Star profile
HIP 69618
Variable starWhat is HIP 69618
In southern Centaurus pulses a blue-white B-class star whose light set out around 1543, just as Copernicus was publishing De revolutionibus and unseating Earth from its pedestal. It is a variable: its brightness breathes, rising and falling in slow cycles, as if the star itself were beating. Far hotter and more massive than the Sun, it reminds us that the universe is a body in constant pulse, not a fixed postcard against a black backdrop.
Where it is and when to see it
HIP 69618 lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is May: the Sun sits at the opposite point of the sky and the star culminates around midnight. How high it climbs above the horizon depends on the latitude you watch from.
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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 HIP 69618
- Constellation
- Centaurus
- Apparent magnitude
- 5.03
- Distance
- 481.8 light years
- Coordinates (J2000)
- RA 213.738° · Dec -57.086°
- Catalogue
- HIP 69618 · HD 124367
A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.
Other stars in Centaurus
Centaurus has 174 stars in Stelvia's catalogue. Here are a few of them.
- Rigil KentaurusAlpha 1 Centauri-0.01
- HadarBeta Centauri0.61
- TolimanAlpha 2 Centauri1.35
- HIP 571755.00
- HIP 600595.01
- HIP 728005.02
- HIP 658105.04
- Omicron 1 Centauri5.07