Search results

Results 1 – 20 of 376
Advanced search

Search in namespaces:

There is a page named "List of extrasolar planets detected by radial velocity" on Wikipedia

View (previous 20 | ) (20 | 50 | 100 | 250 | 500)
  • following is a list of 456 extrasolar planets that were only detected by radial velocity method –– 31 confirmed and 323 candidates, sorted by orbital periods...
    36 KB (286 words) - 20:08, 22 December 2023
  • Thumbnail for Lists of planets
    of planets in fiction, see: Fictional planets of the Solar System, Extrasolar planets in fiction § List, and List of Star Wars planets and moons List...
    9 KB (782 words) - 00:54, 2 July 2024
  • Thumbnail for Exoplanet
    detection of planets near the star; thus, 85% of the exoplanets detected are inside the tidal locking zone. In several cases, multiple planets have been...
    147 KB (15,908 words) - 19:37, 2 July 2024
  • Thumbnail for Methods of detecting exoplanets
    astronomers have generally had to resort to indirect methods to detect extrasolar planets. As of 2016, several different indirect methods have yielded success...
    134 KB (15,194 words) - 19:55, 5 July 2024
  • George (21 January 2021). "A Decade of Radial-velocity Monitoring of Vega and New Limits on the Presence of Planets". The Astronomical Journal. 161 (4):...
    63 KB (3,715 words) - 22:09, 8 July 2024
  • Thumbnail for List of nearest stars
    S2CID 221150644 Accepted for publication by ApJS "The Extrasolar Planet Encyclopaedia — Catalog Listing". Extrasolar Planets Encyclopaedia. Archived from the...
    116 KB (5,396 words) - 01:22, 9 July 2024
  • Thumbnail for Radial velocity
    detect planets around stars, in the way that the movement's measurement determines the planet's orbital period, while the resulting radial-velocity amplitude...
    14 KB (1,791 words) - 05:54, 24 March 2024
  • Thumbnail for Epsilon Eridani b
    AU with a period of around 7.6 years, and has a mass around 0.6 times that of Jupiter. As of 2023[update], both the Extrasolar Planets Encyclopaedia and...
    21 KB (1,743 words) - 23:11, 1 March 2024
  • Thumbnail for List of nearest exoplanets
    some known extrasolar bodies, including nearby exoplanets, through the NameExoWorlds project. Planets named in the 2015 event include the planets around Epsilon...
    135 KB (7,432 words) - 19:44, 29 June 2024
  • Thumbnail for Upsilon Andromedae b
    Andromedae b was detected by the variations in its star's radial velocity caused by the planet's gravity. The variations were detected by making sensitive...
    17 KB (1,550 words) - 15:44, 2 May 2024
  • Thumbnail for List of directly imaged exoplanets
    This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit...
    48 KB (3,408 words) - 03:24, 6 July 2024
  • This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity...
    68 KB (4,423 words) - 11:49, 9 July 2024
  • Thumbnail for 51 Pegasi b
    named Dimidium /dɪˈmɪdiəm/, is an extrasolar planet approximately 50 light-years (15 parsecs) away in the constellation of Pegasus. It was the first exoplanet...
    16 KB (1,602 words) - 13:31, 21 February 2024
  • Thumbnail for Exomoon
    Exomoon (redirect from Extrasolar satellite)
    exomoon or extrasolar moon is a natural satellite that orbits an exoplanet or other non-stellar extrasolar body. Exomoons are difficult to detect and confirm...
    33 KB (4,120 words) - 22:11, 2 May 2024
  • Thumbnail for List of multiplanetary systems
    microlensing List of exoplanets detected by radial velocity List of exoplanets detected by timing List of directly imaged exoplanets List of transiting...
    260 KB (8,676 words) - 21:37, 8 July 2024
  • Thumbnail for Proxima Centauri d
    Proxima Centauri d (category Exoplanets detected by radial velocity)
    Centauri system. It is the least massive exoplanet detected with the radial velocity method as of 2022[update]. Although Proxima d orbits too close to...
    6 KB (342 words) - 01:22, 5 March 2024
  • Exoplanet naming convention). Some exoplanets, especially those detected by radial velocity, can turn out to be brown dwarfs if their mass is higher than...
    63 KB (845 words) - 20:36, 16 June 2024
  • Thumbnail for Discoveries of exoplanets
    was announced that 30 new planets were discovered, all were detected by the radial velocity method. It is the most planets ever announced in a single...
    83 KB (8,219 words) - 08:44, 24 April 2024
  • Thumbnail for Gliese 436 b
    Gliese 436 b (category Exoplanets detected by radial velocity)
    radial velocity method. Together with 55 Cancri e, it was the first of a new class of planets with a minimum mass (M sini) similar to Neptune. The planet was...
    24 KB (2,119 words) - 21:56, 29 June 2024
  • Thumbnail for Upsilon Andromedae c
    detected by measuring variations in its star's radial velocity as a result of the planet's gravity. This was done by making precise measurements of the...
    11 KB (1,075 words) - 21:56, 31 January 2024
View (previous 20 | ) (20 | 50 | 100 | 250 | 500)