Author
Listed:
- Kevin B. Stevenson
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
- Joseph Harrington
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
- Sarah Nymeyer
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
- Nikku Madhusudhan
(Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA)
- Sara Seager
(Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA)
- William C. Bowman
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
- Ryan A. Hardy
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
- Drake Deming
(Planetary Systems Laboratory, NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA)
- Emily Rauscher
(Columbia University, New York, New York 10027, USA)
- Nate B. Lust
(Planetary Sciences Group, University of Central Florida, Orlando, Florida 32816, USA)
Abstract
A 'hot Neptune' low on gas New observations in the infrared provide the first indications of the atmospheric composition of a 'hot Neptune' extrasolar planet, Gliese 436b (GJ 436b). A companion to an M-dwarf star, GJ 436b exhibits a high abundance of carbon monoxide. Water and trace amounts of carbon dioxide are also present but the concentration of methane, expected to be the dominant carbon-bearing species in a hydrogen-dominated atmosphere, is 100,000 times less than predicted for a planet in thermochemical equilibrium. Possible disruptive influences include vertical mixing and methane polymerization. The measurements were accomplished at six wavelengths using the Spitzer Space Telescope while the planet passed behind its parent star on a short, 2.64-day orbit.
Suggested Citation
Kevin B. Stevenson & Joseph Harrington & Sarah Nymeyer & Nikku Madhusudhan & Sara Seager & William C. Bowman & Ryan A. Hardy & Drake Deming & Emily Rauscher & Nate B. Lust, 2010.
"Possible thermochemical disequilibrium in the atmosphere of the exoplanet GJ 436b,"
Nature, Nature, vol. 464(7292), pages 1161-1164, April.
Handle:
RePEc:nat:nature:v:464:y:2010:i:7292:d:10.1038_nature09013
DOI: 10.1038/nature09013
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