Methane and its isotopologues on Saturn from Cassini/CIRS observations

By L. Fletcher, G. Orton, Nicholas A. Teanby, P. Irwin, G. Bjoraker. 2009

170 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/9c476e03a44660be73c8b435ef3ad7c189e850fc

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. N. Madhusudhan
2. Jon Fortney
3. M. Line
4. A. Showman
5. J. D'esert
6. Laura Kreidberg
7. Sara Seager
8. D. Deming

In Atmospheric Science

1. Jon Fortney
2. N. Madhusudhan
3. A. Showman
4. J. D'esert
5. Derek Homeier
6. M. Line
7. G. Henry
8. Laura Kreidberg

Citations in the corpus

• THE MASS–METALLICITY RELATION FOR GIANT PLANETS (2015, background): “Spectroscopy of the solar system’s giants points to enhancements in the mixing ratio of carbon (as seen in CH4) of ∼4, 10, 80, and 80, in Jupiter, Saturn, Uranus, and Neptune, respectively (Wong et al. 2004; Fletcher et al. 2009).”
• A PRECISE WATER ABUNDANCE MEASUREMENT FOR THE HOT JUPITER WASP-43b (2014, background): “Jupiter’s methane abundance is from the Galileo probe (Wong et al. 2004), while those of the other planets are from infrared spectroscopy (Fletcher et al. 2009; Karkoschka & Tomasko 2011; Sromovsky et al. 2011).”
• Exoplanetary Atmospheres: Key Insights, Challenges, and Prospects (2019, methodology): “Determination of the Minimum Masses of Heavy Elements in the Envelopes of Jupiter and Saturn.”