Please use this identifier to cite or link to this item:
https://www.um.edu.mt/library/oar/handle/123456789/45935| Title: | Spin axis and shape model for 1117 Reginita |
| Authors: | Franco, Lorenzo Marchini, Alessandro Galdies, Charles Grech, Winston |
| Keywords: | Photometry Asteroids |
| Issue Date: | 2019 |
| Publisher: | The Minor Planetary Bulletin |
| Citation: | Franco, L., Marchini, A., Galdies, C., Brincat, S. M., & Grech, W. (2019). Spin axis and shape model for 1117 Reginita. Minor Planet Bulletin, 46, 269-271. |
| 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. |
| URI: | https://www.um.edu.mt/library/oar/handle/123456789/45935 |
| Appears in Collections: | Scholarly Works - InsESEMP |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Franco, Marchini, Galdies, Grech (2019) MPB 46(3) - 269-271.pdf | 805.39 kB | Adobe PDF | View/Open |
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