User contributions
- 16:22, 28 February 2018 diff hist +260 N File:46622 1365ctxcontextccf.jpg Context view of hirise image 46622_1365, as seen by CTX Concentric crater fill Source: http://viewer.mars.asu.edu/planetview/inst/ctx/G15_023941_1374_XN_42S140W#P=G15_023941_1374_XN_42S140W&T=2 Image credit: NASA/MSS current
- 14:21, 28 February 2018 diff hist +193 N File:ESP 037461 2255scallopstop.jpg Scalloped ground as seen by hirise under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_037461_2255 Image credit: NASA/JPL/University of Arizona current
- 14:15, 28 February 2018 diff hist +370 N File:45290 2350icelayerscloseer.jpg Close view of depression that contains layers of ice under only 1-2 meters of covering debris, as seen by HiRISE under HiWish program Location is the Diacria quadrangle. Arrows indicate thin covering over ice layers. Source: http://hirise.lpl.arizona.... current
- 14:05, 28 February 2018 diff hist +6 m Martian features that are signs of water ice →Triangular depressions
- 14:03, 28 February 2018 diff hist +48 m File:ESP 045290 2350triangulardepression.jpg →Summary current
- 14:02, 28 February 2018 diff hist +218 N File:ESP 045290 2350triangulardepression.jpg Triangular depression that is associated with ice under a thin cover of debris. Image from HiRISE under HiWish program Image credit: http://hirise.lpl.arizona.edu/ESP_045290_2350
- 13:30, 28 February 2018 diff hist -44 m Martian features that are signs of water ice
- 13:27, 28 February 2018 diff hist +2 m Martian features that are signs of water ice
- 13:25, 28 February 2018 diff hist +1 m Martian features that are signs of water ice →Triangular depressions
- 09:51, 28 February 2018 diff hist +250 N Talk:Martian features that are signs of water ice Created page with "I have done much work on this article. I will come back later today to edit some of the mistakes, especially the pictures that did not appear.~~~~" current
- 09:50, 28 February 2018 diff hist -20 m Martian features that are signs of water ice →Upper Plains Unit
- 09:48, 28 February 2018 diff hist +1 m Martian features that are signs of water ice
- 09:48, 28 February 2018 diff hist +8 m Martian features that are signs of water ice →Upper Plains Unit
- 09:46, 28 February 2018 diff hist +9 m Martian features that are signs of water ice →Scalloped topography
- 09:45, 28 February 2018 diff hist +6 m Martian features that are signs of water ice →Glacial Features
- 09:44, 28 February 2018 diff hist +3 m Martian features that are signs of water ice →Glacial Features
- 09:43, 28 February 2018 diff hist +2 m Martian features that are signs of water ice →Pedestal Craters
- 09:42, 28 February 2018 diff hist +12 m Martian features that are signs of water ice →Pedestal Craters
- 09:41, 28 February 2018 diff hist -3 m Martian features that are signs of water ice →Latitude Dependent Mantle
- 09:41, 28 February 2018 diff hist -4 m Martian features that are signs of water ice →Appendix
- 09:40, 28 February 2018 diff hist -5 m Martian features that are signs of water ice
- 09:38, 28 February 2018 diff hist +36,252 N Martian features that are signs of water ice added long article with pictures about ice
- 09:36, 28 February 2018 diff hist +15 m Hellas Planitia
- 09:36, 28 February 2018 diff hist +133 m Hellas Planitia
- 12:46, 27 February 2018 diff hist +366 N File:Iceincraterscomparison.jpg Ice in craters, as seen by HiRISE Picture on left shows ice exposed in small crater. In the later picture on right most of the ice is gone. Picture is from ESP_011574_2235 in the Cebrenia quadrangle. Source: https://www.nasa.gov/mission_pages/MRO...
- 12:40, 27 February 2018 diff hist +360 N File:MRO CRISM prelaunch 2.jpg CRISM, the first visible-infrared spectrometer to fly on a NASA Mars mission, will look for the residue of minerals that form in the presence of water – the “fingerprints” left by evaporated hot springs, thermal vents, lakes or ponds. Source:... current
- 12:36, 27 February 2018 diff hist +560 N File:Mars Reconnaissance Orbiter spacecraft model.png Artist's rendering, from NASA, of the Mars Reconnaissance Orbiter spacecraft, in mission configuration. The spacecraft spent its prime mission in orbit around Mars, with its main objectives concerning more detailed and specialised studies of the planet... current
- 12:31, 27 February 2018 diff hist +530 N File:Phoenix landing.jpg An artist's rendition of the Phoenix Mars probe during landing. The sophisticated landing system on Phoenix allows the spacecraft to touch down within 10 kilometres (6.2 mi) of the targeted landing area. Thrusters are started when the lander is 570 met... current
- 12:26, 27 February 2018 diff hist +271 N File:Mars Odyssey spacecraft model.png Artist's view of Mars Odyssey spacecraft Mars Odyssey mapped distribution of water on Mars Source: Published source': "Spacecraft Icons" at NASA Science Direct source: Image hosted by smd-prod.s3.amazonaws.com. Image credit: NASA current
- 12:21, 27 February 2018 diff hist +210 N File:ESP 052405 2595icelayers.jpg Ice layers in northern ice cap, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_052405_2595 Image credit: NASA/JPL/University of Arizona current
- 12:10, 27 February 2018 diff hist +268 N File:Esp 037167 1445mantle.jpg Parts of surface with and without mantle, as seen by HiRISE under HiWish program Mantle may supply future colonists with water. Source: http://hirise.lpl.arizona.edu/ESP_037167_1445 Image credit: NASA/JPL/University of Arizona current
- 12:03, 27 February 2018 diff hist +322 N File:45917 2220gulliesmantle.jpg Close view of latitude dependent mantle, as seen by HiRISE under HiWish program A certain percentage of the mantle is ice; hence we may obtain water from this for future colonists. Source: http://hirise.lpl.arizona.edu/ESP_045917_2220 Image Credit:... current
- 11:59, 27 February 2018 diff hist +246 N File:46444 2225mantle.jpg Latitude dependent mantle, as seen by HiRISE under HiWish program A certain percentage of mantle is ice. Source: http://hirise.lpl.arizona.edu/ESP_046444_2225 Image Credit: NASA/JPL/University of Arizona current
- 11:51, 27 February 2018 diff hist +259 N File:Melting pingo wedge ice.jpg Pingo on Earth with melting near Tuktoyaktuk, Northwest Territories, Canada. Source: Originally uploaded to English Wikipedia by en:User:ChrisNF 16 August 2007, as w:Image:Melting pingo wedge ice.jpg. Author: Emma Pike current
- 11:46, 27 February 2018 diff hist +247 N File:ESP 046359 1250-2pingoscale.jpg Possible pingo, as seen by HiRISE under HiWish program Location is the Phaethontis quadrangle. Source: http://hirise.lpl.arizona.edu/ESP_046359_1250 Image credit: NASA/JPL/University of Arizona/Secosky
- 11:39, 27 February 2018 diff hist +232 N File:ESP 047193 1440tongues.jpg Tongue shaped glaciers in Hellas quadrangle, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_047193_1440 Image credit: NASA/JPL/University of Arizona/Secosky current
- 20:25, 26 February 2018 diff hist +241 N File:ESP 042198 2235pyramid.jpg Upper plains unit breaking up, by starting with cracks Image taken with HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_042198_2235 Image credit: NASA/JPL/University of Arizona
- 20:18, 26 February 2018 diff hist +319 N File:ESP 028339 2245headarticle.jpg Ribbed terrain in the upper plains unit, as seen by HiRISE under the HiWish program Small cracks become larger and larger because the more surface area the more sublimation. Source: http://hirise.lpl.arizona.edu/ESP_028339_2245 Image credit: NA...
- 17:15, 26 February 2018 diff hist +209 N File:ESP 019778 1385pyramid.jpg Layers in upper plains unit, as seen by HiRISE, under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_019778_1385 Image credit: NASA/JPL/University of Arizona
- 17:13, 26 February 2018 diff hist +202 N File:48011 1370upperunit.jpg Upper plains unit breaking up, as seen by HiRISE under HiWish program Source:hirise.lpl.arizona.edu/ESP_048011_1370 Image credit: NASA/JPL/University of Arizona current
- 16:58, 26 February 2018 diff hist +170 N File:ESP 047615 1275pedestal.jpg Pedestal crater in Hellas quadrangle, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_047615_1275
- 16:52, 26 February 2018 diff hist +162 N File:26055ringmoldcrater.jpg Close view of ring mold crater, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_026055_1445 current
- 16:50, 26 February 2018 diff hist +165 N File:26055cratermesaswide.jpg Wide view of ring-mold craters, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_026055_1445
- 16:46, 26 February 2018 diff hist +120 N File:Ringmolddiagramlabeled.jpg Series of diagrams showing how ring mold craters are formed. Author: Jim Secosky current
- 16:43, 26 February 2018 diff hist +63 m File:45917 2220brainsopenclosed.jpg →Summary
- 16:42, 26 February 2018 diff hist +230 N File:45917 2220brainsopenclosed.jpg Labeled picture of open and closed brain terrain, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_045917_2220 Image credit: NASA/JPL/University of Arizona
- 14:43, 26 February 2018 diff hist +223 N File:ESP 046622 1365ccfclosecolor.jpg Close, color view of concentric crater fill, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_046622_1365 Image credit: NASA/JPL/University of Arizona/ current
- 14:40, 26 February 2018 diff hist +64 m File:1024px-46622 1365contextccf.jpg →Summary current
- 14:36, 26 February 2018 diff hist +145 N File:ESP 046622 1365ccf.jpg Concentric crater fill, as seen by HiRISE under HiWish program Image credit: NASA/JPL/University of Arizona
- 14:32, 26 February 2018 diff hist -84 m File:1024px-46622 1365contextccf.jpg →Summary