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Star · K V

BD+05 4868 A

BD+05 4868 A is a main-sequence star of spectral type K V in the constellation Pegasus, 142.2 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 107587
ConstellationPegasus
Distance142.2 light-years (43.6 pc)
Apparent magnitudemagnitude 10.16
Absolute magnitudemagnitude 6.96
Spectral typeK V
Surface temperature4,600 K
Luminosity0.192 L☉
Radius0.69 R☉
Mass0.7 M☉
Age11.1 billion years
Metallicity [Fe/H]-0.05
Right ascension (J2000)21h 47m 26.5s
Declination (J2000)+6° 36′ 17″
Space velocity (relative to the Sun)54.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 10.16. Visible from the whole Northern Hemisphere and south to latitude 83° S. 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 1884. 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 BD+05 4868 A, the Sun would look like a star of magnitude 8.03, in the direction where our sky has the constellation Sextans. 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.