Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-19T04:45:14.644Z Has data issue: false hasContentIssue false

Spectroscopic Observations of Solar System Objects: Pushing the Limits

Published online by Cambridge University Press:  07 August 2017

Anita L. Cochran*
Affiliation:
The University of Texas, McDonald Observatory

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Targets within the solar system generally fall into one of two types: a) major planets (except Pluto) and our Moon; b) minor planets, comets, Pluto and planetary satellites. The first group is noteworthy for being reasonably bright. Most are also spatially extended. The inner planets never achieve large solar elongation. The second group comprises bodies which are generally faint. Comets are spatially extended. The minor planets and comets may be in orbits which are highly inclined or viewed at small solar elongations. Comets may even be in retrograde orbits. Planetary satellites may be bright or faint but suffer from being in the glare of the parent planet.

Type
Section I — Review Papers
Copyright
Copyright © Kluwer 1995 

References

Bell, J. F., Hawke, B. R., Owensby, P. D., and Gaffey, M. J. 1988 Lunar Planet. Sci. Conf. XIX, 57.Google Scholar
Binzel, R. P. and Xu, S. 1993 Science 260, 186.Google Scholar
Binzel, R. P., Xu, S., Bus, S. J., Skrutskie, M. F., Meyer, M. R., Knezek, P. and Barker, E. S. 1993 Science 262, 1541.CrossRefGoogle Scholar
Chapman, C. R. and Gaffey, M. J. 1979 in Asteroids, Gehreis, T., ed., The University of Arizona Press, Tucson, p. 1064.Google Scholar
Chapman, C. R., Morrison, D. and Zellner, B. 1975 Icarus 25, 104.Google Scholar
Kleine, M. 1994 Carbon Isotope Abundance Ratios in Comets, Ph.D. thesis, Arizona State University.Google Scholar
Kleine, M., Wyckoff, S., Wehinger, P. A. and Peterson, B. A. 1994 ApJ 436, 885.Google Scholar
Kleine, M., Wyckoff, S., Wehinger, P. A. and Peterson, B. A. 1995a ApJ 439, 1021.CrossRefGoogle Scholar
Kleine, M., Wyckoff, S., Wehinger, P. A. and Peterson, B. A. 1995b ApJ 439, 1021.Google Scholar
McFadden, L. A., Bell, J. F. and McCord, T. B. 1980 Icarus 44, 410.CrossRefGoogle Scholar
Potter, A. E. and Morgan, T. H. 1988 Science 241, 675.CrossRefGoogle Scholar
Sawyer, S. R. 1991 Ph.D. thesis, The University of Texas at Austin.Google Scholar
Spencer, J. R., Calvin, W. M. and Person, M. J. 1994 JGR Planets, submitted.Google Scholar
Tholen, D. J. 1984 Ph.D. thesis, Univ. of Arizona.Google Scholar
Vilas, F. and McFadden, L. A. 1992 Icarus 100, 85.CrossRefGoogle Scholar
Woodman, J. H., Cochran, W. D. and Slavsky, D. B. 1979 Icarus 37, 73.CrossRefGoogle Scholar
Xu, S., Binzel, R. P., Burbine, T. H. and Bus, S. J. 1994 Submitted to Icarus.Google Scholar