Star profile

37 Pegasi

3D likeness based on its real data · class F · ~6,500 K

What is 37 Pegasi

37 Pegasi lies about 169 light-years away, within the great square of the winged horse that rules the autumn skies. It is a yellowish type-F star, slightly hotter and whiter than the Sun. The light now settling on Earth set out in the mid-nineteenth century, when the first transatlantic telegraph lines were still being drawn.

Where it is and when to see it

37 Pegasi lies in the northern 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 43° above the horizon.
From New York it culminates about 54° above the horizon.
From Sydney it culminates about 52° above the horizon.

It can be seen from anywhere north of 86° S.

It ranks no. 52 in brightness among the 98 stars of Pegasus in our catalogue. To find it, start from Enif, the brightest: it lies about 13° away (a fist at arm's length covers about 10°).

The light you see today left it about 170 years ago.

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Astronomical data for 37 Pegasi

Constellation: Pegasus
Apparent magnitude: 5.51
Distance: 169.2 light years
Coordinates (J2000): RA 337.491° · Dec 4.432°
Catalogue: HIP 111062 · HD 213235

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Other stars in Pegasus

Pegasus has 98 stars in Stelvia's catalogue. Here are a few of them.

See all 98 stars in Pegasus