Scientists have discovered six new exoplanets, taking the total to 5,502. With advancements in technology, the field of exoplanet research has grown exponentially since the first discovery in 1992, and upcoming instruments promise even deeper insights. On August 24, 2023, over three decades after
This planet was discovered using the transit method.
Completes an orbit every 1.52 days, meaning it is very close to its star. While it is extremely rare for giant planets like this to orbit so closely to Sun-like stars, it is even rarer for them to orbit M-dwarf stars as is the case here.c is a giant protoplanet that orbits a very young star. This star still has its protoplanetary disk, which is a rotating disc of gas and dust that can surround a young star.Was found carving spiral arms into its star’s protoplanetary disk.
NASA’s Transiting Exoplanet Survey Satellite launched in 2018 and has identified thousands of exoplanet candidates and confirmed over 320 planets.have also been used to discover and study exoplanets.is set to launch in May 2027. Roman will be carrying a technology demonstration called the Roman Coronagraph Instrument. This coronagraph will work by using a series of complex masks and mirrors to distort the light coming from far-away stars.
With the success of the Roman Coronagraph Instrument, NASA could push the envelope even further with is a concept for the mission the Habitable Worlds Observatory, which would search for “signatures of life on planets outside of our solar system,”These six exoplanets were discovered by different teams as part of five separate studies:“An M dwarf accompanied by a close-in giant orbiter with SPECULOOS” by Amaury H M J Triaud, Georgina Dransfield, Taiki Kagetani, Mathilde Timmermans, Norio Narita,...
“Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095” by F. Murgas, A. Castro-González, E. Pallé, F. J. Pozuelos, S. Millholland, O. Foo, J. Korth, E. Marfil, P. J. Amado, J. A. Caballero, J. L. Christiansen, D. R. Ciardi, K. A. Collins, M. Di Sora, A. Fukui, T. Gan, E. J. Gonzales, Th. Henning, E. Herrero, G. Isopi, J. M. Jenkins, J. Lillo-Box, N. Lodieu, R. Luque, F. Mallia, J. C. Morales, G. Morello, N. Narita, J. Orell-Miquel, H. Parviainen, M.
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