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Topic: Atmosphere

NASA finds Red Dwarf Star with several Earth Size Planets in Orbit

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A bumper crop of Earth-size planets huddled around an ultra-cool, red dwarf star could be little more than chunks of rock blasted by radiation, or cloud-covered worlds as broiling hot as Venus.

Or they could harbor exotic lifeforms, thriving under skies of ruddy twilight.

Scientists are pondering the possibilities after this week’s announcement: the discovery of seven worlds orbiting a small, cool star some 40 light-years away, all of them in the ballpark of our home planet in terms of their heft (mass) and size (diameter). Three of the planets reside in the “habitable zone” around their star, TRAPPIST-1, where calculations suggest that conditions might be right for liquid water to exist on their surfaces—though follow-up observations are needed to be sure.

This illustration shows the seven planets orbiting TRAPPIST-1, and ultra-cool dwarf star, as they might look as viewed from Earth using a fictional, incredibly powerful telescope. (NASA-JPL/Caltech)

This illustration shows the seven planets orbiting TRAPPIST-1, and ultra-cool dwarf star, as they might look as viewed from Earth using a fictional, incredibly powerful telescope. (NASA-JPL/Caltech)

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NASA’s Spitzer Space Telescope discover Star with Seven Earth Sized Planets in Orbit

 

Written by Elizabeth Landau
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Spitzer Space Telescope has revealed the first known system of seven Earth-size planets around a single star. Three of these planets are firmly located in the habitable zone, the area around the parent star where a rocky planet is most likely to have liquid water.

The discovery sets a new record for greatest number of habitable-zone planets found around a single star outside our solar system. All of these seven planets could have liquid water — key to life as we know it — under the right atmospheric conditions, but the chances are highest with the three in the habitable zone.

The TRAPPIST-1 star, an ultra-cool dwarf, has seven Earth-size planets orbiting it. This artist's concept appeared on the cover of the journal Nature in Feb. 23, 2017 announcing new results about the system. (NASA/JPL-Caltech)

The TRAPPIST-1 star, an ultra-cool dwarf, has seven Earth-size planets orbiting it. This artist’s concept appeared on the cover of the journal Nature in Feb. 23, 2017 announcing new results about the system. (NASA/JPL-Caltech)

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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 to send Stratospheric Aerosol and Gas Experiment III (SAGE III) to International Space Station

 

Written by Eric Gillard
NASA Langley Research Center

NASA - National Aeronautics and Space AdministrationHampton, VA – Brooke Thornton has devoted eight years to a project that aims to check on the atmospheric health of the Earth. Needless to say, when NASA’s Stratospheric Aerosol and Gas Experiment III on the International Space Station (SAGE III on ISS) launches, she’ll be among the many cheering and working for its success in space.

“After seeing SAGE III mature from concept, to development, to assembly and testing, and preparing for mission ops … I’m excited to see it launch so we get the science we have worked so hard for,” she said.

NASA's Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument. (NASA)

NASA’s Stratospheric Aerosol and Gas Experiment III (SAGE III) instrument. (NASA)

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NASA’s SMAP mission provides Climate, Weather and Agriculture data

 

Written by Alan Buis
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – A new study of the first year of observational data from NASA’s Soil Moisture Active Passive (SMAP) mission is providing significant surprises that will help in modeling Earth’s climate, forecasting our weather and monitoring agricultural crop growth.

The findings are presented in a paper published recently in the journal Nature Geosciences by scientists from the Massachusetts Institute of Technology (MIT), Cambridge; and NASA’s Jet Propulsion Laboratory, Pasadena, California. They used SMAP measurements to estimate soil moisture memory in the top 2 inches (5 centimeters) of Earth’s topsoils.

Artist's rendering of NASA's Soil Moisture Active Passive satellite. (NASA/JPL-Caltech)

Artist’s rendering of NASA’s Soil Moisture Active Passive satellite. (NASA/JPL-Caltech)

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NASA’s SOFIA telescope data reveals composition of dwarf planet Ceres

 

NASA’s Ames Research Center

NASA - National Aeronautics and Space AdministrationMoffett Field, CA – New observations show that Ceres, the largest body in the asteroid belt, does not appear to have the carbon-rich surface composition that space- and ground-based telescopes previously indicated.

Using data primarily from NASA’s Stratospheric Observatory for Infrared Astronomy, SOFIA, a team of astronomers has detected the presence of substantial amounts of material on the surface of Ceres that appear to be fragments of other asteroids containing mostly rocky silicates.

The column of material at and just below the surface of dwarf planet Ceres (box) – the top layer contains anhydrous (dry) pyroxene dust accumulated from space mixed in with native hydrous (wet) dust, carbonates, and water ice. (Bottom) Cross section of Ceres showing the surface layers that are the subject of this study plus a watery mantle and a rocky-metallic core. (Pierre Vernazza, LAM–CNRS/AMU)

The column of material at and just below the surface of dwarf planet Ceres (box) – the top layer contains anhydrous (dry) pyroxene dust accumulated from space mixed in with native hydrous (wet) dust, carbonates, and water ice. (Bottom) Cross section of Ceres showing the surface layers that are the subject of this study plus a watery mantle and a rocky-metallic core. (Pierre Vernazza, LAM–CNRS/AMU)

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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 advances Exploration Objectives in 2016

 

Written by Bob Jacobs / Allard Beutel
NASA Headquarters

NASA - National Aeronautics and Space AdministrationWashington, D.C. – In 2016, NASA drove advances in technology, science, aeronautics and space exploration that enhanced the world’s knowledge, innovation, and stewardship of Earth.

“This past year marked record-breaking progress in our exploration objectives,” said NASA Administrator Charles Bolden. “We advanced the capabilities we’ll need to travel farther into the solar system while increasing observations of our home and the universe, learning more about how to continuously live and work in space, and, of course, inspiring the next generation of leaders to take up our Journey to Mars and make their own discoveries.”

This illustration depicts NASA's Juno spacecraft at Jupiter, with its solar arrays and main antenna pointed toward the distant sun and Earth. (NASA/JPL-Caltech)

This illustration depicts NASA’s Juno spacecraft at Jupiter, with its solar arrays and main antenna pointed toward the distant sun and Earth. (NASA/JPL-Caltech)

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NASA’s Cassini spacecraft takes first look at Saturn’s Atmosphere

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Cassini spacecraft has sent to Earth its first views of Saturn’s atmosphere since beginning the latest phase of its mission. The new images show scenes from high above Saturn’s northern hemisphere, including the planet’s intriguing hexagon-shaped jet stream.

Cassini began its new mission phase, called its Ring-Grazing Orbits, on November 30th. Each of these weeklong orbits — 20 in all — carries the spacecraft high above Saturn’s northern hemisphere before sending it skimming past the outer edges of the planet’s main rings.

This view from NASA's Cassini spacecraft was obtained about half a day before its first close pass by the outer edges of Saturn's main rings during its penultimate mission phase. (NASA/JPL-Caltech/Space Science Institute)

This view from NASA’s Cassini spacecraft was obtained about half a day before its first close pass by the outer edges of Saturn’s main rings during its penultimate mission phase. (NASA/JPL-Caltech/Space Science Institute)

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NASA’s Cassini spacecraft completes first dive into outer edges of Saturn’s Rings

 

Written by Preston Dyches
NASA’s Jet Propulsion Laboratory

NASA - National Aeronautics and Space AdministrationPasadena, CA – NASA’s Saturn-orbiting Cassini spacecraft has made its first close dive past the outer edges of Saturn’s rings since beginning its penultimate mission phase on November 30th.

Cassini crossed through the plane of Saturn’s rings on December 4th at 5:09am PST (8:09am EST) at a distance of approximately 57,000 miles (91,000 kilometers) above Saturn’s cloud tops. This is the approximate location of a faint, dusty ring produced by the planet’s small moons Janus and Epimetheus, and just 6,800 miles (11,000 kilometers) from the center of Saturn’s F ring.

This graphic shows the closest approaches of Cassini's final two orbital phases. Ring-grazing orbits are shown in gray (at left); Grand Finale orbits are shown in blue. The orange line shows the spacecraft's Sept. 2017 final plunge into Saturn. (NASA/JPL-Caltech)

This graphic shows the closest approaches of Cassini’s final two orbital phases. Ring-grazing orbits are shown in gray (at left); Grand Finale orbits are shown in blue. The orange line shows the spacecraft’s Sept. 2017 final plunge into Saturn. (NASA/JPL-Caltech)

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