Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866
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 dis...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
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De Gruyter
2023-08-01
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| Series: | Open Astronomy |
| Subjects: | |
| Online Access: | https://doi.org/10.1515/astro-2022-0227 |
| _version_ | 1797736208739074048 |
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| author | Eglitis Ilgmars Kristers Nagainis |
| author_facet | Eglitis Ilgmars Kristers Nagainis |
| author_sort | Eglitis Ilgmars |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-03-12T13:09:22Z |
| format | Article |
| id | doaj.art-7b25d5d387244e2caa138aeb64561808 |
| institution | Directory Open Access Journal |
| issn | 2543-6376 |
| language | English |
| last_indexed | 2024-03-12T13:09:22Z |
| publishDate | 2023-08-01 |
| publisher | De Gruyter |
| record_format | Article |
| series | Open Astronomy |
| spelling | doaj.art-7b25d5d387244e2caa138aeb645618082023-08-28T06:15:30ZengDe GruyterOpen Astronomy2543-63762023-08-013212276810.1515/astro-2022-0227Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866Eglitis Ilgmars0Kristers Nagainis1Institute of Astronomy, University of Latvia, Riga, LV-1586, LatviaInstitute of Astronomy, University of Latvia, Riga, LV-1586, LatviaThe 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.https://doi.org/10.1515/astro-2022-0227main belt asteroidslight curverotation period |
| spellingShingle | Eglitis Ilgmars Kristers Nagainis Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 Open Astronomy main belt asteroids light curve rotation period |
| title | Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 |
| title_full | Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 |
| title_fullStr | Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 |
| title_full_unstemmed | Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 |
| title_short | Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866 |
| title_sort | light curve analysis of main belt asteroids 4747 5255 11411 15433 17866 |
| topic | main belt asteroids light curve rotation period |
| url | https://doi.org/10.1515/astro-2022-0227 |
| work_keys_str_mv | AT eglitisilgmars lightcurveanalysisofmainbeltasteroids47475255114111543317866 AT kristersnagainis lightcurveanalysisofmainbeltasteroids47475255114111543317866 |