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Star · F7IV

σ Peg

σ Peg is a subgiant star of spectral type F7IV in the constellation Pegasus, 89.2 light-years from the Sun.

Other namesGJ 9801A · HIP 112935
ConstellationPegasus
Distance89.2 light-years (27.4 pc)
Apparent magnitudemagnitude 5.16
Absolute magnitudemagnitude 2.97
Spectral typeF7IV
Surface temperature6,450 K
Luminosity5.54 L☉
Radius1.89 R☉
Mass1.53 M☉ (estimated)
Right ascension (J2000)22h 52m 24.1s
Declination (J2000)+9° 50′ 08″
Space velocity (relative to the Sun)68.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.16). Visible from the whole Northern Hemisphere and south to latitude 80° S. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1937. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around σ Peg, the Sun would look like a star of magnitude 7.02, in the direction where our sky has the constellation Crater. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.