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Andromeda (constellation)}} is a {}-based template to be used at the bottom of articles about astronomical objects beyond the Solar System, located in the constellation of Andromeda. The template is divided into categories of stars, star clusters, nebulae, exoplanets, galaxies, galaxy clusters, and a miscellaneous "other" category.
Groombridge 34 is a binary star system in the northern constellation of Andromeda.It was listed as entry number 34 in A Catalogue of Circumpolar Stars, published posthumously in 1838 by British astronomer Stephen Groombridge. [11]
HD 895 is a multiple star system in the constellation Andromeda.Its apparent magnitude is 6.277, [2] so it can be seen by the naked eye under very favourable conditions. Based on parallax measured by Hipparcos, the system is located around 54 parsecs (180 ly) away, [4] and it is made of two different spectroscopic binary pairs.
a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 14.5 at minimum brightness to a magnitude of 9.9 at maximum brightness, with a period of approximately 238.3 days.
HD 5789 and HD 5788 is a pair of stars comprising a binary star [12] system in the northern constellation of Andromeda.Located approximately 151 parsecs (490 ly) away, the primary is a hot, massive blue star with an apparent magnitude of 6.06 while the secondary is slightly smaller and cooler, with an apparent magnitude of 6.76.
Zeta Andromedae (Zeta And, ζ Andromedae, ζ And) is a star system in the constellation Andromeda. It is approximately 189 light-years from Earth. Zeta Andromedae is the star's Bayer designation. It also has the Flamsteed designation 34 Andromedae and multiple other designations in stellar catalogues.
Theta Andromedae is a binary star [11] system in the northern constellation of Andromeda. Theta Andromedae, Latinized from θ Andromedae, is its Bayer designation.It is located at a distance of approximately 173 light-years (53 parsecs) from the Sun, [1] and has an apparent visual magnitude of 4.6. [2]
Delta Andromedae, Latinized from δ Andromedae, is a triple star [12] system in the northern constellation of Andromeda. The system is visible to the naked eye as a point of light with a combined apparent visual magnitude of 3.28. [2] Based upon parallax measurements, it is located at a distance of approximately 105.5 light-years (32.3 parsecs ...