Abstract
The main belt asteroids 4747, 5255, 11411, 15433, and 17866 were studied at the Baldone Astrophysical Observatory in the time span range 2018-2022. The obtained light curve data together with published Minor Planet Center data are analyzed with Fourier series, Lomb-Scargle periodogram, and phase dispersion minimization methods. A plan of analysis is given. The results computed from different observatories' data are compared, and mean-weighted periods are obtained.
| Original language | English |
|---|---|
| Article number | 20220227 |
| Pages (from-to) | 1-9 |
| Journal | Baltic Astronomy |
| Volume | 32 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jan 2023 |
OECD Field of Science
- 1.3 Physical Sciences
Keywords
- light curve
- main belt asteroids
- rotation period
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