| absmag_v= {{Val|−2.06|0.07}}[11]
}}{{Starbox orbit
| reference = [11]
| period_unitless = 7.38090 d
| axis =
| axis_unitless =
| eccentricity = {{Val|0.344|0.021}}
| inclination =
| node =
| periastron = {{Val|2455143.254|0.067|u=HJD}}
| periarg = {{Val|160.5|4.5}}
| periarg_primary =
| k1 = {{Val|0.344|0.021}}
| k2 =
}}{{Starbox detail
| component1 = μ Eri A
| mass = {{Val|6.2|0.2}}[11]
| radius = 6.1[7]
| luminosity = 1,905[7]
| temperature = 15,668[7]
| gravity = 3.5[11]
| metal_fe = 0[11]
| rotational_velocity = {{Val|130|3}}[7]
| rotation =
| age_myr =
}}{{Starbox catalog
| names = μ Eri, BD-03° 876, 57 Eridani, FK5 176, HD 30211, HIP 22109, HR 1520, SAO 131468.[20]
}}{{Starbox reference
| Simbad = mu+Eri
}}{{Starbox end}}Mu Eridani (μ Eridani) is a binary star system in the constellation Eridanus. It is visible to the naked eye with an apparent visual magnitude of 4.00.[3] Based upon an annual parallax shift of 0.00625 arcseconds,[ it is located roughly 520 light years from the Sun.]
In 1910, this was determined to be a single-lined spectroscopic binary star system. The pair orbit each other with a period of 7.38 days and an eccentricity of 0.344, during which they undergo Algol-like eclipses.[11] The primary is a slowly pulsating B-type star[7] with a stellar classification of B5 IV.[4] It has a relatively high rate of rotation with a projected rotational velocity of 130 km/s, which is at least 30% of the star's break-up velocity.[7] The star has about six times the Sun's mass and radius, and it shines with 1,905 times the solar luminosity from its outer atmosphere at an effective temperature of 15,668 K.[11][7]
References
1. ^1 2 3 4 5 6 7 8 {{citation | title=Oscillation modes in the rapidly rotating slowly pulsating B-type star μ Eridani | display-authors=1 | last1=Daszyńska-Daszkiewicz | first1=J. | last2=Dziembowski | first2=W. A. | last3=Jerzykiewicz | first3=M. | last4=Handler | first4=G. | journal=Monthly Notices of the Royal Astronomical Society | volume=446 | issue=2 | pages=1438–1448 | date=January 2015 | doi=10.1093/mnras/stu2216 | bibcode=2015MNRAS.446.1438D | arxiv=1410.6283 | postscript=. }}
2. ^1 2 3 4 {{citation | display-authors=1 | last1=Crawford | first1=D. L. | last2=Barnes | first2=J. V. | last3=Golson | first3=J. C. | title=Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere | journal=The Astronomical Journal | year=1971 | pages=1058 | volume=76 | bibcode=1971AJ.....76.1058C | doi=10.1086/111220 | postscript=. }}
3. ^1 2 {{citation | last1=Levato | first1=H. | title=Rotational velocities and spectral types for a sample of binary systems | journal=Astronomy and Astrophysics Supplement Series | volume=19 | pages=91–99 | date=January 1975 | bibcode=1975A&AS...19...91L | postscript=. }}
4. ^1 2 3 4 5 6 7 {{citation | title=μ Eridani from MOST and from the ground: an orbit, the SPB component's fundamental parameters and the SPB frequencies | display-authors=1 | last1=Jerzykiewicz | first1=M. | last2=Lehmann | first2=H. | last3=Niemczura | first3=E. | last4=Molenda-Żakowicz | first4=J. | last5=Dymitrov | first5=W. | last6=Fagas | first6=M. | last7=Guenther | first7=D. B. | last8=Hartmann | first8=M. | last9=Hrudková | first9=M. | last10=Kamiński | first10=K. | last11=Moffat | first11=A. F. J. | last12=Kuschnig | first12=R. | last13=Leto | first13=G. | last14=Matthews | first14=J. M. | last15=Rowe | first15=J. F. | last16=Ruciński | first16=S. M. | last17=Sasselov | first17=D. | last18=Weiss | first18=W. W. | journal=Monthly Notices of the Royal Astronomical Society | volume=432 | issue=2 | pages=1032–1045 | date=June 2013 | doi=10.1093/mnras/stt522 | bibcode=2013MNRAS.432.1032J | arxiv=1303.6812 | postscript=. }}
5. ^1 {{cite simbad | title=mu. Eri | accessdate=2016-11-01 | postscript=. }}