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Star · G0 V

HD 216435

HD 216435 is a subgiant star of spectral type G0 V in the constellation Grus, 108.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesτ¹ Gru · GJ 9802 · HIP 113044
ConstellationGrus
Distance108.0 light-years (33.1 pc)
Apparent magnitudemagnitude 6.03
Absolute magnitudemagnitude 3.43
Spectral typeG0 V
Surface temperature6,000 K
Luminosity3.6 L☉
Radius1.8 R☉
Mass1.3 M☉
Age3.0 billion years
Metallicity [Fe/H]0.24
Right ascension (J2000)22h 53m 37.9s
Declination (J2000)−48° 35′ 54″
Space velocity (relative to the Sun)36.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.03). Visible from the whole Southern Hemisphere and north to latitude 41° N. South of latitude 41° S it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1918. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.

The Sun seen from there

From a planet around HD 216435, the Sun would look like a star of magnitude 7.43, in the direction where our sky has the constellation Ursa Major. 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.