Physical Characterization of Fast rotating NEOs From Spectroscopy Back to Spectrophotometry
Abstract
Required technique for physical characterization of fast rotating asteroids (with H>22, and V magnitude between 18.0 and 19.5) remains Spectrophotometry. Nevertheless, comparison of the relative reflectance spectrum of the object with the actual spectra from SMASSI, SMASSII, and laboratories is necessary.
- Publication:
-
EPSC-DPS Joint Meeting 2019
- Pub Date:
- September 2019
- Bibcode:
- 2019EPSC...13..365K