Participation in the Consolidated Infrared Spectrometer (CIRS) as Co-Investigator

Details Participation in the Consolidated Infrared Spectrometer (CIRS) as Co-Investigator Participation in the Consolidated Infrared Spectrometer (CIRS) as Co-Investigator

Jan 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000stin...0127888o&link_type=abstract

Technical Report, Hawaii Univ. Honolulu, HI United States Inst. for Astronomy

Astronomy and Astrophysics

Astronomy

Infrared Spectrometers, Nitrogen Isotopes, Saturn Atmosphere, Ammonia, Spectral Bands, Nuclear Fusion, Earth Atmosphere, Galileo Probe, Jupiter Atmosphere, Dredging, Enrichment, Errors, Mass Spectrometers, Mass Spectra, Gas Giant Planets

Scientific paper

During the period under review, Owen-pursued the question of a determination of N-15/N-14 in the atmosphere of Saturn, to be carried out by CIRS when Cassini is in orbit about the planet. There are presently no determinations of this important isotope ratio in Saturn, but a study of the 10 microns spectral region of Jupiter has led to the identification of (N-15)H3 lines with the short Wavelength Spectrometer (SWS) of ISO. The resulting determination was a value of N-15/N-14 = 1.9 (+0.9/-1.0) x 10-3 for this giant planet. This number is decidedly lower than the terrestrial value of 3.66 x 10-3 for molecular nitrogen in the Earth's atmosphere. It is much lower than a direct measurement of N-15/N-14 =5 (+2 /-1) x 10-3 in the solar wind by Kallenbach et al. The latter discrepancy is especially surprising in that Jupiter and the sun are expected to have identical isotope ratios: deep mixing on the sun that would dredge up products of nucleosynthesis from the solar interior is not known to occur. Both Fouchet et al. and Kallenbach et al. suggested that some as yet unknown fractionation process in Jupiter's upper atmosphere might act to enrich N-14 above the NH3 clouds, at the 400 mb pressure level corresponding to the ISO observation. A new measurement of the nitrogen isotopes on Jupiter has just become available from the in situ mass spectra recorded by the Galileo Probe Mass Spectrometer. It is N-15/N-14 = 2.3 +/- 0.3 x 10-3. This determination refers to a pressure level greater than 0.8 mb, weighted toward 2 bars. This new result validates the essential correctness of the Fouchet et al. measurement while greatly reducing the uncertainty. It thus appears that the Kallenbach et al. value must somehow be in error. Further support for this conclusion comes from the upper limit of N-15/N-14 less than 2.8 x 10-3 set for solar wind nitrogen implanted in lunar grains.

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