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4 Ursae Minoris

Index 4 Ursae Minoris

4 Ursae Minoris is a binary star system in the northern circumpolar constellation Ursa Minor. [1]

16 relations: Apparent magnitude, Astronomical spectroscopy, Binary star, Circumpolar constellation, Effective temperature, Hydrogen, Light-year, Orbital eccentricity, Orbital period, Photosphere, Radial velocity, Red giant, Solar luminosity, Solar radius, Stellar parallax, Ursa Minor.

Apparent magnitude

The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.

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Astronomical spectroscopy

Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light and radio, which radiates from stars and other celestial objects.

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Binary star

A binary star is a star system consisting of two stars orbiting around their common barycenter.

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Circumpolar constellation

In astronomy, a circumpolar constellation is a constellation (group of stars) that never sets below the horizon, as viewed from a location on Earth.

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Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation.

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Hydrogen

Hydrogen is a chemical element with symbol H and atomic number 1.

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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 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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Orbital period

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

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Photosphere

The photosphere is a star's outer shell from which light is radiated.

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Radial velocity

The radial velocity of an object with respect to a given point is the rate of change of the distance between the object and the point.

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Red giant

A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses) in a late phase of stellar evolution.

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Solar luminosity

The solar luminosity,, is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.

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Solar radius

Solar radius is a unit of distance used to express the size of stars in astronomy.

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Stellar parallax

Stellar parallax is the apparent shift of position of any nearby star (or other object) against the background of distant objects.

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Ursa Minor

Ursa Minor (Latin: "Lesser Bear", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the Northern Sky.

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Redirects here:

B Ursae Minoris.

References

[1] https://en.wikipedia.org/wiki/4_Ursae_Minoris

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