Post on 09-Jan-2016
description
2009--1
View Mars by Hubble Space TelescopeFlight into Mariner Valley
603817 1960~1975 1964~19711975-121976~199217198811992~19921996 21/
NASA
2009-2020
200920112013201620182020MSLScoutGround Breaking (GBMSR)ScoutScoutMSLScoutScoutScoutMSLScoutMSR with RoverScoutMSLScoutGround Breaking (GBMSR)Scout
ESA Aurora Aurora2033
21 1 2 3 4 5
12
40
10-6CO2N240ArO2COH2O95.32.70.60.130.070.0339ArNeKrXeO352.530.080.040.2
61035Km -33o100o17o-22o-123o- -133o
65851600
Olympus55025
5S, 297E, 2004-03-26, by G. Neukum
Mssbauer spectra show jarositeOpportunity/MRO, 2004-03-02small-scale cross bedding
Concentrations of Mg, Al, Cl and Br versus S in rocks and soils indicates water alteration L. A. Haskin et al., 2005, Nature Letters, Vol. 436
10W2E5N6STES hematite abundance, is overlain on a daytime THEMISChristensen et al., 2001, JGR
Mars Hematite
The change of CO2 and H2O ice in North Polar
MARS ICE
Martian north polar layered deposits
Fishbaugh, 2006, JGR
Colour view of crater with water ice(70.5 N,103 E, 35 Km wide, 2 km depth, 15 m/pixel)2 Feb. 2005, from G. Neukum
Nanedi VallisParana Valles
Olympica Fossae, 25.98N, 113.18W , http://www.msss.com/moc_gallery/ 2001-02-152000-03-19
Gullies in Newton Basin (MOC2-320 )39.0S, 166.1WNASA/JPL, 2002-10-07
Gullies Formation mechanismMGS_88923, 65S,15 W, NASA/JPL, 1997-12-29
Groundwater sapping Nirgal vallisJaumann, Reiss, 2002Recent (few Myr) outflow from Cerberus fossaeBurr et al., GRL, 2002
Colour nadir view of Nicholson Crater (100Km wide, 0.0 S, 195.5E, 15.3 m/pixel)
Hock, 2004
2.23, 356.75, MOC Release No. MOC2-316, 2002-06-27 Partially-Exhumed Crater in Northern Terra Meridiani
West Arabia Terra, 8N, 7W MOC Release No. MOC2-261, 2000-10-4 Terra Meridiani mesas, 16.87, 331.23MOC Release No. M20-01357, 2000-10-23
Eberswalde Delta, MGS MOC Release No. MOC2-1225, 2005-09-20In northeast of Holden Crater near 24.0S, 33.7W
Water Alteration at Gusev Crater Rocks in the Gusev Crater show evidence for interaction with waterhighly elevated levels of S, Cl, K, P, Br basaltic chemistry, but highly oxidized and lacking in primary basaltic minerals, IR spectrum fit well by basaltic glassgoethite ( FeO(OH), Hydrated Iron Oxide )fine to coarse layered sedimentsSpirit landing site
MGS
MGS TES Basalt MapBasalt (Type 1 spectra) concentrated in Southern HighlandsBandfield et al. (2000), Hamilton et al. (2001)
MGS TES Andesite MapAndesite (type 2 spectra) appears concentrated in Northern Lowlands, but also intermixed with basalt in Southern Highlands.Bandfield et al. (2000), Hamilton et al. (2001)
1997X
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Apollo(3300)10-9 T 32
3219
14%25%37%
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[McKay, 1996 #82] (PAHs)[McKay, 1996 #82] (biofilm)
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20122017
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1234C, H, O, N, P , S56
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