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Giant World Orbiting Red Dwarf Star Gliese 876

Giant World Orbiting Red Dwarf Star Gliese 876
This is an artist's concept of a gas giant planet orbiting the cool, red dwarf star Gliese 876, located 15 light-years away in the autumn constellation Aquarius. The planet was discovered in 1998. But new Hubble Space Telescope measurements of the star's wobble, caused by the gravitational tug of the planet, firmly establish the planet's mass as being no more than approximately twice that of Jupiter's. The planet is only one fifth the distance from the star as the Earth is from the Sun. Though it is too far away to be photographed by present day telescopes, the planet is presumably a gas giant world that might be encircled by moons, as imagined in this illustration. Gliese 876 also has an inner planet with a mass only half that of Jupiter's, as estimated by earlier ground-based observations. The inner gas planet in the system appears as a bright star-like object near the red dwarf. Despite its close proximity to Earth, the red dwarf star is one third the mass of our Sun and is too faint to be seen by the naked eye.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    22h 53m 16.73s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -14° 15' 49.3"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Aquarius
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    15.19 light-years (4.66 parsecs)

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    Principal Astronomers: T. Forveille (CFHT/Observatoire de Grenoble), G. F. Benedict and B. McArthur (McDonald Observatory), X. Delfosse (Observatoire de Grenoble), E. Nelan (STScI), R. P. Butler (Carnegie Institute), W. Spiesman (McDonald Observatory), G. W. Marcy (UC Berkeley), B. Goldman (NMSU), C. Perrier (Observatorie de Grenoble), W. Jefferys (University of Texas), M. Mayor (Observatorie de Geneve)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>FGS
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    June - August, November 1999; May 2000; November 2001, Exposure Time: 4 hours
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Gliese 876b; Gl 876b; GJ 876b; Ross 780b
  • Object Description
    Object DescriptionThe type of astronomical object.
    Extrasolarplanet; Companion to Star Gliese 876 (Ross 780)
  • Release Date
    December 3, 2002
  • Science Release
    Hubble Makes Precise Measure of Extrasolar World’s True Mass
  • Credit
    NASA and G. Bacon (STScI)

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov