Polarization of asteroid (387) Aquitania: the newest member of a class of large inversion angle asteroids

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12 pages, 2 figures, accepted to Icarus

Scientific paper

10.1016/j.icarus.2008.10.003

We present new imaging polarimetric observations of two Main Belt asteroids, (234) Barbara and (387) Aquitania, taken in the first half of 2008 using the Dual-Beam Imaging Polarimeter on the University of Hawaii 2.2 meter telescope, located on Mauna Kea, Hawaii. Barbara had been previously shown to exhibit a very unusual polarization-phase curve by Cellino, et al. (2006). Our observations confirm this result and add Aquitania to the growing class of large inversion angle objects. Interestingly, these asteroids show spinel features in their IR spectra suggesting a mineralogical origin to the phase angle-dependent polarimetric features. As spinel is associated with calcium-aluminum-rich inclusions and carbonaceous chondrites, these large inversion angle asteroids may represent some of the oldest surfaces in the solar system. Circular as well as linear polarization measurements were obtained but circular polarization was not detected.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Polarization of asteroid (387) Aquitania: the newest member of a class of large inversion angle asteroids does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Polarization of asteroid (387) Aquitania: the newest member of a class of large inversion angle asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarization of asteroid (387) Aquitania: the newest member of a class of large inversion angle asteroids will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-590215

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.