Unidentified Lines In The High-resolution 3-micron Spectra of Jupiter And Titan

Details Unidentified Lines In The High-resolution 3-micron Spectra of Jupiter And Titan Unidentified Lines In The High-resolution 3-micron Spectra of Jupiter And Titan

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dps....42.1112s&link_type=abstract

American Astronomical Society, DPS meeting #42, #11.12; Bulletin of the American Astronomical Society, Vol. 42, p.1019

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We introduce unidentified lines detected in the high-resolution spectra of Jupiter and Titan which were reported by Seo et al. (2009), Kim et al. (2005) and Kim et al. (2010). We have reanalyzed the high-resolution spectra of Titan and Jupiter in the 2.87 - 3.4 micron range in order to find appropriate molecular bands which are responsible for those unidentified lines. We used the theoretical and laboratory IR databases for molecular ro-vibrational spectra available in literature. We present a preliminary result for the identification and suggest low-temperature laboratory observations, which might help the identifications.
References :
Seo, H. et al. 2009, Icarus 199, 449-457
Kim, S.J. et al. 2005, Icarus 173, 522-532
Kim, S.J. et al. 2010, Icarus 208, 837-849

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