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Venus Has a Surprisingly Chilly Layer

The Blank Face of Venus (NASA/Gordan Ugarkovic)

Although similar in size to Earth, the planet-next-door Venus is typically perceived as a hellish inferno of caustic clouds, crushing pressures and kiln-like temperatures. And while those are indeed all very much the case, Venus has recently been found to have a cooler side too… although it’s 125 km (77 miles) up in its atmosphere.

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Phoenix’s Sense of Snow

Martian Polar Plains

Martian Polar Plains

The results are in: Mars has (or had) a favorable environment for life.

Microbial life, sure, but life nonetheless.

This is according to the results posted in this week’s edition of the journal Science, from the Phoenix Mars polar lander. The data indicates that the region around the lander has subsurface layers of perchlorate, a water-friendly compound that could allow microbial life to exist just beneath the surface of the Martial soil.

“Not only did we find water ice, as expected, but the soil chemistry and minerals we observed lead us to believe this site had a wetter and warmer climate in the recent past — the last few million years — and could again in the future,” said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Read the entire press release here.

The Phoenix lander, launched on August 4, 2007, landed in the north polar region of Mars with the objective of finding out if the planet has or once had favorable conditions for life. It has been silent since December of last year, when the harsh Martian winter set in and depleted its energy levels.

The results also indicate instances of snow in the Martian atmosphere. Apparently Mars has some very Earth-like precipitation at higher latitudes.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

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