Keck Observatory
Brendan Bowler and Michael Liu, IfA/Hawaii
Spectrum of Young Extrasolar Planet Yields Surprising Results
30 Aug 2010, 18:00 UTC
Brendan Bowler and Michael Liu, IfA/Hawaii
Kamuela, HI - Astronomers at the University of Hawaii have measured the temperature of a young gas-giant planet around another star using the W. M. Keck Observatory, and the results are puzzling. They have found that its atmosphere is unlike that of any previously studied extrasolar planet. By obtaining a spectrum of its emitted light, the astronomers determined the temperature of the planet. As a result, they found that current theoretical models of gas-giant planets did a poor job of explaining all the data. The team suspects that the reason is dust in the planet’s atmosphere. Models with normal amounts…
Note: All formatting and links have been removed - click title or image to see full article.




