Astronomers Pinpoint Rare Binary Brown Dwarf
Arthur T Knackerbracket has found the following story:
Astronomers working on 'first light' results from a newly commissioned telescope in Chile made a chance discovery that led to the identification of a rare eclipsing binary brown dwarf system.
The discovery, published today in Nature Astronomy, was led by an international team of researchers, including scientists at the University of Birmingham, working on the SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) project. SPECULOOS involves the University of Birmingham in collaboration with the University of Liige, the University of Cambridge, the University of Bern, the Institute of Astrophysics of the Canaries, the Massachusetts Institute of Technology, and other partner institutions.
SPECULOOS' mission is to investigate planets surrounding ultra-cool dwarfs, a category that includes the smallest stars that exist, as well as objects called 'brown dwarfs'. Brown dwarfs are 'sub-stellar' objects, meaning they have less mass than a star but more than a planet. Brown dwarfs are unable to sustain the fusion of hydrogen into helium, a process that powers the light from normal stars like the Sun.
Astronomers predict that these ultra-cool dwarfs should host large populations of close-by, potentially habitable rocky planets, offering a wealth of opportunity to explore a diversity of atmospheres and climates. An example is the 7-planet system TRAPPIST-1, which was discovered by members of the same team.
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Amaury H. M. J. Triaud, Adam J. Burgasser, Artem Burdanov, Vedad Kunovac HodA3/4iA, Roi Alonso, Daniella Bardalez Gagliuffi, Laetitia Delrez, Brice-Olivier Demory, Julien de Wit, Elsa Ducrot, Frederic V. Hessman, Tim-Oliver Husser, Emmanuil Jehin, Peter P. Pedersen, Didier Queloz, James McCormac, Catriona Murray, Daniel Sebastian, Samantha Thompson, Vali(C)rie Van Grootel, Michail Gillon. An eclipsing substellar binary in a young triple system discovered by SPECULOOS[$]. Nature Astronomy, 2020; DOI: 10.1038/s41550-020-1018-2
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