Centaur 29P/Schwassmann-Wachmann 1 and its near-nucleus environment from a stellar occultation
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| Main Authors: | , , , , , , , , , , , |
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| Format: | Preprint |
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2024
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| author | Pereira, C. L. Braga-Ribas, F. Sicardy, B. Morgado, B. E. Ortiz, J. L. Assafin, M. Miles, R. Desmars, J. Camargo, J. I. B. Benedetti-Rossi, G. Kretlow, M. Vieira-Martins, R. |
| author_facet | Pereira, C. L. Braga-Ribas, F. Sicardy, B. Morgado, B. E. Ortiz, J. L. Assafin, M. Miles, R. Desmars, J. Camargo, J. I. B. Benedetti-Rossi, G. Kretlow, M. Vieira-Martins, R. |
| contents | Comets offer valuable insights into the early Solar System's conditions and processes. Stellar occultations enables detailed study of cometary nuclei typically hidden by their coma. Observing the star's light passing through the coma helps infer dust's optical depth near the nucleus and determine dust opacity detection limits. 29P/Schwassmann-Wachmann 1, a Centaur with a diameter of approximately 60 km, lies in a region transitioning from Centaurs to Jupiter-Family comets. Our study presents the first-ever observed occultation by 29P, allowing in the future a more refined orbit and thus better predictions for other occultations. The light curve reveals a solid-body detection lasting $3.65\pm0.05$ seconds, corresponding to a chord length of approximately 54 km. This provides a lower limit for the object's radius, measured at $27.0\pm0.7$ km. We identified features on both sides of the main-body occultation around 1,700 km from the nucleus in the sky plane for which upper limits on apparent opacity and equivalent width were determined. Gradual dimming within 23 km of the nucleus during ingress only is interpreted as a localised dust cloud/jet above the surface, with an optical depth of approximately $τ\sim 0.18$. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2411_16358 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Centaur 29P/Schwassmann-Wachmann 1 and its near-nucleus environment from a stellar occultation Pereira, C. L. Braga-Ribas, F. Sicardy, B. Morgado, B. E. Ortiz, J. L. Assafin, M. Miles, R. Desmars, J. Camargo, J. I. B. Benedetti-Rossi, G. Kretlow, M. Vieira-Martins, R. Earth and Planetary Astrophysics Comets offer valuable insights into the early Solar System's conditions and processes. Stellar occultations enables detailed study of cometary nuclei typically hidden by their coma. Observing the star's light passing through the coma helps infer dust's optical depth near the nucleus and determine dust opacity detection limits. 29P/Schwassmann-Wachmann 1, a Centaur with a diameter of approximately 60 km, lies in a region transitioning from Centaurs to Jupiter-Family comets. Our study presents the first-ever observed occultation by 29P, allowing in the future a more refined orbit and thus better predictions for other occultations. The light curve reveals a solid-body detection lasting $3.65\pm0.05$ seconds, corresponding to a chord length of approximately 54 km. This provides a lower limit for the object's radius, measured at $27.0\pm0.7$ km. We identified features on both sides of the main-body occultation around 1,700 km from the nucleus in the sky plane for which upper limits on apparent opacity and equivalent width were determined. Gradual dimming within 23 km of the nucleus during ingress only is interpreted as a localised dust cloud/jet above the surface, with an optical depth of approximately $τ\sim 0.18$. |
| title | Centaur 29P/Schwassmann-Wachmann 1 and its near-nucleus environment from a stellar occultation |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2411.16358 |