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Star · G V

HIP 94235

HIP 94235 is a main-sequence star of spectral type G V in the constellation Pavo, 191.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationPavo
Distance191.0 light-years (58.5 pc)
Apparent magnitudemagnitude 8.31
Absolute magnitudemagnitude 4.47
Spectral typeG V
Surface temperature5,990 K
Luminosity1.37 L☉
Radius1.08 R☉
Mass1.09 M☉
Age0.1 billion years
Metallicity [Fe/H]0.00
Right ascension (J2000)19h 10m 57.9s
Declination (J2000)−60° 16′ 20″
Space velocity (relative to the Sun)29.7 km/s

In the sky

Too faint for the naked eye (magnitude 8.31); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 30° N. South of latitude 30° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1835. 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 HIP 94235, the Sun would look like a star of magnitude 8.67, in the direction where our sky has the constellation Lynx. 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.