Epsilon Canis Majoris

ε Canis Majoris

Template:Location mark Location of ε Canis Majoris (circled)
Observation data Epoch J2000      Equinox J2000
Constellation	Canis Major
ε CMa A
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	1.50
ε CMa B
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	+7.5
Characteristics
ε CMa A
Evolutionary stage	Blue giant, main sequence or stellar merger product
Spectral type	B2 II or B2 III-II
U−B Template:Engvar	−0.93
B−V Template:Engvar	−0.21
Astrometry
ε CMa A
Radial velocity (Rv)	+Template:Val km/s
Proper motion (μ)	RA: +3.24 mas/yr Dec.: +1.33 mas/yr
Parallax (π)	8.05±0.14 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	Template:Val
ε CMa B
Radial velocity (Rv)	+Template:Val km/s
Proper motion (μ)	RA: +1.802 mas/yr Dec.: Template:Val mas/yr
Parallax (π)	7.6159±0.0223 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Details
ε CMa A
Mass	Template:Val Template:Solar mass
Radius	Template:Val Template:Solar radius
Luminosity	Template:Val Template:Solar luminosity Template:Val Template:Solar luminosity
Surface gravity (log g)	Template:Val cgs
Temperature	Template:Val K
Rotation	5 days
Rotational velocity (v sin i)	25 km/s
Age	17.5Template:Snd19 Myr
ε CMa B
Mass	1.54 Template:Solar mass
Radius	1.54 Template:Solar radius
Luminosity	6.13 Template:Solar luminosity
Surface gravity (log g)	4.15 cgs
Temperature	7,315 K
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
ε CMa A
SIMBAD	data
ε CMa B
SIMBAD	data

Epsilon Canis Majoris is a binary star system and the second-brightest star in the constellation of Canis Major. Its name is a Bayer designation that is Latinised from ε Canis Majoris, and abbreviated Epsilon CMa or ε CMa. This is the 22nd-brightest star in the night sky with an apparent magnitude of 1.50. About 4.7 million years ago, it was the brightest star in the night sky, with an apparent magnitude of −3.99. Based upon parallax measurements obtained during the Hipparcos and the Gaia mission, it is about Template:Val light-years distant.

The two components are designated ε Canis Majoris A, officially named Adhara Template:IPAc-en – the traditional name of the system, and B.

Nomenclature

ε Canis Majoris (Latinised to Epsilon Canis Majoris) is the binary system's Bayer designation. The designations of the two components as ε Canis Majoris A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).

ε Canis Majoris bore the traditional name Adhara (sometimes spelled Adara, Adard, Udara or Udra), derived from the Arabic word عذارى 'aðāra', "virgins". In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire star systems. It approved the name Adhara for the star ε Canis Majoris A on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.

In the 17th-century catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Aoul al Adzari (أول العذاري awwal al-adhara), which was translated into Latin as Prima Virginum, meaning First of the Virgins. Along with δ Canis Majoris (Wezen), η Canis Majoris (Aludra) and ο² Canis Majoris (Thanih al Adzari), these stars were Al ʽAdhārā (العذاري), 'the Virgins'.

In Chinese, (), meaning Bow and Arrow, refers to an asterism consisting of ε Canis Majoris, δ Canis Majoris, η Canis Majoris, κ Canis Majoris, ο Puppis, π Puppis, χ Puppis, c Puppis and k Puppis. Consequently, ε Canis Majoris itself is known as (, Template:Langx).

Physical properties

ε Canis Majoris is a binary star. The primary, ε Canis Majoris A, has an apparent magnitude of +1.5 and belongs to the spectral classification B2. Its color is blue or blueish-white, due to the surface temperature of Template:Val. It emits a total radiation equal to 38,700 times that of the Sun. This star is the brightest source of extreme ultraviolet in the night sky. It is the strongest source of photons capable of ionizing hydrogen atoms in interstellar gas near the Sun, and is very important in determining the ionization state of the Local Interstellar Cloud. Its rotation period is estimated to be about 5 days.

The exact evolutionary status of Template:Nobr is uncertain. Spectroscopically it has been given the class B2 II, with the luminosity class of II indicating that is a bright giant, more luminous than a typical giant (luminosity class III). However, it appear less luminous than the expected for this luminosity class, and is more likely of class B2 III-II. Two studies suggest Template:Nobr is still in the late main sequence (TAMS), rather than being a giant. One of these even suggested it could be the final product of a stellar merger.

The +7.5-magnitude (the absolute magnitude amounts to +1.9) companion star, ε Canis Majoris B, is Template:Val away with a position angle of 161° of the main star. Despite the relatively large angular distance the components can only be resolved in large telescopes, since the primary is approximately 250 times brighter than its companion.

A few million years ago, ε Canis Majoris was much closer to the Sun than it is at present, causing it to be a much brighter star in the night sky. About 4.4 million years ago, Adhara was Template:Convert light-years from the Sun, and was the brightest star in the night sky with a magnitude of Template:Val.Template:Efn No other star has attained this brightness since, nor will any other star attain this brightness for at least five million years.

In culture

USS Adhara (AK-71) was a U.S. Navy Crater-class cargo ship named after the star.

ε Canis Majoris appears on the national flag of Brazil, symbolising the state of Tocantins.