Star profile
HIP 3505
What is HIP 3505
In Cetus, the cosmic whale grazing along the celestial equator, shines this yellow-white F-type star, slightly hotter than the Sun. Its light set out around 1939, when Edwin Armstrong demonstrated FM radio and the world first glimpsed clean sound. It now reaches Earth as a continuous broadcast, free of static, from 87 years ago.
Where it is and when to see it
HIP 3505 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 culminates about 16° above the horizon.
- From New York it culminates about 27° above the horizon.
- From Sydney it culminates about 78° above the horizon.
It can be seen from anywhere south of 68° N.
It ranks no. 38 in brightness among the 111 stars of Cetus in our catalogue. To find it, start from Diphda, the brightest: it lies about 4° away (a fist at arm's length covers about 10°).
The light you see today left it about 87 years ago.
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Leave your signature on HIP 3505
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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 3505
- Constellation
- Cetus
- Apparent magnitude
- 5.22
- Distance
- 87.2 light years
- Coordinates (J2000)
- RA 11.185° · Dec -22.006°
- Catalogue
- HIP 3505 · HD 4247
A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.
Other stars in Cetus
Cetus has 111 stars in Stelvia's catalogue. Here are a few of them.
- DiphdaBeta Ceti2.04
- MenkarAlpha Ceti2.54
- Eta Ceti3.46
- HIP 23815.17
- Phi 2 Ceti5.17
- 13 Ceti5.20
- HIP 117385.27
- 69 Ceti5.29