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Star · K3 V

HD 48948

HD 48948 is a main-sequence star of spectral type K3 V in the constellation Lynx, 54.9 light-years from the Sun. It is orbited by 3 confirmed exoplanet(s).

Other namesGl 247 · HIP 32769
ConstellationLynx
Distance54.9 light-years (16.8 pc)
Apparent magnitudemagnitude 8.59
Absolute magnitudemagnitude 7.46
Spectral typeK3 V
Surface temperature4,590 K
Luminosity0.163 L☉
Radius0.679 R☉
Mass0.686 M☉
Age11.5 billion years
Metallicity [Fe/H]-0.21
Right ascension (J2000)6h 49m 57.0s
Declination (J2000)+60° 20′ 08″
Space velocity (relative to the Sun)65.2 km/s

In the sky

Too faint for the naked eye (magnitude 8.59); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 30° S. North of latitude 30° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1971. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 974 thousand years.

The Sun seen from there

From a planet around HD 48948, the Sun would look like a star of magnitude 5.96, in the direction where our sky has the constellation Pavo. It would be visible to the naked eye.

Planets

Neighbours

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

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