Category Astronomy/Space

The gravitational lensed system BG1429+1202. This picture shows how strong gravitational lensing by a massive galaxy (red color) acts on the light of a very distant galaxy (with bluish color), producing in this case four separate images and increasing the total flux. Without this effect, the detailed study of distant galaxies like BG1429+1202 requires the next generation of extremely large telescopes, like TMT and E-ELT. Credit: Gabriel Pérez (IAC), GTC, Isaac Newton Group, andthe DECaLS project.

An international team has discovered one of the brightest “non-active” galaxies in the early universe...

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...

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...

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...