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The name was discussed by IAU WGSN in 2018 but no action was taken. The name may be revisited in a future WGSN meeting.   
The name was discussed by IAU WGSN in 2018 but no action was taken. The name may be revisited in a future WGSN meeting.   


Mu Aquilae lacks a proper name in SIMBAD, [[wikipedia:Mu_Aquilae|wikipedia]], Bright Star Catalog (4th, 5th editions), and Kunitzsch & Smart (2006).  
As of early 2026, through search of astronomical catalogs and books currently available to WGSN yielded no previously known historical names for the star μ Aql (Mu Aquilae), including popular sources like [https://simbad.cds.unistra.fr/simbad/sim-id?Ident=mu+Aql SIMBAD], [[wikipedia:Mu_Aquilae|wikipedia]], Bright Star Catalog (4th, 5th editions), and Kunitzsch & Smart (2006). The star μ Aql (HR 7429, HD 184406, HR 7429, GJ 9661) is a relatively nearby (34 parsecs) K giant with apparent Johnson V magnitude of 4.45. It does not have any known stellar or planetary companions as of early 2026. 
 
Note that μ Aql (sometimes abbreviated as mu Aql or the Latinized Mu Aquilae) is NOT the same as the variable star MU Aql. 
 
== Weblinks ==
== Weblinks ==



Revision as of 16:07, 6 June 2026

Wardaman constellations and star names in Aquila from Cairns and Harney (2004, 198).

Bardardi, a ceremonial meeting place, is a name for an asterism in Aquila from the Australian Wardaman people.

Etymology and History

"Bardardi" is the Wardaman Aboriginal name from Cairns & Harney (2003,[1] p.198) for a ceremonial meeting place.

Mythology

IAU Working Group on Star Names

The name was discussed by IAU WGSN in 2018 but no action was taken. The name may be revisited in a future WGSN meeting.

As of early 2026, through search of astronomical catalogs and books currently available to WGSN yielded no previously known historical names for the star μ Aql (Mu Aquilae), including popular sources like SIMBAD, wikipedia, Bright Star Catalog (4th, 5th editions), and Kunitzsch & Smart (2006). The star μ Aql (HR 7429, HD 184406, HR 7429, GJ 9661) is a relatively nearby (34 parsecs) K giant with apparent Johnson V magnitude of 4.45. It does not have any known stellar or planetary companions as of early 2026.

Note that μ Aql (sometimes abbreviated as mu Aql or the Latinized Mu Aquilae) is NOT the same as the variable star MU Aql.

Reference

  1. ↑ Cairns, H. and Harney, B.Y. (2003) Dark Sparklers - Yidumduma's Aboriginal Astronomy. H.C. Cairns, Merimbula, NSW