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• Lichen
  ...ecover quickly when conditions are favorable. Although lichens can grow in regions with more rainfall, they actually require little rainfall to survive.<ref>h
  2 KB (289 words) - 18:31, 25 July 2020
• Glossary of Mars features
  ...of each Martian surface feature. Use examples from the [[:Category:Regions|Regions Category]].
  2 KB (266 words) - 14:58, 17 December 2018
• Origin of Mars and its Elemental Composition
  ...o 100 million years in a process that mixed planetesimals from neighboring regions of the rotating disk. ...rent distances form the proto sun and since planetesimals from neighboring regions mixed in forming these planets, the elemental compositions of Mars and Eart
  2 KB (313 words) - 18:14, 10 November 2020
• Needed explorations
  *average wind speed in a Martian year for several regions ...] feed the hope of finding underground warm spots near the surface in some regions. A specialized rover can be sent to Mars to drill holes, measure temperatur
  2 KB (332 words) - 06:56, 7 November 2023
• Albedo
  ...]]. Albedo may be increased by surface features (i.e. ice or snow in polar regions) or atmospherics (i.e. clouds), so any changes in climate strongly influenc
  1 KB (165 words) - 12:42, 24 July 2018
• Chromium
  ...with other metals, either in cooled lava chambers, asteroid impacts or in regions of hydrothermal vents.
  1 KB (183 words) - 07:55, 2 May 2024
• Xanthe Terra
  ...jpg|thumb|500px|left|MOLA map showing boundaries of Xanthe Terra and other regions]] ...aos was highly suggestive that huge floods came out of the ground in chaos regions and formed large outflow channels. Orson Welles Crater was named after Ors
  3 KB (443 words) - 12:42, 10 November 2020
• Mercury
  ...has a metal rich regolith along with what appears to be permanently shaded regions at the poles that may harbor water or possibly other volatiles<ref>https://
  2 KB (296 words) - 16:31, 17 February 2023
• Solar wind
  ...03, '''1997''']</ref> and is located above equatorial closed magnetic flux regions (i.e. the streamer belt).
  4 KB (616 words) - 16:26, 6 May 2021
• Coronal Mass Ejections
  ...y of a protective magnetic field, and does not experience aurorae in polar regions.
  5 KB (701 words) - 08:06, 27 May 2022
• Energy Infrastructure
  ...ial and industrial, and 240/120V for residential. Different countries and regions use different voltages and DC frequencies.
  2 KB (309 words) - 08:42, 26 September 2022
• Crew 200 EVA Reports
  ...radio communication between EVA crew and HabCom, in northern and southern regions 2) Test how EVAs can safely and effectively be conducted with three-member ...rove with Curiosity to the north, then to the south to explore and map the regions of communication strength/readibility. We applied a communication protocol
  7 KB (1,162 words) - 16:23, 7 March 2019
• Crew 182
  ...and identifying some possible solutions to be applied in arid and semiarid regions, verifying issues related to the operation of self-sustainable habitats. Th ...nologies Applied to Mars and Semiarid, Mars Research Group – Mars and Arid Regions Settlements Sustainability, and the Museu Espaço Marte. He is also creati
  7 KB (1,133 words) - 12:06, 7 March 2019
• Crew 182-Team Peru V
  ...and identifying some possible solutions to be applied in arid and semiarid regions, verifying issues related to the operation of self-sustainable habitats. Th ...nologies Applied to Mars and Semiarid, Mars Research Group – Mars and Arid Regions Settlements Sustainability, and the Museu Espaço Marte. He is also creati
  7 KB (1,130 words) - 12:32, 16 March 2019
• Back contamination
  == Other regions of dangerous contamination ==
  8 KB (1,351 words) - 22:04, 15 May 2022
• Extremophiles
  ...day of the year (approximately room temperature) to -153o C in the polar regions. (NASA 2013) Even on the warmest day on Mars, the temperature plummets at
  9 KB (1,306 words) - 11:23, 17 December 2018
• Natural fiber
  ...d in ropes and rigging. Hemp bridges still span canyons and rivers in some regions on Earth. It has been replaced by [[synthetic fiber]] in many applications.
  3 KB (500 words) - 11:51, 5 October 2022
• Dust storms
  ...n part of the planet, mainly from the Hellas basin and the Acidalia/Chryse regions. Large storms can last about a month, but have also lasted up to six.
  4 KB (661 words) - 12:30, 29 November 2022
• Margaritifer Terra
  ...mb|600px|left|MOLA map showing boundaries for Margaritifer Terra and other regions. Color indicates elevation.
  3 KB (470 words) - 06:47, 23 March 2020
• Galactic Cosmic Rays
  ...s can be directed by the Earth's magnetic field and to impact at the polar regions. Higher energy cosmic rays move so fast, that they have not the time to be
  4 KB (659 words) - 20:09, 20 April 2024
• Phoenix Mars Mission
  ...-extractable water for fuel production and industrial processes. The polar regions were expected to be the most likely places to find [[water|water ice]]. ...Below Phoenix.jpg|thumb|200px|right|View under Phoenix spacecraft Bright regions are probably top of an ice sheet.]]
  8 KB (1,143 words) - 15:14, 12 April 2020
• Orbital debris
  ...cause re-entry. Usually the debris is allowed to burn up over unpopulated regions of Earth (i.e. the Pacific Ocean or Australian Outback), and should any mas
  4 KB (589 words) - 00:05, 18 December 2018
• Arsia Mons
  ...hape; the grooves on the wall mark former flow levels. Pits near volcanic regions of Mars may be openings to caves like this.]]
  4 KB (597 words) - 18:50, 8 January 2020
• Luna-Mars Trade
  ...rogen]], and [[Carbon]] outside of volatiles trapped in Permanently Shaded Regions near the poles<ref>https://www.hou.usra.edu/meetings/lunarvolatiles2018/pdf
  4 KB (648 words) - 02:26, 25 July 2020
• Volcano
  ...hort history of plate tectonics, so it is likely that the Martian volcanic regions are based on various hot spots. ...the planet increases the odds that we can find geothermal power in other regions of the planet.
  9 KB (1,402 words) - 11:52, 5 January 2023
• Observing Mars with a Telescope
  ...small telescope, the planet’s surface features begin to appear.Three main regions can be seen: the polar caps, lighter areas of rust-colored dust, and darker Similarly, the darker regions, or albedo markings, were thought to be seas or large patches of vegetation
  13 KB (2,038 words) - 12:05, 18 September 2019
• Hellas Planitia
  ...left|thumb|300px|Map showing locations of Hellas Planitia and other nearby regions]]
  4 KB (676 words) - 20:14, 7 January 2020
• Water
  ...ander confirmed in 2008 that water ice is not limited to the extreme polar regions.<ref>Smith, P., et al. 2009. H_<sup>2O at the Phoenix Landing S .... <nowiki>https://sci.esa.int/web/mars-express/-/51824-4-probing-the-polar-regions</nowiki></ref> Although it has been known for many years that the poles hav
  22 KB (3,416 words) - 16:26, 20 March 2023
• Terra Sirenum
  ...g|thumb|300px|right|MOLA map showing boundaries of Terra Sirenum and other regions]] ...OLA map showing boundaries of Terra Sirenum near the south pole and other regions]]
  10 KB (1,480 words) - 17:48, 9 November 2020
• Mars Reconnaissance Orbiter
  ...places for changes over time, and acquire stereo (3D) coverage of special regions and potential future landing sites.<ref>Malin, M. C.; et al. (2007). "Conte
  11 KB (1,695 words) - 15:12, 6 September 2019
• Noachis quadrangle
  ...rra and the western part of Hellas Planitia, which are classical names for regions on Mars. The name "Noachis" means the land of Noah. Noachis is considered among the oldest regions on Mars since it is so densely covered with impact craters. The oldest par
  19 KB (2,977 words) - 08:57, 20 February 2024
• Olympus Mons
  ...down before landing. Moreover, Olympus Mons stands in one of the dustiest regions of Mars. This would likely make rock samples hard to come by and the dust l
  5 KB (853 words) - 20:54, 20 August 2021
• Atmosphere
  --- Ground fogs are found in low laying regions such as the [[Hellas Basin]], [[Noctis Labyrinthus]], and [[Valles Marineri ...ure varies little from the equator to the higher mid latitudes. The polar regions are much colder. For this reason, transient surface winds are less powerfu
  35 KB (5,867 words) - 06:50, 15 December 2022
• Gusev Crater
  ...spectra of the dust was similar to spectra of bright, low thermal inertia regions like Tharsis and Arabia that have been detected by orbiting satellites. A
  6 KB (917 words) - 19:04, 8 January 2020
• Periodic climate changes on Mars
  ...Van Gaselt, M. Olvmo. 2011. Landscape evolution in Martian mid-latitude regions: insights from analogous periglacial landforms in Svalbard. In: Balme, M. ...long periods under a few meters of dirt and rock. Many of these supposed regions of underground ice generally begin around 30 degrees of latitude on both si
  13 KB (1,801 words) - 18:20, 29 December 2023
• Interplanetary Internet
  ...able-delay environment using a generalized suite of protocols. Examples of regions might include the terrestrial Internet as a region, a region on the surface
  14 KB (2,041 words) - 11:20, 5 October 2022
• Medusae Fossae
  Its roughly-shaped regions extend from just south of [[Olympus Mons]] to Apollinaris Patera, with a sm
  6 KB (880 words) - 07:29, 8 January 2024
• Crew 200 Sol Summaries
  ...ity Summary: Crew conducted first 3-crew member EVA to explore and map the regions of communication strength. We planned contingency plans for loss of signal ...g Camel Ridge East to explore the limits of walkie talkie comms in certain regions. Comms checks were performed every minute between HabCom and EVA, and GPS c
  16 KB (2,564 words) - 16:52, 7 March 2019
• Spirit
  ...spectra of the dust was similar to spectra of bright, low thermal inertia regions like Arabia and Tharsis that have been detected by orbiting satellites. A ...ed the presence of large amounts of carbonate-rich rocks, which means that regions of the planet may have once harbored water. As the Martian atmosphere cont
  15 KB (2,283 words) - 14:41, 9 February 2019
• Magnetosphere
  ...path, until they hit the Earth's atmosphere over the north or south polar regions, forming the aurorae. However, Eskimo are not constantly dying of radiatio
  8 KB (1,217 words) - 09:01, 27 May 2022
• Layers on Mars
  ...ow layers. Both of these are the remains of layers that once covered wide regions. They often owe their existence to an erosion-resistant top layer. Someti Many other past lakes have been proposed for craters and other low regions.<ref>De Hon, R. 1992. Martian lake basins and lacustrine plains. Earth Moon
  19 KB (2,816 words) - 10:23, 2 January 2024
• Interplanetary commerce
  ...has a metal rich regolith along with what appears to be permanently shaded regions at the poles that may harbor water or possibly other volatiles<ref>https://
  9 KB (1,398 words) - 14:52, 2 October 2020
• Martian Meteorites
  ...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
  9 KB (1,466 words) - 08:56, 25 August 2021
• Cosmic radiation
  ...nd the sky would reduce this radiation to levels approaching high altitude regions on Earth. See [[Radiation shielding]] for more details.
  10 KB (1,660 words) - 22:07, 26 April 2024
• Lunae Palus quadrangle
  ...ikimolaargyre.jpg | MOLA map showing boundaries for Lunae Planum and other regions. Colors indicate elevations.]] MOLA map showing boundaries for Lunae Planum and other regions. Colors indicate elevations.
  19 KB (2,910 words) - 17:58, 24 December 2023
• Oxia Palus quadrangle
  ...//planetarynames.wr.usgs.gov/</ref> This quadrangle covers parts of many regions: Chryse Planitia, Arabia Terra, Xanthe Terra, Margaritifer Terra, Meridiani ...the strong impression that something abruptly disturbed the ground. Chaos regions formed long ago. By counting craters (more craters in any given area means
  40 KB (6,274 words) - 10:53, 23 December 2023
• Iapygia quadrangle
  ...outh latitude and from 270° to 315° west longitude (90-45 E). Parts of the regions called Tyrrhena Terra and Terra Sabaea are found in this quadrangle. The la ...n is a Russian term because this type of dune was first seen in the desert regions of Turkistan.<ref>| url=http://www.britannica.com/EBchecked/topic/53068/bar
  20 KB (3,015 words) - 06:56, 20 April 2024
• Crew 187 GreenHab Reports
  During my first day, I have divided the crops in 8 regions in order to compare each day the changes using picture
  14 KB (2,152 words) - 11:35, 24 March 2019
• Eridania quadrangle
  ...n is a Russian term because this type of dune was first seen in the desert regions of Turkistan.<ref>http://www.britannica.com/EBchecked/topic/53068/barchan</ ESP 049302 1385mantle.jpg|Wide view of crater with regions of latitude dependent mantle
  28 KB (4,220 words) - 06:09, 17 April 2024
• MAVEN
  ...J., R. Phillips. 2007. Hydrological modeling of outflow channels and chaos regions on Mars. Journal of Geophysical Research: Planets Volume 112, Issue E8 </re
  10 KB (1,524 words) - 14:33, 9 February 2019
• Casius quadrangle
  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
• Crew 186 Science Reports
  ...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
• Crew 197 Mission Summary
  ...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
• Martian features that are signs of water ice
  ...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
• Diacria quadrangle
  ...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 quadrangle
  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
• Mars
  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
• Amenthes quadrangle
  ...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
• Coprates quadrangle
  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
• Sinus Sabaeus quadrangle
  ...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
• Thaumasia quadrangle
  ...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
• Ismenius Lacus quadrangle
  ...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
• Hellas quadrangle
  ...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
• Margaritifer Sinus quadrangle
  ...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
• Crew 192 EVA Reports
  ...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
• Cebrenia quadrangle
  ...). "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
• Mariner 4
  ...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
• Crew 186 Mission Summary
  Geologic EVAs were performed to the following regions:
  13 KB (2,194 words) - 12:37, 30 September 2022
• CREW 191 – ASIA TEAM
  ...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
• Cost of energy on Mars
  ...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
• Mare Acidalium quadrangle
  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
• The beauty of Mars from 150 miles
  ...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
• Crew 188 Sol Summaries
  ...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
• Aeolis quadrangle
  ...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
• Argyre quadrangle
  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
• Oceans on Mars
  ...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
• Crew 186 Sol Summaries
  ...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
• Elysium quadrangle
  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
• Glaciers on Mars
  ...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
• Mare Tyrrhenum quadrangle
  ...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
• Mare Australe quadrangle
  ...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
• Crew 187 Mission Summary
  ...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
• Crew 202 Sol Summaries
  ...Kissing Camel Range, to collect clay and shale samples and identify sandy regions.
  24 KB (4,065 words) - 14:56, 7 March 2019
• What Mars Actually Looks Like!
  ...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
• Phoenicis Lacus quadrangle
  ...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
• Rivers on Mars
  ...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
• Syrtis Major quadrangle
  ...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
• Geological processes that have shaped Mars: Why Mars looks like it does
  ...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
• Crew 205 EVA Reports
  Purpose of EVA: Region Exploration and Sample Collection from Moon Regions
  25 KB (4,054 words) - 17:56, 7 March 2019
• Arcadia quadrangle
  ...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
• Crew 190 Journalism Reports
  ...which can then be assembled with surrounding maps to create maps of whole regions.
  24 KB (4,209 words) - 10:26, 24 March 2019
• HiWish program
  ...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
• Amazonis quadrangle
  ...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
• Crew 186 EVA Reports
  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
• Radioisotope Thermoelectric Generators: Advantages and Disadvantages
  ...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
• Arabia quadrangle
  ...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
• Crew 3 - Crew Reports
  ...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
• The Observational History of Mars as a Pathway for a Human Mission
  ...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
• Martian gullies
  ...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
• Extant Life on Mars
  ...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
• Crew 2 - Crew Reports
  ...seepage. Such a feature might possibly be similar to larger gully outflow regions identified on Mars. This feature had gone unnoticed during previous EVAs th ...more abundant. Large drought-resistant woody plants flourish in low-lying regions of valleys and canyons.
  173 KB (29,116 words) - 08:06, 29 October 2019
• Crew 200 Mission Summary
  ...communication between EVA crew and HabCom, and driving EVA to map further regions. One EVA member would drive the rover, while the other EVA member would pro
  42 KB (6,606 words) - 16:56, 7 March 2019
• Crew 1b - Crew Reports
  ...trate surface runoff into the canyon because the mudstone underneath these regions is more undercut as evidenced by U-shaped depressions running down the cany ...lenses of sandstone layers. The conglomerate is non-uniform with different regions of concentrations of different sized clasts. The sandstone is medium-graine
  190 KB (31,918 words) - 09:28, 12 October 2019
• Crew 4 - Crew Reports
  We use CO2 output as a measure of biological richness in the arctic regions for Global Carbon Models. These data will be analyzed for trends across sam ...bon Models, and utilization of this technique is also applicable in desert regions. Samples were taken from as many microhabitats as could be located along se
  287 KB (46,756 words) - 18:19, 19 December 2019
• Crew 1a - Crew Reports
  ...lenses of sandstone layers. The conglomerate is non-uniform with different regions of concentrations of different sized clasts. The sandstone is medium-graine
  127 KB (20,888 words) - 21:33, 4 October 2019
• Crew 6 - Crew Reports
  Some of the tafonified regions here seem to be associated with extensive horizontal oyster bed layers. Som
  118 KB (20,168 words) - 17:24, 16 March 2020