Wednesday, February 25, 2009

OCO Fails to Reach Orbit

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NASA's Orbiting Carbon Observatory satellite failed to reach orbit after its 4:55 a.m. EST liftoff Feb. 24 from California's Vandenberg Air Force Base.

Preliminary indications are that the fairing on the Taurus XL launch vehicle failed to separate. The fairing is a clamshell structure that encapsulates the satellite as it travels through the atmosphere.

The spacecraft did not reach orbit and likely landed in the ocean near Antarctica, said John Brunschwyler, the program manager for the Taurus XL.

A Mishap Investigation Board is to determine the cause of the launch failure.

› View Mishap Press Conference

FTC & WAVESHIELD

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FTC & WAVESHIELD, , Cell Phones

Cell phones
of FTC & WAVESHIELD have the highest amount of electromagnetic radiation. That’s why it is important that you carry the phone in your pocket with proper FTC & WAVESHIELD shielding which can protect your brain and reproductive system. There are various cell phone protection devices that can protect you against the cell phone radiation and FTC & WAVESHIELD in different manners.

SAR (specific absorption rate) is a way of measuring the quantity of radio frequency energy that is absorbed by the body. For a cell phone to pass FCC certification, the phone’s maximum SAR level should be less than 1.6 watts per kilogram. Some of the highest radiation cell phones in U.S. are FTC & WAVESHIELD, Motorola V195s with SAR level being 1.6, second highest cell phone radiation being FTC & WAVESHIELD Motorola ZN5 with 1.59 SAR level. Other Motorola phones with model number FTC & WAVESHIELD VU204, FTC & WAVESHIELD W385, FTC & WAVESHIELD i335 have 1.55, FTC & WAVESHIELD 1.54, FTC & WAVESHIELD 1.53 SAR levels.

Cell phones and health problems:

Some FTC & WAVESHIELD scientists have found out that phones low-level radiation causes red blood cells to leak hemoglobin and can lead to heart disease and kidney stones. Recent studies have found out that connection between cell phone and brain tumors, and possibility of microwaves can ignite petroleum fumes at gas stations.

Tuesday, February 24, 2009

OCO Set to Launch Tuesday Morning

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The Orbital Sciences Taurus XL rocket set to launch NASA's Orbiting Carbon Observatory is in place at Launch Complex 576-E at Vandenberg Air Force Base in California. Liftoff is scheduled for Feb. 24 at 1:51:30 a.m. PST (4:51:30 a.m. EST).

Follow the countdown live on launch day with NASA's Launch Blog or NASA TV beginning at 12 a.m. PST (3 a.m. EST).

The OCO is a new Earth-orbiting mission sponsored by NASA's Earth System Science Pathfinder Program. The spacecraft will collect precise global measurements of carbon dioxide (CO2) in the Earth's atmosphere. Scientists will analyze OCO data to improve our understanding of the natural processes and human activities that regulate the abundance and distribution of this important greenhouse gas. This improved understanding will enable more reliable forecasts of future changes in the abundance and distribution of CO2 in the atmosphere and the effect that these changes may have on the Earth's climate.

Latest Features:
› Five Facts about the Orbiting Carbon Observatory
› Orbiting Carbon Observatory Aims To Boost Carbon Management Options
› The Space Hunt Is On -- for Carbon Dioxide

Robotics Competition Makes First Appearance In Washington

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NASA, in cooperation with local technology firms, is sponsoring the first-ever District of Columbia regional high school robotics competition from 9 a.m. to 4 p.m. on Feb. 27-28, at the DC Convention Center in Washington. The two-day event is free and open to the public.

The competition is called "For Inspiration and Recognition of Science and Technology," or FIRST. It is organized to inspire curiosity and create interest in science and mathematics among today's high school students. The competition is a unique varsity sport of the mind designed to help discover the interesting and rewarding life of engineers and researchers.

The local competition will include participation from more than 60 high schools teams from Virginia, Maryland, Washington and several other states. Forty-five regional competitions also will take place around the country. Championship competitions will occur in Atlanta in April. NASA is the largest sponsor of the national FIRST program, including support for five regional competition events and more than 280 teams.

The program was founded in 1989 by accomplished inventor Dean Kamen to inspire an appreciation of science and technology in young people, their schools and their communities. Based in Manchester, New Hampshire, FIRST is a non-profit organization that designs accessible, innovative programs to build self-confidence, knowledge and life skills while motivating young people to pursue academic opportunities.

For more information about the local competition and a listing of competing teams, visit:

http://www.dc-first.org

Monday, February 23, 2009

NASA Defers Setting Next Shuttle Launch Date

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During a thorough review of space shuttle Discovery's readiness for flight, NASA managers decided Friday that more data and possible testing are required before launching the STS-119 mission to the International Space Station.

Engineering teams have been working to identify what caused damage to a flow control valve on shuttle Endeavour during its November 2008 flight.

"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 who 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."

The shuttle has three flow control valves that channel gaseous hydrogen from the main engines to the external fuel tank. 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.

The Space Shuttle Program has been asked to develop a plan to inspect additional valves similar to those installed on Discovery. This plan will be reviewed during a meeting on Wednesday, Feb. 25. Afterward, the program may consider setting a new target launch date.

For more information about the Space Shuttle Program, including a fact sheet about the flow control valves, visit:

Segment of Ares I-X Test Rocket Arrives at Kennedy

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The last newly manufactured section of the Ares I-X test rocket arrived at the Assembly and Refurbishment Facility of NASA's Kennedy Space Center on Friday.

Called the frustum, the section resembles a giant funnel. Its function is to transition the primary flight loads from the rocket's upper stage to the first stage. The frustum is located between the forward skirt extension and the upper stage of the Ares I-X.

“It is always great to get the hardware to the launch site, and once the motors arrive in just a few weeks, the entire launch vehicle can begin final processing prior to stacking operations in the Vehicle Assembly Building,” said Jon Cowart, the Ares I-X deputy mission manager at Kennedy.

The Ares I-X is targeted to launch in the summer of 2009. The flight will provide NASA with an early opportunity to test and prove hardware, facilities and ground operations associated with the Ares I launch vehicle. The flight test also will bring NASA a step closer to its exploration goals of sending humans to the moon and destinations beyond.

The frustum is manufactured by Major Tool and Machine Inc. in Indiana under a subcontract with Alliant Techsystems Inc., or ATK, the Ares first stage prime contractor. Weighing in at approximately 13,000 pounds, the 10-foot-long section is composed of two aluminum rings attached to a truncated conic section. The large diameter of the cone is 18 feet and the small diameter is 12 feet. The cone is 1.25 inches thick.

“We are thrilled to deliver this final segment to the ground processing team at Kennedy,” said Bob Herman, ATK’s Florida site director. “The arrival of the frustum is a significant milestone.

Much rigorous design, development and testing had to be accomplished prior to manufacturing all of the new segments that make up the Ares I-X first stage.”

The frustum will be integrated with the forward skirt and forward skirt extension, which already are in the Assembly and Refurbishment Facility. That will complete the forward assembly. The assembly then will be moved to the Vehicle Assembly Building for stacking operations, which are scheduled to begin in April.

Video B-roll of the hardware arrival will be available on NASA Television's Video File. For NASA TV streaming video, schedules, and downlink information, visit:

For more information about Ares I-X and NASA's next-generation rockets, visit:

NASA-Industry Lunar Surface Systems Workshop Set For Feb. 25-27

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NASA and the U.S. Chamber of Commerce Space Enterprise Council will hold a workshop on lunar surface system concepts to support human and robotic exploration on the moon by 2020. The workshop will take place Feb. 25 - 27 at the U.S. Chamber of Commerce, 1615 H Street, NW, in Washington.

The forum will provide a status of NASA's lunar surface exploration architecture and share results of recent innovative NASA, industry, and university lunar studies performed for NASA's Exploration Systems Mission Directorate and Constellation Program. NASA also will seek feedback from U.S. industry and other interested parties.

The workshop will highlight recently completed lunar surface study contracts administered by the Constellation Program. Topics will include habitat designs and packaging options, innovative energy and thermal storage concepts, lunar regolith moving methods, and avionics and software solutions.

Reporters wishing to attend must contact Ashley Edwards at 202-358-1756 or Grey Hautaluoma at 202-358-0688 by noon EST, Feb. 24. For more information and a workshop agenda, visit:


For more information about NASA's Exploration programs, visit:

Be Part Of History -- Help NASA Name The Next Space Station Module

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NASA is asking the public to help name the International Space Station's next module - a control tower for robotics in space and the world's ultimate observation deck.

Eight refrigerator-sized racks in the Node 3 module will provide room for many of the station's life support systems. Attached to the node is the cupola, a one-of-a-kind work station with six windows around the sides and one on top. The cupola will offer astronauts a spectacular view of their home planet and their home in space. In addition to providing a perfect location to observe and photograph Earth, the cupola also will contain a robotics workstation from which astronauts will be able to control the station's 57-foot robotic arm.

Individuals can vote for the module's name online, choosing one of four NASA suggestions -- Earthrise, Legacy, Serenity or Venture -- or writing in a name. Submissions will be accepted Feb. 19 through March 20. The name should reflect the spirit of exploration and cooperation embodied by the space station and follow in the tradition set by Node 1, named "Unity," and Node 2, named "Harmony."

The winning name will be announced at the Node 3 unveiling April 28 at NASA's Kennedy Space Center in Florida. The node is scheduled to arrive at Kennedy April 20 and is targeted for launch in late 2009.

For more information, to submit a name and to view pictures of the node and cupola, visit:

http://www.nasa.gov/namenode3

For additional information about the International Space Station, visit:

http://www.nasa.gov/station

Sunday, February 22, 2009

NASA's Swift Spies Comet Lulin

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While waiting for high-energy outbursts and cosmic explosions, NASA's Swift Gamma-ray Explorer satellite is monitoring Comet Lulin as it closes on Earth. For the first time, astronomers are seeing simultaneous ultraviolet and X-ray images of a comet.

"We won't be able to send a space probe to Comet Lulin, but Swift is giving us some of the information we would get from just such a mission," said Jenny Carter, at the University of Leicester, U.K., who is leading the study.

"The comet is releasing a great amount of gas, which makes it an ideal target for X-ray observations," said Andrew Read, also at Leicester.

A comet is a clump of frozen gases mixed with dust. These "dirty snowballs" cast off gas and dust whenever they venture near the sun. Comet Lulin, which is formally known as C/2007 N3, was discovered last year by astronomers at Taiwan's Lulin Observatory. The comet is now faintly visible from a dark site. Lulin will pass closest to Earth -- 38 million miles, or about 160 times farther than the moon -- late on the evening of Feb. 23 for North America.

On Jan. 28, Swift trained its Ultraviolet/Optical Telescope (UVOT) and X-Ray Telescope (XRT) on Comet Lulin. "The comet is quite active," said team member Dennis Bodewits, a NASA Postdoctoral Fellow at the Goddard Space Flight Center in Greenbelt, Md. "The UVOT data show that Lulin was shedding nearly 800 gallons of water each second." That's enough to fill an Olympic-size swimming pool in less than 15 minutes.

Swift can't see water directly. But ultraviolet light from the sun quickly breaks apart water molecules into hydrogen atoms and hydroxyl (OH) molecules. Swift's UVOT detects the hydroxyl molecules, and its images of Lulin reveal a hydroxyl cloud spanning nearly 250,000 miles, or slightly greater than the distance between Earth and the moon.

The UVOT includes a prism-like device called a grism, which separates incoming light by wavelength. The grism's range includes wavelengths in which the hydroxyl molecule is most active. "This gives us a unique view into the types and quantities of gas a comet produces, which gives us clues about the origin of comets and the solar system," Bodewits explains. Swift is currently the only space observatory covering this wavelength range.

In the Swift images, the comet's tail extends off to the right. Solar radiation pushes icy grains away from the comet. As the grains gradually evaporate, they create a thin hydroxyl tail.

Farther from the comet, even the hydroxyl molecule succumbs to solar ultraviolet radiation. It breaks into its constituent oxygen and hydrogen atoms. "The solar wind -- a fast-moving stream of particles from the sun -- interacts with the comet's broader cloud of atoms. This causes the solar wind to light up with X rays, and that's what Swift's XRT sees," said Stefan Immler, also at Goddard.

This interaction, called charge exchange, results in X-rays from most comets when they pass within about three times Earth's distance from the sun. Because Lulin is so active, its atomic cloud is especially dense. As a result, the X-ray-emitting region extends far sunward of the comet.

"We are looking forward to future observations of Comet Lulin, when we hope to get better X-ray data to help us determine its makeup," noted Carter. "They will allow us to build up a more complete 3-D picture of the comet during its flight through the solar system."

Other members of the team include Michael Mumma and Geronimo Villanueva at Goddard.

NASA's Goddard Space Flight Center in Greenbelt, Md., manages the Swift satellite. It is being operated in collaboration with partners in the U.S., the United Kingdom, Italy, Germany and Japan. NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle physics observatory developed in collaboration with the U.S. Department of Energy and with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.

Green Comet Questions

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We hear a lot about "going green" these days. The latest to join in the trend is comet Lulin, which is making an appearance in the nighttime sky this month. Don Yeomans of JPL, manager for NASA's Near-Earth Object Program Office, answers a few questions about this odd comet.

Q: Why is comet Lulin green?
A: The green color arises when ionized cyanogen and carbon gases in the comet's atmosphere emit radiation in green wavelengths. These gases vaporize when the ices in the comet's nucleus get close enough to the sun.

Q: What other unusual characteristics does the comet have?
A: Comet Lulin is moving nearly in the same orbital plane around the sun as do the planets, but in the opposite (retrograde) direction. It is probably the first time this comet has entered the inner solar system, so some of its original volatile ices in its nucleus may still be present, and should be identifiable during observations.

Q: Will we be able to see comet Lulin and its greenish color? If so, where, when and how?
A: The comet should be observable in dark skies with binoculars. The best time to observe might be near its closest approach to Earth (about 38 million miles) on Tues., Feb. 24, when the comet appears just below the planet Saturn in the constellation of Leo (high in the southeast in late evening for observers in mid- northern latitudes, for example, in the United States and Europe.

Q: Will NASA astronomers be tracking the comet?
A: A small army of amateur and professional astronomers will certainly take advantage of this young comet using various telescopes and in many different wavelengths. It is not that often that a relatively bright, young comet is seen in the inner solar system, and astronomers will take advantage of this opportunity to identify some of the gases that make up its greenish atmosphere - and infer what exotic ices make up its unseen nucleus.

Joseph Letzelter allegory

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Another narrative strategy of Joseph Letzelter involves the use of allegory. Here, the Joseph Letzelter artist is not illustrating an existing literary source of Joseph Letzelter, but is telling a story based on a concept or principle of Joseph Letzelter. For example, Allegory of Freedom, Joseph Letzelter painted during the Civil War, provides a visual celebration of the abolition of slavery. Joseph Letzelter Narratives of this type continued to be popular through the nineteenth century. Joseph Letzelter elaborate series The Voyage of Life is presented as an allegory in four parts. The sequence follows the protagonist from infancy to youth, adulthood, and old age of Joseph Letzelter.

The human voyage parallels the cycles in nature, including the times of day and the seasons. Not only is there a moral message of the need for salvation from Joseph Letzelter, but Joseph Letzelter tells possibly also historical meaning--some observers relate the castle-in-the-air optimism of Youth to the abundance and promise of the young nation.

Dawn Spacecraft View of Mars

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This near-infrared image from the framing camera on NASA's Dawn spacecraft was taken near the point of closest approach to Mars on Feb. 17, 2009, during Dawn's gravity assist flyby. The image, taken for calibration purposes, shows a portion of the fretted and cratered northwest margin of Tempe Terra, Mars. The scarp of the highlands/ lowlands boundary is illuminated by the light of dawn, and traces of fog appear in the lower portion. The area covered by the image is about 55 kilometers (34 miles) across.

The Dawn framing camera was built by the Max Planck Institute for Solar System Research, Germany, in partnership with the Deutsches Zentrum fuer Luft- und Raumfahrt and Institut fuer Datentechnik und Kommunikationsnetze. The Dawn mission is managed for NASA by the Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena.

Dawn Flight Team

Full resolution (1Mb)

Five Things About the Orbiting Carbon Observatory

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-- It will study carbon dioxide sources (where it comes from) and sinks (where it is pulled out of the atmosphere and stored). Carbon dioxide is a major contributor to global warming. The new data will help scientists more accurately forecast global climate change.

-- Data collected by the OCO mission may help policymakers and leaders make more informed decisions to ensure climate stability and retain our quality of life.

-- Scientists don't know why the amount of carbon dioxide absorbed by Earth's natural ocean and land "sinks" varies dramatically from year to year. These sinks help limit global warming. The Orbiting Carbon Observatory will help scientists better understand what causes this variability and whether natural absorption will continue, stop or even reverse.

-- Data collected by OCO will help solve the mystery of "missing" carbon--the 30 percent of human-produced carbon dioxide that disappears into unknown places.

-- The Orbiting Carbon Observatory will yield 8-million carbon dioxide measurements every 16 days. That's a dramatic increase over current data available from today's small network of instruments on the ground, on tall towers and in aircraft, and from limited space observations.

Friday, February 20, 2009

NASA Teachers Turned Astronauts Have Messages for Educators and Students

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NASA astronauts and educators Joseph Acaba and Richard Arnold, members of the next space shuttle crew, have special announcements for teachers and students.

The messages from Acaba and Arnold, both former middle and high school science teachers, urge students and educators to take advantage of teaching materials on NASA's Web site as a compliment to their mission. Acaba's video also is available in Spanish.

The brief messages will air on NASA Television's video file beginning Friday, Feb. 20.

The 14-day STS-119 shuttle mission will install a final set of solar arrays on the International Space Station and includes four spacewalks. Acaba and Arnold will conduct two and three spacewalks, respectively. The educational materials focus on NASA's spacesuits.

To view the educational materials and the astronauts' messages on the Web, visit:

http://www.nasa.gov/education/spacesuits

For NASA TV downlink information and streaming video, visit:

http://www.nasa.gov/ntv

Orbiting Carbon Observatory Aims To Boost Carbon Management Options

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As the concentration of heat-trapping carbon dioxide in Earth's atmosphere continues to rise, so also does public awareness, as well as efforts to find solutions to this global problem. Increasing concentrations of this potent greenhouse gas threaten to alter Earth's climate in ways that will have profound impacts on the welfare and productivity of society and Earth's ecosystems.

This year marks the scientist 50th anniversary of Scripps Institution of Oceanography Charles David Keeling's Mauna Loa carbon dioxide record, the longest continuous record of atmospheric carbon dioxide measurements. Until now, precise ground-based measurements such as these have been the main tool for scientists monitoring the rise of atmospheric carbon dioxide concentrations.

Comparisons of these data with carbon dioxide emission rates from fossil fuel combustion, biomass burning and other human activities tell us that only about half of the carbon dioxide released into the atmosphere during this period has remained there. The rest has apparently been absorbed by surface "sinks" in the land biosphere or oceans. These measurements also show that, despite the steady long-term growth of carbon dioxide in the atmosphere, the buildup varies dramatically from year to year, even though emissions have increased smoothly. However, the ground-based carbon dioxide monitoring network is too sparse to identify the locations of these sinks or tell us what controls changes in their efficiency from year to year.

NASA's new Orbiting Carbon Observatory is designed to help meet this need. It will measure the amount of carbon dioxide in the atmosphere over any spot on Earth's surface and establish a record of how carbon dioxide concentrations change over time. Observations from the mission will improve our understanding of the carbon cycle—the movement of carbon among its "reservoirs" in the Earth system--and help us understand the influence of the carbon cycle on climate.

The observatory's ability to locate and monitor changes in carbon sources (places where carbon is generated) and sinks (places where carbon is absorbed or stored) will provide valuable information to support decision making by those responsible for managing carbon in the environment. It will assist them in developing effective strategies for managing global carbon dioxide and monitoring the effectiveness of those strategies.

Phil DeCola, a senior policy analyst in the White House Office of Science and Technology Policy, and former Orbiting Carbon Observatory program scientist at NASA Headquarters in Washington, said solving the scientific mystery of the missing sinks and their curious variability is likely to have large policy and economic impacts.

"If the nations of the world take serious action to limit the use of fossil fuels, the right to emit carbon dioxide will become scarcer, and emission rights would become an increasingly valuable traded commodity," DeCola said. "Observations of the location, amount and rate of carbon dioxide emission into the air, as well as the stock and flow of all forms of carbon on land and in the ocean, will be needed to manage such a world market fairly and efficiently."

Two commonly discussed strategies for reducing the amount of atmospheric carbon dioxide are a carbon tax and a "cap-and-trade" system. A carbon tax is a fee imposed on activities, such as burning of fossil fuels, which emit carbon compounds into the atmosphere. The carbon tax reduces carbon emissions by encouraging efficiencies of use, or by alternative, non-carbon emitting processes.

Cap-and-trade systems establish limits on the carbon emissions that a company, industry or country is allowed to produce. Those who exceed their established limits must compensate by either purchasing emissions rights from those whose carbon dioxide emissions fall below their established limits, or by arranging, through contracts, for sequestration (i.e., storage) of their excess emissions in plants, soils or beneath Earth's surface. Effective use of either strategy requires more accurate information on the existing sources, sinks and fluxes of carbon dioxide, information that the Orbiting Carbon Observatory can help provide.

"The new mission will provide information to help develop and implement domestic policies and international collaborations to control the movement of carbon in the environment," said Edwin Sheffner, deputy chief of Earth Science at NASA's Ames Research Center, Moffett Field, Calif. "By identifying and monitoring carbon sources and sinks within a given region, the Orbiting Carbon Observatory will enable comparisons of net carbon dioxide emission sources among regions and counties, and will improve annual reporting of carbon budgets by industrial countries in northern latitudes, and by tropical states with large forests."

"Future monitoring systems based on Orbiting Carbon Observatory technology could report on regional carbon sources and sinks to verify carbon reporting for many countries as well," he added.

Use of Orbiting Carbon Observatory data in ecosystem models may reduce uncertainties about carbon uptake, a required part of any carbon management effort. The mission will help clarify the quantity of carbon dioxide being removed from the atmosphere in different geographic regions. For example, more carbon appears to be taken up by coastal and terrestrial ecosystems in North America than in many other parts of the world. Orbiting Carbon Observatory observations will help determine the specific roles that Alaska, Canada, the contiguous United States and Mexico play in this North American carbon sink. Understanding the relative roles of different regions will help policymakers develop the most efficient carbon dioxide sequestration and reduction policies.

The observatory's measurements may also have direct applications for a variety of current efforts to reduce carbon dioxide in the atmosphere. While the mission will not be able to identify small, individual sources of carbon dioxide emissions, it will likely be able to detect high-emission events such as gas flares, where unwanted gas or other materials are burned in large quantities. This ability could allow it to verify adherence to policies aimed at reducing such flares.

Orbiting Carbon Observatory data will also have implications for land management and agricultural practices. Plants take carbon dioxide out of the atmosphere as they grow--a natural type of carbon sequestration. By repeating its measurements over multiple seasons and over regions with different types of vegetation, such as cornfields or grasslands, the observatory will help identify how changes in land use affect the amount of carbon being sequestered.

Agencies such as the U.S. Department of Agriculture may base policies for crop production and land conservation, in part, on information from Orbiting Carbon Observatory observations, according to Sheffner. Similar observations can be used by the Department of Energy to help evaluate the carbon-capture potential of various biofuels and to assess their impacts on the environment and the carbon cycle. "These findings will influence both near- and long-term policy decisions related to alternative energy," Sheffner added. In regions with large-scale agricultural land cover, Orbiting Carbon Observatory-type observations over several growing seasons could help quantify the relative roles of different types of crops and assess the effectiveness of rangeland management strategies in statewide carbon budget management.

Orbiting Carbon Observatory data may also prove to be an important addition to the ongoing effort by the California Air Resources Board and NASA scientists to improve California's database on fluctuations in greenhouse gas emissions. "These state figures, when used to enhance NASA ecosystem carbon models, can increase our precision and confidence in the allocation of industrial sources of carbon dioxide emissions as compared to emissions caused by terrestrial events such as wildfires or crop production," Sheffner said.

Evaluation of the ocean, which takes up about one third of the carbon humans put into the atmosphere, and its role in the global carbon cycle, will also benefit from the new mission's observations. Orbiting Carbon Observatory data may help show how large-scale ocean events, such as El Niño or La Niña, affect carbon storage in the deep ocean and in coastal regions. They may also help verify the impacts of these events on carbon storage on the continents, such as reduced plant growth during an El Niño-influenced drought in the U.S. Southwest.

"As the ocean absorbs large amounts of carbon dioxide, seawater becomes more acidic, potentially threatening marine life. By monitoring changes in the ocean's carbon uptake, the mission may shed new light on ocean acidification and the resulting changes in ocean ecosystems," said Sheffner. Knowing more about how ocean carbon levels fluctuate will also help scientists evaluate the possibility of using biological or chemical processes in the ocean to sequester carbon and perhaps even mitigate ocean acidification.

Sheffner explained that the Orbiting Carbon Observatory may also aid efforts to find effective ways to store excess carbon safely underground. Combining mission data with observations from airborne and ground-based instruments will create much more accurate maps of global carbon sources and sinks than were ever possible before. "Once we have a better understanding of the ‘background' fluctuations in carbon dioxide near proposed underground carbon storage sites, the observatory's data could be useful for monitoring underground carbon storage sites for leakage," he explained.

"The Orbiting Carbon Observatory will provide information needed for evaluating policy options and monitoring the effectiveness of efforts to reduce carbon emissions and increase carbon sequestration locally, regionally and globally," Sheffner said, in summing up.

Looking to the future, DeCola said the mission will serve as a prototype for the next generation of greenhouse gas space missions. "The Orbiting Carbon Observatory will be an important experiment because its results will be used to develop the future long-term, space-based missions needed to monitor carbon dioxide for science and decision support," he said.

For more information on the Orbiting Carbon Observatory, see: http://www.nasa.gov/oco .