Star profile

HIP 24927

3D likeness based on its real data · class A · ~8,500 K

What is HIP 24927

In Lepus, right beneath Orion's feet, this white A-type star emits the crisp, clean glow that defines its class, dominated by hot hydrogen. Its light set out 416 years ago, just as Galileo first turned his telescope toward the sky in 1610. Hotter and more luminous than the Sun, it concentrates in a single point the austere elegance of young stars only beginning their journey along the main sequence.

Where it is and when to see it

HIP 24927 lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is December, when it culminates around midnight.

From London it culminates about 17° above the horizon.
From New York it culminates about 28° above the horizon.
From Sydney it culminates about 77° above the horizon.

It can be seen from anywhere south of 69° N.

It ranks no. 13 in brightness among the 45 stars of Lepus in our catalogue. To find it, start from Arneb, the brightest: it lies about 4° away (a fist at arm's length covers about 10°).

The light you see today left it about 420 years ago.

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Astronomical data for HIP 24927

Constellation: Lepus
Apparent magnitude: 4.70
Distance: 416.1 light years
Coordinates (J2000): RA 80.112° · Dec -21.240°
Catalogue: HIP 24927 · HD 34968

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

Other stars in Lepus

Lepus has 45 stars in Stelvia's catalogue. Here are a few of them.

See all 45 stars in Lepus