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Comparing key compositional indicators in Jupiter with those in extra-solar giant planets

Lunine, Jonathan I. and Greene, Tom and Beichman, Charles and Bean, Jacob and Hammel, Heidi B. and Marley, Mark S. (2019) Comparing key compositional indicators in Jupiter with those in extra-solar giant planets. Astro2020 Science White Paper, . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20191126-091657483

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Abstract

Spectroscopic transiting observations of the atmospheres of hot Jupiters around other stars, first with Hubble Space Telescope and then Spitzer, opened the door to compositional studies of exoplanets. The James Webb Space Telescope will provide such a profound improvement in signal-to-noise ratio that it will enable detailed analysis of molecular abundances, including but not limited to determining abundances of all the major carbon- and oxygen-bearing species in hot Jupiter atmospheres. This will allow determination of the carbon-to-oxygen ratio, an essential number for planet formation models and a motivating goal of the Juno mission currently around Jupiter.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1904.00054arXivDiscussion Paper
ORCID:
AuthorORCID
Lunine, Jonathan I.0000-0003-2279-4131
Greene, Tom0000-0002-8963-8056
Beichman, Charles0000-0002-5627-5471
Bean, Jacob0000-0003-4733-6532
Hammel, Heidi B.0000-0001-8751-3463
Marley, Mark S.0000-0002-5251-2943
Additional Information:Submitted to the Astro2020 Decadal Survey as a white paper; thematic areas "Planetary Systems" and "Star and Planet Formation."
Series Name:Astro2020 Science White Paper
Record Number:CaltechAUTHORS:20191126-091657483
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191126-091657483
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100057
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:26 Nov 2019 17:46
Last Modified:26 Nov 2019 17:46

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