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Transiting Exoplanet Survey Satellite (TESS) is a space telescope for NASA's Explorer program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission. [6]
Discovered in 2023, TOI-700 e is a terrestrial exoplanet that NASA claims to be an "earth-like" planet, with 95 percent of the Earth’s radius. Discovered by NASA's TESS (Transitioning Exoplanet Survey Satellite), TOI-700 e has a mass of about 0.818 Earths and takes 27.8 days to orbit once around its star. [ 13 ]
Project 1640: Active 0+ Qatar Exoplanet Survey (QES) Active 9 [31] Search for extraterrestrial intelligence (SETI) Active 0 SOPHIE échelle spectrograph: Active 0+ [32] Spectro-Polarimetric High-Contrast Exoplanet Research (SPHERE) Active 1+ [33] SPECULOOS: Commissioning - Searching 1,200 nearby "Ultra Cool Dwarfs" (M7 and later). Successor to ...
Combined data from Cheops and TESS, or the Transiting Exoplanet Survey Satellite, hinted that the anomaly might be due to something intriguing occurring in the atmosphere above the dayside.
The TKS aims to measure the mass for about 100 exoplanets [2] and has been awarded some of the largest time allocations in the histories of Keck I and APF. [1] The program has four main science themes: [2] the bulk compositions of small planets; dynamical temperatures and system architectures; a larger, more refined sample for future ...
The Next-Generation Transit Survey (NGTS) is a ground-based robotic search for exoplanets. [1] The facility is located at Paranal Observatory in the Atacama Desert in northern Chile, about 2 km from ESO's Very Large Telescope and 0.5 km from the VISTA Survey Telescope. Science operations began in early 2015. [2]
TOI-715 b is a super-Earth exoplanet in the habitable zone of its parent M-type star, TOI-715. [1] [2] [3] The planet is 1.55 times larger than Earth, and is located at 0.083 astronomical units (12,400,000 km) from its star. [4] The planet orbits in the habitable zone of its star and has an equilibrium temperature of 234 K (−39 °C). [4]
TOI-2119 is a binary star system composed of a M-type main sequence star and a brown dwarf, discovered by the Transiting Exoplanet Survey Satellite (TESS) in 2020 and announced in 2022. [7] [5] It became the first example of a brown dwarf orbiting an M-dwarf to have the obliquity of the system measured using the Rossiter–McLaughlin effect. [4]