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Iota Persei

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Iota Persei

Stars of Perseus
Observation data
Epoch J2000      Equinox J2000
Constellation Perseus
Right ascension 03h 09m 04.02s
Declination +49° 36′ 47.8″
Apparent magnitude (V) 4.05
Characteristics
Spectral type G0 V
U−B color index 0.12
B−V color index 0.60
Variable type None
Astrometry
Radial velocity (Rv)+50.0 km/s
Proper motion (μ) RA: 1262.18 mas/yr
Dec.: -91.60 mas/yr
Parallax (π)94.93 ± 0.67 mas
Distance34.4 ± 0.2 ly
(10.53 ± 0.07 pc)
Absolute magnitude (MV)3.94
Details
Mass1.3 M
Radius1.08 R
Luminosity2.2 L
Temperature5,945 K
Metallicity108% Sun
Rotation<10 km/s.
Age8.1 × 109 years
Other designations
GJ 124, HR 937, BD +49°857, HD 19373, LHS 166, LTT 11020, GCTP 647.00, SAO 38597, FK5 112, LFT 256, HIP 14632.

Iota Persei (ι Per / ι Persei) is a main sequence dwarf star in the constellation Perseus. It is somewhat larger and greater in mass than the Sun, and is located about 34 light years distant. Iota Persei has a relatively high proper motion across the sky, and moves at a net velocity of 92 km/s, relative to the Sun.

No sub-stellar companions to this star have yet been found. There is a 12th-magnitude line of sight companion star that is not believed to be gravitationally associated with Iota Persei.

Cultural references

  • "Iota Persei". SolStation. Retrieved 2006-07-25.
  • "Gl 124". ARICNS. Retrieved 2006-07-25.
  • "Iota Per". Prof. Jim Kaler. Retrieved 2006-07-25.
  • "HD 19373 -- High proper-motion Star". SIMBAD. Retrieved 2006-07-25.
  • "ι Persei". Alcyone ephemeris. Retrieved 2006-07-25.