Recurrent Cometary Activity Discovered on Quasi-Hilda Jupiter Family Comet 362P/(457175) 2008 GO98
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| Format: | Preprint |
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2025
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| _version_ | 1866918103120609280 |
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| author | Farrell, Kennedy A. Chandler, Colin Orion Trujillo, Chadwick A. Oldroyd, William J. DeSpain, Jarod A. Magbanua, Mark Jesus Mendoza Frissell, Maxwell K. Stone, Phineas |
| author_facet | Farrell, Kennedy A. Chandler, Colin Orion Trujillo, Chadwick A. Oldroyd, William J. DeSpain, Jarod A. Magbanua, Mark Jesus Mendoza Frissell, Maxwell K. Stone, Phineas |
| contents | We report the discovery of recurrent activity on quasi-Hilda comet (QHC) 362P/(457175) 2008 GO98. The first activity epoch was discovered during the perihelion passage of 362P. The first activity epoch was discovered during the perihelion in 2016 (Garcia-Migani & Gil-Hutton 2018), so we were motivated to observe it for recurrent cometary activity near its next perihelion passage (UT 2024 July 20). We obtained observations with the Lowell Discovery Telescope (LDT), the Astrophysical Research Consortium (ARC) telescope, and the Vatican Advanced Technology Telescope (VATT) and identified a second activity epoch when 362P had a true anomaly (v) as early as 318.1 deg. We conducted archival searches of numerous repositories and identified images obtained with Canada-France-Hawaii Telescope (CFHT) MegaCam, Dark Energy Camera (DECam), Pan-STARRS 1, SkyMapper, Zwicky Transient Facility (ZTF), and Las Cumbres Observatory Global Telescope (LCOGT) network data. Using these data, we identified activity from a previously unreported timespan, and we did not detect activity when 362P was away from perihelion, specifically 83 deg < v < 318 deg. Detection of activity near perihelion and absence of activity away from perihelion suggest thermally-driven activity and volatile sublimation. Our dynamical simulations suggest 362P is a QHC and it will remain in a combined Jupiter-family comet (JFC) and quasi-Hilda orbit over the next 1 kyr, though it will become increasingly chaotic nearing the end of this timeframe. Our backward simulations suggest 362P may have migrated from the orbit of a Long Period Comet (~53%) or Centaur (~32%), otherwise it remained a JFC (~15%) over the previous 100 kyr. We recommend additional telescope observations from the community as 362P continues outbound from its perihelion on UT 2024 July 20, as well as continued observations for a third activity epoch. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2507_17808 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Recurrent Cometary Activity Discovered on Quasi-Hilda Jupiter Family Comet 362P/(457175) 2008 GO98 Farrell, Kennedy A. Chandler, Colin Orion Trujillo, Chadwick A. Oldroyd, William J. DeSpain, Jarod A. Magbanua, Mark Jesus Mendoza Frissell, Maxwell K. Stone, Phineas Earth and Planetary Astrophysics We report the discovery of recurrent activity on quasi-Hilda comet (QHC) 362P/(457175) 2008 GO98. The first activity epoch was discovered during the perihelion passage of 362P. The first activity epoch was discovered during the perihelion in 2016 (Garcia-Migani & Gil-Hutton 2018), so we were motivated to observe it for recurrent cometary activity near its next perihelion passage (UT 2024 July 20). We obtained observations with the Lowell Discovery Telescope (LDT), the Astrophysical Research Consortium (ARC) telescope, and the Vatican Advanced Technology Telescope (VATT) and identified a second activity epoch when 362P had a true anomaly (v) as early as 318.1 deg. We conducted archival searches of numerous repositories and identified images obtained with Canada-France-Hawaii Telescope (CFHT) MegaCam, Dark Energy Camera (DECam), Pan-STARRS 1, SkyMapper, Zwicky Transient Facility (ZTF), and Las Cumbres Observatory Global Telescope (LCOGT) network data. Using these data, we identified activity from a previously unreported timespan, and we did not detect activity when 362P was away from perihelion, specifically 83 deg < v < 318 deg. Detection of activity near perihelion and absence of activity away from perihelion suggest thermally-driven activity and volatile sublimation. Our dynamical simulations suggest 362P is a QHC and it will remain in a combined Jupiter-family comet (JFC) and quasi-Hilda orbit over the next 1 kyr, though it will become increasingly chaotic nearing the end of this timeframe. Our backward simulations suggest 362P may have migrated from the orbit of a Long Period Comet (~53%) or Centaur (~32%), otherwise it remained a JFC (~15%) over the previous 100 kyr. We recommend additional telescope observations from the community as 362P continues outbound from its perihelion on UT 2024 July 20, as well as continued observations for a third activity epoch. |
| title | Recurrent Cometary Activity Discovered on Quasi-Hilda Jupiter Family Comet 362P/(457175) 2008 GO98 |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2507.17808 |