Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius.The combined apparent visual magnitude of the pair is +3.04, making it one of the brighter members of Scorpius. The combined apparent visual magnitude of the pair is +3.04,[2] making it one of the brighter members of Scorpius. [10] It approved the name Xamidimura for the component Mu¹ Scorpii Aa on 5 September 2017 (along with Pipirima for the partner of Mu¹ Scorpii) and it is now so included in the List of IAU-approved Star Names.

Mu Scorpii Reviews They are separated too by the different asterism in Chinese astronomy.

[8], In 2016, the IAU organized a Working Group on Star Names (WGSN)[9] to catalog and standardize proper names for stars.

Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). Keep reading for comprehensive facts and information.

Mu Scorpii Sargas. [12], Astronomical Society of Southern Africa (2013), Monthly Notices of the Royal Astronomical Society, Commonwealth Scientific and Industrial Research Organisation, "WG Triennial Report (2015-2018) - Star Names", https://en.wikipedia.org/w/index.php?title=Mu1_Scorpii&oldid=949957563, Articles with Chinese-language sources (zh), Articles containing Chinese-language text, Creative Commons Attribution-ShareAlike License, This page was last edited on 9 April 2020, at 13:48. Location It is formed by Sargas with Xamidimura (Mu 1 Scorpii), Larawag (Epsilon Scorpii), Zeta 1 and Zeta 2 Scorpii, Eta Scorpii, Iota 1 Scorpii, Kappa Scorpii, Shaula (Lambda Scorpii), and Lesath (Upsilon Scorpii). The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.

It is the primary component of the Theta Scorpii binary star system. Antares. Theta Scorpii is an evolved bright yellow giant star of spectral type F0 II. The secondary is a smaller B-type main sequence star with a classification of Mu Scorpii B6. For other star systems with this Bayer designation, see Mu Scorpii.. Mu² Scorpii (μ² Sco, μ² Scorpii) is a star in the constellation Scorpius.. μ² Scorpii is a blue-white B-type subgiant with an apparent magnitude of +3.56.

In Polynesian mythology, Nu Scorpii (ν Scorpii, abbreviated Nu Sco, ν Sco) is a multiple star system in the constellation of Scorpius.It is most likely a septuple star system, consisting of two close groups (designated Nu Scorpii AB and CD) that are separated by 41 arcseconds. [16], Monthly Notices of the Royal Astronomical Society, Centre de données astronomiques de Strasbourg, AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日, The beautiful maidens from the Once, Upon a Reef, https://en.wikipedia.org/w/index.php?title=Mu2_Scorpii&oldid=973582434, Articles with Chinese-language sources (zh), Articles with unsourced statements from April 2019, Creative Commons Attribution-ShareAlike License, This page was last edited on 18 August 2020, at 01:47. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. In Tahiti, a traditional story is told of a brother and sister, named Pipiri and Rehua, who flee their parents into the sky and become stars. [7], The pair of stars Mu¹ and Mu² Scorpii are known as the xami di mura 'eyes of the lion' by the Khoikhoi people of South Africa. Primary / Proper / Traditional Name: Pipirima: Alternative Names: Mu2 Scorpii, Mu.02 Sco, HD 151985, HIP 82545, HR 6252: Spectral Type: B2IV: Constellation's Main Star Jabbah is a Subgiant Star type star. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. It has an apparent visual magnitude of +3.56,[2] which is bright enough to be seen with the naked eye.

μ¹ Scorpii was a member of asterism 尾 (Wěi), Tail and μ² Scorpii was the sole star in asterism 神宮 (Shéngōng), Changing Room (of the temple). by admin; Posted on 2020-07-25 2020-07-25; Binary Stars; Sargas, Theta Scorpii A (θ Sco A), is a white giant star located in the constellation Scorpius. Mu¹ Scorpii is an eclipsing binary of the Beta Lyrae type. The "optical" double Mu Sco lies directly above it. Jabbah is not part of the Scorpius constellation outline but is within the borders of the constellation.

[13], In 2016, the IAU organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Pipirima for this star on 5 September 2017 (along with Xamidimura for its partner) and it is now so included in the List of IAU-approved Star Names. Above Mu, find Epsilon. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: .

Mu² Scorpii (μ² Scorpii, abbreviated Mu² Sco, μ² Sco), also named Pipirima /pɪˈpɪrɪmə/,[11] is a star in the zodiac constellation of Scorpius. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. Jabbah is a B2IV subgiant star based on the spectral type that was recorded in the Hipparcos star catalogue. The secondary is a smaller B-type main sequence star with a classification of about B6.5 V, having 5.3 times the Sun's mass and 4.4 times the radius of the Sun. [1] It is a member of the Upper Centaurus-Lupus subgroup of the Scorpius–Centaurus Association. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: They are separated too into different asterism in Chinese astronomy. ; Based on the spectral type (B2IV) of the star, the star's colour is blue . Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius. [citation needed] (In a similar version of the story told in the Cook Islands, they become Omega¹ and Omega² Scorpii). With a combined apparent magnitude of […] Read More. [3] It has an estimated 7 times the radius of the Sun, almost 9 times the Sun's mass,[6] and shines with 2,385 times the Sun's luminosity. [11] Consequently, the Chinese name for Mu¹ Scorpii itself is 尾宿一 (Wěi Xiù yī), "the First Star of Tail". Jabbah Facts.

The designations of the primary as Mu¹ Scorpii Aa derives from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). μ¹ Scorpii - a binary star whose primary is named Xamidimura; μ² Scorpii (named Pipirima); They are separated by 0.1° in the sky. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. Both of Mu Scorpii were lied in Tail mansion. The brighter component is an eclipsing binary that varies between magnitudes 2.9 and 3.2 every …

The two stars revolve each other along a circular orbit with the components separated by 12.9 times the Sun's radius. [3], The primary (Mu¹ Scorpii Aa) is formally named Xamidimura /ˌkæmidiˈmʊərə/, from the Khoekhoe xami di mûra IPA: [xami ti mũːɾa] 'the (two) eyes of the lion'.[5]. [11], In Chinese astronomy, Mu² Scorpii is called 尾宿增二. Both asterisms are part of the Tail mansion. Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs).

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Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius.The combined apparent visual magnitude of the pair is +3.04, making it one of the brighter members of Scorpius. The combined apparent visual magnitude of the pair is +3.04,[2] making it one of the brighter members of Scorpius. [10] It approved the name Xamidimura for the component Mu¹ Scorpii Aa on 5 September 2017 (along with Pipirima for the partner of Mu¹ Scorpii) and it is now so included in the List of IAU-approved Star Names.

Mu Scorpii Reviews They are separated too by the different asterism in Chinese astronomy.

[8], In 2016, the IAU organized a Working Group on Star Names (WGSN)[9] to catalog and standardize proper names for stars.

Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). Keep reading for comprehensive facts and information.

Mu Scorpii Sargas. [12], Astronomical Society of Southern Africa (2013), Monthly Notices of the Royal Astronomical Society, Commonwealth Scientific and Industrial Research Organisation, "WG Triennial Report (2015-2018) - Star Names", https://en.wikipedia.org/w/index.php?title=Mu1_Scorpii&oldid=949957563, Articles with Chinese-language sources (zh), Articles containing Chinese-language text, Creative Commons Attribution-ShareAlike License, This page was last edited on 9 April 2020, at 13:48. Location It is formed by Sargas with Xamidimura (Mu 1 Scorpii), Larawag (Epsilon Scorpii), Zeta 1 and Zeta 2 Scorpii, Eta Scorpii, Iota 1 Scorpii, Kappa Scorpii, Shaula (Lambda Scorpii), and Lesath (Upsilon Scorpii). The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.

It is the primary component of the Theta Scorpii binary star system. Antares. Theta Scorpii is an evolved bright yellow giant star of spectral type F0 II. The secondary is a smaller B-type main sequence star with a classification of Mu Scorpii B6. For other star systems with this Bayer designation, see Mu Scorpii.. Mu² Scorpii (μ² Sco, μ² Scorpii) is a star in the constellation Scorpius.. μ² Scorpii is a blue-white B-type subgiant with an apparent magnitude of +3.56.

In Polynesian mythology, Nu Scorpii (ν Scorpii, abbreviated Nu Sco, ν Sco) is a multiple star system in the constellation of Scorpius.It is most likely a septuple star system, consisting of two close groups (designated Nu Scorpii AB and CD) that are separated by 41 arcseconds. [16], Monthly Notices of the Royal Astronomical Society, Centre de données astronomiques de Strasbourg, AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日, The beautiful maidens from the Once, Upon a Reef, https://en.wikipedia.org/w/index.php?title=Mu2_Scorpii&oldid=973582434, Articles with Chinese-language sources (zh), Articles with unsourced statements from April 2019, Creative Commons Attribution-ShareAlike License, This page was last edited on 18 August 2020, at 01:47. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. In Tahiti, a traditional story is told of a brother and sister, named Pipiri and Rehua, who flee their parents into the sky and become stars. [7], The pair of stars Mu¹ and Mu² Scorpii are known as the xami di mura 'eyes of the lion' by the Khoikhoi people of South Africa. Primary / Proper / Traditional Name: Pipirima: Alternative Names: Mu2 Scorpii, Mu.02 Sco, HD 151985, HIP 82545, HR 6252: Spectral Type: B2IV: Constellation's Main Star Jabbah is a Subgiant Star type star. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. It has an apparent visual magnitude of +3.56,[2] which is bright enough to be seen with the naked eye.

μ¹ Scorpii was a member of asterism 尾 (Wěi), Tail and μ² Scorpii was the sole star in asterism 神宮 (Shéngōng), Changing Room (of the temple). by admin; Posted on 2020-07-25 2020-07-25; Binary Stars; Sargas, Theta Scorpii A (θ Sco A), is a white giant star located in the constellation Scorpius. Mu¹ Scorpii is an eclipsing binary of the Beta Lyrae type. The "optical" double Mu Sco lies directly above it. Jabbah is not part of the Scorpius constellation outline but is within the borders of the constellation.

[13], In 2016, the IAU organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Pipirima for this star on 5 September 2017 (along with Xamidimura for its partner) and it is now so included in the List of IAU-approved Star Names. Above Mu, find Epsilon. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: .

Mu² Scorpii (μ² Scorpii, abbreviated Mu² Sco, μ² Sco), also named Pipirima /pɪˈpɪrɪmə/,[11] is a star in the zodiac constellation of Scorpius. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. Jabbah is a B2IV subgiant star based on the spectral type that was recorded in the Hipparcos star catalogue. The secondary is a smaller B-type main sequence star with a classification of about B6.5 V, having 5.3 times the Sun's mass and 4.4 times the radius of the Sun. [1] It is a member of the Upper Centaurus-Lupus subgroup of the Scorpius–Centaurus Association. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: They are separated too into different asterism in Chinese astronomy. ; Based on the spectral type (B2IV) of the star, the star's colour is blue . Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius. [citation needed] (In a similar version of the story told in the Cook Islands, they become Omega¹ and Omega² Scorpii). With a combined apparent magnitude of […] Read More. [3] It has an estimated 7 times the radius of the Sun, almost 9 times the Sun's mass,[6] and shines with 2,385 times the Sun's luminosity. [11] Consequently, the Chinese name for Mu¹ Scorpii itself is 尾宿一 (Wěi Xiù yī), "the First Star of Tail". Jabbah Facts.

The designations of the primary as Mu¹ Scorpii Aa derives from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). μ¹ Scorpii - a binary star whose primary is named Xamidimura; μ² Scorpii (named Pipirima); They are separated by 0.1° in the sky. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. Both of Mu Scorpii were lied in Tail mansion. The brighter component is an eclipsing binary that varies between magnitudes 2.9 and 3.2 every …

The two stars revolve each other along a circular orbit with the components separated by 12.9 times the Sun's radius. [3], The primary (Mu¹ Scorpii Aa) is formally named Xamidimura /ˌkæmidiˈmʊərə/, from the Khoekhoe xami di mûra IPA: [xami ti mũːɾa] 'the (two) eyes of the lion'.[5]. [11], In Chinese astronomy, Mu² Scorpii is called 尾宿增二. Both asterisms are part of the Tail mansion. Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs).

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Sargas (θ Scorpii) Facts Theta Scorpii is located at around 300 light-years away from the Sun. At the western bend in the tail in south central Scorpius lies Zeta Scorpii, which consists of nearby (Zeta-2) and one of the most luminous stars of the Galaxy, Zeta-1. [3] Due to occultation of each component by the other, the apparent magnitude of the system decreased by 0.3 and 0.4 magnitudes over the course of the binary's orbit, which takes 34 hours 42.6 minutes to complete. [5], In Chinese, 尾宿 (Wěi Xiù), meaning Tail, refers to an asterism consisting of Mu¹ Scorpii, Epsilon Scorpii, Zeta¹ Scorpii and Zeta² Scorpii, Eta Scorpii, Theta Scorpii, Iota¹ Scorpii and Iota² Scorpii, Kappa Scorpii, Lambda Scorpii and Upsilon Scorpii. It is approximately 517 light years from Earth.This star has 7.0 times the radius of the Sun and its outer atmosphere has an effective temperature of 23,113 K. [1] Rho Ophiuchi, seen in proper context in Ophiuchus, is above and slightly to the left of Antares. "[13][14] In one account, the children become Shaula and Lesath in the tip of the tail of Scorpio,[13] and in another they become Mu² and Mu¹ Scorpii. μ² Scorpii (Latinised to Mu² Scorpii) is the star's Bayer designation. The Chinese Tail asterism is part of the Tail mansion and represents the tail of the Azure Dragon. [12], This is a blue-white, B-type subgiant star with a stellar classification of B2 IV. Shaula, Lambda Scorpii (λ Sco), is a triple star system located at a distance of about 570 light years from Earth in the direction of the constellation Scorpius.With an apparent magnitude of 1.62, it is the second brightest star in Scorpius, fainter only than the red supergiant Antares.. Shaula is the 24th brightest star in … Based on parallax measurements, it is approximately 470 light-years from the Sun.. The effective temperature of the outer atmosphere for each star is 23,725 K for the primary and 16,850 K for the secondary. Mu² Scorpii (μ² Scorpii, abbreviated Mu² Sco, μ² Sco), also named Pipirima / p i ˈ p iː r i m ɑː /, is a star in the zodiac constellation of Scorpius.It has an apparent visual magnitude of +3.56, which is bright enough to be seen with the naked eye. [1], Index of articles associated with the same name, AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日, https://en.wikipedia.org/w/index.php?title=Mu_Scorpii&oldid=933044532, Articles with Chinese-language sources (zh), Short description is different from Wikidata, Creative Commons Attribution-ShareAlike License, This page was last edited on 29 December 2019, at 17:40.

Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius.The combined apparent visual magnitude of the pair is +3.04, making it one of the brighter members of Scorpius. The combined apparent visual magnitude of the pair is +3.04,[2] making it one of the brighter members of Scorpius. [10] It approved the name Xamidimura for the component Mu¹ Scorpii Aa on 5 September 2017 (along with Pipirima for the partner of Mu¹ Scorpii) and it is now so included in the List of IAU-approved Star Names.

Mu Scorpii Reviews They are separated too by the different asterism in Chinese astronomy.

[8], In 2016, the IAU organized a Working Group on Star Names (WGSN)[9] to catalog and standardize proper names for stars.

Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs). Keep reading for comprehensive facts and information.

Mu Scorpii Sargas. [12], Astronomical Society of Southern Africa (2013), Monthly Notices of the Royal Astronomical Society, Commonwealth Scientific and Industrial Research Organisation, "WG Triennial Report (2015-2018) - Star Names", https://en.wikipedia.org/w/index.php?title=Mu1_Scorpii&oldid=949957563, Articles with Chinese-language sources (zh), Articles containing Chinese-language text, Creative Commons Attribution-ShareAlike License, This page was last edited on 9 April 2020, at 13:48. Location It is formed by Sargas with Xamidimura (Mu 1 Scorpii), Larawag (Epsilon Scorpii), Zeta 1 and Zeta 2 Scorpii, Eta Scorpii, Iota 1 Scorpii, Kappa Scorpii, Shaula (Lambda Scorpii), and Lesath (Upsilon Scorpii). The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.

It is the primary component of the Theta Scorpii binary star system. Antares. Theta Scorpii is an evolved bright yellow giant star of spectral type F0 II. The secondary is a smaller B-type main sequence star with a classification of Mu Scorpii B6. For other star systems with this Bayer designation, see Mu Scorpii.. Mu² Scorpii (μ² Sco, μ² Scorpii) is a star in the constellation Scorpius.. μ² Scorpii is a blue-white B-type subgiant with an apparent magnitude of +3.56.

In Polynesian mythology, Nu Scorpii (ν Scorpii, abbreviated Nu Sco, ν Sco) is a multiple star system in the constellation of Scorpius.It is most likely a septuple star system, consisting of two close groups (designated Nu Scorpii AB and CD) that are separated by 41 arcseconds. [16], Monthly Notices of the Royal Astronomical Society, Centre de données astronomiques de Strasbourg, AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日, The beautiful maidens from the Once, Upon a Reef, https://en.wikipedia.org/w/index.php?title=Mu2_Scorpii&oldid=973582434, Articles with Chinese-language sources (zh), Articles with unsourced statements from April 2019, Creative Commons Attribution-ShareAlike License, This page was last edited on 18 August 2020, at 01:47. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. In Tahiti, a traditional story is told of a brother and sister, named Pipiri and Rehua, who flee their parents into the sky and become stars. [7], The pair of stars Mu¹ and Mu² Scorpii are known as the xami di mura 'eyes of the lion' by the Khoikhoi people of South Africa. Primary / Proper / Traditional Name: Pipirima: Alternative Names: Mu2 Scorpii, Mu.02 Sco, HD 151985, HIP 82545, HR 6252: Spectral Type: B2IV: Constellation's Main Star Jabbah is a Subgiant Star type star. Its distance from the Sun is about 474 light-years, as determined by parallax measurements. It has an apparent visual magnitude of +3.56,[2] which is bright enough to be seen with the naked eye.

μ¹ Scorpii was a member of asterism 尾 (Wěi), Tail and μ² Scorpii was the sole star in asterism 神宮 (Shéngōng), Changing Room (of the temple). by admin; Posted on 2020-07-25 2020-07-25; Binary Stars; Sargas, Theta Scorpii A (θ Sco A), is a white giant star located in the constellation Scorpius. Mu¹ Scorpii is an eclipsing binary of the Beta Lyrae type. The "optical" double Mu Sco lies directly above it. Jabbah is not part of the Scorpius constellation outline but is within the borders of the constellation.

[13], In 2016, the IAU organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Pipirima for this star on 5 September 2017 (along with Xamidimura for its partner) and it is now so included in the List of IAU-approved Star Names. Above Mu, find Epsilon. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: .

Mu² Scorpii (μ² Scorpii, abbreviated Mu² Sco, μ² Sco), also named Pipirima /pɪˈpɪrɪmə/,[11] is a star in the zodiac constellation of Scorpius. Discovered to be a spectroscopic binary by Solon Irving Bailey in 1896, it was only the third such eclipsing pair to be discovered. Jabbah is a B2IV subgiant star based on the spectral type that was recorded in the Hipparcos star catalogue. The secondary is a smaller B-type main sequence star with a classification of about B6.5 V, having 5.3 times the Sun's mass and 4.4 times the radius of the Sun. [1] It is a member of the Upper Centaurus-Lupus subgroup of the Scorpius–Centaurus Association. The Bayer designation Mu Scorpii (μ Sco, μ Scorpii) is shared by two star systems, in the constellation Scorpius: They are separated too into different asterism in Chinese astronomy. ; Based on the spectral type (B2IV) of the star, the star's colour is blue . Mu¹ Scorpii (μ¹ Scorpii, abbreviated Mu¹ Sco, μ¹ Sco) is a binary star system in the southern zodiac constellation of Scorpius. [citation needed] (In a similar version of the story told in the Cook Islands, they become Omega¹ and Omega² Scorpii). With a combined apparent magnitude of […] Read More. [3] It has an estimated 7 times the radius of the Sun, almost 9 times the Sun's mass,[6] and shines with 2,385 times the Sun's luminosity. [11] Consequently, the Chinese name for Mu¹ Scorpii itself is 尾宿一 (Wěi Xiù yī), "the First Star of Tail". Jabbah Facts.

The designations of the primary as Mu¹ Scorpii Aa derives from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). μ¹ Scorpii - a binary star whose primary is named Xamidimura; μ² Scorpii (named Pipirima); They are separated by 0.1° in the sky. This is a semidetached binary system where the secondary is close to filling its Roche lobe, or it may even be overflowing. Both of Mu Scorpii were lied in Tail mansion. The brighter component is an eclipsing binary that varies between magnitudes 2.9 and 3.2 every …

The two stars revolve each other along a circular orbit with the components separated by 12.9 times the Sun's radius. [3], The primary (Mu¹ Scorpii Aa) is formally named Xamidimura /ˌkæmidiˈmʊərə/, from the Khoekhoe xami di mûra IPA: [xami ti mũːɾa] 'the (two) eyes of the lion'.[5]. [11], In Chinese astronomy, Mu² Scorpii is called 尾宿增二. Both asterisms are part of the Tail mansion. Based upon parallax measurements, the distance of this system from the Sun is roughly 500 light-years (150 parsecs).

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