Astronomers have found evidence of a substellar companion — a low-mass brown dwarf or a giant planet — orbiting Roque 12, a member of the young stellar cluster Pleiades.
An artist’s impression of the Roque 12 binary system in the Pleiades cluster. Image credit: Sci-News.com / NASA / ESA / AURA / Caltech.
The Pleiades is an open star cluster about 440 light-years from Earth in the constellation of Taurus.
The combination of its nearness and youth makes its rapidly cooling brown dwarfs bright and easy to detect.
Also referred to as NPL 36, BPL 172 and EPIC 211090981 in various catalogues, the object has a spectral type of M7.5 and a mass of 63 times that of Jupiter.
Now University of St Andrews astronomer Aleks Scholz and colleagues report the discovery of a deep, singular eclipse in Roque 12.
The event was observed in 2002 with two telescopes at the German Spanish Astronomical Centre on Calar Alto, Almería province, Spain. It was 0.6 mag deep and lasted around 1.3 hours.
“The best explanation for the eclipse is the presence of a companion on an eccentric orbit,” the astronomers said.
They found that the substellar object orbits Roque 12 in less than 70 days.
It has most probably a mass between 10 and 42 Jupiter masses, and therefore could be either a giant planet or a brown dwarf.
“The Roque 12 system could be one of very few known eclipsing binaries in the brown dwarf domain, the first with high eccentricity and long period,” Dr. Scholz and co-authors said.
“A system like that would be uniquely suited to test evolutionary models for substellar objects.”
“We encourage the astronomical community to help hunting for the putative second eclipse of Roque 12.”
Aleks Scholz et al. 2020. The one that got away: A unique eclipse in the young brown dwarf Roque 12. Open Journal of Astrophysics, to be submitted for review; arXiv: 2006.03582