Three fast-rotating Jovian Trojans identified by TESS set new population density limits Article Swipe
YOU?
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· 2025
· Open Access
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· DOI: https://doi.org/10.48550/arxiv.2501.18440
Here we report on the identification of the three fastest rotating Jovian Trojans with reliable population assignment, using light curve data from the Transiting Exoplanet Satellite Survey mission, also confirmed by Zwicky Transient Facility data. For two of our targets the rotation periods are moderately below the previously accepted ~5 h Jovian Trojan breakup limit (4.26 and 4.75 h), however, the rotation period of (13383) was found to be P = 2.926 h, leading to a density estimate of $ρ$ $\approx$ 1.6 $g cm^{-3}$, higher than the generally accepted $\leq$ 1 $g cm^{-3}$ density limit of Jovian Trojans. If associated with lower densities, this rotation rate requires considerable cohesion in the order of a few kPa. The relatively high albedo (pV $\approx$ 0.11) and fast rotation suggest that (13383) may have undergone an energetic collision that spun up the body and exposed bright material to the surface.
Related Topics
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2501.18440
- https://arxiv.org/pdf/2501.18440
- OA Status
- green
- Related Works
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- OpenAlex ID
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Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W4407012517Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.48550/arxiv.2501.18440Digital Object Identifier
- Title
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Three fast-rotating Jovian Trojans identified by TESS set new population density limitsWork title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2025Year of publication
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2025-01-30Full publication date if available
- Authors
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Csaba Kiss, Nóra Takács, Csilla Kalup, Róbert Szakáts, L. Molnár, E. Plachy, K. Sárneczky, R. Szabó, Gyula M. Szabó, Attila Bódi, András PálList of authors in order
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https://arxiv.org/abs/2501.18440Publisher landing page
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https://arxiv.org/pdf/2501.18440Direct link to full text PDF
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YesWhether a free full text is available
- OA status
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greenOpen access status per OpenAlex
- OA URL
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https://arxiv.org/pdf/2501.18440Direct OA link when available
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Jovian, Set (abstract data type), Population, Astronomy, Astrobiology, Physics, Astrophysics, Computer science, Planet, Sociology, Demography, Saturn, Programming languageTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.suggest | 126 |
| abstract_inverted_index.targets | 39 |
| abstract_inverted_index.Facility | 33 |
| abstract_inverted_index.Trojans. | 97 |
| abstract_inverted_index.accepted | 48, 88 |
| abstract_inverted_index.cm^{-3}$ | 92 |
| abstract_inverted_index.cohesion | 108 |
| abstract_inverted_index.estimate | 77 |
| abstract_inverted_index.however, | 59 |
| abstract_inverted_index.material | 143 |
| abstract_inverted_index.mission, | 27 |
| abstract_inverted_index.reliable | 14 |
| abstract_inverted_index.requires | 106 |
| abstract_inverted_index.rotating | 10 |
| abstract_inverted_index.rotation | 41, 61, 104, 125 |
| abstract_inverted_index.surface. | 146 |
| abstract_inverted_index.$\approx$ | 80, 121 |
| abstract_inverted_index.Exoplanet | 24 |
| abstract_inverted_index.Satellite | 25 |
| abstract_inverted_index.Transient | 32 |
| abstract_inverted_index.cm^{-3}$, | 83 |
| abstract_inverted_index.collision | 134 |
| abstract_inverted_index.confirmed | 29 |
| abstract_inverted_index.energetic | 133 |
| abstract_inverted_index.generally | 87 |
| abstract_inverted_index.undergone | 131 |
| abstract_inverted_index.Transiting | 23 |
| abstract_inverted_index.associated | 99 |
| abstract_inverted_index.densities, | 102 |
| abstract_inverted_index.moderately | 44 |
| abstract_inverted_index.population | 15 |
| abstract_inverted_index.previously | 47 |
| abstract_inverted_index.relatively | 117 |
| abstract_inverted_index.assignment, | 16 |
| abstract_inverted_index.considerable | 107 |
| abstract_inverted_index.identification | 5 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 11 |
| citation_normalized_percentile |