Archivo de imágenes de Hubble

Mundo gigante orbitando la estrella enana roja 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 gra...

Fecha
Jan 1, 2002
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2002-27-1254-image
Por

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.

Credits

NASA and G. Bacon (STScI)

Detalles de la imagen

About The Object
Object NameGliese 876b; Gl 876b; GJ 876b; Ross 780b
Object DescriptionExtrasolarplanet; Companion to Star Gliese 876 (Ross 780)
R.A. Position22h 53m 16.73s
Dec. Position-14° 15' 49.3"
ConstellationAquarius
Distance15.19 light-years (4.66 parsecs)
About The Data
Data DescriptionPrincipal 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)
InstrumentHST>FGS
Exposure DatesJune - August, November 1999; May 2000; November 2001, Exposure Time: 4 hours

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