
Star profile
Sigma Persei
What is Sigma Persei
Sigma Persei is an orange giant glowing on the flank of the hero Perseus, some three hundred and sixty light-years away from us. Its warm tone contrasts with the brilliant white and bluish stars that dominate the rest of the constellation, an elegant reminder that the sky is built from very different stellar generations. The light we now see set out when the Inquisition was still interrogating Galileo in Rome and modern astronomy was barely emerging from the newly invented telescope.
Where it is and when to see it
Sigma Persei lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is November, when it culminates around midnight.
- From London it never sets and culminates about 86° up.
- From New York it culminates about 83° above the horizon.
- From Sydney it culminates about 8° above the horizon.
It can be seen from anywhere north of 42° S.
It ranks no. 23 in brightness among the 99 stars of Perseus in our catalogue. To find it, start from Mirfak, the brightest: it lies about 2° away (a fist at arm's length covers about 10°).
The light you see today left it about 360 years ago.
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A public signature from a real person. The chosen name is a symbolic denomination within Stelvia, with no official standing or IAU recognition: the sky is not for sale and belongs to no one.
Astronomical data for Sigma Persei
- Constellation
- Perseus
- Apparent magnitude
- 4.36
- Distance
- 359.6 light years
- Coordinates (J2000)
- RA 52.644° · Dec 47.995°
- Catalogue
- HIP 16335 · HD 21552
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Other stars in Perseus
Perseus has 99 stars in Stelvia's catalogue. Here are a few of them.
- MirfakAlpha Persei1.79
- AlgolBeta Persei2.09
- Zeta Persei2.84
- Lambda Persei4.25
- 58 Persei4.25
- Psi Persei4.32
- 17 Persei4.56
- HIP 200704.60