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HD 128311 b

Index HD 128311 b

HD 128311 b is an exoplanet located approximately 54 light-years away in the constellation of Boötes. [1]

13 relations: Astronomical unit, Boötes, California, Constellation, Doppler spectroscopy, Exoplanet, HD 128311, Jupiter mass, Light-year, Minimum mass, Orbital eccentricity, R. Paul Butler, Star.

Astronomical unit

The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.

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Boötes

Boötes is a constellation in the northern sky, located between 0° and +60° declination, and 13 and 16 hours of right ascension on the celestial sphere.

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California

California is a state in the Pacific Region of the United States.

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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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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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HD 128311

HD 128311 or HN Boötis is an orange main-sequence star located approximately 54 light-years away in the constellation of Boötes.

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Jupiter mass

Jupiter mass, also called Jovian mass is the unit of mass equal to the total mass of the planet Jupiter.

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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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Minimum mass

In astronomy, minimum mass is the lower-bound calculated mass of observed objects such as planets, stars and binary systems, nebulae, and black holes.

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Orbital eccentricity

The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle.

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R. Paul Butler

R.

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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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Redirects here:

HD 128311b, HN Boötis b, HN Boötisb.

References

[1] https://en.wikipedia.org/wiki/HD_128311_b

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