DF.3.03 — A Transiting Extrasolar Ring System: Indirect Evidence for Exosatellite Formation?

Date & Time

Aug 7th at 4:40 PM until 5:00 PM




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Author(s): Eric E Mamajek1

Institution(s): 1. University of Rochester

The young star 1SWASP J140747.93-394542.6 ("J1407") is a 16-million-year-old pre-main sequence star in Sco-Cen, the nearest OB association. In 2012, we reported that time series photometry data from the SuperWASP and ASAS programs show that the star J1407 had a series of extremely complex eclipses over a two-month span in early 2007, with ~95% of the star's light blocked out near minimum. The star J1407 shows no evidence for accretion nor any circumstellar disk blueward of the WISE4 IR band. The eclipses have been modeled as due to a set of (at least 30) concentric dust rings with total mass of approximately 1 Earth mass, with radii ranging from approximately 30-90 million km. There is at least one very clean gap in the ring system at radius ~0.4 AU which may be cleared by a sub-Earth-size exosatellite. While popularly described as a "super-Saturn" with "rings", given the age of the system, and the size and inferred mass of the rings, it seems plausible that we are detecting a circumplanetary (or protoexosatellite) disk. The disk would appear to fill a non-negligible fraction of its Hill radius, and the appearance of gaps would suggest that system is in the process of spawning exosatellites. I will summarize the current knowledge about the J1407 system: including archival and on-going photometric searches for additional eclipses, imaging and Doppler constraints on the companion of the ringed companion, and future prospects for discovering eclipsing disks girding young exoplanets and substellar objects.