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Mu Coronae Borealis
Star in the constellation Corona Borealis
Star in the constellation Corona Borealis
| b-v = +1.64 | u-b = +2.01 Mu Coronae Borealis, Latinized from μ Coronae Borealis, is a solitary, ruby-hued star located in the northern constellation of Corona Borealis. It is faintly visible to the naked eye, having an apparent visual magnitude of 5.12. Based upon an annual parallax shift of 5.92 mas, it is located roughly 551 light years from the Sun. This is an evolved red giant star with a stellar classification of M1.5 IIIb. It is currently on the asymptotic giant branch and is a variable star of uncertain type, showing a change in brightness with an amplitude of 0.0147 magnitude and a frequency of 0.02455 cycles per day, or 40.7 days/cycle. On average, it is radiating 2,512 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,600 K.
References
References
- {{cite Gaia DR3. 1377362206141270272
- (2021). "Direct Measurements of Giant Star Effective Temperatures and Linear Radii: Calibration against Spectral Types and V - K Color". The Astrophysical Journal.
- (2020). "Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era". Astronomy and Astrophysics.
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