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[[File:ExtantLife1.jpg|200px|left|Extant Life on Mars|link=Extant Life on Mars]]
[[File:mdrs.jpg|300px|left|Mars Desert Research Station|link=Mars Desert Research Station]]
<div align="justify" style="text-align:justify;padding:0 5px;">The habitability of Mars is the key to discovering '''[[Extant Life on Mars]]'''. The question of whether Mars had conditions for life to arise and persist will be explored. The planet Mars has a high probability of extant life due to the many prerequisites for life that exist on the planet, as determined by the one example we have, Earth. Further research needs to be conducted to prove extant life exists on Mars. Defining life is paramount to any discovery of biological organisms, this will be examined by comparing the fossil records of early life on Earth and the examples of extremophiles presently being studied. Magnetic field pockets have been detected on Mars, which is thought to be necessary for life forms to be protected from harmful solar particles. Marsquakes are being detected by the InSight lander, contemporaneously with this publication, potentially solidifying the presence of a magnetic field, however that alone does not determine the existence of life on Mars. (InSight) Minerals that exist in the regolith are not a sole indicator of life. The mineral content of Mars [CHNOPS], including biologically available N, is conducive to supporting organisms that we know eke out a living in the same type of environment on Earth. A more complete record of prebiotic chemistry needs to be determined. Amino acids, the building blocks of DNA, have been found in meteorites from Mars. Mars has water in liquid form that occasionally erupts from below the surface and persists for short periods of time as a brine on the surface, allowing the liquid form to exist in the cold temperature and low pressure. Water is present in the subsurface of Mars. (McKay 2020) The presence of water does not equate to life, but every example of life on Earth depends on water to survive. Mars has organic material, including methane, which is commonly associated with biological processes. Methane on Earth is formed from biological sources 90% of the time. Yet, due to the possibility of serpentinization of minerals and geological cycling of methane, further research needs to be done to determine the biological or geological origin of CH4. (Astrobio) These facts alone are not unequivocal proof of extant life on Mars, but together they make a compelling case.</div>
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The '''[[Mars Desert Research Station]]''' (MDRS) is a Mars analog research facility run by [[The Mars Society]] in the southern Utah desert — the second of the Society's analog stations and one of the longest-running Mars surface simulations in the world. Since its habitat was built in 2001, rotating crews have lived "in simulation" near Hanksville, wearing analog spacesuits for surface excursions and rationing water, power, and communications much as an early Mars settlement would.
<div style="text-align:justify;padding:0 5px;">'''[[Extant Life on Mars|Read More]]''' </div>
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The campus has grown into a cluster of connected modules — the two-story Hab, the GreenHab greenhouse, the Science Dome laboratory, the RAM engineering workshop, and the Musk Mars Desert Observatory. Each field season (roughly October–May) hosts crews of six or seven scientists, engineers, and students from around the world; by 2025 more than 300 crews had completed rotations, carrying out research in geology, biology, engineering, and human factors. '''[[Mars Desert Research Station|Read more &rarr;]]'''
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Latest revision as of 13:11, 5 July 2026

Mars Desert Research Station
Mars Desert Research Station

The Mars Desert Research Station (MDRS) is a Mars analog research facility run by The Mars Society in the southern Utah desert — the second of the Society's analog stations and one of the longest-running Mars surface simulations in the world. Since its habitat was built in 2001, rotating crews have lived "in simulation" near Hanksville, wearing analog spacesuits for surface excursions and rationing water, power, and communications much as an early Mars settlement would.

The campus has grown into a cluster of connected modules — the two-story Hab, the GreenHab greenhouse, the Science Dome laboratory, the RAM engineering workshop, and the Musk Mars Desert Observatory. Each field season (roughly October–May) hosts crews of six or seven scientists, engineers, and students from around the world; by 2025 more than 300 crews had completed rotations, carrying out research in geology, biology, engineering, and human factors. Read more →