WHAT IS NEW ABOUT THE NEW COMET YANAKA (1988R)

Citation
Jm. Greenberg et al., WHAT IS NEW ABOUT THE NEW COMET YANAKA (1988R), The Astrophysical journal, 414(1), 1993, pp. 120000045-120000048
Citations number
44
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
0004637X
Volume
414
Issue
1
Year of publication
1993
Part
2
Pages
120000045 - 120000048
Database
ISI
SICI code
0004-637X(1993)414:1<120000045:WINATN>2.0.ZU;2-Y
Abstract
A deficiency in the observed abundances of C2 and CN in comet Yanaka ( 1988r) is explained in terms of the properties of its organic refracto ry dust component and the fact that it is a new comet. Because the maj or fraction of the carbon in comets is in a mixture of complex organic molecules which earlier explained the ''missing'' carbon mystery it i s shown that substantial carbon depletions are impossible. The low C2 and CN production rates may be understood as consequences of Yanaka (1 988r) being a new comet in combination with the small central area of coma observed. The surface of new comets resulting from cosmic-ray pro cessing in the Oort cloud gives rise to dust which is relatively nonfr agile and which remains relatively large and cool within the limits of a small diaphragm making the comet appear to be dust poor. This dust yields smaller abundances of carbon-rich species by evaporation than c ustomary for the smaller and hotter fragmented particles further out i n the coma.