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- | caption = HIP 65426 b is on the lower left of the image, with the circle representing what Neptune's orbit would look like around the sta | discovery_method = [[Methods of detecting exoplanets#Direct imaging|Direct imaging]] ...12 KB (1,655 words) - 23:55, 15 February 2025
- {{Short description|Red dwarf star with Earth-like planet}} | names = {{odlist | name = SPECULOOS-2 | 2MASS = J04163114-2818526 | LP = 890-9 | ...8 KB (941 words) - 13:56, 31 January 2025
- | discovery_method = [[Methods of detecting exoplanets#Transit photometry|Transit]] ...Astronomical Union|IAU]] |access-date=27 August 2022}}</ref> The approved names, proposed by a team from [[Bahrain]], were announced in June 2023. WASP-121 ...22 KB (2,972 words) - 08:25, 1 March 2025
- |names=CWISE J153429.19-104318.9, [[Wide-field Infrared Survey Explorer|WISEA The brown dwarf is 50 light years from Earth, with a transverse velocity of over 200 km/s – over 25% faster than the next fast ...14 KB (1,981 words) - 17:30, 17 January 2025
- | names = LUH 16,{{r|Mamajek2013}} Luhman–WISE 1,{{r|Mamajek2013}} [[Wide-field Inf ...ch other at a distance of about 3.5 [[astronomical unit]]s{{r|Luhman2013}} with an [[orbital period]] of approximately 26.6 years.<ref name="Bedin2024"/> ...43 KB (6,000 words) - 06:40, 6 February 2025
- {{redirect-distinguish|Space velocity (astronomy)|radial velocity|proper motion|peculiar velocity}} ...ars in the period 1985–2005. Barnard's Star is the star with the highest [[proper motion]].<ref name=Kaler>{{cite web|first=James B.|last=Kaler|url=http://ww ...61 KB (8,592 words) - 01:54, 20 January 2025
- | names ={{abbr|2MUDC|2MASS UltraCool Dwarves catalog}} 12171,{{sfn|Martínez-Rodríg ...Milky Way]].{{sfn|Gargaud|Amils|Quintanilla|Cleaves|2011|loc=Red Dwarf}}}} with seven known [[exoplanet]]s. It lies in the constellation [[Aquarius (conste ...187 KB (25,955 words) - 17:28, 25 February 2025