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TRAPPIST-1e

TRAPPIST-1e is a rocky, close-to-Earth-sized exoplanet orbiting within the habitable zone around the ultracool dwarf star TRAPPIST-1, located 40.7 light-years away from Earth in the constellation of Aquarius. Astronomers used the transit method to find the exoplanet, a method that measures the dimming of a star when a planet crosses in front of it.

Physical characteristics
Mass, radius, density, composition and temperature TRAPPIST-1e was detected with the transit method, where the planet blocked a small percentage of its host star's light when passing between it and Earth. This allowed scientists to accurately determine the planet's radius at , with a small uncertainty of about . Transit-timing variations and advanced computer simulations helped constrain the planet's mass, which turned out to be , or about 15% less massive than Venus. it is Earth's greenhouse gases that raise its surface temperatures to the levels we experience. If TRAPPIST-1e has a thick atmosphere, its surface could be much warmer than its equilibrium temperature. Host star The planet orbits an (late M-type) ultracool dwarf star named TRAPPIST-1. The star has a mass of 0.089 —near the boundary between a brown dwarf and low-mass star—and a radius of 0.121 . It has a temperature of and is 7.6 billion years old. In comparison, the Sun is 4.6 billion years old and has a temperature of . The star is metal-rich, with a metallicity ([Fe/H]) of 0.04, or 109% the solar amount. This is particularly odd as such low-mass stars near the boundary between brown dwarfs and hydrogen-fusing stars should be expected to have considerably less metal content than the Sun. Its luminosity () is 0.0522% of that of the Sun. The star's apparent magnitude, or how bright it appears from Earth's perspective, is 18.8. Therefore, it is far too dim to be seen with the naked eye. Orbit TRAPPIST-1e orbits its host star quite closely. One full revolution around TRAPPIST-1 takes only 6.099 Earth days (~146 hours) to complete. It orbits at a distance of , or just under 3% the separation between Earth and the Sun. For comparison, the closest planet in the Solar System, Mercury, takes 88 days to orbit the Sun at a distance of . Despite its close proximity to its host star, TRAPPIST-1e gets only about 60% the starlight that Earth gets from the Sun due to the low luminosity of its star. The star would cover an angular diameter of about 2.17 degrees from the surface of the planet, and so would appear about four times larger than the Sun does from Earth. Atmosphere Transit observations with James Webb Space Telescope suggested no clear answer about the existence of an atmosphere, but it did rule out many atmosphere scenarios. See the "Habitability" studies below. ==Habitability==
Habitability
The exoplanet was announced to be orbiting within the habitable zone of its parent star, the region where, with the correct conditions and atmospheric properties, liquid water may exist on the surface of the planet. TRAPPIST-1e has a radius of around 0.91 , so it is likely a rocky planet. Its host star is a red ultracool dwarf, with only about 8% of the mass of the Sun (close to the boundary between brown dwarfs and hydrogen-fusing stars). As a result, stars like TRAPPIST-1 have the potential to remain stable for up to 12 trillion years, which is over 2,000 times longer than the Sun. Because of this ability to live for such a long period of time, it is likely TRAPPIST-1 will be one of the last remaining stars in the Universe, when the gas needed to form new stars will be exhausted, and the existing stars begin to die off. 2018 studies Despite being likely tidally locked—meaning one hemisphere permanently faces the star while the other does not—which may reduce the habitability of the planet, more detailed studies of TRAPPIST-1e and the other TRAPPIST-1 planets released in 2018 determined that the planet is in fact one of the most Earth-sized worlds found, with 91% the radius, 77% the mass, 102.4% the density (5.65 g/cm3), and 93% the surface gravity. TRAPPIST-1e is confirmed to be a terrestrial planet with a solid, rocky surface. It is cool enough for liquid water to pool on the surface, but not so cold that it would freeze like on TRAPPIST-1f, g, and h. to , == Discovery ==
Discovery
A team of astronomers headed by Michaël Gillon used the TRAPPIST (Transiting Planets and Planetesimals Small Telescope) telescope at the La Silla Observatory in the Atacama Desert, Chile, The team made their observations from September–December 2015 and published its findings in the May 2016 issue of the journal Nature. == Gallery ==
Gallery
Videos File:PIA21427 - TRAPPIST-1 Planetary Orbits and Transits.ogg|Video (01:32) – Artistic representation of TRAPPIST-1 exoplanets transiting their host star File:PIA21468 - TRAPPIST-1 Planets - Flyaround Animation.ogg|Video (01:10) – Fly-around animation of the planets of the TRAPPIST-1 system, including TRAPPIST-1e ==See also==
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