Aging red giant star in the constellation Hercules
98 Herculis
Observation data Epoch J2000 Equinox J2000
Constellation
Hercules
Right ascension
18h 06m 01.90000s[1]
Declination
+22° 13′ 07.9396″[1]
Apparent magnitude (V)
4.96[2]
Characteristics
Spectral type
M3-SIII[3] or M3IIIBa0.2[4]
B−V color index
1.656±0.062[2]
Variable type
suspected[5]
Astrometry
Radial velocity (Rv)
−19.48±0.21[2] km/s
Proper motion (μ)
RA: −12.028[1] mas/yr Dec.: −6.067[1] mas/yr
Parallax (π)
5.5201 ± 0.1610 mas[1]
Distance
590 ± 20 ly (181 ± 5 pc)
Absolute magnitude (MV)
−1.78[2]
Details
Radius
85.39+10.72 −8.50[1]R☉
Luminosity
1,329.7±44.7[1]L☉
Temperature
3,772+203 −217[1] K
Other designations
98 Her, NSV 10208, BD+22°3273, HD 165625, HIP 88657, HR 6765, SAO 85725[6]
Database references
SIMBAD
data
98 Herculis is a single[7] star located approximately 590[1] light years from the Sun in the northern constellation Hercules. It is visible to the naked eye as a dim, red-hued point of light with an apparent visual magnitude of 4.96.[2] The brightness of the star is diminished by an extinction of 0.19 due to interstellar dust.[8] The star is moving closer to the Earth with a heliocentric radial velocity of −19 km/s.[2]
This is an aging red giant star on the asymptotic giant branch[9] with a stellar classification of M3-SIII,[3] where the suffix notation indicating this is an S-type star. It is a mild barium star with an intensity class of 0.2,[10][4] and is a suspected variable star, although Percy and Shepherd (1992) were unable to confirm this.[11] With the hydrogen at its core exhausted, the star has expanded to around 85[1] times the Sun's radius. It is radiating 1,330[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,772 K.[1]
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^Cite error: The named reference Percy1992 was invoked but never defined (see the help page).
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