Extrasolar
planets could have hospitable climates
A modeling
study in the International Journal of Astrobiology suggests that
some planets with high obliquity—those whose axes are tilted
more strongly than Earth’s—have more potential for life-supporting
climates than previously thought. Darren Williams (Penn State Erie,
the Behrend College) and David Pollard (EMS Environment Institute, Pennsylvania
State University) simulated the climates for 12 planetary scenarios
that varied in their obliquity, level of atmospheric carbon dioxide,
and configuration of continents. Using the GENESIS global circulation
model, Williams and Pollard found that, as obliquity goes up for an
Earthlike planet, high latitudes tend to warm while the tropics typically
cool, with a slight global warming overall. They note that obliquity’s
effect on climate occurs only for certain arrangements of continents,
where seasonal extremes are magnified. The GENESIS simulations for other
types of planets showed the greatest temperature extremes—with
monthly surface temperatures averaging as high as 80 to 100°C (176
to 212°F)—occurred where high-latitude continents were most
prevalent. However, Williams and Pollard found that none of the seasonal
extremes in their high-obliquity scenarios were enough to generate
a climate catastrophe in the form of a runaway greenhouse effect or
global ice sheets. “Therefore, most Earth-like planets should
be hospitable to life at high obliquity,” say the authors. Williams
hopes to see the work used in modeling visible and infrared light curves
of extrasolar planets for such efforts as the Space Interferometry Mission
and the Terrestrial Planet Finder.