File:Centaurus_constellation_map.svg · Wikimedia Commons · See Wikimedia Commons
Agena
Sign in to saveAlso known as HR 5267, HIP 68702, HIC 68702, HD 122451, Hadar, β Cen, β Centauri
ster
Beta Centauri is a bright star system located in the Centaurus constellation in the southern sky. It is one of the notable stars in that region and serves as an important reference point for observers studying the southern celestial sphere.
AI-generated from the Wikipedia summary — may contain errors.
In the Vinony graph
Vinony's link graph records 300 inbound references to Agena, and connects out to Alpha Centauri, year and Centaurus.
It is catalogued under topics including Bayer objects, Beta Cephei variables and Brightest stars.
Vinony links it to 54 Wikipedia language editions.
Wikidata facts
- Distance from Earth
- 50
- Radius
- 7.07
- Image
- Centaurus constellation map.svg
Show 14 more facts
- catalog code
- WEB 12025
- spectral class
- B1
- Commons category
- Beta Centauri
- apparent magnitude
- 1.278
- right ascension component of proper motion
- -21
- absolute magnitude
- -5.42
- luminosity
- 41700
- right ascension
- 210.955855623
- declination
- -60.373035162
- effective temperature
- 26720
- radial velocity
- -12.0
- parallax
- 8.32
- stellar rotational velocity
- 105
- declination component of proper motion
- -25
via Wikidata · CC0
Article · Nederlands
Agena (beta Centauri) is een heldere dubbelster in het sterrenbeeld Centaur (Centaurus). Het is een hete, witte dubbelster, waarvan de gegevens moeilijk te achterhalen zijn omdat er een groot helderheidsverschil is tussen beide sterren. De periode wordt geschat op enkele honderden jaren. De ster staat ook bekend als Hadar.
Abstract from DBpedia / Wikipedia · CC BY-SA