| Download | - View final version: OSSOS. XXIII. 2013 VZ₇₀ and the temporary coorbitals of the giant planets (PDF, 1.3 MiB)
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| DOI | Resolve DOI: https://doi.org/10.3847/PSJ/ac1c6b |
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| Author | Search for: Alexandersen, MikeORCID identifier: https://orcid.org/0000-0003-4143-8589; Search for: Greenstreet, SarahORCID identifier: https://orcid.org/0000-0002-4439-1539; Search for: Gladman, Brett J.ORCID identifier: https://orcid.org/0000-0002-0283-2260; Search for: Bannister, Michele T.ORCID identifier: https://orcid.org/0000-0003-3257-4490; Search for: Chen, Ying-TungORCID identifier: https://orcid.org/0000-0001-7244-6069; Search for: Gwyn, Stephen D. J.1ORCID identifier: https://orcid.org/0000-0001-8221-8406; Search for: Kavelaars, JJ1ORCID identifier: https://orcid.org/0000-0001-7032-5255; Search for: Petit, Jean-MarcORCID identifier: https://orcid.org/0000-0003-0407-2266; Search for: Volk, KathrynORCID identifier: https://orcid.org/0000-0001-8736-236X; Search for: Lehner, Matthew J.ORCID identifier: https://orcid.org/0000-0003-4077-0985; Search for: Wang, Shiang-YuORCID identifier: https://orcid.org/0000-0001-6491-1901 |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Funder | Search for: Herzberg Astronomy and Astrophysics |
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| Format | Text, Article |
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| Physical description | 11 p. |
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| Subject | Kuiper belt; trans-Neptunian objects; resonant Kuiper belt objects; centaur group; small Solar System bodies; Trojan asteroids; Jupiter trojans; Neptune trojans; scattered disk objects; orbital resonances; asteroid dynamics; planetary dynamics |
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| Abstract | We present the discovery of 2013 VZ₇₀, the first known horseshoe coorbital companion of Saturn. Observed by the Outer Solar System Origins Survey for 4.5 yr, the orbit of 2013 VZ₇₀ is determined to high precision, revealing that it currently is in “horseshoe” libration with the planet. This coorbital motion will last at least thousands of years but ends ∼10 kyr from now; 2013 VZ₇₀ is thus another example of the already-known “transient coorbital” populations of the giant planets, with this being the first known prograde example for Saturn (temporary retrograde coorbitals are known for Jupiter and Saturn). We present a theoretical steady-state model of the scattering population of trans-Neptunian origin in the giant planet region (2–34 au), including the temporary coorbital populations of the four giant planets. We expose this model to observational biases using survey simulations in order to compare the model to the real detections made by a set of well-characterized outer solar system surveys. While the observed number of coorbitals relative to the scattering population is higher than predicted, we show that the number of observed transient coorbitals of each giant planet relative to each other is consistent with a trans-Neptunian source. |
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| Publication date | 2021-10-13 |
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| Publisher | IOP |
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| Licence | |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 2e21afc4-ee70-4f3c-acce-7715d5bab80e |
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| Record created | 2022-11-01 |
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| Record modified | 2022-11-01 |
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