Tau Herculids 2022 from the McDonald Observatory, Texas -- a progress report
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arXiv
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| Main Authors: | , , , , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866914771379421184 |
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| author | Szabó, Norton Olivér Igaz, Antal Kiss, László L. Rózsahegyi, Márton Sárneczky, Krisztián Csák, Balázs Deme, Lívia Vinkó, József |
| author_facet | Szabó, Norton Olivér Igaz, Antal Kiss, László L. Rózsahegyi, Márton Sárneczky, Krisztián Csák, Balázs Deme, Lívia Vinkó, József |
| contents | As part of an intensive effort to observe the predicted 2022 Tau Herculids outburst, we recorded almost 800 individual meteor streaks on May 30th and 31st, 2022, using a high-sensitivity Sony~$α$7 camera. The video recordings were obtained under perfect conditions at the McDonald Observatory, Texas, USA. The meteor sample is dominated by the predicted Tau Herculids shower, however, we also noted significant activity of sporadic meteors and other possible weak showers. We found that the time of the maximum activity matched very well the predictions, while we note the large fraction of faint meteors that were not detectable visually. We determined the radiant, and the time evolution of the activities and currently we are working on the determination of the brightness statistics. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2404_17007 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Tau Herculids 2022 from the McDonald Observatory, Texas -- a progress report Szabó, Norton Olivér Igaz, Antal Kiss, László L. Rózsahegyi, Márton Sárneczky, Krisztián Csák, Balázs Deme, Lívia Vinkó, József Earth and Planetary Astrophysics As part of an intensive effort to observe the predicted 2022 Tau Herculids outburst, we recorded almost 800 individual meteor streaks on May 30th and 31st, 2022, using a high-sensitivity Sony~$α$7 camera. The video recordings were obtained under perfect conditions at the McDonald Observatory, Texas, USA. The meteor sample is dominated by the predicted Tau Herculids shower, however, we also noted significant activity of sporadic meteors and other possible weak showers. We found that the time of the maximum activity matched very well the predictions, while we note the large fraction of faint meteors that were not detectable visually. We determined the radiant, and the time evolution of the activities and currently we are working on the determination of the brightness statistics. |
| title | Tau Herculids 2022 from the McDonald Observatory, Texas -- a progress report |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2404.17007 |