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Star · G2IV

HIP 104788

HIP 104788 is a subgiant star of spectral type G2IV in the constellation Cepheus, 139.4 light-years from the Sun.

ConstellationCepheus
Distance139.4 light-years (42.8 pc)
Apparent magnitudemagnitude 6.38
Absolute magnitudemagnitude 3.23
Spectral typeG2IV
Surface temperature5,870 K
Luminosity4.68 L☉
Radius2.09 R☉
Mass1.47 M☉ (estimated)
Right ascension (J2000)21h 13m 42.5s
Declination (J2000)+64° 24′ 14″
Space velocity (relative to the Sun)37.1 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.38). Visible from the whole Northern Hemisphere and south to latitude 26° S. North of latitude 26° N it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1887. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.5 million years.

The Sun seen from there

From a planet around HIP 104788, the Sun would look like a star of magnitude 7.98, in the direction where our sky has the constellation Carina. 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.