Category: crater

Craters on Moon:1° From crater Theophilus (100…

Craters on Moon:

1° From crater Theophilus (100km diameter) below to crater Langrenus above.

2° From bottom to top, dark titanium rich lava in the Sea of Fertility then the diamond shaped patch is the Marsh of Sleep. Small bright crater Proclus is thought to be a recent impact crater and has thrown out bright ejecta that is much lighter than the surrounding ancient weathered rock. Above is the rather hexagonal Mare Crisium.

3° From the Sinus Iridium top left through the Mare Imbrium with the Alpine Valley in the centre. (This original image is horizontal)

4° At the middle and bottom of this image, sunlight is shining on a mountain peak in the Alexander crater which lies beyond the day/night terminator.

Image credit: John Purvis

Slopes at Hale (Mars) Mineral salts that a…

Slopes at Hale (Mars)

Mineral salts that attract water on these slopes at Hale crater. The streaks are formed by liquid water. The blue color seen upslope of the dark streaks is thought not to be related to their formation, but instead is from the presence of the mineral pyroxene.

Credit: NASA

Dunes, peaks and craters on Mars obtained by H…

Dunes, peaks and craters on Mars obtained by HiRISE (High Resolution Imaging Science Experiment), a camera on board the Mars Reconnaissance Orbiter.

Image credit: NASA/JPL/University of Arizona

Characteristics of the moons of Saturn

Saturn has 62 natural satellites. Here are some features of some of its moons, with mountains,…

Image credit:  Bartosz Wojczyński

Image credit: 

Bartosz Wojczyński

Iapetus – The strange moon of Saturn Iapetus was discovered by…

Iapetus – The strange moon of Saturn

Iapetus was discovered by Giovanni Domenico Cassini, an Italian astronomer, in October 1671.

Iapetus is the third-largest natural satellite of Saturn, eleventh-largest in the Solar System, and the largest body in the Solar System known not to be in hydrostatic equilibrium. Iapetus is best known for its dramatic “two-tone” coloration.

Scientists have long wondered why one hemisphere of Iapetus is so dark in comparison to its other hemisphere, and in comparison to other surfaces in the Saturn system. Iapetus may be sweeping up particles from the more-distant dark moon, Phoebe. If that is the darkening mechanism, it should be steadily renewing the dark surface because very few fresh bright craters are detected within the dark terrain. An alternate theory is that there might be ice volcanism distributing darker material to the surface. Volcano-like eruptions of hydrocarbons might form the dark surfaces, particularly after chemical reactions caused by solar radiation.

Discoveries by the Cassini mission in 2007 revealed several other unusual features, such as a massive equatorial ridge running three-quarters of the way around the moon.


While Cassini keep docked Iapetus, the starry sky runs on the bottom. Among all the stars, the brightest, eclipsed for 7 frames, is Bellatrix, in the Orion constellation.

Image credit: NASA/ JPL/ CICLOPS / Space Science Institute/ Kevin Gill

Animation: AliveUniverseImages

Learn more at: Wikipedia | NASA | spaceflightnow

Hyperion – moon of Saturn Credit: NASA/JPL/Space Science…

Hyperion – moon of Saturn

Credit: NASA/JPL/Space Science Institute