation and checkout of the new Tranquility node.

Mission Specialists Nicholas Patrick and Robert Behnken spent the first three hours of their day working on tools and preparations of the station’s airlock for the last planned spacewalk on Tuesday.

Pilot Terry Virts and Mission Specialist Kathryn Hire kicked off the day monitoring the depressurization of the cupola module. While they operated Canadarm2, station Commander Jeff Williams operated the common berthing mechanisms for the relocation of cupola from Tranquility’s outboard hatch to the Earth-facing side of the module.

Cupola will then be repressurized and monitored for an airtight seal by flight controllers in Houston. At the same time shuttle Commander George Zamka, Mission Specialist Stephen Robinson, and station Flight Engineers Max Suraev and T.J. Creamer will resume outfitting and activation of Tranquility.

At 10:24 p.m. EST, Virts and Hire took time to answer questions about their mission prepared by students at NASA Explorer Schools. At 6:04 a.m. Monday Virts and Behnken will talk about the flight in interviews with WOR Radio New York’s John Gambling and television stations KTVI-TV in St. Louis and WREG-TV in Memphis.Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Layers Piled in a Mars Crater Record a History of Changes

Near the center of a Martian crater about the size of Connecticut, hundreds of exposed rock layers form a mound as tall as the Rockies and reveal a record of major environmental changes on Mars billions of years ago.

The history told by this tall parfait of layers inside Gale Crater matches what has been proposed in recent years as the dominant planet-wide pattern for early Mars, according to a new report by geologists using instruments on NASA's Mars Reconnaissance Orbiter.

"Looking at the layers from the bottom to the top, from the oldest to the youngest, you see a sequence of changing rocks that resulted from changes in environmental conditions through time," said Ralph Milliken of NASA's Jet Propulsion Laboratory, Pasadena, Calif. "This thick sequence of rocks appears to be showing different steps in the drying-out of Mars."

Using geological layers to understand stages in the evolution of a planet's climate has a precedent on Earth. A change about 1.8 billion years ago in the types of rock layers formed on Earth became a key to understanding a dramatic change in Earth's ancient atmosphere.

Milliken and two co-authors report in Geophysical Research Letters that clay minerals, which form under very wet conditions, are concentrated in layers near the bottom of the Gale stack.

Above that, sulfate minerals are intermixed with the clays. Sulfates form in wet conditions and can be deposited when the water in which they are dissolved evaporates. Higher still are sulfate-containing layers without detectable clays. And at the top is a thick formation of regularly spaced layers bearing no detectable water-related minerals.

Rock exposures with compositions like various layers of the Gale stack have been mapped elsewhere on Mars, and researchers, including Jean-Pierre Bibring of the University of Paris, have proposed a Martian planetary chronology of clay-producing conditions followed by sulfate-producing conditions followed by dry conditions. However, Gale is the first location where a single series of layers has been found to contain these clues in a clearly defined sequence from older rocks to younger rocks.

"If you could stand there, you would see this beautiful formation of Martian sediments laid down in the past, a stratigraphic section that's more than twice the height of the Grand Canyon, though not as steep," said Bradley Thomson of the Johns Hopkins University Applied Physics Laboratory, Laurel, Md. He and John Grotzinger of the California Institute of Technology in Pasadena are Milliken's co-authors.

NASA selected Gale Crater in 2008 as one of four finalist sites for the Mars Science Laboratory rover, Curiosity, which has a planned launch in 2011. The finalist sites all have exposures of water-related minerals, and each has attributes that distinguish it from the others. This new report is an example of how observations made for evaluating the landing-site candidates are providing valuable science results even before the rover mission launches.

Three instruments on NASA's Mars Reconnaissance Orbiter have provided key data about the layered mound in Gale Crater. Images from the High Resolution Imaging Science Experiment camera reveal details used to map hundreds of layers. Using stereo pairs of the images, the U.S.

Geological Survey has generated three-dimensional models used to discern elevation differences as small as a meter (about a yard). Observations by the Compact Reconnaissance Imaging Spectrometer for Mars yielded information about minerals on the surface. The Context Camera provided broader-scale images showing how the layers fit geologically into their surroundings.

Thomson said, "This work demonstrates the synergy of the instruments on the Mars Reconnaissance Orbiter. We wouldn't have as complete a picture if we were missing any of the components." Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Astronauts Enter Tranquility Node, Cupola on Space Station

Astronauts

Endeavour and space station astronauts entered the outpost's new "room with a view" for the first time late Friday.

ISS Commander Jeff Williams opened the hatch into Tranquility at 9:17 p.m. EST on Friday entering it for the first time with STS-130 Commander George Zamka and Mission Specialist Stephen Robinson. The hatch into the cupola was opened afterwards at 11:32 p.m.

Opening Night for Tranquility

The doors leading to the final U.S. components of the International Space Station were opened at 9:17 p.m. EST. The crews of space shuttle Endeavour and the station entered Tranquility and began internal outfitting of the module and the cupola.

While Pilot Terry Virts and Mission Specialist Kathryn Hire took the controls of the space station’s robotic arm for a walkoff from its base on the Harmony module to the Destiny laboratory, Mission Specialist Stephen Robinson and station Commander Jeff Williams began outfitting the vestibule between Tranquility and the Unity node.

While internal outfitting proceeds Virts and Flight Engineer Soichi Noguchi will move components of the Advanced Resistive Exercise Device and the Air Revitalization System rack into the new node.

Spacewalkers Robert Behnken and Nicholas Patrick are preparing a new spacesuit for Patrick to use during the second spacewalk scheduled to begin Saturday at 9:09 p.m. It was discovered that his original suit had a temporary slight decrease in the speed in its cooling fan during the first spacewalk.

Behnken and Patrick took a break at 2:29 a.m. Saturday to answer questions about the mission that have been gathered by astronaut and spacecraft communicator Mike Massimino on his Twitter account.Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Solar Dynamics Observatory Launches!

Solar Dynamics

The Atlas V roared to life Thursday morning to send the Solar Dynamics Observatory into space on its mission to evaluate the complex mechanisms of the sun. Liftoff came on-time at 10:23 a.m. EST from Launch Complex 41 at Cape Canaveral Air Force Station on Florida's Atlantic Coast.

The SDO spacecraft is in good shape midway through the launch phase that will eventually place it in an elongated orbit reaching more than 21,000 miles high. Eventually, SDO's orbit will be circularized and will reach about 22,300 miles in what is called geosynchronous orbit.

From that altitude, the spacecraft will point its instruments at the sun and relay the readings instantly to a ground station in New Mexico. The research is expected to reveal the sun's inner workings by constantly taking high resolution images of the sun, collecting readings from inside the sun and measuring its magnetic field activity.

This data is expected to give researchers the insight they need to eventually predict solar storms and other activity on the sun that can affect spacecraft in orbit, astronauts on the International Space Station and electronic and other systems on Earth.Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Endeavour Arrives at International Space Station

EndeavourSpacewalk preparations and water recovery system maintenance highlight the work schedule for the first full day of joint docked operations by the astronauts on space shuttle Endeavour and the International Space Station.


First up for Mission Specialists Nicholas Patrick and Bob Behnken will be time to configure tools they’ll take outside on the first spacewalk of the mission Thursday evening. Shuttle Commander George Zamka and station Flight Engineer Soichi Noguchi will resize a spare spacesuit for Behnken after a power harness on his original suit failed.

Station Commander Jeff Williams began his day by beginning the installation of a new Distillation Assembly and Flow Control Pump Assembly in the station’s Water Recovery System as part of the plan to reactivate the equipment that processes urine into drinking water for station crews.

Flight Engineers Max Suraev and Oleg Kotov will continue to pack items in a Progress supply ship and T.J. Creamer is scheduled to be monitoring several scientific payloads. Shuttle Pilot Terry Virts and Mission Specialists Kay Hire and Steve Robinson will continue moving new equipment and supplies from Endeavour onto the station.

All 11 crew members are scheduled for some off duty time in the latter portion of their day before a spacewalk procedures review at 4:09 a.m. EST Thursday.

The International Space Station has been moving steadily closer to completion for the past several years. But what house is complete without a utility room, a gym and a picture window?

During the STS-130 mission, space shuttle Endeavour will deliver the Tranquility node and its cupola, a dome-shaped extension from Tranquility made up of seven windows. They will be the last major U.S. modules to be added to the space station, and together they’ll help clear out premium workspace in other areas of the station – as well as offer a window on the world.

At 15 feet wide and 23 feet long, the Tranquility node will provide a centralized home for the station’s environmental control equipment – one of the systems that remove carbon dioxide from the station’s air, one of the station’s bathrooms and the equipment that converts urine into drinkable water, all of which is currently taking up space in the Destiny laboratory.

And there’s enough room left over to house the station’s new treadmill and its microgravity equivalent of a weight machine, moving it out of the Unity node where it’s in the way whenever spacewalk preparations are going on inside the adjacent Quest airlock.

“It gives us a much needed addition to the house, so to speak,” said Bob Dempsey, lead space station flight director for the mission. “We’re getting to the point where we’re really cramped for space. You might be surprised at that, considering we’re essentially the volume of a 747 and we’ve been adding modules for the last couple of years.

You might think we’d be sitting around in a big empty house. But no – every inch is really getting packed up there. Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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Solar Dynamics Observatory Set to Launch Today

Solar Dynamics

The Solar Dynamics Observatory is set for an unprecedented mission to study the sun and its dynamic behavior.

The Solar Dynamics Observatory and its Atlas V rocket rolled out to the launch pad at Launch Complex 41 at Cape Canaveral Air Force Station in Florida. The Tuesday morning move sets the stage for a liftoff Wednesday at 10:26 a.m. EST.

Weather for launch day stands at 40 percent "go" at liftoff time due to wind, cloud thickness and a slight chance of showers. The temperature at launch time is expected to be a chilly 51 degrees.

Live coverage of the launch will begin at 7:15 a.m. Wednesday on NASA TV and NASA's Launch Blog.

SDO's unprecedented mission will study the sun and its dynamic behavior. Onboard telescopes will scrutinize sunspots and solar flares using more pixels and colors than any other observatory in the history of solar physics. And SDO will reveal the sun’s hidden secrets in a prodigious rush of pictures.
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Dark-Orange And Charcoal-Black Terrain

Dark-Orange And Charcoal-Black Terrain

NASA today released the most detailed set of images ever taken of the distant dwarf planet Pluto. The images taken by NASA's Hubble Space Telescope show an icy and dark molasses-colored, mottled world that is undergoing seasonal changes in its surface color and brightness. Pluto has become significantly redder, while its illuminated northern hemisphere is getting brighter.

These changes are most likely consequences of surface ices sublimating on the sunlit pole and then refreezing on the other pole as the dwarf planet heads into the next phase of its 248-year-long seasonal cycle. The dramatic change in color apparently took place in a two-year period, from 2000 to 2002.

The Hubble images will remain our sharpest view of Pluto until NASA's New Horizons probe is within six months of its Pluto flyby. The Hubble pictures are proving invaluable for picking out the planet's most interesting-looking hemisphere for the New Horizons spacecraft to swoop over when it flies by Pluto in 2015.

Though Pluto is arguably one of the public's favorite planetary objects, it is also the hardest of which to get a detailed portrait because the world is small and very far away. Hubble resolves surface variations a few hundred miles across, which are too coarse for understanding surface geology.

But in terms of surface color and brightness Hubble reveals a complex-looking and variegated world with white, dark-orange and charcoal-black terrain. The overall color is believed to be a result of ultraviolet radiation from the distant sun breaking up methane that is present on Pluto's surface, leaving behind a dark and red carbon-rich residue.

When Hubble pictures taken in 1994 are compared with a new set of images taken in 2002 to 2003, astronomers see evidence that the northern polar region has gotten brighter, while the southern hemisphere has gotten darker. These changes hint at very complex processes affecting the visible surface, and the new data will be used in continued research.
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Solar Dynamics Observatory Set to Launch on Feb. 10

Solar Dynamics ObservatoryThe Solar Dynamics Observatory, or SDO, is set to launch on Feb. 10 at 10:26 a.m. EST from Launch Complex 41 at Cape Canaveral Air Force Station in Florida. Weather for launch day stands at a 60 percent chance of "go" for liftoff.

A prelaunch news conference will be held at 1 p.m. on Tuesday, followed by the mission science briefing. Both will be carried live on NASA TV. Live coverage of the launch will begin at 7:30 a.m. Wednesday on NASA TV and the launch blog.

SDO's unprecedented mission will study the sun and its dynamic behavior. Onboard telescopes will scrutinize sunspots and solar flares using more pixels and colors than any other observatory in the history of solar physics. And SDO will reveal the sun’s hidden secrets in a prodigious rush of pictures.

The Solar Dynamics Observatory (SDO) will be taking a closer look at the Sun, the source of all Space Weather. Space Weather affects not only our lives here on Earth, but the Earth itself, and everything outside its atmosphere (astronauts and satellites out in space and even the other planets).

The Sun, our closest star, is still a great mystery to scientists. SDO will help us understand where the Sun's energy comes from, how the inside of the Sun works, and how energy is stored and released in the Sun's atmosphere... yes, the Sun has an atmosphere! By better understanding the Sun and how it works, we will be able to better predict and better forecast the "weather out in space" providing earlier warnings to protect our astronauts and satellites floating around out there.

SDO is the first satellite under the Living with a Star (LWS) program at NASA. The spacecraft is being designed to fly for five years. However, since satellites go through a lot of testing and retesting, they often keep working long past their initial mission life. SOHO for example, which was built to fly for five years, in 2005 celebrated its 10 year anniversary in 2005!

SDO is unlike any other satellite. It will be collecting huge amounts of data everyday. In fact SDO will produce enough data to fill a single CD every 36 seconds.Patio misting systems | Misting cooling system | Mist cooling | Outdoor cooling systems | Patio cooling systems | Misting fan

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