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Beta Trianguli and Delta Trianguli

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Beta Trianguli and Delta Trianguli

Beta Trianguli vs. Delta Trianguli

Beta Trianguli (Beta Tri, β Trianguli, β Tri) is the Bayer designation for a binary star system in the constellation Triangulum, located about 127 light years from Earth. Delta Trianguli (Delta Tri, δ Trianguli, δ Tri) is a spectroscopic binary star system approximately away in the constellation of Triangulum.

Similarities between Beta Trianguli and Delta Trianguli

Beta Trianguli and Delta Trianguli have 27 things in common (in Unionpedia): Apparent magnitude, Astronomical unit, Binary star, Bond (Chinese constellation), Centre de données astronomiques de Strasbourg, Chi Andromedae, Chinese language, Constellation, Durchmusterung, Epoch (astronomy), Gamma Andromedae, Gamma Trianguli, Henry Draper Catalogue, Hipparcos, Infrared excess, Main sequence, Monthly Notices of the Royal Astronomical Society, Orbital eccentricity, Phi Persei, Star, Stellar classification, Tau Andromedae, Triangulum, Upsilon Andromedae, 49 Andromedae, 51 Andromedae, 56 Andromedae.

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 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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Binary star

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

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Bond (Chinese constellation)

Leu (or Low) sieu meaning "the Train of a garment", was one of the twenty-eight lunar mansions of the traditional Chinese astronomy.

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Centre de données astronomiques de Strasbourg

The Centre de Données astronomiques de Strasbourg (CDS; English translation: Strasbourg Astronomical Data Center) is a data hub which collects and distributes astronomical information.

Beta Trianguli and Centre de données astronomiques de Strasbourg · Centre de données astronomiques de Strasbourg and Delta Trianguli · See more »

Chi Andromedae

Chi Andromedae (χ Andromedae, χ And) is the Bayer designation for a star in the northern constellation of Andromeda.

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Chinese language

Chinese is a group of related, but in many cases mutually unintelligible, language varieties, forming a branch of the Sino-Tibetan language family.

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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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Durchmusterung

In astronomy, Durchmusterung or Bonner Durchmusterung (BD), is the comprehensive astrometric star catalogue of the whole sky, compiled by the Bonn Observatory (Germany) from 1859 to 1903.

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Epoch (astronomy)

In astronomy, an epoch is a moment in time used as a reference point for some time-varying astronomical quantity, such as the celestial coordinates or elliptical orbital elements of a celestial body, because these are subject to perturbations and vary with time.

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Gamma Andromedae

Gamma Andromedae (γ Andromedae, abbreviated Gam And, γ And) is the third-brightest point of light in the constellation of Andromeda.

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Gamma Trianguli

Gamma Trianguli (Gamma Tri, γ Trianguli, γ Tri) is a star in the constellation Triangulum located approximately 112 light years from Earth.

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Henry Draper Catalogue

The Henry Draper Catalogue (HD) is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension (HDE), published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the Henry Draper Extension Charts (HDEC), published from 1937 to 1949 in the form of charts, which gave classifications for 86,933 more stars.

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Hipparcos

Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993.

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Infrared excess

An infrared excess is a measurement of an astronomical source, typically a star, that in their spectral energy distribution has a greater measured infrared flux than expected by assuming the star is a blackbody radiator.

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Main sequence

In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.

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Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics.

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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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Phi Persei

Phi Persei (Phi Per, φ Persei, φ Per) is a Class B2Vpe, fourth-magnitude star in the constellation Perseus.

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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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Stellar classification

In astronomy, stellar classification is the classification of stars based on their spectral characteristics.

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Tau Andromedae

Tau Andromedae (τ And, τ Andromedae) is the Bayer designation for a star in the northern constellation of Andromeda.

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Triangulum

Triangulum is a small constellation in the northern sky.

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Upsilon Andromedae

Upsilon Andromedae (υ Andromedae, abbreviated Upsilon And, υ And) is a binary star located approximately 44 light-years from Earth in the constellation of Andromeda.

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49 Andromedae

49 Andromedae (abbreviated 49 And) is a star in the constellation Andromeda.

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51 Andromedae

51 Andromedae (abbreviated 51 And), also named Nembus, is the 5th brightest (4th magnitude) star in the constellation of Andromeda.

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56 Andromedae

56 Andromedae (abbreviated 56 And) is a double star in the constellation Andromeda.

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The list above answers the following questions

Beta Trianguli and Delta Trianguli Comparison

Beta Trianguli has 40 relations, while Delta Trianguli has 43. As they have in common 27, the Jaccard index is 32.53% = 27 / (40 + 43).

References

This article shows the relationship between Beta Trianguli and Delta Trianguli. To access each article from which the information was extracted, please visit:

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