Multiband photometry of a Patroclus-Menoetius mutual event: Constraints on surface heterogeneity
arXiv:1904.06379 · doi:10.3847/1538-3881/ab18f4
Abstract
We present the first complete multiband observations of a binary asteroid mutual event. We obtained high-cadence, high-signal-to-noise photometry of the UT 2018 April 9 inferior shadowing event in the Jupiter Trojan binary system Patroclus-Menoetius in four Sloan bands , , , and . We use an eclipse lightcurve model to fit for a precise mid-eclipse time and estimate the minimum separation of the two eclipsing components during the event. Our best-fit mid-eclipse time of is 19 minutes later than the prediction of Grundy et al. (2018); the minimum separation between the center of Menoetius' shadow and the center of Patroclus is km slightly larger than the predicted 69.5 km. Using the derived lightcurves, we find no evidence for significant albedo variations or large-scale topographic features on the Earth-facing hemisphere and limb of Patroclus. We also apply the technique of eclipse mapping to place an upper bound of 0.15 mag on wide-scale surface color variability across Patroclus.
5 pages, 3 figures, accepted for publication in AJ
References in corpus (5)
- The Correlated Colors of Transneptunian Binaries
- A hypothesis for the color bimodality of Jupiter Trojans
- Taxonomy of asteroid families among the Jupiter Trojans: Comparison between spectroscopic data and the Sloan Digital Sky Survey colors
- The differing magnitude distributions of the two Jupiter Trojan color populations
- The Upcoming Mutual Event Season for the Patroclus - Menoetius Trojan Binary
Cited by in corpus (3)
- JWST near-infrared spectroscopy of the Lucy Jupiter Trojan flyby targets: Evidence for OH absorption, aliphatic organics, and CO
- 2021 occultations and transits of Linus orbiting (22) Kalliope: I. Polygonal and `cliptracing' algorithm
- Evidence of Possible Spectral Variability in the Patroclus-Menoetius Binary System