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Combined display of all available logs of Marspedia. You can narrow down the view by selecting a log type, the username (case-sensitive), or the affected page (also case-sensitive).

Logs
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  • 06:18, 18 March 2022 Suitupandshowup talk contribs created page File:ZhurongChina.jpg (Zhurong, as seen by HiRISE. The Chinese Zhurong rover landed on Mars in May 2021. (It was 14 May in the United States, but 15 May China.) This HiRISE image was acquired on 11 March 2022. Its wheel tracks left on the surface are indicated with blue arrow. Source: https://www.uahirise.org/hipod/ESP_073225_2055 Image credit: NASA/JPL/University of Arizona)
  • 06:18, 18 March 2022 Suitupandshowup talk contribs uploaded File:ZhurongChina.jpg (Zhurong, as seen by HiRISE. The Chinese Zhurong rover landed on Mars in May 2021. (It was 14 May in the United States, but 15 May China.) This HiRISE image was acquired on 11 March 2022. Its wheel tracks left on the surface are indicated with blue arrow. Source: https://www.uahirise.org/hipod/ESP_073225_2055 Image credit: NASA/JPL/University of Arizona)
  • 17:02, 3 March 2022 Suitupandshowup talk contribs created page File:Curiosityblackthorn.jpg (Feature called "Blackthorn" as seen by Curiosity in Gale Crater. It was a type of concretion. Source: https://mars.nasa.gov/raw_images/1029787/?site=msl Image Credit: NASA/JPL-Caltech/MSSS)
  • 17:02, 3 March 2022 Suitupandshowup talk contribs uploaded File:Curiosityblackthorn.jpg (Feature called "Blackthorn" as seen by Curiosity in Gale Crater. It was a type of concretion. Source: https://mars.nasa.gov/raw_images/1029787/?site=msl Image Credit: NASA/JPL-Caltech/MSSS)
  • 06:42, 24 January 2022 Suitupandshowup talk contribs created page File:PSP 010277 1650fallingdunes.croppedjpg.jpg (Falling dunes, as seen by HiRISE. Source: https://www.uahirise.org/PSP_010277_1650 Image credit: NASA/JPL/University of Arizona/Secosky This image shows a transect of approximately 8-kilometers of Coprates Chasma wall stratigraphy, which includes (moving down sequence): the southern plateau, wall spurs, fans of eroded material, gullies, sand dunes, and canyon floor. Dunes located in the center left show slip faces on the downhill side and aligned with the local gradient, indicating down sl...)
  • 06:42, 24 January 2022 Suitupandshowup talk contribs uploaded File:PSP 010277 1650fallingdunes.croppedjpg.jpg (Falling dunes, as seen by HiRISE. Source: https://www.uahirise.org/PSP_010277_1650 Image credit: NASA/JPL/University of Arizona/Secosky This image shows a transect of approximately 8-kilometers of Coprates Chasma wall stratigraphy, which includes (moving down sequence): the southern plateau, wall spurs, fans of eroded material, gullies, sand dunes, and canyon floor. Dunes located in the center left show slip faces on the downhill side and aligned with the local gradient, indicating down sl...)
  • 16:56, 20 January 2022 Suitupandshowup talk contribs created page File:CuriosityjpegPIA23974.width-1440.jpg (Stitched together from 28 images, this view from NASA's Curiosity Mars rover was captured on April 9, 2020, the 2,729th Martian day, or sol, of the mission after the rover ascended a steep slope, part of a geologic feature called "Greenheugh Pediment." In the foreground is the crusty sandstone cap that stretches the length of the pediment, forming an overhanging ledge in some parts. At center is the "clay-bearing unit," a region with a unique story to tell about the history of water on Mount...)
  • 16:56, 20 January 2022 Suitupandshowup talk contribs uploaded File:CuriosityjpegPIA23974.width-1440.jpg (Stitched together from 28 images, this view from NASA's Curiosity Mars rover was captured on April 9, 2020, the 2,729th Martian day, or sol, of the mission after the rover ascended a steep slope, part of a geologic feature called "Greenheugh Pediment." In the foreground is the crusty sandstone cap that stretches the length of the pediment, forming an overhanging ledge in some parts. At center is the "clay-bearing unit," a region with a unique story to tell about the history of water on Mount...)
  • 09:04, 20 January 2022 Suitupandshowup talk contribs created page File:ESP 071502 1750longitudecrater.jpg (Crater at the zero longitude on Mars, as seen by HiRISE Source: hirise.lpl.arizona.edu/ESP_071502_1750 Image credit: NASA/JPL/University of Arizona/)
  • 09:04, 20 January 2022 Suitupandshowup talk contribs uploaded File:ESP 071502 1750longitudecrater.jpg (Crater at the zero longitude on Mars, as seen by HiRISE Source: hirise.lpl.arizona.edu/ESP_071502_1750 Image credit: NASA/JPL/University of Arizona/)
  • 07:15, 13 January 2022 Suitupandshowup talk contribs created page File:71634 1880layersfaultslabeled.jpg (Faults in layered terrain, as seen by HiRISE under HiWish program Some faults are indicated with white arrow. The location is Danielson Crater in the Oxia Palus quadrangle at 7.688 N and 353.101 E (ESP_071634_1880). Source: hirise.lpl.arizona.edu/ESP_071634_1880 Image credit: NASA/JPL/University of Arizona/Secosky)
  • 07:15, 13 January 2022 Suitupandshowup talk contribs uploaded File:71634 1880layersfaultslabeled.jpg (Faults in layered terrain, as seen by HiRISE under HiWish program Some faults are indicated with white arrow. The location is Danielson Crater in the Oxia Palus quadrangle at 7.688 N and 353.101 E (ESP_071634_1880). Source: hirise.lpl.arizona.edu/ESP_071634_1880 Image credit: NASA/JPL/University of Arizona/Secosky)
  • 09:24, 18 December 2021 Suitupandshowup talk contribs created page File:Perseveranceseith 122237583 map-nc.png (Map showing distribution of minerals in Jezero delta. Source: https://www.bbc.com/news/science-environment-59677383 Image credit: ASAA/JPL_CALTECH/MSSS)
  • 09:24, 18 December 2021 Suitupandshowup talk contribs uploaded File:Perseveranceseith 122237583 map-nc.png (Map showing distribution of minerals in Jezero delta. Source: https://www.bbc.com/news/science-environment-59677383 Image credit: ASAA/JPL_CALTECH/MSSS)
  • 09:42, 22 November 2021 Suitupandshowup talk contribs created page File:ESP 046876 1465secondarycraters.jpg (This image of a southern mid-latitude crater was intended to investigate the lineated material on the crater floor. At the higher resolution of HiRISE, the image reveals a landscape peppered by small impact craters. These craters range from about 30 meters in diameter down to the resolution limit (about 2 meter diameter in this image acquired by averaging 2 by 2 picture elements). Such dense clusters of small craters are frequently formed by secondary craters, caused by the impact of materia...)
  • 09:42, 22 November 2021 Suitupandshowup talk contribs uploaded File:ESP 046876 1465secondarycraters.jpg (This image of a southern mid-latitude crater was intended to investigate the lineated material on the crater floor. At the higher resolution of HiRISE, the image reveals a landscape peppered by small impact craters. These craters range from about 30 meters in diameter down to the resolution limit (about 2 meter diameter in this image acquired by averaging 2 by 2 picture elements). Such dense clusters of small craters are frequently formed by secondary craters, caused by the impact of materia...)
  • 11:11, 31 October 2021 Suitupandshowup talk contribs created page File:ESP 032011 1425newgullies.jpg (Changes in gullies, as seen by HiRISE This observation is evidence that something other than flowing water can make gullies. Observations like this show that gullies are forming today. Although we cannot pin down the season of this event, locations where HiRISE has been able to image more often demonstrate that this sort of event generally occurs in the winter, when liquid water is very unlikely. Despite their resemblance to water-formed ravines on Earth, carbon dioxide may play a key role...)
  • 11:11, 31 October 2021 Suitupandshowup talk contribs uploaded File:ESP 032011 1425newgullies.jpg (Changes in gullies, as seen by HiRISE This observation is evidence that something other than flowing water can make gullies. Observations like this show that gullies are forming today. Although we cannot pin down the season of this event, locations where HiRISE has been able to image more often demonstrate that this sort of event generally occurs in the winter, when liquid water is very unlikely. Despite their resemblance to water-formed ravines on Earth, carbon dioxide may play a key role...)
  • 16:21, 13 October 2021 Suitupandshowup talk contribs created page File:Claymap.jpg (Map showing locations where clays and hydrated minerals have been found on Mars. Clay needs water to form and it is good for preserving fossils and organic material. Image Credit: NASA/JPL-Caltech/JHU-APL Source:https://mars.nasa.gov/resources/3433/regions-of-mars-with-clays-and-hydrated-minerals-identified-from-orbit/)
  • 16:21, 13 October 2021 Suitupandshowup talk contribs uploaded File:Claymap.jpg (Map showing locations where clays and hydrated minerals have been found on Mars. Clay needs water to form and it is good for preserving fossils and organic material. Image Credit: NASA/JPL-Caltech/JHU-APL Source:https://mars.nasa.gov/resources/3433/regions-of-mars-with-clays-and-hydrated-minerals-identified-from-orbit/)
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