
Star profile
Chi Phoenicis
What is Chi Phoenicis
Chi Phoenicis is an orange K-type star in the southern Phoenix, a constellation that the Dutch navigators Keyser and de Houtman drew at the close of the sixteenth century during their voyages to the East Indies. About 375 light-years away, its warm hue contrasts with the more common blues of the recent southern figures, giving it a discreet role in the plumage of the bird reborn from its ashes.
Where it is and when to see it
Chi Phoenicis lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is September, when it culminates around midnight.
- From London it never rises above the horizon.
- From New York it culminates about 5° above the horizon.
- From Sydney it culminates about 79° above the horizon.
It can be seen from anywhere south of 45° N.
It ranks no. 18 in brightness among the 39 stars of Phoenix in our catalogue. To find it, start from Ankaa, the brightest: it lies about 17° away (a fist at arm's length covers about 10°).
The light you see today left it about 380 years ago.
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Astronomical data for Chi Phoenicis
- Constellation
- Phoenix
- Apparent magnitude
- 5.15
- Distance
- 375.4 light years
- Coordinates (J2000)
- RA 30.427° · Dec -44.714°
- Catalogue
- HIP 9459 · HD 12524
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Other stars in Phoenix
Phoenix has 39 stars in Stelvia's catalogue. Here are a few of them.
- AnkaaAlpha Phoenicis2.40
- Beta Phoenicis3.32
- Gamma Phoenicis3.41
- Nu Phoenicis4.97
- Phi Phoenicis5.12
- Pi Phoenicis5.13
- Sigma Phoenicis5.18
- Upsilon Phoenicis5.21