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| Auteurs principaux: | , , , , |
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| Format: | Preprint |
| Publié: |
2023
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| Sujets: | |
| Accès en ligne: | https://arxiv.org/abs/2310.14193 |
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| _version_ | 1866914677017018368 |
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| author | Wakjira, Hawi Yohanis Mosunova, D. A. Postnikova, E. S. Chupina, N. V. Vereshchagin, S. V. |
| author_facet | Wakjira, Hawi Yohanis Mosunova, D. A. Postnikova, E. S. Chupina, N. V. Vereshchagin, S. V. |
| contents | We study of possible encounters in past epochs of the open star cluster NGC 1977 with host stars. For this purpose, the age of the cluster was determined based on our catalog data. Stars with planetary systems were selected from the NASA Archive. The age of the cluster was determined using the color - absolute magnitude diagram and the isochron system. By extending the track of the movement of the cluster and stars in past epochs, 10 Myr. The time of the maximum approach 32 pc of the host star with planetary system TOI-2796 with the NGC 1977 are found. The place of approach in the sky is shown, this point can be considered as the place of appearance of interstellar comets. Thus, the result of our work is that the we found approach of the host star to the cluster entailed effects associated with the gravitational influence of the cluster on the nuclei of comets located in the outer parts of the Oort cloud of the planetary system. The effect of approach on comets is estimated. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2310_14193 |
| institution | arXiv |
| publishDate | 2023 |
| record_format | arxiv |
| spellingShingle | Approach of the NGC 1977 star cluster to the TOI-2796 host star Wakjira, Hawi Yohanis Mosunova, D. A. Postnikova, E. S. Chupina, N. V. Vereshchagin, S. V. Astrophysics of Galaxies We study of possible encounters in past epochs of the open star cluster NGC 1977 with host stars. For this purpose, the age of the cluster was determined based on our catalog data. Stars with planetary systems were selected from the NASA Archive. The age of the cluster was determined using the color - absolute magnitude diagram and the isochron system. By extending the track of the movement of the cluster and stars in past epochs, 10 Myr. The time of the maximum approach 32 pc of the host star with planetary system TOI-2796 with the NGC 1977 are found. The place of approach in the sky is shown, this point can be considered as the place of appearance of interstellar comets. Thus, the result of our work is that the we found approach of the host star to the cluster entailed effects associated with the gravitational influence of the cluster on the nuclei of comets located in the outer parts of the Oort cloud of the planetary system. The effect of approach on comets is estimated. |
| title | Approach of the NGC 1977 star cluster to the TOI-2796 host star |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2310.14193 |