Your Eyes In Space Open the simulation

Star · K4 V

HD 125595

HD 125595 is a main-sequence star of spectral type K4 V in the constellation Centaurus, 92.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 545.1 · HIP 70170
ConstellationCentaurus
Distance92.0 light-years (28.2 pc)
Apparent magnitudemagnitude 9.03
Absolute magnitudemagnitude 6.78
Spectral typeK4 V
Surface temperature4,690 K
Luminosity0.241 L☉
Radius0.74 R☉
Mass0.29 M☉
Age3.5 billion years
Metallicity [Fe/H]0.08
Right ascension (J2000)14h 21m 23.2s
Declination (J2000)−40° 23′ 39″
Space velocity (relative to the Sun)75.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.03. Visible from the whole Southern Hemisphere and north to latitude 50° N. South of latitude 50° S it never sets. It stands highest at midnight in April, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1934. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around HD 125595, the Sun would look like a star of magnitude 7.08, in the direction where our sky has the constellation Andromeda. 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.