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106 Herculis
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Binary star system in the constellation Hercules
250px A light curve for 106 Herculis, plotted from TESS data
J2000
Hercules
18 20 17.91482
+21 57 40.6622
4.96
AGB
M0 III
+1.58
+1.98
suspected SR
-35.20 0.29
+18.105
-59.631
8.5067
0.1739
−0.664
44.32 2.70 5.89
3789 6 commas
414.1 9.7
1.56 0.09
0.00 0.03
5.0 1.0
106 Her +21°3390 168720 89861 6868 85941 24405
106+Her
106 Herculis is a variable star in the northern constellation Hercules. It is visible to the naked eye as a faint, red-hued point of light with a baseline apparent visual magnitude of 4.96. Based on its parallax, it is estimated to lie 383 ly pc off away from the Sun. The star is moving closer to the Earth with a heliocentric radial velocity of -35 km/s.
Eggleton and Tokovinin (2008) listed this as a suspected binary star system consisting of two roughly equal components. It appears as an ageing red giant with a stellar classification of M0III. This is a suspected semiregular variable star with a very small amplitude and a period of 40 days or more. Having exhausted the supply of hydrogen at its core, it has expanded to 44 times the Sun's radius. It is radiating around 414 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of about commas 3,789 K.
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Category:M-type giants
Category:Semiregular variable stars
Category:Hercules (constellation)
Category:Durchmusterung objects
Herculis, 106
168720
089861
6868
Category:Suspected variables