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Star · K5V

HIP 948

HIP 948 is a main-sequence star of spectral type K5V in the constellation Sculptor, 113.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationSculptor
Distance113.8 light-years (34.9 pc)
Apparent magnitudemagnitude 9.92
Absolute magnitudemagnitude 7.21
Spectral typeK5V
Surface temperature4,500 K
Luminosity0.175 L☉
Radius0.688 R☉
Mass0.71 M☉
Right ascension (J2000)0h 11m 41.7s
Declination (J2000)−39° 13′ 48″
Space velocity (relative to the Sun)125.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.92. Visible from the whole Southern Hemisphere and north to latitude 51° N. South of latitude 51° S it never sets. 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 1912. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.0 million years.

The Sun seen from there

From a planet around HIP 948, the Sun would look like a star of magnitude 7.54, in the direction where our sky has the constellation Canes Venatici. It would be invisible 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.