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Star · G3V

HD 199509

HD 199509 is a main-sequence star of spectral type G3V in the constellation Octans, 79.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesHIP 104436
ConstellationOctans
Distance79.4 light-years (24.4 pc)
Apparent magnitudemagnitude 6.98
Absolute magnitudemagnitude 5.05
Spectral typeG3V
Surface temperature5,800 K
Luminosity0.824 L☉
Radius0.92 R☉
Mass1.04 M☉
Age1.6 billion years
Metallicity [Fe/H]-0.31
Right ascension (J2000)21h 09m 20.9s
Declination (J2000)−82° 01′ 38″
Space velocity (relative to the Sun)38.3 km/s

In the sky

Too faint for the naked eye (magnitude 6.98); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 8° N. South of latitude 8° S it never sets.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1947. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.4 million years.

The Sun seen from there

From a planet around HD 199509, the Sun would look like a star of magnitude 6.76, in the direction where our sky has the constellation Camelopardalis. 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.