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• Mars
  ...a of Earth. The Martian [[Atmosphere]] is almost unique in that the South Pole gets so cold in winter that the main atmospheric constituent will freeze ou ...res range widely from as little as 140° K (-133° C, -207° F) at the winter pole to almost 300° K (27° C, 80° F) on the dayside during summer.
  11 KB (1,851 words) - 08:12, 27 May 2022
• Crew 187 EVA Reports
  ...rew left the airlock at 10:35 and headed south in 4 ATVs, upon finding the pole 1101 trough Cow Dung road, after about half an hour of traverse, we proceed ...and camera) was lost, so a search formation was done, and the crew headed south, being able to find the device, and resuming the walk back north. The walk
  19 KB (3,259 words) - 11:19, 24 March 2019
• Interplanetary commerce
  ...Fd8OUrOYo</ref> would be able to compete against fuel mined from the south pole of Luna, reducing the cost and improving the stability of supply of fuel to
  9 KB (1,398 words) - 14:52, 2 October 2020
• Crew 202
  ...ton, where she designed robotic traverses and geological maps at the south pole far side of the Moon.
  8 KB (1,205 words) - 15:03, 7 March 2019
• Periodic climate changes on Mars
  ...xide ice tend to migrate during a Martian year from the North Pole, to the South (and back again) each year. This puts more CO2 and water vapour in the atm ...latitude bands in the mid-latitudes: 30-60 degrees North and 30-60 degrees South latitudes.
  13 KB (1,801 words) - 18:20, 29 December 2023
• Terra Sirenum
  ...b|300px|right|MOLA map showing boundaries of Terra Sirenum near the south pole and other regions]]
  10 KB (1,480 words) - 17:48, 9 November 2020
• Eridania quadrangle
  ...ess: Tucson, 1992.</ref> The Eridania quadrangle lies between 30° and 65° south latitude and 180° and 240° west longitude (180-120 E). Most of the class ...h magnetic pole of one pointing up from the surface and the north magnetic pole of the next pointing down.<ref>ISBN|978-0-521-82956-4</ref> When similar st
  28 KB (4,220 words) - 06:09, 17 April 2024
• Noachis quadrangle
  The Noachis quadrangle covers the area from 30° to 65° south latitude and 300° to 360° west longitude (60-0 E). It lies between Argy ...dust when the climate was different due to changes in the tilt of the Mars pole.<ref>doi=10.1038/nature02114 |pmid=14685228 |title=Recent ice ages on Mars
  19 KB (2,977 words) - 08:57, 20 February 2024
• Mariner 4
  ...so bright (second only to Sirius) and that it was near the south ecliptic pole.<ref>Glasstone, S. 1968. The Book of Mars. NASA. Washington D.C.</ref>
  14 KB (2,150 words) - 15:24, 15 May 2019
• Geological processes that have shaped Mars: Why Mars looks like it does
  ...at the top of the depression contains pure ice. This wall faces the south pole. <ref>Supplementary Materials Exposed subsurface ice sheets in the Martian ...190-MC-30-MareAustraleRegion-19980605.jpg |right|thumb|px| Region of South Pole with ice cap Southern ice cap is much smaller than the North’s.]]
  75 KB (11,585 words) - 04:00, 24 January 2024
• Phaethontis quadrangle
  The Phaethontis quadrangle lies between 30° and 65 ° south latitude and 120° and 180 ° west longitude (240-180 E). This latitude ra ...north wall of crater that lies west of the crater Newton (41.3047 degrees south latitude, 192.89 east longitide). Image taken with [[Mars Global Surveyor]
  41 KB (6,106 words) - 10:20, 29 December 2023
• What Mars Actually Looks Like!
  ...nd on steep slopes. A high concentration occurs near 40 degrees north and south of the equator. Usually, each gully has an ''alcove'' at its head, a fan- ...scalloped depression displays a gentle equator-facing slope and a steeper pole-facing scarp.<ref>http://www.uahirise.org/ESP_038821_1235</ref> <ref>https:
  65 KB (9,935 words) - 10:41, 11 April 2024
• Hellas quadrangle
  The Hellas quadrangle covers the area from 30° to 65° south latitude and 240° to 300° west longitude (120-60 E ). When an asteroid sl ...he same places where glaciers are observed. Water is transported from the south polar area to northern Hellas and falls as precipitation.<ref>Forget, F., e
  59 KB (8,788 words) - 06:48, 4 May 2024
• Martian features that are signs of water ice
  ...sily seen as triangular depressions with one steep wall that faces the pole.<ref>https://www.uahirise.org/ESP_074914_1225</ref> These exposed ice sh The sites are at latitudes from about 55 to 58 degrees north and south of the equator, suggesting that there is shallow ground ice under roughly a
  42 KB (6,301 words) - 14:48, 27 March 2024
• Iapygia quadrangle
  The Iapygia quadrangle covers the area from 0° to 30° south latitude and from 270° to 315° west longitude (90-45 E). Parts of the reg ...ear 30% of the carbon dioxide in the atmosphere freezes out and covers the pole that is experiencing winter, so there is a great potential for strong winds
  20 KB (3,015 words) - 06:56, 20 April 2024
• Nuclear power
  ...out as the ice cave grows <ref name=":3">Rodwell, Raul Rodriguez '' South Pole Station - Rodwells '', https://www.southpolestation.com/trivia/rodwell/rodw
  22 KB (3,579 words) - 10:30, 23 November 2022
• Diacria quadrangle
  ...ic and tectonic features related to the huge volcanoes Olympus Mons to the south and Alba Mons to the east. Much of the tectonic features on Mars are cause ...ern lowland plains of Mars and cover portions of Amazonis Planitia (in the south), Arcadia Planitia (west central), and Vastitas Borealis (in the north). Th
  36 KB (5,518 words) - 14:50, 27 March 2024
• Glaciers on Mars
  ...an, G.J. and J.W. Head, III. 2002. Candidate subglacial volcanoes in the south polar region of Mars: morphology, morphometry, and eruption conditions. J.
  40 KB (5,752 words) - 16:26, 1 January 2024
• Crew 184 - Journalist Report
  ...edical Officer Sczepaniak and me had the privilege to be in group one. The pole position also helped to clear some problems for the rest of the team. It to ...sion to evacuate for the night of Saturday to an emergency pod a few miles south of the Habitat. Equipped with the most relevant life sustaining technologie
  45 KB (8,279 words) - 14:55, 27 March 2019
• HiWish program
  ...jets formed by sublimation beneath translucent slab ice in Mars' seasonal south polar ice cap. Nature: 442(7104):793-6.</ref> <ref>https://mars.nasa.gov/re ...scalloped depression displays a gentle equator-facing slope and a steeper pole-facing scarp.<ref>https://www.uahirise.org/hipod/PSP_001938_2265</ref> <ref
  81 KB (12,252 words) - 10:42, 11 April 2024

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