TRAPPIST-1 in the context of "List of multiplanetary systems"

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⭐ Core Definition: TRAPPIST-1

TRAPPIST-1 is an ultra-cool red dwarf star with seven known planets. It lies in the constellation Aquarius approximately 40.66 light-years away from Earth, and it has a surface temperature of about 2,566 K (2,290 °C; 4,160 °F). Its radius is slightly larger than Jupiter's and it has a mass of about 9% of the Sun. It is estimated to be 7.6 billion years old, making it older than the Solar System. The discovery of the star was first published in 2000.

Observations in 2016 from TRAPPIST–South (Transiting Planets and Planetesimals Small Telescope project) at La Silla Observatory in Chile and other telescopes led to the discovery of two terrestrial planets in orbit around TRAPPIST-1. In 2017, further analysis of the original observations identified five more terrestrial planets. The seven planets take between 1.5 and 19 days to orbit the star in circular orbits. They are all likely tidally locked to TRAPPIST-1, and it is believed that each planet is in permanent day on one side and permanent night on the other. Their masses are comparable to that of Earth and they all lie in the same plane; seen from Earth, they pass in front of the star. This placement allowed the planets to be detected: when they pass in front of the star, its apparent magnitude dims.

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👉 TRAPPIST-1 in the context of List of multiplanetary systems

From the total of 4,490 stars known to have exoplanets (as of October 2, 2025), there are a total of 1,017 known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar System. This list includes systems with at least three confirmed planets or two confirmed planets where additional candidates have been proposed. The stars with the most confirmed planets are the Sun (the Solar System's star) and Kepler-90, with eight confirmed planets each, followed by TRAPPIST-1 with seven planets.

The 1,013 multiplanetary systems are listed below according to the star's distance from Earth. Proxima Centauri, the closest star to the Solar System, has at least two planets (the confirmed b, d and the disputed c). The nearest system with four or more confirmed planets is Barnard Star, with four known. The farthest confirmed system with two or more planets is OGLE-2012-BLG-0026L, at 13,300 light-years (4,100 pc) away.

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TRAPPIST-1 in the context of ASTELCO

The company ASTELCO Systems is a manufacturer of telescopes, telescope control systems, domes/enclosures and related technology for professional astronomical research or public use. ASTELCO is located in Sauerlach near Munich and was founded in 2004.

The company built the telescope and mount of the TRAPPIST Telescopes, famous for the discovery of the TRAPPIST-1 system, a red dwarf with seven terrestrial planets. The company also built the telescopes and mounts for the SPECULOOS Southern and Northern Observatory, which are searching for terrestrial planets around ultracool dwarfs and brown dwarfs in the habitable zone. Other projects include the 60 cm Robotic Telescope BOOTES-5 in Mexico, the COATLI robotic 50 cm telescope in Sierra San Pedro Mártir and the prototype for ESO VLT Laser Guide Star Telescope.

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TRAPPIST-1 in the context of Ultra-cool dwarf

An ultra-cool dwarf is a stellar or sub-stellar object that has an effective temperature lower than 2,700 K (2,430 °C; 4,400 °F). This category of dwarf stars was introduced in 1997 by J. Davy Kirkpatrick, Todd J. Henry, and Michael J. Irwin. It originally included very low mass M-dwarf stars with spectral types of M7 but was later expanded to encompass stars ranging from the coldest known to brown dwarfs as cool as spectral type T6.5. Altogether, ultra-cool dwarfs represent about 15% of the astronomical objects in the stellar neighborhood of the Sun. One of the best known examples is TRAPPIST-1.

Models of the formation of planets suggest that due to their low masses and the small size of their proto-planetary disks, these stars could host a relatively abundant population of terrestrial planets ranging from Mercury-sized to Earth-sized bodies, rather than a population of super-Earths and Jupiter-massed planets. The discovery of the TRAPPIST-1 planetary system, consisting of seven Earth-sized planets, would appear to validate this accretion model.

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