[Previous] | [Session 22] | [Next]
B. Bhattacharya, W.T. Reach (SIRTF Science Center), G. G. Fazio (Smithsonian Astrophysical Observatory)
We present mid-infrared observations of solar system objects (SSO's) at 3.6, 4.5, 5.8, and 8.0 microns. These objects have been observed during the initial calibration and verification phase of the SIRTF mission. We also provide specifications on spacecraft tracking of moving objects.
If you would like more information about this abstract, please follow the link to Bidushi Bhattacharya. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: 1200 E. California Blvd., MS 220-6, Pasadena
[Previous] | [Session 22] | [Next]
Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.