Light fog drifts through a dry Martian gully in an artist's rendering
In the dead of Martian winter, the snowflakes that blanket the planet's poles are no bigger than red blood cells, according to a new study of the icy particles.
The results suggest that, rather than resembling a blizzard, Mars snow would probably look like fog as it fell.
But when temperatures drop in winter to -193 degrees Fahrenheit (-125 degrees Celsius), it gets cold enough for carbon dioxide in the Martian atmosphere to freeze, creating clouds of dry ice that can reach from the poles to halfway to the equator.
So far, no Mars landers have survived near the poles during winter. So to learn more about the carbon dioxide snow, researchers at the Massachusetts Institute of Technology analyzed data spanning 15 years and gathered by NASA orbiters.
Measuring Snowflakes From Orbit
Information from the
Mars Reconnaissance Orbiter helped scientists predict where the clouds are likely to form, based on the temperature and pressure conditions under which such snow can develop.
In addition, the snow and frost deposits add enough mass each winter to alter the planet's gravitational field by a tiny amount.
Using gravity data from the
Mars Global Surveyor, the team estimated how much carbon dioxide snow piles up at both poles seasonally. That probe also showed the amount of light reflected by snow clouds, which helped the researchers determine the clouds' density.
Combining the data, the team was able to pinpoint the number and sizes of snow particles within the clouds.
Around the south pole, carbon dioxide snow particles ranged from 4 to 13 microns—for comparison, the average human red blood cell is 6 to 8 microns wide.
Around the north pole, where the atmosphere is much denser, snow particles range from 8 to 22 microns. On Earth snowflakes tend to be much bigger, around ten millimeters wide.
Snow Size Affects Mars Climate?
Knowing the size of snowflakes on Mars could be "very helpful" in understanding the overall properties of the Martian atmosphere, according to study co-author
Kerri Cahoy of MIT.
Drops of precipitation, including snow crystals, usually form around atmospheric particles such as dust.
But it could be that carbon dioxide snow particles don't need dust grains to form—instead they somehow coalesce directly from the air, Cahoy said.
In addition, the size and composition of Martian snow influences which wavelengths of sunlight the ice crystals absorb and reflect, said study co-author
Renyu Hu, also at MIT.
A better understanding of how the snow particles range in size may therefore yield insight into how much of the sun's energy the planet absorbs—the process that drives Martian climate.
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