Iota Persei
A yellow-white main-sequence star 34.5 light years away.
Iota Persei is a single star in the northern constellation Perseus, visible to the naked eye as a faint, yellow-white point of light. It is a late F- or early G-type main-sequence star located 34.5 light years from the Sun, with a relatively high proper motion and a radial velocity of +49 km/s.
Quick Facts
- Apparent visual magnitude
- 4.1
- Distance from sun
- 34.5 light years
- Radial velocity
- +49 km/s
- Stellar classification
- around G0V
- Mass
- 1.1 times the Sun
- Radius
- 1.383 times the Sun
- Luminosity
- 2.02 times the Sun
- Effective temperature
- 5,849 K
Facts from the source article.
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