9 Equulei
{{Short description|Star in the constellation Equuleus}}
{{Starbox begin
|name = 9 Equulei
}}
{{Starbox observe
|epoch = J2000
|constell = Equuleus
}}
{{Starbox character
}}
{{Starbox astrometry
|radial_v = {{val|-21.82|0.30}}
|prop_mo_ra = {{val|43.871|0.274}}
|prop_mo_dec = {{val|-17.822|0.261}}
|parallax = 4.3895
|p_error = 0.1647
|dist_ly =
|dist_pc =
}}
{{Starbox detail
|mass =
|metal_fe =
|gravity =
|rotational_velocity=
|age_byr =
}}
{{Starbox catalog
|names = HIP 105413, HD 203291, HR 8163, SAO 126719
}}
{{Starbox reference|Simbad=9+Equ}}
{{Starbox end}}
9 Equulei is an M-type star in the constellation Equuleus. It is an asymptotic giant branch (AGB) star, a star that has exhausted its core helium and is now fusing both hydrogen and helium in shells outside the core. It is also a suspected variable star with an amplitude of about 0.05 magnitudes.
The spectral type is M2IIIa, meaning it is a relatively cool giant star. As an AGB star, it is burning hydrogen and helium in shells around an inert carbon-oxygen core. It has expanded to 58 times the radius of the Sun, and it radiates 720 times as much electromagnetic radiation from a photosphere with an effective temperature of {{val|3,920|fmt=commas|ul=K}}.
References
{{Reflist|refs=
{{cite DR2|1739724370656639360}}
}}
{{Stars of Equuleus}}
{{DEFAULTSORT:9 Equulei}}