Bursts of methane may have warmed early Mars
Early Mars presents a paradox: water related activity was most abundant when the Sun was several tens of percent dimmer than at present. Here, the authors provide a possible solution to the faint young Sun problem at Mars, finding that collision induced absorptions in a reduced Martian atmosphere would have been more efficient at trapping heat than previously believed.
The presence of water on ancient Mars is a paradox. There’s plenty of geographical evidence that rivers periodically flowed across the planet’s surface. Yet in the time period when these waters are supposed to have run — three to four billion years ago — Mars should have been too cold to support liquid water.
So how did it stay so warm?..more
- Article Category
- Research Letters
Transient reducing greenhouse warming on early Mars
- First Published:
- | Vol:
- | DOI:
Eos.org: Earth & Space Science News
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The atmosphere varies naturally on all length scales from millimeters to thousands of kilometers, and on all time scales from seconds to decades and longer. This special collection of Geophysical Research Letters synthesizes and summarizes that variability through a phenomenological census. The collection brings together some of the most influential and definitive papers to have been published in this journal in recent years. The topics covered include turbulence on time scales of seconds and minutes, gravity waves on time scales of hours, weather systems on time scales of days, atmospheric blocking on time scales of weeks, the Madden–Julian Oscillation on time scales of months, the Quasi-Biennial Oscillation and El Niño–Southern Oscillation on time scales of years, and the North Atlantic, Arctic, Antarctic, Pacific Decadal, and Atlantic Multi-decadal Oscillations on time scales of decades. The collection is accompanied by a Commentary article, which provides an authoritative, concise, and accessible point of reference for the most important modes of atmospheric variability.
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