Eta Persei

Eta Persei (η Persei, abbreviated Eta Per, η Per), is a binary star and the 'A' component of a triple star system (the 'B' component is the star HD 237009) in the constellation of Perseus. It is approximately 1331 light-years away from Earth.

η Persei
Location of η Per (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 02h 50m 41.766s
Declination +55° 53 43.7876
Apparent magnitude (V) 3.79
Characteristics
Spectral type K3 Ib
U−B color index +1.90
B−V color index +1.69
Astrometry
Radial velocity (Rv)1.07 ± 0.27 km/s
Proper motion (μ) RA: +16.574 mas/yr
Dec.: 12.709 mas/yr
Parallax (π)4.2061 ± 0.3744 mas
Distance780 ± 70 ly
(240 ± 20 pc)
Absolute magnitude (MV)4.29
Details
Radius134 R
Luminosity4,130 L
Temperature3,986±170 K
Rotational velocity (v sin i)5.8 km/s
Other designations
Miram, η Persei, η Per, Eta Per, 15 Persei, BD+55 714, CCDM J02506+5553A, FK5 99, GC 3390, HD 17506, HIP 13268, HR 834, IDS 02434+5529 A, PPM 28039, SAO 23655, WDS J02507+5554A
Database references
SIMBADdata

The two components of Eta Persei itself are designated Eta Persei A (officially named Miram /ˈmræm/, a recent name for the system) and B.

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