paper

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)

Cited by in corpus (3)