Category Astronomy/Space

Mercury’s Thin, Dense Crust

Though Mercury may look drab to the human eye, different minerals appear in a rainbow of colors in this image from NASA's MESSENGER spacecraft. Credit: NASA/Johns Hopkins University APL/Carnegie Institution of Washington

Though Mercury may look drab to the human eye, different minerals appear in a rainbow of colors in this image from NASA’s MESSENGER spacecraft. Credit: NASA/Johns Hopkins University APL/Carnegie Institution of Washington

Mercury’s crust is thinner than anyone thought, new mathematical calculations reveal. A planetary scientist has used careful mathematical calculations to determine the density of Mercury’s crust, which is thinner than anyone thought. Mercury is small, fast and close to the sun, making the rocky world challenging to visit. Only one probe has ever orbited the planet and collected enough data to tell scientists about the chemistry and landscape of Mercury’s surface. Learning about what is beneath the surface, however, requires careful estimation.

After the probe’s mission end...

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Molecular Evolution: How the Building Blocks of Life may Form in Space

Star forming region (Pillars of Creation) in the Eagle Nebula. Low-energy electrons, created in matter by space radiation (e.g., galactic cosmic rays, GCR, etc.), can induce formation of glycine (2HN-CH2-COOH) in astrophysical molecular ices; here, icy grains of interstellar dust (or ices on planetary satellites) are simulated by ammonia, methane and carbon dioxide condensed at 20 K on Pt in UHV, and irradiated by 0-70 eV LEEs. Credit: NASA, Hubble, STScI

Star forming region (Pillars of Creation) in the Eagle Nebula. Low-energy electrons, created in matter by space radiation (e.g., galactic cosmic rays, GCR, etc.), can induce formation of glycine (2HN-CH2-COOH) in astrophysical molecular ices; here, icy grains of interstellar dust (or ices on planetary satellites) are simulated by ammonia, methane and carbon dioxide condensed at 20 K on Pt in UHV, and irradiated by 0-70 eV LEEs. Credit: NASA, Hubble, STScI

New research offers evidence that humans – and the rest of life on Earth – may have been able to form with the right combination of star dust and radiation...

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Magma Ocean may be Responsible for the Moon’s early Magnetic Field

The bottom-most layer of the moon's mantle melts to form a metal-rich "basal magma ocean" that sits on top of the moon's metal core. Convection in this layer may have driven a dynamo, creating a magnetic field which would have been recorded at the surface by the cooling lunar crust, including the samples brought back by Apollo astronauts. Credit: Aaron Scheinberg

The bottom-most layer of the moon’s mantle melts to form a metal-rich “basal magma ocean” that sits on top of the moon’s metal core. Convection in this layer may have driven a dynamo, creating a magnetic field which would have been recorded at the surface by the cooling lunar crust, including the samples brought back by Apollo astronauts. Credit: Aaron Scheinberg

Around 4 billion years ago, the Moon had a magnetic field that was about as strong as Earth’s magnetic field is today. How the Moon, with a much smaller core than Earth’s, could have had such a strong magnetic field has been an unsolved problem in the history of the Moon’s evolution...

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Projectile Cannon Experiments show how Asteroids can Deliver Water

Special delivery. Experiments using a high-powered projectile cannon suggest that asteroids can deliver surprising amounts of water when they smash into planetary bodies. Credit: Schultz Lab / Brown University

Special delivery. Experiments using a high-powered projectile cannon suggest that asteroids can deliver surprising amounts of water when they smash into planetary bodies. Credit: Schultz Lab / Brown University

Experiments using a high-powered projectile cannon show how impacts by water-rich asteroids can deliver surprising amounts of water to planetary bodies. The research, by scientists from Brown University, could shed light on how water got to the early Earth and help account for some trace water detections on the Moon and elsewhere. “The origin and transportation of water and volatiles is one of the big questions in planetary science,” said Terik Daly, a postdoctoral researcher at Johns Hopkins University who led the research while completing his Ph.D. at Brown...

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