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Star · G5 V

HD 207832

HD 207832 is a main-sequence star of spectral type G5 V in the constellation Piscis Austrinus, 193.1 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

Other namesHIP 107985
ConstellationPiscis Austrinus
Distance193.1 light-years (59.2 pc)
Apparent magnitudemagnitude 8.78
Absolute magnitudemagnitude 4.92
Spectral typeG5 V
Surface temperature5,730 K
Luminosity0.776 L☉
Radius0.89 R☉
Mass1.05 M☉
Age1.4 billion years
Metallicity [Fe/H]0.14
Right ascension (J2000)21h 52m 36.3s
Declination (J2000)−26° 01′ 36″
Space velocity (relative to the Sun)56.7 km/s

In the sky

Too faint for the naked eye (magnitude 8.78); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 64° N. South of latitude 64° S 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 1833. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.4 million years.

The Sun seen from there

From a planet around HD 207832, the Sun would look like a star of magnitude 8.69, in the direction where our sky has the constellation Leo. 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.