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Star · K5 V

HIP 54373

HIP 54373 is a main-sequence star of spectral type K5 V in the constellation Crater, 61.1 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

ConstellationCrater
Distance61.1 light-years (18.7 pc)
Apparent magnitudemagnitude 10.38
Absolute magnitudemagnitude 9.02
Spectral typeK5 V
Surface temperature4,020 K
Luminosity0.0599 L☉
Radius0.565 R☉
Mass0.57 M☉
Right ascension (J2000)11h 07m 27.7s
Declination (J2000)−19° 17′ 29″
Space velocity (relative to the Sun)21.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 10.38. Visible from the whole Southern Hemisphere and north to latitude 71° N. South of latitude 71° S it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1965. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.1 million years.

The Sun seen from there

From a planet around HIP 54373, the Sun would look like a star of magnitude 6.19, in the direction where our sky has the constellation Pegasus. It would be visible to the naked eye.

Planets

Neighbours

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

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.