- Surface temperature
- 3,520 K
- Radius
- 0.07 × the Sun
- Luminosity
- 0.001 × the Sun
- Spectral type
- M5Ve
Cataloged star · Database record + computed analysis
HIP 34603
HIP 34603
A real star from the HYG catalog in the constellation Auriga.
M-type: red dwarf
Its spectral type is M5Ve: the galaxy's most common stars: small, cool, dim, flare-prone, and able to burn for trillions of years. From its measured color, its surface temperature is roughly 3,516 K (3,242 °C), an estimate computed from the catalog's color index.
How far away is it?
It lies 20.5 light-years away (6.29 parsecs, from its measured parallax), within the Sun's wider neighborhood; its light is only 20.5 years old when it reaches your eye.
How powerful is it?
Its computed luminosity is only 0.000755 of the Sun's output, a modest lamp by stellar standards (derived from its brightness and distance).
Can you see it?
At apparent magnitude 11.65, it is a telescope target only. It favors northern observers.
It varies
This is a catalogued variable star (QY): its brightness measurably changes over time, whether by pulsation, eclipses in a double system, or surface activity.
Everything above is computed from the catalog’s measured values for this star. Where a value is missing, the statement is omitted rather than guessed.
About this record
Data: the HYG stellar database v4.1 (Hipparcos + Yale + Gliese, CC BY-SA, © David Nash / astronexus). Want the full stories? Our deep star guides cover Sirius, Betelgeuse, Proxima Centauri, Vega and three dozen more. You can also browse the catalog or learn how stars live and die.