Stars And Stellar Phenomena Codexery

Beta Centauri

Triple star system and pointer to the Southern Cross.

Beta Centauri

Wikipedia / Wikimedia Commons

Beta Centauri, also known as Hadar, is a triple star system in the southern constellation of Centaurus. It is the second-brightest object in Centaurus and the eleventh brightest star in the night sky, with a combined apparent visual magnitude of 0.61. The system is well known in the Southern Hemisphere as one of the two 'Pointers' to the Southern Cross, aiding navigation.

Bayer designation
β Centauri
Traditional names
Hadar, Agena
Apparent magnitude
0.61
Distance
about 361 light-years (111 parsecs)
Spectral type
B1 (all three components)
Number of stars
3 (Aa, Ab, B)
Variable type
β Cephei (component Aa)

Lore & Background

The system bears the traditional names Hadar and Agena. Hadar comes from the Arabic root meaning 'to be present' or 'settled area,' while Agena is thought to derive from Latin genua, meaning 'knees,' referring to its position on the left knee of the centaur in the constellation Centaurus. In 2016, the International Astronomical Union approved the name Hadar for the star β Centauri Aa. The Chinese name is 马腹一 (Mandarin: mǎ fù yī, 'the First Star of the Horse's Abdomen'). The Boorong people of Australia named it Bermbermgle (with α Centauri), two brothers who spear and kill Tchingal, 'The Emu' (Coalsack Nebula). The Mursi people of Ethiopia call it Waar.

Reader's Guide

Beta Centauri is significant as a bright navigational aid in the Southern Hemisphere, forming the inner of the two 'Pointers' to the Southern Cross. A line from Alpha Centauri through Beta Centauri leads near Gacrux, helping navigators determine south. The system is also notable for its triple-star nature: a close binary pair (Aa and Ab) with a 357-day orbit and high eccentricity, plus a wider companion (B) separated by 1.3 arcseconds. Both Aa and Ab are giant stars of spectral type B1 III, with masses 12.02 and 10.58 times that of the Sun, respectively. They are massive enough to eventually explode as supernovas, while component B will become a white dwarf. The system's brightness and variability—component Aa is a β Cephei variable—make it a subject of astrophysical study.

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