These pictures show the distribution of surface ice at the Moon’s south pole (left) and north pole (right) as detected by thes Moon Mineralogy Mapper instrument. The blue areas are the icy regions plotted over images of the lunar surface with the gray scale corresponding to surface temperature (darker representing colder areas and lighter shades indicating warmer zones). As expected, the ice is concentrated at the darkest and coldest locations, the shadows of craters. This data is the first direct, definitive evidence of water ice on the Moon’s surface.
Image Credits: NASA
One of most famous spiral galaxies is Messier 104, aka The Sombrero Galaxy because of its particular shape its dominant nuclear bulge is composed mainly of mature stars. It is located in the constellation Virgo about 30 million light-years away. This luminous and massive galaxy has a total mass of about 800 billion time that of our Sun. from our point of vies it’s a nearly edge-on disc composed of stars, gas, and dust. The complexity of this dust is apparent directly in front of the bright nucleus, but also shows up in the dark absorbing lanes throughout the disc.
Image Credit: ESO
This is Messier 96, a spiral galaxy a bit more than 35 million light-years away in the constellation of Leo (The Lion). It is roughly the same mass and size as the Milky Way, but unlike our more or less symmetrical galaxy, M96 is lopsided. Its dust and gas are unevenly spread throughout its weak spiral arms, and its core is not exactly at the apparent galactic center. Its arms are also asymmetrical, perhaps because of the gravitational pull of other galaxies within the same group as Messier 96.
Image Credit: ESA / NASA
Astronomers have assembled one of the most comprehensive portraits yet of the universe’s evolutionary history. It’s based on a broad spectrum of observations by the Hubble Space Telescope and other space and ground-based telescopes. In particular, Hubble’s ultraviolet vision has been used to track the birth of stars over the last 11 billion years, going all the way back to the cosmos’ busiest star-forming period about 3 billion years after the big bang. This composite image encompasses a sea of around 15,000 galaxies widely distributed in time and space. About 12,000 of them are undergoing star formation. This mosaic is 14 times the area of the Hubble Ultra Violet Ultra Deep Field released in 2014. Right click on the image to embiggen it.
Image Credits: NASA / ESA / P. Oesch (University of Geneva) / M. Montes (University of New South Wales)
This is a view of Saturn partially lit in crescent phase, a view that can only be seen when the object is between the observer and the Sun. From the Earth, we can only see Mercury and Venus in varying crescent phases and Mars and the other outer planets fully lit. Because the Moon can be either between the Earth and the Sun or farther away, we see it go through all the phases from New to Full to New again.
This picture of Saturn was made by the Cassini spacecraft.
Image Credit: NASA
Saturn’s rings are mostly water ice in chunks that range in size from smaller than a grain of sand to mountains. The ring system extends 282,000 km from the planet, but it’s only about 10 m thick in most places. Looking from some angles, it’s possible to see through the rings—as in this that looks from south to north. The Cassini spacecraft took the images stitched together in this natural-color mosaic in April, 2007, when it was about 725,000 kim from Saturn.
Image Credit: NASA