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HIP 6191 The Sun
Surface temperature
3,890 K
Radius
10 × the Sun
Luminosity
20.8 × the Sun
Spectral type
M6III
Diagram, not a photograph. Colour from the star’s measured colour index; size from its luminosity and temperature, drawn to one scale with the Sun. Source: HYG stellar database.

Cataloged star · Database record + computed analysis

HIP 6191

HIP 6191 · HD 7861

A real star from the HYG catalog in the constellation Cassiopeia.

776.6 light-years away Apparent magnitude 8.44

M-type: red dwarf

Its spectral type is M6III: 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 3,894 K (3,621 °C), an estimate computed from the catalog's color index.

How far away is it?

It lies about 777 light-years away (238.1 parsecs, from its measured parallax). The light reaching Earth tonight left it around the year 1,249.

How powerful is it?

Its computed luminosity is about 20.8 times the Sun's output (derived from its brightness and distance).

Can you see it?

At apparent magnitude 8.44, it is invisible to the naked eye, though binoculars will show it. It favors northern observers.

It varies

This is a catalogued variable star (AA): 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.