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This star has a mass of about 13–14 times the [[Solar mass|mass of the Sun]]<ref name=aaa459_2_589/> with 8–11 times the [[Solar radius|Sun's radius]].<ref name=mnras369_1_L61/> The [[effective temperature]] of the star's outer envelope is about 23,150 K, which is much higher than the Sun's at 5,778 K. The energy emitted at the high temperature of the former is what gives this star a blue-white hue characteristic of a [[B-type star]].<ref name=aaa501_1_297/><ref name=csiro/> The estimated age of Mirzam is {{nowrap|12–13 million years}}, which is long enough for a star of this mass to have [[stellar evolution|evolved]] into a [[giant star]]. The [[stellar classification]] of B1 II-III<ref name=apj573_1_359/> indicates that the [[stellar spectrum|spectrum]] matches a star part way between a giant star and a [[bright giant]]. |
This star has a mass of about 13–14 times the [[Solar mass|mass of the Sun]]<ref name=aaa459_2_589/> with 8–11 times the [[Solar radius|Sun's radius]].<ref name=mnras369_1_L61/> The [[effective temperature]] of the star's outer envelope is about 23,150 K, which is much higher than the Sun's at 5,778 K. The energy emitted at the high temperature of the former is what gives this star a blue-white hue characteristic of a [[B-type star]].<ref name=aaa501_1_297/><ref name=csiro/> The estimated age of Mirzam is {{nowrap|12–13 million years}}, which is long enough for a star of this mass to have [[stellar evolution|evolved]] into a [[giant star]]. The [[stellar classification]] of B1 II-III<ref name=apj573_1_359/> indicates that the [[stellar spectrum|spectrum]] matches a star part way between a giant star and a [[bright giant]]. |
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Beta Canis Majoris is located near the far end of the [[Local Bubble]],<ref name=Welsh/> a cavity in the local [[interstellar medium]] through which the [[Sun]] is traveling. Beta Canis Majoris was the [[historical brightest stars|brightest star]] in the night sky around four million years ago, peaking with an apparent magnitude of -3.65, or more than seven times as bright as [[Sirius]] today.<ref name=tomkin1998>{{cite journal|last=Tomkin|first=Jocelyn|date=April 1998|title=Once and Future Celestial Kings|journal=Sky and Telescope|volume=95|issue=4|pages=59–63|bibcode=1998S&T....95d..59T}} – based on computations from [[HIPPARCOS]] data. (The calculations exclude stars whose distance or [[proper motion]] is uncertain.) [ftp://tlgleonid.asuscomm.com/HITACHI/BOOK_ASTRO/S&T/SkyandTelescope_1998%20-%20astronomy/04/199804059063.pdf PDF]{{dead link|date=November 2017 |bot=InternetArchiveBot |fix-attempted=yes }}</ref> |
Beta Canis Majoris is located near the far end of the [[Local Bubble]],<ref name=Welsh/> a cavity in the local [[interstellar medium]] through which the [[Sun]] is traveling. It is located within the [[Mirzam Tunnel]], a region of less dense concentration between the stars and HII regions surrounding the Ori OB1 and Vel OB2 associations. Beta Canis Majoris was the [[historical brightest stars|brightest star]] in the night sky around four million years ago, peaking with an apparent magnitude of -3.65, or more than seven times as bright as [[Sirius]] today.<ref name=tomkin1998>{{cite journal|last=Tomkin|first=Jocelyn|date=April 1998|title=Once and Future Celestial Kings|journal=Sky and Telescope|volume=95|issue=4|pages=59–63|bibcode=1998S&T....95d..59T}} – based on computations from [[HIPPARCOS]] data. (The calculations exclude stars whose distance or [[proper motion]] is uncertain.) [ftp://tlgleonid.asuscomm.com/HITACHI/BOOK_ASTRO/S&T/SkyandTelescope_1998%20-%20astronomy/04/199804059063.pdf PDF]{{dead link|date=November 2017 |bot=InternetArchiveBot |fix-attempted=yes }}</ref> |
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==In culture== |
==In culture== |
Location of β Canis Majoris (circled) | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Major |
Right ascension | 06h22m 41.98535s[1] |
Declination | −17° 57′ 21.3073″[1] |
Apparent magnitude (V) | 1.985[2] (1.97 - 2.01[3]) |
Characteristics | |
Spectral type | B1 II-III[4] |
U−B color index | −0.99[2] |
B−V color index | −0.235[2] |
Variable type | β Cep[5] |
Astrometry | |
Radial velocity (Rv) | +33.7[6] km/s |
Proper motion (μ) | RA: −3.23[1] mas/yr Dec.: −0.78[1] mas/yr |
Parallax (π) | 6.62 ± 0.22 mas[1] |
Distance | 490 ± 20 ly (151 ± 5 pc) |
Absolute magnitude (MV) | −4.1[7] |
Details | |
Mass | 13.5 ± 0.5[8] M☉ |
Radius | 9.7 ± 1.3[9] R☉ |
Luminosity | 26600[9] L☉ |
Surface gravity (log g) | 3.79 ± 0.20[9] cgs |
Temperature | 25,000[10] K |
Metallicity [Fe/H] | 0.04 ± 0.10[8] dex |
Rotational velocity (v sin i) | 31 ± 5[8] km/s |
Age | 12.4 ± 0.7[8] Myr |
Other designations | |
Mirzam, Murzim, Mirza,[11] 2 Canis Majoris, HR 2294, BD−17°1467, HD 44743, SAO 151428, FK5 243, HIP 30324, GC 8223, CCDM 06227-1757[12] | |
Database references | |
SIMBAD | data |
Beta Canis Majoris (β Canis Majoris, abbreviated Beta CMa, β CMa), also named Mirzam /ˈmɜːrzəm/,[13] is a star in the southern constellationofCanis Major, the "Great Dog", located at a distance of about 500 light-years (150 parsecs) from the Sun.[1] In the modern constellation it lies at the position of the dog's front leg.
Beta Canis Majoris is the star's Bayer designation. The traditional names Mirzam, Al-MurzimorMurzim,[11] derive from the Arabic (مرزم) for 'The Herald', and probably refers to its position, heralding (i.e., rising before) Sirius in the night sky. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[14] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[15] included a table of the first two batches of names approved by the WGSN; which included Mirzam for this star.
InChinese, 軍市 (Jūn Shì), meaning 'Market for Soldiers', refers to an asterism consisting of β Canis Majoris, Nu3 Canis Majoris, 15 Canis Majoris, Pi Canis Majoris, Omicron1 Canis Majoris and Xi1 Canis Majoris.[16] Consequently, β Canis Majoris itself is known as 軍市一 (Jūn Shì yī, English: the First Star of Market for Soldiers).[17] From this Chinese name arose the name Kuen She.[11]
The Dunhuang Star Chart noted β Canis Majoris as Yeji "Pheasant Cock", though was located about 10 degrees too far north of its correct position.[18]
Beta Canis Majoris was called Oupo by the people of the Tuamotus.[19]
Frequency (day−1) |
Amplitude (km s−1) |
---|---|
3.9793 | 2.7 |
3.9995 | 2.6 |
4.1832 | 0.7 |
Mirzam is a Beta Cephei variable that varies in apparent magnitude between +1.97 and +2.01 over a six-hour period, a change in brightness that is too small to be discerned with the naked eye. It exhibits this variation in luminosity because of periodic pulsations in its outer envelope, which follow a complex pattern with three different cycles; all about six hours in length. The two dominant pulsation frequencies have a combined beat period of roughly 50 days. The strongest pulsation mode is a radial first overtone, while the second is non-radial.[8]
This star has a mass of about 13–14 times the mass of the Sun[8] with 8–11 times the Sun's radius.[9] The effective temperature of the star's outer envelope is about 23,150 K, which is much higher than the Sun's at 5,778 K. The energy emitted at the high temperature of the former is what gives this star a blue-white hue characteristic of a B-type star.[10][21] The estimated age of Mirzam is 12–13 million years, which is long enough for a star of this mass to have evolved into a giant star. The stellar classification of B1 II-III[4] indicates that the spectrum matches a star part way between a giant star and a bright giant.
Beta Canis Majoris is located near the far end of the Local Bubble,[22] a cavity in the local interstellar medium through which the Sun is traveling. It is located within the Mirzam Tunnel, a region of less dense concentration between the stars and HII regions surrounding the Ori OB1 and Vel OB2 associations. Beta Canis Majoris was the brightest star in the night sky around four million years ago, peaking with an apparent magnitude of -3.65, or more than seven times as bright as Sirius today.[23]
Mirzam appears on the flag of Brazil, symbolising the state of Amapá.[24]
Murzim (AK-95) was a United States Navy Crater class cargo ship named after one of the star's alternative traditional names.
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