
Star profile
Pi Coronae Borealis
What is Pi Coronae Borealis
Pi Coronae Borealis is a yellow G-type giant some 243 light-years away, set in the small northern crown. This constellation, a semicircle of faint stars, evokes the crown of Ariadne thrown into the sky by Dionysus in Greek myth. Pi is one of the secondary lights surrounding bright Alphecca, the jewel of the band, lending volume and depth to the delicate celestial arc.
Where it is and when to see it
Pi Coronae Borealis lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is May, when it culminates around midnight.
- From London it culminates about 71° above the horizon.
- From New York it culminates about 82° above the horizon.
- From Sydney it culminates about 24° above the horizon.
It can be seen from anywhere north of 57° S.
It ranks no. 20 in brightness among the 26 stars of Corona Borealis in our catalogue. To find it, start from Alphecca, the brightest: it lies about 6° away (a fist at arm's length covers about 10°).
The light you see today left it about 240 years ago.
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Astronomical data for Pi Coronae Borealis
- Constellation
- Corona Borealis
- Apparent magnitude
- 5.57
- Distance
- 243.4 light years
- Coordinates (J2000)
- RA 235.997° · Dec 32.516°
- Catalogue
- HIP 77048 · HD 140716
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Other stars in Corona Borealis
Corona Borealis has 26 stars in Stelvia's catalogue. Here are a few of them.
- AlpheccaAlpha Coronae Borealis2.22
- NusakanBeta Coronae Borealis3.66
- Gamma Coronae Borealis3.81
- Nu 2 Coronae Borealis5.40
- Lambda Coronae Borealis5.43
- Omicron Coronae Borealis5.51
- HIP 782765.61
- HIP 793585.62