Star

Iota Persei

Iota Persei is a main-sequence or subgiant star included in the CosmoInsider stellar archive.

Verified 2026-10-02

Overview

This profile synchronizes the identity, classification and physical parameters of Iota Persei. Its adopted radius is 1.4124 solar radii. The measurement comes from Boyajian et al. · 2013 · tabla 3 and retains its method and uncertainty when available.

Essential data

Key fact
stellar_scale
Key fact
1.4124
Key fact
G0IV-V
Key fact
Perseo

Physical properties

Measurement
1.4124
Radius
982606.68
Measurement
5838
Measurement
1.097
Measurement
2.0781
Measurement
34.32
Distance
10.5407
Measurement
49.5

Sources and references

  1. Boyajian et al. · 2013 · tabla 3 arXiv
  2. HD 19373 — SIMBAD object record Centre de Données astronomiques de Strasbourg
  3. HYG 4.1-c7f7f883 HYG