Category Astronomy/Space

Don’t Judge an Asteroid by its Cover: Mid-infrared Data from SOFIA Shows Ceres’ True Composition

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. Credits: 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. Credits: Pierre Vernazza, LAM–CNRS/AMU

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...

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A Colorful ‘Landing’ on Pluto

Video: A colorful ‘landing’ on Pluto

The original black-and-white Pluto “landing” movie can be viewed at: http://pluto.jhuapl.edu/News-Center/News-Article.php?page=20160714-2

What would it be like to actually land on Pluto? This movie was made from more than 100 images taken by NASA’s New Horizons spacecraft over 6 weeks of approach and close flyby in the summer of 2015. The video offers a trip down onto the surface of Pluto—starting with a distant view of Pluto and its largest moon, Charon—and leading up to an eventual ride in for a “landing” on the shoreline of Pluto’s informally named Sputnik Planitia.

To create a movie that makes viewers feel as if they’re diving into Pluto, mission scientists had to interpolate some of the panchromatic (black and white) frames based on what they know Pluto looks like to make it as sm...

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Cassini Gets Up Close and Personal With Saturn’s ‘Wavemaker’ Moon Daphnis

Cassini Gets Up Close and Personal With Saturn's 'Wavemaker' Moon Daphnis

As this almost surreal observation of Saturn’s tiny moon Daphnis shows, we’re finally getting a really good look at the small-scale processes that are at work in Saturn’s rings Credit: NASA/JPL/Space Science Institute

The wavemaker moon, Daphnis, is featured in this view, taken as NASA’s Cassini spacecraft made one of its ring-grazing passes over the outer edges of Saturn’s rings on Jan. 16, 2017. This is the closest view of the small moon obtained yet. Daphnis (5 miles) orbits within the 26-mile wide Keeler Gap. Cassini’s viewing angle causes the gap to appear narrower than it actually is, due to foreshortening.

The little moon’s gravity raises waves in the edges of the gap in both the horizontal and vertical directions...

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Violations of Energy Conservation in the Early Universe may explain Dark Energy

universe

This is the “South Pillar” region of the star-forming region called the Carina Nebula. Like cracking open a watermelon and finding its seeds, the infrared telescope “busted open” this murky cloud to reveal star embryos tucked inside finger-like pillars of thick dust. Credit: NASA

Physicists have proposed that violations of energy conservation in the early universe, as predicted by certain modified theories of quantum mechanics and quantum gravity, may explain the cosmological constant problem, which is sometimes referred to as “the worst theoretical prediction in the history of physics.” “The main achievement of the work was the unexpected relation between two apparently very distinct issues, namely the accelerated expansion of the universe and microscopic physics,” Josset said.

Einstein ...

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