Star profile
HIP 116250
What is HIP 116250
Within the lonely Octans, almost over the celestial south pole, shines a yellow G-type star 102 light-years away. Its light set out around 1923, when Edwin Hubble identified variable stars in Andromeda and proved that we live in a universe full of galaxies. A close sister of the Sun in colour and temperature, its surface hovers near 5,700 degrees and its golden light is barely distinguishable from our own.
Where it is and when to see it
HIP 116250 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, when it culminates around midnight.
- From London it never rises above the horizon.
- From New York it never rises above the horizon.
- From Sydney it never sets and culminates about 47° up.
It can be seen from anywhere south of 13° N.
It ranks no. 28 in brightness among the 35 stars of Octans in our catalogue. To find it, start from Nu Octans, the brightest: it lies about 6° away (a fist at arm's length covers about 10°).
The light you see today left it about 100 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 HIP 116250
- Constellation
- Octans
- Apparent magnitude
- 5.82
- Distance
- 102.5 light years
- Coordinates (J2000)
- RA 353.331° · Dec -77.385°
- Catalogue
- HIP 116250 · HD 221420
A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.
Other stars in Octans
Octans has 35 stars in Stelvia's catalogue. Here are a few of them.
- Nu Octans3.73
- Beta Octans4.13
- Delta Octans4.31
- HIP 1014275.76
- Upsilon Octans5.76
- HIP 10745.78
- Omega Octans5.88
- HIP 76015.88