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  • Polygonal, patterned ground is quite common in some regions of Mars, especially in scalloped topography or scalloped terrain.<ref>Malin ...Van Gaselt, M. Olvmo. 2011. Landscape evolution in Martian mid-latitude regions: insights from analogous periglacial landforms in Svalbard. In: Balme, M.
    36 KB (5,458 words) - 10:17, 23 December 2023
  • ...lfates, and recent evaporites. Most of those minerals are present close to regions of geological interest on Mars, and are dug on Earth for construction and o Six geologic EVAs have been performed by the crew, visiting the following regions: URC North Site, area East of Greenstone Road, and The Moons (Morrison Form
    33 KB (5,314 words) - 12:08, 24 March 2019
  • ...e 2 of MarsVR. Working with Dr. Rupert, we identified several interesting regions surrounding the MDRS such as Candor Chasma, the Summerville, Lith Canyon, a
    11 KB (1,766 words) - 17:41, 7 March 2019
  • ...Below Phoenix.jpg|thumb|200px|right|View under Phoenix spacecraft Bright regions are probably top of an ice sheet.]] ...Reconnaissance Orbiter (MRO). Much evidence of underground ice in vast regions of Mars has already been found by past studies, but this study found that t
    42 KB (6,301 words) - 14:48, 27 March 2024
  • ...e Below Phoenix.jpg|thumb|200px|left|View under Phoenix spacecraft Bright regions are probably top of an ice sheet.]] Polygonal, patterned ground is quite common in some regions of Mars.<ref>http://www.diss.fu-berlin.de/diss/servlets/MCRFileNodeServlet/
    36 KB (5,518 words) - 14:50, 27 March 2024
  • Memnonia includes parts of the following classical regions of Mars: Arcadia Planitia, Amazonis Planitia, Lucus Planum, Terra Sirenum, '''Yardangs''' are common in some regions on Mars, especially in what's called the "Medusae Fossae Formation."<ref>ht
    26 KB (3,975 words) - 15:23, 23 December 2023
  • Large, but not global, weak magnetic fields exist in various regions of Mars. This unexpected finding was made by Mars Global Surveyor just days
    11 KB (1,851 words) - 08:12, 27 May 2022
  • ...Here we are going by a system where the surface of Mars is divided into 30 regions, called quadrangles. Nearly all of the quadrangles use the classical names
    13 KB (2,036 words) - 15:17, 23 December 2023
  • The Coprates quadrangle contains parts of many of the old classical regions of Mars: Sinai Planum, Solis Planum, Thaumasia Planum, Lunae Planum, Noachi ...water.<ref>McEwen, A., et al. 2014. Recurring slope lineae in equatorial regions of Mars. Nature Geoscience 7, 53-58. doi:10.1038/ngeo2014</ref><ref>McEwe
    26 KB (4,014 words) - 08:58, 1 January 2024
  • ...west longitude (45-0 E). The Sinus Sabaeus quadrangle contains parts of regions that have classical names: Noachis Terra and Terra Sabaea.
    14 KB (2,201 words) - 16:09, 16 November 2023
  • ...tude (300-240 E). It encompasses many different regions or parts of many regions that have classical names. The northern part includes Thaumasia plateau. T
    26 KB (3,907 words) - 18:00, 23 December 2023
  • ...his region and is described below. The Ismenius Lacus quadrangle contains regions called Deuteronilus Mensae and Protonilus Mensae, two places that are of sp ...dwind.arc.nasa.gov/.</ref> The Ismenius Lacus quadrangle contains parts of regions named Acidalia Planitia, Arabia Terra, Vastitas Borealis, and Terra Sabaea.
    70 KB (10,556 words) - 06:01, 28 March 2024
  • ...Van Gaselt, M. Olvmo. 2011. Landscape evolution in Martian mid-latitude regions: insights from analogous periglacial landforms in Svalbard. In: Balme, M. ...tilt cause significant changes in the distribution of water ice from Polar Regions down to latitudes equivalent to Texas. During certain climate period’s,
    59 KB (8,788 words) - 06:48, 4 May 2024
  • ...th evidence of lakes, deltas, ancient rivers, inverted channels, and chaos regions that released water.<ref>Grotzinger, J. and R. Milliken (eds.) 2012. Sedi ...pxr|Jones Crater, as seen by CTX camera (on Mars Reconnaissance Orbiter). Regions on the floor containing layers, fans, and dunes are labeled.]]
    38 KB (5,857 words) - 15:46, 24 December 2023
  • ...ory reconnaissance of the Reservoir Dam, Tank Wash, and Factory Butte View regions. The EVA was conducted using a combination of ATV and dismounted scouting.
    15 KB (2,289 words) - 19:22, 7 March 2019
  • ...). "Mariner 9 Evidence for Wind Erosion in the Equatorial and Mid-Latitude Regions of Mars". Journal of Geophysical Research. 78 (20): 4123–4137(JGRHomepage ...xias Chaos in the Cebrenia quadrangle is different from most other chaotic regions. It does not have outflow channels, and it does not show a great elevation
    37 KB (5,472 words) - 16:15, 3 November 2020
  • ...akes. There is also much evidence for an ocean. Drainage systems in some regions point to precipitation as a cause. Clearly, these must have formed when Ma
    14 KB (2,150 words) - 15:24, 15 May 2019
  • Geologic EVAs were performed to the following regions:
    13 KB (2,194 words) - 12:37, 30 September 2022
  • ...and satellite telecom engineer. Supporting activities of research in polar regions with technology and experiences.
    13 KB (2,098 words) - 10:03, 24 March 2019
  • ...ions of years to lose their heat, so there is every reason to suspect that regions of Mars could have useful amounts of geothermal heat within drilling distan
    17 KB (2,767 words) - 06:46, 7 November 2023
  • Many regions with classical names are located here. Most of the region called Acidalia Polygonal, patterned ground is quite common in some regions of Mars.<ref>http://www.diss.fu-berlin.de/diss/servlets/MCRFileNodeServlet/
    31 KB (4,688 words) - 03:55, 24 January 2024
  • ...SE observations of gas sublimation-driven activity in Mars' southern polar regions: II. Surficial deposits and their origins". Icarus. 205 (1): 296–310.</re
    17 KB (2,665 words) - 07:46, 30 March 2024
  • ...EVA 9 will take the crew to a site first explored by Crew 187 in the south regions of our exploration zone. Crew members will work on various projects at the ...critical waypoints, calibrate GPS equipment, familiarize the crew with the regions, and ensure safe exploration of all future EVAs. Crewmembers will be workin
    35 KB (5,701 words) - 12:50, 30 September 2022
  • ...225° W (180-135 E) and 0° to 30° south on Mars, and contains parts of the regions Elysium Planitia and Terra Cimmeria. A small part of the Medusae Fossae Fo Some regions in the Aeolis quadrangle show inverted relief.<ref>Ori, G., I. Di Pietro,
    51 KB (7,713 words) - 06:14, 11 April 2024
  • This region, as with many other regions on Mars, shows evidence of water in the past. Well-formed channels are pre
    17 KB (2,550 words) - 07:07, 20 February 2024
  • ...ed that lobe and rampart shapes appeared in smaller craters than in other regions. Consequently, the team concluded that the ice was shallower in the deeper ..., R. Phillips. 2007. Hydrological modeling of outflow channels and chaos regions on Mars. Journal of Geophysical Research: Planets Volume 112, Issue E8</re
    49 KB (7,482 words) - 13:10, 27 December 2023
  • ...t EVA to the Moons region was cut short, so we revisited each of the Moons regions and collected a sample of the clay and salt at each site that we had not be ...Hanksville Repeater “communication satellite” on EVA to bridge some of the regions where direct communication between the Hab and the EVA team was otherwise n
    34 KB (5,868 words) - 12:02, 24 March 2019
  • Some regions in the Elysium quadrangle display strata or layers. Some layers break up in
    18 KB (2,848 words) - 16:04, 24 December 2023
  • ...e. [[Sublimation]] along the cracks turns the cracks into small valleys. Regions called Nilosyrtis Mensae, Protonilus Mensae and Deuteronilus Mensae display ...uate ridges and gullies in the degradation of craters in the Newton Basin regions of Mars. Icarus: 178, 465-486.</ref> <ref>cite journal
    40 KB (5,752 words) - 16:26, 1 January 2024
  • ...very old volcano). The Mare Tyrrhenum quadrangle encompasses parts of the regions Tyrrhena Terra, Hesperia Planum, and Terra Cimmeria. Mare Tyrrhenum's larg
    18 KB (2,705 words) - 15:55, 24 December 2023
  • ...SE observations of gas sublimation-driven activity in Mars' southern polar regions: I. Erosion of the surface | journal= Icarus | volume= 205 | issue= 1 |pag ...a/images/dune_defrost_6_2001/</ref><ref>SPRING DEFROSTING OF MARTIAN POLAR REGIONS: MARS GLOBAL SURVEYOR MOC AND TES MONITORING OF THE RICHARDSON CRATER DUNE
    40 KB (6,134 words) - 19:14, 23 December 2023
  • ...cturing services at low costs, it has been accepted as one of the supplier regions of the most important companies and space agencies.
    18 KB (3,025 words) - 12:14, 24 March 2019
  • ...Kissing Camel Range, to collect clay and shale samples and identify sandy regions.
    24 KB (4,065 words) - 14:56, 7 March 2019
  • ...ter in Casius quadrangle These layered features are quite common in some regions of Mars. ...like features common on dust-covered slopes, especially in the equatorial regions.<ref name=Chuang10>Chuang, F.C.; Beyer, R.A.; Bridges, N.T. (2010). Modific
    65 KB (9,935 words) - 10:41, 11 April 2024
  • ...arts of this quadrangle are Syria Planum, and Claritas Fossae. The classic regions Daedalia Planum, Sinai Planum, and Solis Planum are found in this quadrangl
    21 KB (3,311 words) - 08:44, 28 March 2024
  • ...J., R. Phillips. 2007. Hydrological modeling of outflow channels and chaos regions on Mars. Journal of Geophysical Research: Planets Volume 112, Issue E8 </re
    21 KB (3,160 words) - 10:42, 29 December 2023
  • ...0° to 315° W (45-90 E). Syrtis Major quadrangle includes some other named regions: Syrtis Major Planum, and parts of Terra Sabaea and [[Isidis Planitia]].<
    21 KB (3,097 words) - 15:11, 8 May 2023
  • ...grained material which was easily eroded to make vast fields of yardangs. Regions called the “Medusa Fossae Formation and Electris deposits contain thousan ...Mariner 9 Evidence for Wind Erosion in the Equatorial and Mid-Latitude Regions of Mars. Journal of Geophysical Research: 78, 4123–4137(JGRHomepage).
    75 KB (11,585 words) - 04:00, 24 January 2024
  • Purpose of EVA: Region Exploration and Sample Collection from Moon Regions
    25 KB (4,054 words) - 17:56, 7 March 2019
  • ...tilt cause significant changes in the distribution of water ice from Polar Regions down to latitudes equivalent to Texas. During certain climate periods, wat
    25 KB (3,838 words) - 04:53, 7 May 2024
  • ...which can then be assembled with surrounding maps to create maps of whole regions.
    24 KB (4,209 words) - 10:26, 24 March 2019
  • ...ter in Casius quadrangle These layered features are quite common in some regions of Mars. ...Mariner 9 Evidence for Wind Erosion in the Equatorial and Mid-Latitude Regions of Mars. Journal of Geophysical Research: 78, 4123–4137(JGRHomepage).
    81 KB (12,252 words) - 10:42, 11 April 2024
  • ...w, avalanche-like features common on dust-covered slopes in the equatorial regions.<ref>Chuang, F.C.; Beyer, R.A.; Bridges, N.T. (2010). Modification of Marti
    29 KB (4,450 words) - 10:40, 11 April 2024
  • Purpose of EVA: Visit the regions of Beige Moon and Yellow Moon, collect samples of salts
    29 KB (5,011 words) - 11:28, 24 March 2019
  • ...rovers and landers who may need to spend long periods of time in obscured regions.<ref name=":0" /> Notably, [[European Space Agency (ESA)|ESA]]’s Rosetta
    31 KB (4,637 words) - 13:31, 7 May 2024
  • ...re subsequently named. Today, we name the quadrangles after old classical regions that are nearby. The Arabia quadrangle contains part of the classic area of
    34 KB (5,229 words) - 09:43, 26 February 2024
  • ...with which to work. We examined the north-south axis of the canyon to find regions of deep shade which could retain water for long periods of time. Although w ...were Gram stained. Dark violet (Gram positive) and fuschia (Gram negative) regions were both observed; however, I suspect much nonspecific staining, perhaps c
    157 KB (25,890 words) - 15:59, 5 November 2019
  • ...Martian day. Cassini also noted white areas on the north and south polar regions, which were thought to be snow and ice. Following up on Cassini’s observa McEwan, A. et.al., 2013. Recurring slope lineae in equatorial regions of Mars. https://www.nature.com/articles/ngeo2014 (Accessed 3 Oct 2020)
    64 KB (10,261 words) - 16:11, 21 December 2020
  • ...tilt cause significant changes in the distribution of water ice from polar regions down to latitudes equivalent to Texas. During certain climate periods water
    38 KB (5,720 words) - 15:45, 4 May 2024
  • ...be found anywhere, but some places make them easier to find such as desert regions and Antarctica. The contrast of the light sand or white snow and the dark McEwen, Alfred S. et. al. 2013. Recurring slope lineae in equatorial regions of Mars. https://www.nature.com/articles/ngeo2014. (Accessed 12 March 2020)
    80 KB (12,727 words) - 12:45, 26 May 2020

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