Back to Search
Start Over
Spin axis and shape model for 1117 Reginita
- Publication Year :
- 2019
- Publisher :
- The Minor Planetary Bulletin, 2019.
-
Abstract
- We present shape and spin axis model for main-belt asteroid 1117 Reginita. The model was achieved with the lightcurve inversion process using combined dense photometric data acquired from nine apparitions between 2003-2018 and sparse data from USNO Flagstaff. Analysis of the resulting data found a sidereal period P = 2.946472 ± 0.000002 hours and two mirrored pole solutions at (λ = 0°, β = 43°) and (λ = 174°, β = 47°) with an uncertainty of ± 5 degrees.<br />peer-reviewed
- Subjects :
- Photometry
Asteroids
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Accession number :
- edsair.od......3549..6f7897fb06a2986bcfe2c8e576a06e99