Cometary constraints on the planet forming environment.
Molecular elemental and isotopic abundances of comets provide sensitive diagnostics for models of the primitive solar nebula. New measurements of the N2, NH and NH2 abundances in comets together with the in situ Giotto mass spectrometer and dust analyzer data provide new constraints for models of the comet forming environment in the solar nebula. An inventory of nitrogen-containing species in comet Halley indicates that NH3 and CN are the dominant N carriers observed in the coma gas. The elemental nitrogen abundance in the gas component of the coma is found to be depleted by a factor approximately 75 relative to the solar photosphere. Combined with the Giotto dust analyzer results for the coma dust component, we find for comet Halley Ngas + dust approximately 1/6 the solar value. The measurement of the CN carbon isotope ratio from the bulk coma gas and dust in comet Halley indicates a significantly lower value, 12C/13C = 65 +/- 9 than the solar system value of 89 +/- 2. Because the dominant CN carrier species in comets remains unidentified, it is not yet possible to attribute the low isotope ratio predominantly to the bulk gas or dust components. The large chemical and isotopic inhomogeneities discovered in the Halley dust particles on 1 mu scales are indicative of preserved circumstellar grains which survived processing in the interstellar clouds, and may be related to the presolar silicon carbide, diamond and graphite grains recently discovered in carbonaceous chondrites. Less than 0.1% of the bulk mass in the primitive meteorites studied consists of these cosmically important grains. A larger mass fraction (approximately 5%) of chemically heterogeneous organic grains is found in the nucleus of comet Halley. The isotopic anomalies discovered in the PUMA 1 Giotto data in comet Halley are probably also attributable to preserved circumstellar grains. Thus the extent of grain processing in the interstellar environment is much less than predicted by interstellar grain models, and a significant fraction of comet nuclei (approximately 5%) may be in the form of preserved circumstellar matter. Comet nuclei probably formed in much more benign environments than primitive meteorites.
Wyckoff
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Department of Physics and Astronomy, Arizona State University, Tempe 85287-1504, USA.
D000641:Ammonia; D002247:Carbon Isotopes; D002248:Carbon Monoxide; D019443:Cosmic Dust / Q000032:analysis*; D003486:Cyanides; D019419:Evolution, Planetary; D018559:Exobiology; D005740:Gases / Q000032:analysis*; D006859:Hydrogen; D019110:Meteoroids; D009584:Nitrogen / Q000737:chemistry; D010100:Oxygen; D016082:Solar System; D013026:Space Flight; D018531:Spacecraft
D002247:Carbon Isotopes; D019443:Cosmic Dust; D003486:Cyanides; D005740:Gases; D000641:Ammonia; D002248:Carbon Monoxide; D006859:Hydrogen; D009584:Nitrogen; D010100:Oxygen