The deuterium abundance in Jupiter and Saturn from ISO-SWS observations

By E. Lellouch, B. Bézard, T. Fouchet, H. Feuchtgruber, T. Encrenaz, T. Graauw. 2001

211 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/b3da823f73b0afdd4bd24a8c37175c7b85f0cc20

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. Martin Asplund
2. N. Grevesse
3. E. Jenkins
4. Pat Scott
5. A. Sauval
6. N. Madhusudhan
7. J. Michael Shull
8. B. Bézard

In Atmospheric Science

1. E. Jenkins
2. N. Grevesse
3. Martin Asplund
4. B. Draine
5. P. Irwin
6. Pat Scott
7. B. Conrath
8. A. Sauval

In Spectroscopy

1. B. Draine
2. P. Irwin

Citations in the corpus

• Photochemistry and diffusion in Jupiter's stratosphere: Constraints from ISO observations and comparisons with other giant planets (2005, methodology): “, 2000; Lellouch et al., 2002; Kunde et al., 2004]. Therefore global-average and 1-D models of oxygen compounds are not very meaningful for Jupiter in the post-SL9 era. Lellouch et al. [2002] provide model-data comparisons that suggest that H2O and CO2 originate from the deposition of oxygen compoun”
• Origin of water in the terrestrial planets (2005, background): “The D/H ratio of the nebular gas is inferred from spectroscopic measurements of CH4 in the atmospheres of Jupiter and Saturn to be 2.1 ± 0.4 × 10−5 (Lellouch et al. 2001), much lower than VSMOW.”
• The chemical composition of the Sun (2009, methodology): “Using ISO spectra of the Jovian atmosphere and taking into account an expected 5−10% enrichment during the planet’s formation, Lellouch et al. (2001) obtained a proto-solar abundance of D/H = (2.1 ± 0.4) · 10−5.”
• What Is the Total Deuterium Abundance in the Local Galactic Disk? (2006, background): “Analysis of Infrared Space Observatory (ISO) spectra of H2, HD, CH4, and CH3D in Jupiter’s atmosphere led Lellouch et al. (2001) to infer (D/H)psc = 21 ± 4 ppm, although there are many assumptions that go into this analysis.”
• The composition of Titan's stratosphere from Cassini/CIRS mid-infrared spectra (2007, background): “This potential problem was noted in ISO observations of Saturn (Lellouch et al., 2001).”