Modeling giant extrasolar ring systems in eclipse and the case of J1407b: sculpting by exomoons?

Abstract

The light curve of 1SWASP J140747.93-394542.6, a $\sim$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. 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. 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 $100M_{Moon}$. The ring system has one clearly defined gap at 0.4 AU (61 million km), which we hypothesize is being cleared out by a $<0.8M_{\oplus }$ 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.

13 pages, 6 figures, 3 tables. Accepted for publication in ApJ. Data and computer code for model at: http://github.com/mkenworthy/exorings

References in corpus (9)

• The fast spin-rotation of a young extrasolar planet
• The first WASP public data release
• On the age of the $\beta$ Pictoris moving group
• A ring system detected around the Centaur (10199) Chariklo
• In the Shadow of the Transiting Disk: Imaging epsilon Aurigae in Eclipse
• The Orbit and Occultations of KH 15D
• The Gemini NICI Planet-Finding Campaign: The Orbit of the Young Exoplanet beta Pictoris b
• Mass and period limits on the ringed companion transiting the young star J1407
• OGLE-BLG182.1.162852: An Eclipsing Binary with a Circumstellar Disk

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