FOSSIL: I. The Spin Rate Limit of Jupiter Trojans
Chan-Kao Chang, Ying-Tung Chen, Wesley C. Fraser, Fumi Yoshida,, Matthew J. Lehner, Shiang-Yu Wang, JJ Kavelaars, Rosemary E. Pike, Mike, Alexandersen, Takashi Ito, Young-Jun Choi, A. Paula Granados Contreras,, Youngmin JeongAhn, Jianghui Ji, Myung-Jin Kim, Samantha M. Lawler

TL;DR
This study measures the rotation periods of small Jupiter Trojans, revealing a spin rate limit near 4 hours and suggesting a rubble-pile structure with a specific bulk density, expanding understanding of their physical properties.
Contribution
First reported rotation periods for JTs smaller than 10 km, establishing a lower spin rate limit and implications for their internal structure.
Findings
Rotation period lower limit near 4 hours.
Bulk density of 0.9 g/cm³ needed for structural integrity.
First periods measured for JTs with D < 10 km.
Abstract
Rotation periods of 53 small (diameters km) Jupiter Trojans (JTs) were derived using the high-cadence light curves obtained by the FOSSIL phase I survey, a Subaru/Hyper Suprime-Cam intensive program. These are the first reported periods measured for JTs with km. We found a lower limit of the rotation period near 4 hr, instead of the previously published result of 5 hr (Ryan et al. 2017; Szabo et al. 2017, 2020) found for larger JTs. Assuming a rubble-pile structure for JTs, a bulk density of 0.9 gcm is required to withstand this spin rate limit, consistent with the value gcm (Marchis et al. 2006; Mueller et al. 2010; Buie et al. 2015; Berthier et al. 2020) derived from the binary JT system, (617) Patroclus-Menoetius system.
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies · Stellar, planetary, and galactic studies
