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Gliese 317 b

Index Gliese 317 b

Gliese 317 b is an extrasolar planet approximately 50 light-years away in the constellation of Pyxis. [1]

15 relations: Constellation, Distance, Doppler spectroscopy, Exoplanet, Giant planet, Gliese 317, Gliese 436 b, Light-year, Orbital speed, Pyxis, Red dwarf, Star, Sun, The Astrophysical Journal, W. M. Keck Observatory.

Constellation

A constellation is a group of stars that are considered to form imaginary outlines or meaningful patterns on the celestial sphere, typically representing animals, mythological people or gods, mythological creatures, or manufactured devices.

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Distance

Distance is a numerical measurement of how far apart objects are.

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Doppler spectroscopy

Doppler spectroscopy (also known as the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star.

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Exoplanet

An exoplanet or extrasolar planet is a planet outside our solar system.

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Giant planet

A giant planet is any massive planet.

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Gliese 317

Gliese 317 is a red dwarf approximately 50 light-years away in the constellation of Pyxis.

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Gliese 436 b

Gliese 436 b (sometimes called GJ 436 b) is a Neptune-sized exoplanet orbiting the red dwarf Gliese 436.

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Light-year

The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.

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Orbital speed

In gravitationally bound systems, the orbital speed of an astronomical body or object (e.g. planet, moon, artificial satellite, spacecraft, or star) is the speed at which it orbits around either the barycenter or, if the object is much less massive than the largest body in the system, its speed relative to that largest body.

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Pyxis

Pyxis is a small and faint constellation in the southern sky.

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Red dwarf

A red dwarf (or M dwarf) is a small and relatively cool star on the main sequence, of M spectral type.

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Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

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Sun

The Sun is the star at the center of the Solar System.

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The Astrophysical Journal

The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.

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W. M. Keck Observatory

The W. M. Keck Observatory is a two-telescope astronomical observatory at an elevation of 4,145 meters (13,600 ft) near the summit of Mauna Kea in the U.S. state of Hawaii.

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Redirects here:

GJ 317 b, Gliese 317b.

References

[1] https://en.wikipedia.org/wiki/Gliese_317_b

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