Correlating IRTF Spectra and Arecibo Radar Observations of Low-Albedo Main-Belt Asteroids

Astronomy and Astrophysics – Astronomy

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Scientific paper

We have coordinated radar observations and spectral observations of low-albedo main-belt asteroids in order to investigate whether there is a radar signature for hydrated minerals. A suggestion of such a correlation from serendipitous observations of 105 Artemis indicated that hydrated minerals might have higher radar albedos. About 30 objects have now been sampled, including re-observing 105 Artemis, and the relationship may not be a simple one. The radar images of many of these asteroids, primarily of taxonomic classes C and P, are remarkably complex, showing bright glints and irregular features. In order to link the radar and spectra together over several weeks, we have asked the amateur astronomy community for lightcurve observations. Their generous response has been extremely valuable. In many cases, we have found that the rotation period differs considerably from the previous best estimates Lightcurve observations also allow us to determine the relative rotation phase of spectra and radar observations made several weeks apart. . We can also improve the interpretation of the radar data considerably if the rotation period is known independently. Results of these combined observations will be presented.
The Arecibo Observatory is part of the National Astronomy and Ionosphere Center, which is operated by Cornell University under a cooperative agreement with the National Science Foundation.
Visiting astronomers at the Infrared Telescope Facility, which is operated by the University of Hawaii, under Cooperative Agreement no. NCC 5-538 with the National Aeronautics and Space Administration, Science Mission Directorate, Planetary Astronomy Program.

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