• Thumbnail for MAVEN
    planet's climate and water. The name is an acronym for "Mars Atmosphere and Volatile Evolution" while the word maven also denotes "a person who has special...
    37 KB (3,981 words) - 18:31, 22 May 2025
  • Thumbnail for Shannon Curry
    planetary physicist and the Principal Investigator of the NASA Mars Scout mission MAVEN (Mars Atmosphere and Volatile Evolution). Curry is an associate...
    6 KB (548 words) - 04:14, 13 April 2025
  • Thumbnail for Solar wind
    which are ripped off by the solar wind. In 2015 the NASA Mars Atmosphere and Volatile Evolution (MAVEN) mission measured the rate of atmospheric stripping...
    57 KB (6,718 words) - 12:33, 29 May 2025
  • Thumbnail for Magnetic field of Mars
    measurements from the Mars Global Surveyor (MGS) magnetic field experiment/electron reflectometer (MAG/ER) and Mars Atmosphere and Volatile Evolution (MAVEN) magnetic-field...
    22 KB (2,148 words) - 00:41, 3 September 2024
  • Thumbnail for Exploration of Mars
    Wayback Machine. Space Daily. Retrieved 19 November 2011. "Mars Atmosphere and Volatile Evolution mission – MAVEN". NASA. 2015-02-24. Archived from the original...
    123 KB (11,279 words) - 20:43, 6 June 2025
  • Thumbnail for Atmosphere of Mars
    The atmosphere of Mars is the layer of gases surrounding Mars. It is primarily composed of carbon dioxide (95%), molecular nitrogen (2.85%), and argon...
    149 KB (15,322 words) - 03:03, 9 June 2025
  • Thumbnail for NASA
    Human exploration, and observed the key chemical ingredients for life to occur. In 2013, the Mars Atmosphere and Volatile Evolution (MAVEN) mission observed...
    223 KB (20,686 words) - 12:37, 10 June 2025
  • Thumbnail for Climate of Mars
    are also important differences, such as much lower thermal inertia. Mars's atmosphere has a scale height of approximately 11 km (36,000 ft), 60% greater...
    114 KB (11,742 words) - 04:00, 9 June 2025
  • Thumbnail for Mars
    20 °C (−243 to 68 °F) and cosmic radiation is high. Mars retains some water, in the ground as well as thinly in the atmosphere, forming cirrus clouds...
    209 KB (18,461 words) - 20:56, 15 May 2025
  • Thumbnail for Water on Mars
    the surface of Mars, limited to traces of dissolved moisture from the atmosphere and thin films, large quantities of ice are present on and under the surface...
    293 KB (30,911 words) - 18:42, 7 June 2025
  • Kaveh; Usui, Tomohiro (2018-07-26). "Water and Volatile Inventories of Mercury, Venus, the Moon, and Mars". Space Science Reviews. 214 (5): 92. Bibcode:2018SSRv...
    21 KB (2,678 words) - 00:08, 10 June 2025
  • biosignatures in the soil and rocks at the planet's surface, and biomarker gases in the atmosphere. Mars is of particular interest for the study of the origins...
    213 KB (20,791 words) - 20:31, 9 June 2025
  • Thumbnail for Atmosphere of Titan
    the Solar System with an atmosphere that is denser than the atmosphere of Earth and is one of two moons with an atmosphere significant enough to drive...
    55 KB (5,914 words) - 13:41, 9 June 2025
  • Thumbnail for Atmosphere of Pluto
    known atmosphere. Its closest analog is the atmosphere of Triton, although in some aspects it resembles even the atmosphere of Mars. The atmosphere of Pluto...
    59 KB (6,083 words) - 21:09, 29 May 2025
  • Thumbnail for List of active Solar System probes
    List of active Solar System probes (category Discovery and exploration of the Solar System)
    Destination: Mars Arrival: 6 August 2012 Institution: NASA MAVEN — Mars Atmosphere and Volatile Evolution. Mission: study the Martian upper atmosphere and its...
    19 KB (2,006 words) - 06:34, 6 June 2025
  • Jane Lee Fox (category Harvard Graduate School of Arts and Sciences alumni)
    hydrocarbons in atmosphere of Titan, one of the moon's of Saturn. Fox was a member of the science team for the Mars Atmosphere and Volatile Evolution (MAVEN)...
    9 KB (694 words) - 18:24, 23 May 2025
  • Thumbnail for Solar System
    and Neptune) formed further out, beyond the frost line, the point between the orbits of Mars and Jupiter where material is cool enough for volatile icy...
    224 KB (21,986 words) - 22:29, 7 June 2025
  • (REPTile) Lunar Atmosphere and Dust Environment Explorer (LADEE) Lunar Dust Experiment (LDEX) MAVEN - Mars Atmosphere and Volatile EvolutioN Mission Magnetospheric...
    5 KB (541 words) - 17:49, 25 October 2024
  • Thumbnail for Terraforming of Mars
    gravity of Mars requires 2.6 times Earth's column airmass to obtain the optimum 100 kPa (15 psi) pressure at the surface. Additional volatiles to increase...
    67 KB (6,471 words) - 20:07, 11 June 2025
  • Thumbnail for Composition of Mars
    Crater on Mars. Hydrogen is present as water (H2O) ice and in hydrated minerals. Carbon occurs as carbon dioxide (CO2) in the atmosphere and sometimes...
    90 KB (9,037 words) - 04:33, 26 March 2025
  • Thumbnail for Terraforming
    Terraforming (section Mars)
    the planet and altering its atmosphere, and NASA has even hosted debates on the subject. Several potential methods for the terraforming of Mars may be within...
    62 KB (7,156 words) - 20:52, 22 May 2025
  • Thumbnail for Venus
    Robert O. (1 July 1991). "On the origin and early evolution of terrestrial planet atmospheres and meteoritic volatiles". Icarus. 92 (1): 2–79. Bibcode:1991Icar...
    224 KB (20,391 words) - 05:52, 12 June 2025
  • Thumbnail for Prebiotic atmosphere
    prebiotic atmosphere is the second atmosphere present on Earth before today's biotic, oxygen-rich third atmosphere, and after the first atmosphere (which...
    41 KB (4,605 words) - 11:37, 22 May 2025
  • Jupiter (spacecraft) (category Lockheed Martin satellites and probes)
    designs of two earlier Lockheed Martin spacecraft: Mars Atmosphere and Volatile Evolution Mission (MAVEN), and the Juno spacecraft. Jupiter is to include a...
    10 KB (1,108 words) - 00:21, 7 March 2025
  • Thumbnail for Formation and evolution of the Solar System
    surface or atmosphere. Such a fate awaits the moons Phobos of Mars (within 30 to 50 million years), Triton of Neptune (in 3.6 billion years), and at least...
    113 KB (13,512 words) - 03:13, 5 June 2025
  • pre-Noachian and Noachian, which is not well known. Volatile outgassing is thought to have occurred during these periods. One way to ascertain whether Mars possessed...
    30 KB (3,666 words) - 15:25, 18 April 2025
  • Pepin, Robert O. (1991). "On the origin and early evolution of terrestrial planet atmospheres and meteoritic volatiles". Icarus. 92 (1): 2–79. Bibcode:1991Icar...
    42 KB (5,115 words) - 06:59, 2 June 2025
  • Thumbnail for Space tug
    designs of two earlier Lockheed Martin spacecraft—Mars Atmosphere and Volatile Evolution Mission and the Juno—as well as a robotic arm from MDA derived...
    37 KB (3,615 words) - 21:42, 23 April 2025
  • Thumbnail for Climate of Triton
    fluctuations that induce global volatile transport between its polar caps, leading to variable atmospheric circulation. The atmosphere of Triton also supports...
    21 KB (2,294 words) - 13:04, 28 May 2025
  • Thumbnail for Mineral evolution
    Water and other volatiles, if present, increase the total. Earth was volatile-rich, with an atmosphere composed of N2, CO2 and water, and an ocean that...
    45 KB (5,027 words) - 03:20, 9 June 2025