TRAPPIST

TRAPPIST is controlled from Liège, Belgium, with some autonomous features. It consists of two reflecting robotic telescopes located at the ESO La Silla Observatory (housed in the dome of the retired Swiss T70 telescope) in Chile and at Oukaïmeden Observatory in Morocco. The 60 cm f/8 Ritchey–Chrétien design telescopes and New Technology Mount NTM-500 were built by ASTELCO Systems, a company in Germany. The CCD camera was built by Finger Lakes Instrumentation (USA), providing a 22 x 22 arcminutes field of view. The camera is fitted with a double filter wheel, allowing 12 different filters and one clear position. The telescope condominium is a joint venture between the University of Liège, Belgium, and the Geneva Observatory, Switzerland, and among other tasks, it specializes in searching for comets and exoplanets. In November 2010, it was one of the few telescopes that observed a stellar occultation of the planetary body Eris, revealing that it may be smaller than Pluto, and it helped observe a stellar occultation by Makemake, when it passed in front of the star NOMAD 1181-0235723. The observations of this event showed it lacked a significant atmosphere. A team of astronomers headed by Michaël Gillon, of the Institut d'Astrophysique et Géophysique at the University of Liège in Belgium, used the telescope to observe the ultracool dwarf star 2MASS J23062928-0502285, now also known as TRAPPIST-1. By utilising transit photometry, they discovered seven terrestrial planets, at least three of which were Earth-sized, orbiting the star; the innermost two were found to be tidally locked to their host star while the outermost appears to lie either within the system's habitable zone or just outside of it. The team published its findings in the May 2016 issue of the Nature journal. While TRAPPIST-1 is the only planetary system discovered by TRAPPIST, other planetary systems have been discovered by SPECULOOS and given SPECULOOS-n designations, with TRAPPIST-1 being SPECULOOS-1.