Mars Express Results |
Mars Express Results |
Feb 20 2005, 11:24 AM
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Rover Driver Group: Members Posts: 1015 Joined: 4-March 04 Member No.: 47 |
http://physicsweb.org/articles/news/9/2/10/1
QUOTE he latest results from Mars Express reveal that the surface of the red planet is much more diverse than previously thought, with evidence for the presence of hydrated sulphates, silicates and various rock-forming minerals. Space scientists working on the European Space Agency mission have just analysed the first nine months of data from the OMEGA instrument and published six papers that give the first detailed inventory of the entire Martian surface. Last year Mars Express identified frozen water at both the north and south poles of the planet.
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Jul 11 2013, 09:03 AM
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Member Group: Members Posts: 247 Joined: 17-February 07 From: ESAC, cerca Madrid, Spain. Member No.: 1743 |
MEX put out some information on 04 Julyl, with nice images of lava flows on the sides of Olympus Mons. It is sort of old news by now, but you may not have seen it.
The web site announcement is here. From the web page: Hundreds of individual lava flows are seen frozen in time on the flanks of Olympus Mons, the largest volcano in the Solar System. The images, taken on 21 January 2013 by ESA’s Mars Express, focus on the southeast segment of the giant volcano, which towers some 22 km above the surrounding plains. This is more than double the height of Mauna Kea, the tallest volcano on Earth at 10 km, when measured from its oceanic base to summit. -------------------- --
cndwrld@yahoo.com |
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