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  2. Epsilon Indi Ab - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Indi_Ab

    Epsilon Indi Ab is a gas giant exoplanet orbiting the star Epsilon Indi A, about 11.9 light-years away in the constellation of Indus. The planet was confirmed to exist in 2018. [ 1 ] It orbits at around 30 AU (almost as far as Neptune from the Sun) with a period of around 180 years and a relatively high eccentricity of 0.4, and has a mass ...

  3. Epsilon Indi - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Indi

    Epsilon Indi, Latinized from ε Indi, is a star system located at a distance of approximately 12 light-years from Earth in the southern constellation of Indus. The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.674. [ 2 ]

  4. List of nearest exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_exoplanets

    Epsilon Indi Ab, 12 light-years away, with its parent star Epsilon Indi A blacked out, as pictured by JWST in 2023. [1] Distribution of nearest known exoplanets as of March 2018 There are 7,408 known exoplanets , or planets outside the Solar System that orbit a star, as of January 26, 2024; only a small fraction of these are located in the ...

  5. Epsilon Eridani b - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Eridani_b

    A paper published in October 2021 determines, using absolute astrometry measurements from the Hipparcos, Gaia DR2 data, and new radial velocity measurements from Keck/NIRC2 Ms-band vortex coronagraph images, a lower absolute mass of 0.65 times that of Jupiter, at an eccentricity close to 0.055 with the planet orbiting at around 3.53 AU inclined ...

  6. Epsilon Eridani - Wikipedia

    en.wikipedia.org/wiki/Epsilon_Eridani

    The magnetic properties can be modelled by assuming that regions with a magnetic flux of about 0.14 T randomly cover approximately 9% of the photosphere, whereas the remainder of the surface is free of magnetic fields. [88] The overall magnetic activity of Epsilon Eridani shows co-existing 2.95 ± 0.03 and 12.7 ± 0.3 year activity cycles. [84]

  7. DENIS 0255−4700 - Wikipedia

    en.wikipedia.org/wiki/DENIS_0255%E2%88%924700

    DENIS 0255−4700 is an extremely faint brown dwarf 15.9 light-years (4.9 parsecs) from the Solar System in the southern constellation of Eridanus. [3] [7] It is the closest isolated L-type brown dwarf (no undiscovered L-dwarfs are expected to be closer), and only after the binary Luhman 16.

  8. Kapteyn's Star - Wikipedia

    en.wikipedia.org/wiki/Kapteyn's_Star

    It came within 7.0 ly (2.1 pc) of the Sun about 10,900 years ago and has been moving away since that time. [17] Kapteyn's Star is distinctive in a number of regards: it has a high radial velocity, [ 13 ] orbits the Milky Way retrograde , [ 16 ] and is the nearest-known halo star to the Sun. [ 18 ] It is a member of a moving group of stars that ...

  9. COCONUTS-2b - Wikipedia

    en.wikipedia.org/wiki/COCONUTS-2b

    COCONUTS-2 b is a gas giant exoplanet that orbits the M-type star L 34-26. With a mass of 8 Jupiters, [5] it takes over one million years to complete one orbit around the star orbiting 7,506 AU away from it. [1] The planet was discovered in 2011 and was initially identified as a T9 free-floating brown dwarf WISEPA J075108.79−763449.6. [2]