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| Main Authors: | , , , , , , , , |
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| Format: | Preprint |
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2026
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2602.04797 |
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| _version_ | 1866918323014336512 |
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| author | Jones, Graham Mauland-Hus, Renate Tveter, Frank Thomas Buckle, Anne Emonet, Sébastien Michelic, Adalbert Smith, Anna Usken, David Thorsen, Steffen |
| author_facet | Jones, Graham Mauland-Hus, Renate Tveter, Frank Thomas Buckle, Anne Emonet, Sébastien Michelic, Adalbert Smith, Anna Usken, David Thorsen, Steffen |
| contents | In a classic 1982 paper in this journal, Jean Meeus used a statistical approach for finding the mean frequency of a total and an annular eclipse of the Sun at a given place on the surface of the Earth. In this current paper we tackle the problem again, taking advantage of the much greater computing power now available. We obtain narrower estimates of once every 373 $\pm$ 7 years for a total eclipse, and once every 226 $\pm$ 4 years for an annular eclipse. In addition, we obtain a result of once every 2.59 $\pm$ 0.02 years for a partial eclipse. We provide further insights into the "latitude effect", showing that solar eclipses occur most frequently around the Arctic and Antarctic Circles. We also show how the gradual shift of aphelion and perihelion with respect to the seasons produces a $\sim$21,000-year cycle in the frequency of eclipses in the Northern and Southern Hemispheres. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_04797 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | The Frequency of Solar Eclipses for a Given Place: A New Approach to a Classic Question Jones, Graham Mauland-Hus, Renate Tveter, Frank Thomas Buckle, Anne Emonet, Sébastien Michelic, Adalbert Smith, Anna Usken, David Thorsen, Steffen Solar and Stellar Astrophysics Earth and Planetary Astrophysics In a classic 1982 paper in this journal, Jean Meeus used a statistical approach for finding the mean frequency of a total and an annular eclipse of the Sun at a given place on the surface of the Earth. In this current paper we tackle the problem again, taking advantage of the much greater computing power now available. We obtain narrower estimates of once every 373 $\pm$ 7 years for a total eclipse, and once every 226 $\pm$ 4 years for an annular eclipse. In addition, we obtain a result of once every 2.59 $\pm$ 0.02 years for a partial eclipse. We provide further insights into the "latitude effect", showing that solar eclipses occur most frequently around the Arctic and Antarctic Circles. We also show how the gradual shift of aphelion and perihelion with respect to the seasons produces a $\sim$21,000-year cycle in the frequency of eclipses in the Northern and Southern Hemispheres. |
| title | The Frequency of Solar Eclipses for a Given Place: A New Approach to a Classic Question |
| topic | Solar and Stellar Astrophysics Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2602.04797 |