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Mars' Frozen Silence: Unique Formation on the Hillside seen by NASA's Perseverance, Curiosity, MRO
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On Mars, as seen by NASA's Perseverance and Curiosity Rovers, ice subjected to frigid temperatures undergoes a singular metamorphosis. Known as sublimation, the transition from solid ice directly into vapor occurs due to the planet's rarefied atmosphere and feeble solar radiation. This atmospheric condition, significantly thinner than Earth's, permits the direct conversion of frozen water or carbon dioxide into gaseous state, bypassing the liquid phase entirely.
The consequence of this unique phenomenon is a sculpted Martian landscape. Ephemeral channels known as "spiders," spanning kilometers in length, appear across ancient riverbeds and crater floors on Mars. These formations, arising over several Martian seasons, contain useful information about past water activity and the distribution of subsurface ice. Atmospheric dynamics are further entwined with sublimation.
Ascending vapor cools and condenses high above the surface, creating clouds that modulate Mars' temperature by reflecting a substantial portion of incoming sunlight back into space. In this video you can see how Martian clouds look like according to Perseverance's onboard cameras. This process influences the planet's climate through feedback loops, altering solar energy absorption and potentially impacting the rate of ice sublimation itself.
Renders of Mars planet in the end of the video - by iGadgetPro
All NASA's RAW-images were colorized, processed and edited by iGadgetPro
Timecodes
0:00 - Introduction to ice sublimation on Mars
0:45 - Factors influencing sublimation rates (altitude, latitude, dust cover)
1:32 - Sublimation rate at mid-latitudes
3:08 - Landforms sculpted by sublimation erosion (mesas, canyons, yardangs)
4:47 - CO2 ice reserves on the Red Planet polar regions
5:56 - Wind's role in shaping the Martian surface (dust devils, channels, dunes)
7:31 - Ongoing research and future Mars missions
#mars #marsin4k #marsclimate #nasamars #marsrover #MartianSublimation
The consequence of this unique phenomenon is a sculpted Martian landscape. Ephemeral channels known as "spiders," spanning kilometers in length, appear across ancient riverbeds and crater floors on Mars. These formations, arising over several Martian seasons, contain useful information about past water activity and the distribution of subsurface ice. Atmospheric dynamics are further entwined with sublimation.
Ascending vapor cools and condenses high above the surface, creating clouds that modulate Mars' temperature by reflecting a substantial portion of incoming sunlight back into space. In this video you can see how Martian clouds look like according to Perseverance's onboard cameras. This process influences the planet's climate through feedback loops, altering solar energy absorption and potentially impacting the rate of ice sublimation itself.
Renders of Mars planet in the end of the video - by iGadgetPro
All NASA's RAW-images were colorized, processed and edited by iGadgetPro
Timecodes
0:00 - Introduction to ice sublimation on Mars
0:45 - Factors influencing sublimation rates (altitude, latitude, dust cover)
1:32 - Sublimation rate at mid-latitudes
3:08 - Landforms sculpted by sublimation erosion (mesas, canyons, yardangs)
4:47 - CO2 ice reserves on the Red Planet polar regions
5:56 - Wind's role in shaping the Martian surface (dust devils, channels, dunes)
7:31 - Ongoing research and future Mars missions
#mars #marsin4k #marsclimate #nasamars #marsrover #MartianSublimation
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