Star profile

HIP 9095

3D likeness based on its real data · class G · ~5,500 K

What is HIP 9095

Phoenix holds it in the southern sky, that constellation burning and reborn among those peeking from below. It is a yellow sun like our own, a distant G-class sibling, suspended 248 light-years away. Its light departed when Galileo s telescopes were already over a century old and the Royal Society was debating the laws of motion. A familiar warmth trapped inside the firebird.

Where it is and when to see it

HIP 9095 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 2° above the horizon.
From Sydney it culminates about 77° above the horizon.

It can be seen from anywhere south of 43° N.

It ranks no. 14 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 250 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 9095

Constellation: Phoenix
Apparent magnitude: 4.82
Distance: 248.2 light years
Coordinates (J2000): RA 29.292° · Dec -47.385°
Catalogue: HIP 9095 · HD 12055

A symbolic commemorative gift: neither the signature nor the chosen name implies ownership of the star or recognition by the IAU.

Other stars in Phoenix

Phoenix has 39 stars in Stelvia's catalogue. Here are a few of them.

See all 39 stars in Phoenix