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Topic: Carbon Dioxide

NASA’s Mars Rover Curiosity’s latest data adds to puzzle of liquid water on Mars

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Mars scientists are wrestling with a problem. Ample evidence says ancient Mars was sometimes wet, with water flowing and pooling on the planet’s surface. Yet, the ancient sun was about one-third less warm and climate modelers struggle to produce scenarios that get the surface of Mars warm enough for keeping water unfrozen.

A leading theory is to have a thicker carbon-dioxide atmosphere forming a greenhouse-gas blanket, helping to warm the surface of ancient Mars. However, according to a new analysis of data from NASA’s Mars rover Curiosity, Mars had far too little carbon dioxide about 3.5 billion years ago to provide enough greenhouse-effect warming to thaw water ice.

Bedrock at this site added to a puzzle about ancient Mars by indicating that a lake was present, but that little carbon dioxide was in the air to help keep a lake unfrozen. (NASA/JPL-Caltech/MSSS)

Bedrock at this site added to a puzzle about ancient Mars by indicating that a lake was present, but that little carbon dioxide was in the air to help keep a lake unfrozen. (NASA/JPL-Caltech/MSSS)

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NASA reports Vortex Coronagraph takes it’s first Planetary System Images

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A new device on the W.M. Keck Observatory in Hawaii has delivered its first images, showing a ring of planet-forming dust around a star, and separately, a cool, star-like body, called a brown dwarf, lying near its companion star.

The device, called a vortex coronagraph, was recently installed inside NIRC2 (Near Infrared Camera 2), the workhorse infrared imaging camera at Keck. It has the potential to image planetary systems and brown dwarfs closer to their host stars than any other instrument in the world.

The vortex mask shown at left is made out of synthetic diamond. Viewed with an scanning electron microscope, right, the "vortex" microstructure of the mask is revealed. (University of Liège/Uppsala University)

The vortex mask shown at left is made out of synthetic diamond. Viewed with an scanning electron microscope, right, the “vortex” microstructure of the mask is revealed. (University of Liège/Uppsala University)

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NASA’s Geostationary Carbon Cycle Observatory to monitor Plant Health from Space

 

Written by Steve Cole
NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – NASA has selected a first-of-its-kind Earth science mission that will extend our nation’s lead in measuring key greenhouse gases and vegetation health from space to advance our understanding of Earth’s natural exchanges of carbon among the land, atmosphere and ocean.

The primary goals of the Geostationary Carbon Cycle Observatory (GeoCARB), led by Berrien Moore of the University of Oklahoma in Norman, are to monitor plant health and vegetation stress throughout the Americas, and to probe, in unprecedented detail, the natural sources, sinks and exchange processes that control carbon dioxide, carbon monoxide and methane in the atmosphere.

From an orbit 22,000 miles above the Americas, the Geostationary Carbon Cycle Observatory will monitor plant health and vegetation stress and probe the natural sources, sinks and exchange processes of key greenhouse gases. (NASA)

From an orbit 22,000 miles above the Americas, the Geostationary Carbon Cycle Observatory will monitor plant health and vegetation stress and probe the natural sources, sinks and exchange processes of key greenhouse gases. (NASA)

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NASA’s Mars Reconnaissance Orbiter observes thawing Carbon Dioxide creating Channels on Mars

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Erosion-carved troughs that grow and branch during multiple Martian years may be infant versions of larger features known as Martian “spiders,” which are radially patterned channels found only in the south polar region of Mars.

Researchers using NASA’s Mars Reconnaissance Orbiter (MRO) report the first detection of cumulative growth, from one Martian spring to another, of channels resulting from the same thawing-carbon-dioxide process believed to form the spider-like features.

This sequence of three HiRISE images from NASA's Mars Reconnaissance Orbiter shows the growth of a branching network of troughs carved by thawing carbon dioxide over the span of three Martian years. This process may also form larger radially patterned channel features known as Martian "spiders." (NASA/JPL-Caltech/Univ. of Arizona)

This sequence of three HiRISE images from NASA’s Mars Reconnaissance Orbiter shows the growth of a branching network of troughs carved by thawing carbon dioxide over the span of three Martian years. This process may also form larger radially patterned channel features known as Martian “spiders.” (NASA/JPL-Caltech/Univ. of Arizona)

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NASA’s Orbiting Carbon Observatory-2 Satellite data used to make Global Carbon Dioxide Emissions Maps

 

Written by Alan Buis
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Scientists have produced the first global maps of human emissions of carbon dioxide ever made solely from satellite observations of the greenhouse gas.

The maps, based on data from NASA’s Orbiting Carbon Observatory-2 (OCO-2) satellite and generated with a new data-processing technique, agree well with inventories of known carbon dioxide emissions.

No satellite before OCO-2 was capable of measuring carbon dioxide in fine enough detail to allow researchers to create maps of human emissions from the satellite data alone. Instead, earlier maps also incorporated estimates from economic data and modeling results.

Human carbon dioxide emissions from fossil fuel burning and other sources have been mapped from OCO-2's global dataset. Traffic and pollution, Cairo, Egypt. (World Bank/Kim Eun Yeul)

Human carbon dioxide emissions from fossil fuel burning and other sources have been mapped from OCO-2’s global dataset. Traffic and pollution, Cairo, Egypt. (World Bank/Kim Eun Yeul)

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Volunteers examine NASA’s Mars Reconnaissance Orbiter images to find areas worth further study

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Ten thousand volunteers viewing images of Martian south polar regions have helped identify targets for closer inspection, yielding new insights about seasonal slabs of frozen carbon dioxide and erosional features known as “spiders.”

From the comfort of home, the volunteers have been exploring the surface of Mars by reviewing images from the Context Camera (CTX) on NASA’s Mars Reconnaissance Orbiter and identifying certain types of seasonal terrains near Mars’ south pole.

This image shows spidery channels eroded into Martian ground. It is a Sept. 12, 2016, example from HiRISE camera high-resolution observations of more than 20 places that were chosen in 2016 on the basis of about 10,000 volunteers' examination of Context Camera lower-resolution views of larger areas. (NASA/JPL-Caltech/Univ. of Arizona)

This image shows spidery channels eroded into Martian ground. It is a Sept. 12, 2016, example from HiRISE camera high-resolution observations of more than 20 places that were chosen in 2016 on the basis of about 10,000 volunteers’ examination of Context Camera lower-resolution views of larger areas. (NASA/JPL-Caltech/Univ. of Arizona)

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NASA’s Mars Reconnaissance Orbiter data shows Gullies on Mars probably not created by Water

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – New findings using data from NASA’s Mars Reconnaissance Orbiter show that gullies on modern Mars are likely not being formed by flowing liquid water. This new evidence will allow researchers to further narrow theories about how Martian gullies form, and reveal more details about Mars’ recent geologic processes.

Scientists use the term “gully” for features on Mars that share three characteristics in their shape: an alcove at the top, a channel, and an apron of deposited material at the bottom.

Martian gullies as seen in the top image from HiRISE on NASA's Mars Reconnaissance Orbiter resemble gullies on Earth that are carved by liquid water. (NASA/JPL-Caltech/UA/JHUAPL)

Martian gullies as seen in the top image from HiRISE on NASA’s Mars Reconnaissance Orbiter resemble gullies on Earth that are carved by liquid water. (NASA/JPL-Caltech/UA/JHUAPL)

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NASA’s Mars Reconnaissance Orbiter observes Carbon Dioxide Frost Agitate the Soil on Mars

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Some dusty parts of Mars get as cold at night year-round as the planet’s poles do in winter, even regions near the equator in summer, according to new NASA findings based on Mars Reconnaissance Orbiter observations.

The surface in these regions becomes so frigid overnight that an extremely thin layer of carbon dioxide frost appears to form. The frost then vaporizes in the morning. Enough dust covers these regions that their heat-holding capacity is low and so the daily temperature swing is large. Daily volatilization of frost crystals that form among the dust grains may help keep the dust fluffy and so sustain this deep overnight chill.

This map shows the frequency of carbon dioxide frost's presence at sunrise on Mars, as a percentage of days year-round. Carbon dioxide ice more often covers the ground at night in some mid-latitude regions than in polar regions, where it is generally absent for much of summer and fall. (NASA/JPL-Caltech)

This map shows the frequency of carbon dioxide frost’s presence at sunrise on Mars, as a percentage of days year-round. Carbon dioxide ice more often covers the ground at night in some mid-latitude regions than in polar regions, where it is generally absent for much of summer and fall. (NASA/JPL-Caltech)

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NASA study shows during winter months Carbon Emissions in Arctic may go Unobserved

 

Written by Alan Buis
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A new NASA-led study has found that in at least part of the Arctic, scientists are not doing as good a job of detecting changes in carbon dioxide during the long, dark winter months as they are at monitoring changes during the short summer.

That’s a concern, because growing Arctic plants can act as a brake on global warming rates by removing carbon from the atmosphere, but increasing cold-season emissions could overwhelm the braking effect and accelerate global warming.

Even after the ground surface freezes in the fall, Alaskan soils can continue to emit carbon. (NOAA/Mandy Lindeberg)

Even after the ground surface freezes in the fall, Alaskan soils can continue to emit carbon. (NOAA/Mandy Lindeberg)

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NASA’s Mars Reconnaissance Orbiter data reveals most recent Ice Age on Mars

 

Written by Guy Webster
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – Scientists using radar data from NASA’s Mars Reconnaissance Orbiter (MRO) have found a record of the most recent Martian ice age recorded in the planet’s north polar ice cap.

The new results agree with previous models that indicate a glacial period ended about 400,000 years ago, as well as predictions about how much ice would have been accumulated at the poles since then.

The results, published in the May 27th issue of the journal Science, help refine models of the Red Planet’s past and future climate by allowing scientists to determine how ice moves between the poles and mid-latitudes, and in what volumes.

Climatic cycles of ice and dust build the Martian polar caps, season by season, year by year, and periodically whittle down their size when the climate changes. This image is a simulated 3-D perspective view, created from image data taken by the THEMIS instrument on NASA's Mars Odyssey spacecraft. (NASA/JPL/Arizona State University, R. Luk)

Climatic cycles of ice and dust build the Martian polar caps, season by season, year by year, and periodically whittle down their size when the climate changes. This image is a simulated 3-D perspective view, created from image data taken by the THEMIS instrument on NASA’s Mars Odyssey spacecraft. (NASA/JPL/Arizona State University, R. Luk)

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