95 Herculis
{{Short description|Double star in the constellation Hercules}}
{{Starbox begin
|name=95 Herculis
}}
{{Starbox image
|image={{Location mark
|image=Hercules constellation map.png|alt=|float=center|width=220
|label=|position=right
|mark=Red circle.svg|mark_width=10
|x=238|y=724
}}
|caption=Location of 95 Herculis in Hercules (circled)
}}
{{Starbox observe 2s
|epoch=J2000
|equinox=J2000
|constell=Hercules
|component1=A
|component2=B
}}
{{Starbox character
|component1=A
|component2=B
|type2=Giant star
}}
{{Starbox astrometry
|component1=A
|radial_v = {{val|-44.86|3.07}}
|prop_mo_ra = +9.200
|prop_mo_dec = +38.438
|parallax = 7.5526
|p_error = 0.0713
|component2 = B
|radial_v2 = {{val|-32.9|0.12}}
|prop_mo_ra2 = +8.995
|prop_mo_dec2 = +36.267
|parallax2 = 7.5492
|p_error2 = 0.0592
}}
{{Starbox detail
|component1 = A
|mass = 2.8
|radius = 6.8
|luminosity = 167
|temperature = 8,000
|rotational_velocity = 233
|component2 = B
|mass2 = 3.2
|radius2 = 19.4
|luminosity2 = 194
|temperature2 = 4,900
|rotational_velocity2 = 5.7
}}
{{Starbox catalog
|names = {{odlist|WDS=J18015+2136|ADS=10993|HIP=88267}}
|component1 = A
|names1 = {{odlist|HD=164669|ADS=10993|HR=6730|TIC=424429430|TYC=1566-3674-1}}
|component2 = B
|names2 = {{odlist|HD=164668|HR=6729|TIC=424429431|TYC=1566-3675-1}}
}}
{{Starbox reference
| Simbad = 95+Her
}}
{{Starbox reference
|no_heading=y
| component = A
| Simbad = 95+Her+A
}}
{{Starbox reference
|no_heading=y
| component = B
| Simbad = 95+Her+B
}}
{{Starbox end}}
95 Herculis is a double stellar system in the constellation Hercules, located 432 light-years from Earth.
Characteristics
From the naked eye, 95 Herculis appears as a single star shining at apparent magnitude 4.31. However, when further scrutinized using a telescope, it is revealed to be a double star, with two components separated by 6.3 arcseconds. This system has a color contrast due to the difference of each star's effective temperature.
The brightest component, called 95 Herculis A, is a white giant or subgiant with an apparent magnitude of 4.8. This evolved star has 2.9 times more mass than the Sun, is 6.8 times wider, and is 167 times more luminous. Its effective temperature of 8,000 Kelvin give it a blue-white hue typical of A-type stars. It is spinning rapidly with an projected rotational velocity of 233 km/s.
The secondary is called 95 Herculis B, a yellow giant of apparent magnitude 5.1. It is the most evolved star in the pair, having reached helium burning stage and now converting carbon into oxygen, while 95 Herculis A is still in the transition from hydrogen burning to helium burning. Albeit fainter than 95 Her A, 95 Her B emmits a significant part of its luminosity in the infrared, and hence the bolometric luminosity is 194 times solar. It is 3.2 times more massive than the Sun and 19 times wider. The effective temperature of the star is 4,900 Kelvin.
Orbit
The orbital elements 95 Herculis are not accurately known and no orbital motion has been detected. However, they projected separation is calculated at 900 astronomical units, with an orbital period of at least 11,000 years.
See also
References
{{Reflist|refs=
{{cite DR3|4576147844112599424}}
{{cite DR3|4576147848417217536}}
{{cite simbad|title=95 Her A|access-date=2024-09-15}}
{{cite simbad|title=95 Her B|access-date=2024-09-15}}
}}
{{Hercules (constellation)}}