
Star profile
HIP 94556
What is HIP 94556
From the Southern Crown, some 298 light-years away, comes the light of this yellow type G star, similar in colour to the Sun. It set out around 1728, when James Bradley discovered stellar aberration and at last proved beyond doubt that the Earth moves. Slightly larger and more luminous than our own star, it glows golden over the small southern crown —a distant echo of our everyday sun.
Where it is and when to see it
HIP 94556 lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is July: 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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The signature wall
Stelvia's sky works like a signature wall: anyone can leave their name and a message on a real star, and that signature goes up on the map for everyone to read. Signing is free.
A signature without a lock can be replaced by someone else's. The lock makes the signature permanent and lets you choose a symbolic name for the star, always shown next to the star's catalogue identifier. How the lock works
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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 94556
- Constellation
- Corona Australis
- Apparent magnitude
- 5.91
- Distance
- 297.9 light years
- Coordinates (J2000)
- RA 288.665° · Dec -45.194°
- Catalogue
- HIP 94556 · HD 179433
A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.
Other stars in Corona Australis
Corona Australis has 29 stars in Stelvia's catalogue. Here are a few of them.
- Beta Coronae Australis4.10
- MeridianaAlpha Coronae Australis4.11
- Gamma Coronae Australis4.23
- Kappa 1 Coronae Australis5.67
- HIP 908425.71
- HIP 935525.73
- HIP 890995.86
- HIP 941575.86