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  • ...-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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...left|thumb|300px|Map showing locations of Hellas Planitia and other nearby regions]]
    4 KB (676 words) - 20:14, 7 January 2020
  • ...ander confirmed in 2008 that water ice is not limited to the extreme polar regions.<ref>Smith, P., et al. 2009. H<sub><sup>2</sub>O 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
  • ...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
  • ...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
  • ...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
  • ...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
  • --- 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
  • ...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
  • ...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
  • ...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
  • 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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...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
  • ...//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
  • ...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
  • 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
  • ...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
  • ...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
  • 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

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