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98 Herculis

Aging red giant star in the constellation Hercules From Wikipedia, the free encyclopedia

98 Herculis is a single[9] 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.[10] The star is moving closer to the Earth with a heliocentric radial velocity of −19 km/s.[2]

Quick facts Constellation, Right ascension ...
98 Herculis
Observation data
Epoch J2000      Equinox ICRS
Constellation Hercules
Right ascension 18h 06m 01.90000s[1]
Declination +22° 13 07.9396[1]
Apparent magnitude (V) 4.96[2]
Characteristics
Evolutionary stage AGB[3]
Spectral type M3-SIII[4] or M3IIIBa0.2[5]
B−V color index 1.656±0.062[2]
Variable type suspected[6]
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]
Distance590 ± 20 ly
(181 ± 5 pc)
Absolute magnitude (MV)−1.78[2]
Details
Mass1.35[7] M
Radius85.39+10.72
−8.50
[1] R
Luminosity1,329.7±44.7[1] L
Surface gravity (log g)1.45[7] cgs
Temperature3,772+203
−217
[1] K
Metallicity [Fe/H]−0.08[7] dex
Other designations
98 Her, NSV 10208, BD+22°3273, HD 165625, HIP 88657, HR 6765, SAO 85725[8]
Database references
SIMBADdata
Close

This is an aging red giant star on the asymptotic giant branch[3] with a stellar classification of M3-SIII,[4] where the suffix notation indicating this is an S-type star. It is a mild barium star with an intensity class of 0.2,[11][5] and is a suspected variable star, although Percy and Shepherd (1992) were unable to confirm this.[12] 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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