really big rings -an extrasolar ring system and exomoon
a tip of the hat to Jim
for those who know what the Roche limit is the paper is on the arXiv
MODELING GIANT EXTRASOLAR RING SYSTEMS IN ECLIPSE AND THE CASE OF J1407B: SCULPTING BY EXOMOONS?
M.A. Kenworthy Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden and E.E. Mamajek Department of Physics and Astronomy, University of Rochester, Rochester, NY 14627-0171, USA
ApJ accepted 2014 Dec 28
The light curve of 1SWASP J140747.93-394542.6, a ∼16 Myr old star in the Sco-Cen OB association, underwent a complex series of deep eclipses that lasted 56 days, centered on April 2007 (Mamajek et al. 2012). This light curve is interpreted as the transit of a giant ring system that is filling up a fraction of the Hill sphere of an unseen secondary companion, J1407b (Mamajek et al. 2012; van Werkhoven et al. 2014; Kenworthy et al. 2015). We fit the light curve with a model of an azimuthally symmetric ring system, including spatial scales down to the temporal limit set by the star’s diameter and relative velocity. The best ring model has 37 rings and extends out to a radius of 0.6 AU (90 million km), and the rings have an estimated total mass on the order of 100MMoon. The ring system has one clearly defined gap at 0.4 AU (61 million km), which we hypothesize is being cleared out by a < 0.8M⊕ exosatellite orbiting around J1407b. This eclipse and model implies that we are seeing a circumplanetary disk undergoing a dynamic transition to an exosatellite-sculpted ring structure and is one of the first seen outside our Solar system.