Washington:After examining a dozen types of suns and a roster of planet surfaces, Cornell University astronomers have developed a practical model -- an environmental colour decoder -- to tease out climate clues for potentially habitable exoplanets in galaxies far away.
"We looked at how different planetary surfaces in the habitable zones of distant solar systems could affect the climate on exoplanets," said Jack Madden, PhD '20, who works in the lab of Lisa Kaltenegger, associate professor of astronomy and director of Cornell's Carl Sagan Institute.
"Reflected light on the surface of planets plays a significant role not only on the overall climate but also on the detectable spectra of Earth-like planets," Madden said.
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Madden and Kaltenegger are co-authors of 'How Surfaces Shape the Climate of Habitable Exoplanets,' released in the monthly notices of the Royal Astronomical Society.
In their research, they combine detail of a planet's surface colour and the light from its host star to calculate a climate. For instance, a rocky, black basalt planet absorbs light well and would be very hot, but add sand or clouds and the planet cools and a planet with vegetation and circling a reddish K-star will likely have cool temperatures because of how those surfaces reflect their suns' light.
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