File list
This special page shows all uploaded files.
| Date | Name | Thumbnail | Size | User | Description | Versions |
|---|---|---|---|---|---|---|
| 02:51, 19 April 2020 | RTGs Cleanup.jpg (file) |  |
20 KB | Sdubois | 1 | |
| 02:47, 19 April 2020 | RTG ComparisonSummary.png (file) |  |
171 KB | Sdubois | 1 | |
| 02:45, 19 April 2020 | RTGs MMRTGAccidents.png (file) |  |
44 KB | Sdubois | 1 | |
| 02:37, 19 April 2020 | RTGs Pu238.jpg (file) |  |
13 KB | Sdubois | 1 | |
| 02:27, 19 April 2020 | RTGs SolarRTGComparison.png (file) |  |
23 KB | Sdubois | 1 | |
| 02:15, 19 April 2020 | RTGs MMRTGPullApart.png (file) |  |
51 KB | Sdubois | 1 | |
| 02:06, 19 April 2020 | RTGs MMRTG.jpg (file) |  |
96 KB | Sdubois | 1 | |
| 01:50, 19 April 2020 | RTGs FutureSolar.png (file) |  |
113 KB | Sdubois | 1 | |
| 01:46, 19 April 2020 | RTGs JunoBus.jpg (file) |  |
16 KB | Sdubois | 1 | |
| 01:35, 19 April 2020 | RTGs PreviousMissions.jpg (file) |  |
107 KB | Sdubois | 1 | |
| 01:13, 19 April 2020 | RTGs Thermocouple.png (file) |  |
18 KB | Sdubois | 1 | |
| 01:04, 19 April 2020 | RTGs OpEnv.png (file) |  |
168 KB | Sdubois | 1 | |
| 08:07, 18 April 2020 | ESP 012531 1435pits.jpg (file) |  |
304 KB | Suitupandshowup | Pits on floor of Hale crater from steam explosions, as seen by HiRISE Hot molted rock fell after impact and caused steam explosions in the ice rich ground. Source: https://www.uahirise.org/https://www.uahirise.org/ESP_012531_1435 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 07:51, 18 April 2020 | ESP 030244 2040secondarycraters.jpg (file) |  |
339 KB | Suitupandshowup | Secondary craters, as seen by HiRISE Source: https://www.uahirise.org/ESP_030244_2040 Image credit: NASA/JPL/University of Arizona | 1 |
| 05:52, 18 April 2020 | PSP 008244 2645northicecaplabeled.jpg (file) |  |
2.66 MB | Suitupandshowup | Lava tubes and lava flows, as seen by HiRISE Source: https://www.uahirise.org/PSP_008244_2645 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 08:41, 17 April 2020 | Marscyclone hst.jpg (file) |  |
31 KB | Suitupandshowup | Cyclone on Mars, as seen by HST. Source: https://apod.nasa.gov/apod/ap990520.html Credit: J. Bell (Cornell), S. Lee (Univ. Colorado), M. Wolff (SSI), et al., NASA | 1 |
| 08:29, 17 April 2020 | PSP 009501 1755lavatube.jpg (file) |  |
2.55 MB | Suitupandshowup | Lava tubes and lava flows, as seen by HiRISE https://www.uahirise.org/PSP_009501_1755 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 08:04, 17 April 2020 | ESP 042625 1655tars.jpg (file) |  |
763 KB | Suitupandshowup | Transverse aeolian ridges (TAR's) Transverse aeolian ridges—or TAR—are mysterious, wind-blown features that are intermediate in size between ripples and much larger sand dunes. Ripples form from hopping sand grains, and dunes form from sand grains being blown over longer distances. One hypothesis for TAR formation is that larger grains like pebbles are rolled on top of smaller ripples; then, finer dust settles into the cracks, “inflating” the pebbles, making the TAR larger than typical rip... | 1 |
| 07:56, 17 April 2020 | ESP 039563 1730tars.jpg (file) |  |
194 KB | Suitupandshowup | Transverse aeolian ridges (TAR's) These are sort of like small sand dunes. We do not understand these totally. Source: https://www.uahirise.org/ESP_039563_1730 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 07:43, 17 April 2020 | ESP 011605 1170defrosting.jpg (file) |  |
320 KB | Suitupandshowup | Defrosting The dark spots are where the ice has melted, allowing us to see the dark undersurface. This takes place each spring. https://www.uahirise.org/ESP_011605_1170 Image credit: NASA/JPL/University of Arizona | 1 |
| 05:57, 17 April 2020 | ESP 011425 1775newcrater.jpg (file) |  |
1.18 MB | Suitupandshowup | New crater The dark represents the dark surface that lies under the dust. It is the dark volcanic rock basalt. Image credit: NASA/JPL/University of Arizona Source: https://www.uahirise.org/ESP_011425_1775 | 1 |
| 11:56, 16 April 2020 | ESP 55095 2170dunes.jpg (file) |  |
70 KB | Suitupandshowup | Close, color view of dunes The location is near Sklodowski Crater in North Arabia Terra in the Ismenius Lacus quadrangle at 36.66 N and 0.787 E (ESP_55095_2170). Picture taken with HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_55095_2170 Image credit is NASA/JPL/University of Arizona. | 1 |
| 09:48, 16 April 2020 | ESP 035801 2210dipping.jpg (file) |  |
46 KB | Suitupandshowup | Dipping layers The location is the Ismenius Lacus quadrangle at Latitude (centered) 40.417° N and Longitude 57.678° E. Source: http://hirise.lpl.arizona.edu/ESP_035801_2210 Image courtesy NASA/JPL/University of Arizona | 1 |
| 10:09, 15 April 2020 | ESP 036619 2275ldalabeled.jpg (file) |  |
808 KB | Suitupandshowup | Lobate debris apron around a mound, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_036619_2275 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 10:06, 15 April 2020 | ESP 035327 2255tongues.jpg (file) |  |
1.56 MB | Suitupandshowup | Tongue-shaped glaciers created when flow ran into an obstacle, causing it to split into two. Source: http://hirise.lpl.arizona.edu/ESP_035327_2255 Image credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 06:09, 15 April 2020 | ESP 046046 2095craterejectarim.jpg (file) |  |
2.18 MB | Suitupandshowup | Parts of crater in Amenthes quadrangle quadrangle, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_046046_2095 Image credit: NASA/JPL/University of Arizona/Jim Secosky | 1 |
| 15:00, 12 April 2020 | Evaporatingicephoenix.jpg (file) |  |
112 KB | Suitupandshowup | These color images were acquired by NASA's Phoenix Mars Lander's Surface Stereo Imager on the 21st and 25th days of the mission, or Sols 20 and 24 (June 15 and 19, 2008). These images show sublimation of ice in the trench informally called "Dodo-Goldilocks" over the course of four days. In the lower left corner of the left image, a group of lumps is visible. In the right image, the lumps have disappeared, similar to the process of evaporation. Date June 15 and June 19, 2008 Source http://ww... | 1 |
| 13:28, 12 April 2020 | Marscopter Attached.jpg (file) |  |
589 KB | Sdubois | 1 | |
| 07:50, 7 April 2020 | 26086 1800fault.jpg (file) |  |
54 KB | Suitupandshowup | Strike-slip fault in Hydaspis Chaos. Location is 0.2 N and 334.7 E (ESP_026086_1800). Background image is CTX image P11_005516_1812. Source: http://hirise.lpl.arizona.edu/ESP_ 26086_1800 Image credit is NASA/JPL/University of Arizona. Image credit is NASA/JPL-Caltech/Malin Space Science Systems for CTX image. | 1 |
| 09:57, 23 March 2020 | MarsPapers Tutorial.compr.pdf (file) |  |
7.99 MB | Frank C | 1 | |
| 06:58, 21 March 2020 | FacectxF23 044929 2199 XI 39N010Wlabeled.jpg (file) |  |
284 KB | Suitupandshowup | Landforms near Face. Mesa, ridges, and possible cirques are present. A '''cirque''' (French, from the Latin word ''circus'') is an amphitheatre-like valley formed by glacial erosion. Alternative names for this landform are '''corrie''' (from Scottish Gaelic coire, meaning a pot or cauldron) and '''cwm''' (Welsh "valley"). A cirque may also be a similarly shaped landform arising from fluvial erosion. The concave shape of a glacial cirque is open on the downhill side, while the cupped secti... | 1 |
| 06:57, 21 March 2020 | FacectxF23 044929 2199 XI 39N010W.jpg (file) |  |
284 KB | Suitupandshowup | Landforms near Face. Mesa, ridges, and possible cirques are present. A '''cirque''' (French, from the Latin word ''circus'') is an amphitheatre-like valley formed by glacial erosion. Alternative names for this landform are '''corrie''' (from Scottish Gaelic coire, meaning a pot or cauldron) and '''cwm''' (Welsh "valley"). A cirque may also be a similarly shaped landform arising from fluvial erosion. The concave shape of a glacial cirque is open on the downhill side, while the cupped secti... | 2 |
| 17:08, 19 March 2020 | Faceg22 026771 2213pedestal.jpg (file) |  |
332 KB | Suitupandshowup | Terrain near the face on Mars. Mud volcano, mesa, and pedestal crater are visible. Possible erosion by glaciers. Source: http://viewer.mars.asu.edu/planetview/inst/ctx/G22_026771_2213 Image credit: NASA/MSSS/Secosky | 1 |
| 17:06, 19 March 2020 | FacectxT01 00807 2205glaciers.jpg (file) |  |
211 KB | Suitupandshowup | Terrain near the face on Mars. Mud volcanoe and brain terrain are visible. Possible erosion by glaciers. Source: http://viewer.mars.asu.edu/planetview/inst/ctx/D02_027892_2219 Image credit: NASA/MSSS/Secosky | 1 |
| 17:03, 19 March 2020 | FacectxD02 027892 2219pyramid.jpg (file) |  |
323 KB | Suitupandshowup | Terrain near the face on Mars. Mud volcanoes are visible. Source: http://viewer.mars.asu.edu/planetview/inst/ctx/D02_027892_2219 Image credit: NASA/MSSS/Secosky | 1 |
| 17:01, 19 March 2020 | FaceG22 026771 2213 XI 41N009W.jpg (file) |  |
246 KB | Suitupandshowup | Terrain to the west of the face on Mars. Source: http://viewer.mars.asu.edu/planetview/inst/ctx/G22_026771_2213_XI_41N009W Image credit: NASA/MSSS/Secosky | 1 |
| 06:09, 19 March 2020 | PspfaceG22 026771 2213 XI 41N009Wctx.4threeviews.jpg (file) |  |
530 KB | Suitupandshowup | Three views of famous face on Mars. One is the original from Viking. Two are from CTX on the MRO. One has half of face blackened to simulate effects of shadows. We could not see the whole face in the original. The half we could see did look like a face. Had we seen the whole face, we may not have thought it was a real face. Pictures were modified by Secosky. Source: PspfaceG22_026771_2213_XI_41N009Wctx Image Credit: NASA | 1 |
| 10:39, 17 March 2020 | 45822 1688duneirb.jpg (file) |  |
225 KB | Suitupandshowup | Dune, as seen by HiRISE under HiWish program Source: http://hirise.lpl.arizona.edu/ESP_045822_1688 Image Credit: NASA/JPL/University of Arizona/Secosky | 1 |
| 10:12, 17 March 2020 | MarsPapers workflow.pdf (file) | |
91 KB | Frank C | 1 | |
| 09:43, 17 March 2020 | MarsPapers TMS Icon white.png (file) |  |
284 KB | Frank C | 1 | |
| 09:40, 17 March 2020 | MarsPapers PermissionForm 2018.pdf (file) | |
143 KB | Frank C | 1 | |
| 09:34, 17 March 2020 | MarsPapers Authors Instructions 2018.pdf (file) | |
364 KB | Frank C | 1 | |
| 17:07, 16 March 2020 | Crew6 MethBlue.jpg (file) |  |
19 KB | Sdubois | 1 | |
| 17:07, 16 March 2020 | Crew6 TafoniPits2.jpg (file) |  |
23 KB | Sdubois | 1 | |
| 17:06, 16 March 2020 | Crew6 TafoniPits.jpg (file) |  |
22 KB | Sdubois | 1 | |
| 17:05, 16 March 2020 | Crew6 TalonatedSurface.jpg (file) |  |
24 KB | Sdubois | 1 | |
| 17:05, 16 March 2020 | Crew6 TalonatedFacies.jpg (file) |  |
22 KB | Sdubois | 1 | |
| 17:04, 16 March 2020 | Crew6 SeriousPolka.jpg (file) |  |
22 KB | Sdubois | 1 | |
| 17:03, 16 March 2020 | Crew6 Dendrites.jpg (file) |  |
21 KB | Sdubois | 1 | |
| 17:03, 16 March 2020 | Crew6 OrangePolka.jpg (file) |  |
24 KB | Sdubois | 1 |
