Castor (star): Difference between revisions
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== Stellar system == | == Stellar system == | ||
<div style="float:left; width:290px; border:solid black 1px; text-align: center; margin: 8px; padding: 4px; font-size: 90%;"> | <div style="float:left; width:290px; border:solid black 1px; text-align: center; margin: 8px; padding: 4px; font-size: 90%;"> | ||
{{chart/start}} | {{tree chart/start}} | ||
{{chart|border=1| | | | |, |- |S1| |S1='''Aa''' }} | {{tree chart|border=1| | | | |, |- |S1| |S1='''Aa''' }} | ||
{{chart|border=0| | |, |- |( |PA| |PA=Period = 9.2128 d }} | {{tree chart|border=0| | |, |- |( |PA| |PA=Period = 9.2128 d }} | ||
{{chart|border=1| | |! | |` |- |S2| |S2='''Ab''' }} | {{tree chart|border=1| | |! | |` |- |S2| |S2='''Ab''' }} | ||
{{chart|border=0| |, |( | | |PB| |PB=Separation = {{Val|3.9|u=arcsec}} }} | {{tree chart|border=0| |, |( | | |PB| |PB=Separation = {{Val|3.9|u=arcsec}} }} | ||
{{chart|border=1| |! |! | |, |- |S3| |S3='''Ba''' }} | {{tree chart|border=1| |! |! | |, |- |S3| |S3='''Ba''' }} | ||
{{chart|border=0| |! |` |- |( |PC| |PC=Period = 2.9283 d }} | {{tree chart|border=0| |! |` |- |( |PC| |PC=Period = 2.9283 d }} | ||
{{chart|border=1|- |( | | |` |- |S4| |S4='''Bb''' }} | {{tree chart|border=1|- |( | | |` |- |S4| |S4='''Bb''' }} | ||
{{chart|border=0| |! | | |PD| |PD=Separation = {{Val|71|u=arcsec}} }} | {{tree chart|border=0| |! | | |PD| |PD=Separation = {{Val|71|u=arcsec}} }} | ||
{{chart|border=1| |! |, |- |S5| |S5='''Ca''' }} | {{tree chart|border=1| |! |, |- |S5| |S5='''Ca''' }} | ||
{{chart|border=0| |` |( |PE| |PE=Period = 0.814 d }} | {{tree chart|border=0| |` |( |PE| |PE=Period = 0.814 d }} | ||
{{chart|border=1| | |` |- |S6| |S6='''Cb''' }} | {{tree chart|border=1| | |` |- |S6| |S6='''Cb''' }} | ||
{{chart/end}} | {{tree chart/end}} | ||
Hierarchy of orbits in the Castor system<ref name=Hussain2012/> | Hierarchy of orbits in the Castor system<ref name=Hussain2012/> | ||
</div> | </div> | ||
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Castor is 49 [[light-year]]s away from Earth, determined from its large annual [[parallax]].<ref name=torres2022/> | Castor is 49 [[light-year]]s away from Earth, determined from its large annual [[parallax]].<ref name=torres2022/> | ||
The two brightest stars are both [[A-type main-sequence star | The two brightest stars are both [[A-type main-sequence star]]s, more massive and brighter than the Sun. The properties of their [[red dwarf]] companions are difficult to determine, but they are known to have masses 39% that of the Sun.<ref name=torres2022/> | ||
[[File:YYGemLightCurve.png|thumb|A [[ | [[File:YYGemLightCurve.png|thumb|A [[Photometric system#Photometric letters|visual band]] [[light curve]] for YY Geminorum (Castor C), adapted from Butler ''et al.'' (2015)<ref name="Butler"/>|none]] | ||
Castor B is an [[Am star]], with particularly strong spectral lines of certain metals. | Castor B is an [[Am star]], with particularly strong spectral lines of certain metals. | ||
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The star was annotated by the [[Arabic]] description ''Al Ras al Taum al Muqadim'', which translates as ''the head of the foremost twin''. In the catalogue of stars in the ''Calendarium of al Achsasi al Mouakket'', this star was designated ''Aoul al Dzira'', which was translated into [[Latin]] as ''Prima Brachii'', meaning ''the first in the paw''.<ref name=knobel1895/> | The star was annotated by the [[Arabic]] description ''Al Ras al Taum al Muqadim'', which translates as ''the head of the foremost twin''. In the catalogue of stars in the ''Calendarium of al Achsasi al Mouakket'', this star was designated ''Aoul al Dzira'', which was translated into [[Latin]] as ''Prima Brachii'', meaning ''the first in the paw''.<ref name=knobel1895/> | ||
In [[Chinese language|Chinese]], {{lang|zh|北河}} ({{lang|zh-Latn|Běi Hé}}), meaning ''[[Well (Chinese constellation)|North River]]'', refers to an asterism consisting of Castor, [[Rho Geminorum]], and [[Beta Geminorum|Pollux]].<ref>{{in lang|zh}} ''中國星座神話'', written by 陳久金. Published by 台灣書房出版有限公司, 2005, {{ISBN|978-986-7332-25-7}}.</ref> Consequently, Castor itself is known as {{lang|zh|北河二}} ({{lang|zh-Latn|Běi Hé èr}}, {{langx|en|the Second Star of North River}}.)<ref>{{cite web |title=亮星中英對照表 |trans-title=Chinese-English Comparison Table of Bright Stars |series=研究資源 [Research Resources] |publisher=香港太空館 [Hong Kong Space Museum] | | In [[Chinese language|Chinese]], {{lang|zh|北河}} ({{lang|zh-Latn|Běi Hé}}), meaning ''[[Well (Chinese constellation)|North River]]'', refers to an asterism consisting of Castor, [[Rho Geminorum]], and [[Beta Geminorum|Pollux]].<ref>{{in lang|zh}} ''中國星座神話'', written by 陳久金. Published by 台灣書房出版有限公司, 2005, {{ISBN|978-986-7332-25-7}}.</ref> Consequently, Castor itself is known as {{lang|zh|北河二}} ({{lang|zh-Latn|Běi Hé èr}}, {{langx|en|the Second Star of North River}}.)<ref>{{cite web |title=亮星中英對照表 |trans-title=Chinese-English Comparison Table of Bright Stars |series=研究資源 [Research Resources] |publisher=香港太空館 [Hong Kong Space Museum] |language=zh |url=http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_c_d.htm |access-date=23 November 2010 |archive-url=https://web.archive.org/web/20090929163750/http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_c_d.htm |archive-date=29 September 2009}}</ref> | ||
In 2016, the [[International Astronomical Union]] organized a [[IAU Working Group on Star Names|Working Group on Star Names]] (WGSN)<ref name="WGSN"/> to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included ''Castor'' for the star α Geminorum Aa.<ref name="WGSN1"/> | In 2016, the [[International Astronomical Union]] organized a [[IAU Working Group on Star Names|Working Group on Star Names]] (WGSN)<ref name="WGSN"/> to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included ''Castor'' for the star α Geminorum Aa.<ref name="WGSN1"/> | ||
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==External links== | ==External links== | ||
* {{ | * {{commons category-inline}} | ||
* {{cite web | * {{cite web | ||
| title=Castor 6 | | title=Castor 6 | ||
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{{Portal bar|Astronomy|Stars|Outer space}} | {{Portal bar|Astronomy|Stars|Outer space}} | ||
{{Sky|07|34|36|+|31|53|18}} | {{Sky|07|34|36|+|31|53|18}} | ||
<!-- Properties --> | |||
{{DEFAULTSORT:Castor (Star)}} | {{DEFAULTSORT:Castor (Star)}} | ||
[[Category:A-type main-sequence stars]] | [[Category:A-type main-sequence stars]] | ||
[[Category:M-type main-sequence stars]] | [[Category:M-type main-sequence stars]] | ||
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[[Category:Castor and Pollux]] | [[Category:Castor and Pollux]] | ||
[[Category:Astronomical objects discovered in 1718]] | [[Category:Astronomical objects discovered in 1718]] | ||
[[Category:Gliese and GJ objects|0278]] | |||
Latest revision as of 00:37, 23 June 2025
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Castor is the second-brightest object in the zodiac constellation of Gemini. It has the Bayer designation α Geminorum, which is Latinised to Alpha Geminorum and abbreviated Alpha Gem or α Gem. With an apparent visual magnitude of 1.58, it is one of the brightest stars in the night sky. Castor appears singular to the naked eye, but it is actually a sextuple star system organized into three binary pairs. Although it is the 'α' (alpha) member of the constellation, it is half a magnitude fainter than 'β' (beta) Geminorum, Pollux.
Stellar system
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Castor is a multiple star system made up of six individual stars; there are three visual components, all of which are spectroscopic binaries. Appearing to the naked eye as a single star, Castor was first recorded as a double star in 1718 by James Pound, but it may have been resolved into at least two sources of light by Cassini as early as 1678. The separation between the binary systems Castor A and Castor B has increased from about 2″ (2 arcseconds of angular measurement) in 1970 to about 6″ in 2017.[15][13] These pairs have magnitudes of 1.9 and 3.0, respectively.
Castor Aa and Ba both have orbits of a few days with a much fainter companion.
Castor C, or YY Geminorum, was discovered to vary in brightness with a regular period. It is an eclipsing binary with additional variations due to areas of different brightness on the surface of one or both stars, as well as irregular flares.[9] The Castor C components orbit in less than a day. Castor C is believed to be in orbit around Castor AB, but with an extremely long period of several thousand years. It is 73″ distant from the bright components.[13]
The combined apparent magnitude of all six stars is +1.58.
Physical properties
Castor is 49 light-years away from Earth, determined from its large annual parallax.[6]
The two brightest stars are both A-type main-sequence stars, more massive and brighter than the Sun. The properties of their red dwarf companions are difficult to determine, but they are known to have masses 39% that of the Sun.[6]
Castor B is an Am star, with particularly strong spectral lines of certain metals.
Castor C is a variable star, classified as a BY Draconis type. BY Draconis variables are cool dwarf stars which vary as they rotate due to starspots or other variations in their photospheres. The two red dwarfs of Castor C are almost identical, with masses around Template:Solar mass and luminosities less than 10% of the Sun.[9] Since 2018 it is suspected a brown dwarf with a mass at least Template:Val times the mass of Jupiter might be orbiting Castor C with a period of 50 years. If it is confirmed, Castor would turn out to be a seven-star system.[17]
All the red dwarfs in the Castor system have emissions lines in their spectra, and all are flare stars.[10]
Etymology and culture
α Geminorum (Latinised to Alpha Geminorum) is the star system's Bayer designation.
Castor and Pollux are the two "heavenly twin" stars that give the constellation Gemini (meaning twins in Latin) its name. The name Castor refers specifically to Castor, one of the twin sons of Zeus and Leda in Greek and Roman mythology.
The star was annotated by the Arabic description Al Ras al Taum al Muqadim, which translates as the head of the foremost twin. In the catalogue of stars in the Calendarium of al Achsasi al Mouakket, this star was designated Aoul al Dzira, which was translated into Latin as Prima Brachii, meaning the first in the paw.[18]
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning North River, refers to an asterism consisting of Castor, Rho Geminorum, and Pollux.[19] Consequently, Castor itself is known as Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[20]
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[21] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Castor for the star α Geminorum Aa.[22]
Castor C also has the variable-star designation YY Geminorum.
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See also
Notes
References
External links
- Template:Commons category-inline
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Template:Stars of Gemini Template:Portal bar Template:Sky
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- Pages with script errors
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- A-type main-sequence stars
- M-type main-sequence stars
- Flare stars
- BY Draconis variables
- Multiple star systems
- Castor Moving Group
- Bayer objects
- Bright Star Catalogue objects
- Durchmusterung objects
- Flamsteed objects
- Gemini (constellation)
- Henry Draper Catalogue objects
- Hipparcos objects
- Objects with variable star designations
- Stars with proper names
- Emission-line stars
- Castor and Pollux
- Astronomical objects discovered in 1718
- Gliese and GJ objects
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