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Logs
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  • 01:35, 19 April 2020 Sdubois talk contribs created page File:RTGs PreviousMissions.jpg
  • 01:35, 19 April 2020 Sdubois talk contribs uploaded File:RTGs PreviousMissions.jpg
  • 01:13, 19 April 2020 Sdubois talk contribs created page File:RTGs Thermocouple.png
  • 01:13, 19 April 2020 Sdubois talk contribs uploaded File:RTGs Thermocouple.png
  • 01:04, 19 April 2020 Sdubois talk contribs created page File:RTGs OpEnv.png
  • 01:04, 19 April 2020 Sdubois talk contribs uploaded File:RTGs OpEnv.png
  • 01:00, 19 April 2020 Sdubois talk contribs created page Radioisotope Thermoelectric Generators: Advantages and Disadvantages (Created page with "{{Stefan}}")
  • 08:07, 18 April 2020 Suitupandshowup talk contribs created page File:ESP 012531 1435pits.jpg (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)
  • 08:07, 18 April 2020 Suitupandshowup talk contribs uploaded File:ESP 012531 1435pits.jpg (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)
  • 07:51, 18 April 2020 Suitupandshowup talk contribs created page File:ESP 030244 2040secondarycraters.jpg (Secondary craters, as seen by HiRISE Source: https://www.uahirise.org/ESP_030244_2040 Image credit: NASA/JPL/University of Arizona)
  • 07:51, 18 April 2020 Suitupandshowup talk contribs uploaded File:ESP 030244 2040secondarycraters.jpg (Secondary craters, as seen by HiRISE Source: https://www.uahirise.org/ESP_030244_2040 Image credit: NASA/JPL/University of Arizona)
  • 05:52, 18 April 2020 Suitupandshowup talk contribs created page File:PSP 008244 2645northicecaplabeled.jpg (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)
  • 05:52, 18 April 2020 Suitupandshowup talk contribs uploaded File:PSP 008244 2645northicecaplabeled.jpg (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)
  • 11:53, 17 April 2020 Suitupandshowup talk contribs created page Geological processes that have shaped Mars: Why Mars looks like it does (added pictures, info, and ref)
  • 08:41, 17 April 2020 Suitupandshowup talk contribs created page File:Marscyclone hst.jpg (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)
  • 08:41, 17 April 2020 Suitupandshowup talk contribs uploaded File:Marscyclone hst.jpg (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)
  • 08:29, 17 April 2020 Suitupandshowup talk contribs created page File:PSP 009501 1755lavatube.jpg (Lava tubes and lava flows, as seen by HiRISE https://www.uahirise.org/PSP_009501_1755 Image credit: NASA/JPL/University of Arizona/Secosky)
  • 08:29, 17 April 2020 Suitupandshowup talk contribs uploaded File:PSP 009501 1755lavatube.jpg (Lava tubes and lava flows, as seen by HiRISE https://www.uahirise.org/PSP_009501_1755 Image credit: NASA/JPL/University of Arizona/Secosky)
  • 08:04, 17 April 2020 Suitupandshowup talk contribs created page File:ESP 042625 1655tars.jpg (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...)
  • 08:04, 17 April 2020 Suitupandshowup talk contribs uploaded File:ESP 042625 1655tars.jpg (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...)
  • 07:56, 17 April 2020 Suitupandshowup talk contribs created page File:ESP 039563 1730tars.jpg (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)
  • 07:56, 17 April 2020 Suitupandshowup talk contribs uploaded File:ESP 039563 1730tars.jpg (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)
  • 07:43, 17 April 2020 Suitupandshowup talk contribs created page File:ESP 011605 1170defrosting.jpg (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)
  • 07:43, 17 April 2020 Suitupandshowup talk contribs uploaded File:ESP 011605 1170defrosting.jpg (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)
  • 05:57, 17 April 2020 Suitupandshowup talk contribs created page File:ESP 011425 1775newcrater.jpg (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)
  • 05:57, 17 April 2020 Suitupandshowup talk contribs uploaded File:ESP 011425 1775newcrater.jpg (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)
  • 11:56, 16 April 2020 Suitupandshowup talk contribs created page File:ESP 55095 2170dunes.jpg (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.)
  • 11:56, 16 April 2020 Suitupandshowup talk contribs uploaded File:ESP 55095 2170dunes.jpg (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.)
  • 09:48, 16 April 2020 Suitupandshowup talk contribs created page File:ESP 035801 2210dipping.jpg (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)
  • 09:48, 16 April 2020 Suitupandshowup talk contribs uploaded File:ESP 035801 2210dipping.jpg (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)
  • 10:09, 15 April 2020 Suitupandshowup talk contribs created page File:ESP 036619 2275ldalabeled.jpg (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)
  • 10:09, 15 April 2020 Suitupandshowup talk contribs uploaded File:ESP 036619 2275ldalabeled.jpg (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)
  • 10:06, 15 April 2020 Suitupandshowup talk contribs created page File:ESP 035327 2255tongues.jpg (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)
  • 10:06, 15 April 2020 Suitupandshowup talk contribs uploaded File:ESP 035327 2255tongues.jpg (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)
  • 06:09, 15 April 2020 Suitupandshowup talk contribs created page File:ESP 046046 2095craterejectarim.jpg (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)
  • 06:09, 15 April 2020 Suitupandshowup talk contribs uploaded File:ESP 046046 2095craterejectarim.jpg (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)
  • 15:00, 12 April 2020 Suitupandshowup talk contribs created page File:Evaporatingicephoenix.jpg (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...)
  • 15:00, 12 April 2020 Suitupandshowup talk contribs uploaded File:Evaporatingicephoenix.jpg (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...)
  • 13:28, 12 April 2020 Sdubois talk contribs created page File:Marscopter Attached.jpg
  • 13:28, 12 April 2020 Sdubois talk contribs uploaded File:Marscopter Attached.jpg
  • 07:50, 7 April 2020 Suitupandshowup talk contribs created page File:26086 1800fault.jpg (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.)
  • 07:50, 7 April 2020 Suitupandshowup talk contribs uploaded File:26086 1800fault.jpg (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.)
  • 09:57, 23 March 2020 Frank C talk contribs created page File:MarsPapers Tutorial.compr.pdf
  • 09:57, 23 March 2020 Frank C talk contribs uploaded File:MarsPapers Tutorial.compr.pdf
  • 06:58, 21 March 2020 Suitupandshowup talk contribs created page File:FacectxF23 044929 2199 XI 39N010Wlabeled.jpg (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...)
  • 06:58, 21 March 2020 Suitupandshowup talk contribs uploaded File:FacectxF23 044929 2199 XI 39N010Wlabeled.jpg (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...)
  • 06:57, 21 March 2020 Suitupandshowup talk contribs uploaded a new version of File:FacectxF23 044929 2199 XI 39N010W.jpg (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...)
  • 06:53, 21 March 2020 Suitupandshowup talk contribs created page File:FacectxF23 044929 2199 XI 39N010W.jpg (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...)
  • 06:53, 21 March 2020 Suitupandshowup talk contribs uploaded File:FacectxF23 044929 2199 XI 39N010W.jpg (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...)
  • 17:08, 19 March 2020 Suitupandshowup talk contribs created page File:Faceg22 026771 2213pedestal.jpg (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)
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