Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2011-03-11
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Accepted for publication in ApJL. 13 pages, 3 figures, 1 table
Scientific paper
We report observations of two consecutive transits of the warm super-Earth exoplanet GJ1214b at 3.6 and 4.5 microns with the Infrared Array Camera instrument on-board the Spitzer Space Telescope. The two transit light curves allow for the determination of the transit parameters for this system. We find these paremeters to be consistent with the previously determined values and no evidence for transit timing variations. The main investigation consists of measuring the transit depths in each bandpass to constrain the planet's transmission spectrum. Fixing the system scale and impact parameters, we measure R_p/R_star=0.1176 (+0.0008/-0.0009) and 0.1163 (+0.0010/-0.0008) at 3.6 and 4.5 microns, respectively. Combining these data with the previously reported MEarth Observatory measurements in the red optical yields constraints on the GJ1214b's transmission spectrum and allows us to rule-out a cloud-free, solar composition (i.e., hydrogen-dominated) atmosphere at 4.5 sigma confidence. This independently confirms a recent finding that was based on a measurement of the planet's transmission spectrum using the VLT. The Spitzer, MEarth, and VLT observations together yield a remarkably flat transmission spectrum over the large wavelength domain spanned by the data. Consequently, cloud-free atmospheric models require more than 30% metals (assumed to be in the form of H2O by volume to be consistent with all the observations.
Bean Jacob
Berta Zachory K.
Burke Christopher J.
Charbonneau David
Desert Jean-Michel
No associations
LandOfFree
Observational evidence for a metal rich atmosphere on the super-Earth GJ1214b does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Observational evidence for a metal rich atmosphere on the super-Earth GJ1214b, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational evidence for a metal rich atmosphere on the super-Earth GJ1214b will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-278065