Issue |
A&A
Volume 533, September 2011
|
|
---|---|---|
Article Number | A114 | |
Number of page(s) | 7 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201117178 | |
Published online | 12 September 2011 |
Detection of a transit of the super-Earth 55 Cancri e with warm Spitzer⋆
1
Department of Earth, Atmospheric and Planetary Sciences,
Department of Physics, Massachusetts Institute of Technology,
77 Massachusetts Ave.,
Cambridge, MA
02139,
USA
e-mail: demory@mit.edu
2
Institut d’Astrophysique et de Géophysique, Université de Liège,
Allée du 6 Août 17, Bat.
B5C, 4000
Liège,
Belgium
3
Department of Astronomy, University of Maryland,
College Park, MD
20742-2421,
USA
4
Observatoire de Genève, Université de Genève,
51 Chemin des
Maillettes, 1290
Sauverny,
Switzerland
5
Planetary Science Group, Department of Physics, University of
Central Florida, Orlando, FL
32816-2385,
USA
Received:
3
May
2011
Accepted:
31
July
2011
We report on the detection of a transit of the super-Earth 55 Cnc e with warm
Spitzer in IRAC’s 4.5 μm band. Our MCMC analysis
includes an extensive modeling of the systematic effects affecting warm Spitzer
photometry, and yields a transit depth of 410 ± 63 ppm, which translates to a
planetary radius of as measured in IRAC
4.5 μm channel. A planetary mass of
is derived from an
extensive set of radial-velocity data, yielding a mean planetary density of
g cm-3.
Thanks to the brightness of its host star (V = 6,
K = 4), 55 Cnc e is a unique target for the thorough characterization of
a super-Earth orbiting around a solar-type star.
Key words: binaries: eclipsing / planetary systems / stars: individual: 55 Cnc / techniques: photometric
The photometric time series used in this work are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/533/A114
© ESO, 2011
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