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Star · K3 V

HD 103949

HD 103949 is a main-sequence star of spectral type K3 V in the constellation Corvus, 86.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 58374
ConstellationCorvus
Distance86.4 light-years (26.5 pc)
Apparent magnitudemagnitude 8.70
Absolute magnitudemagnitude 6.58
Spectral typeK3 V
Surface temperature4,790 K
Luminosity0.269 L☉
Radius0.753 R☉
Mass0.77 M☉
Metallicity [Fe/H]-0.07
Right ascension (J2000)11h 58m 11.7s
Declination (J2000)−23° 55′ 26″
Space velocity (relative to the Sun)25.0 km/s

In the sky

Too faint for the naked eye (magnitude 8.70); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 66° N. South of latitude 66° 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 1940. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.5 million years.

The Sun seen from there

From a planet around HD 103949, the Sun would look like a star of magnitude 6.95, in the direction where our sky has the constellation Pegasus. It would be invisible 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.