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Star · K0

Kepler-409

Kepler-409 is a main-sequence star of spectral type K0 in the constellation Cygnus, 222.2 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCygnus
Distance222.2 light-years (68.1 pc)
Apparent magnitudemagnitude 9.72
Absolute magnitudemagnitude 5.55
Spectral typeK0
Surface temperature5,420 K
Luminosity0.628 L☉
Radius0.897 R☉
Mass0.913 M☉
Age5.8 billion years
Metallicity [Fe/H]0.05
Right ascension (J2000)19h 34m 43.0s
Declination (J2000)+46° 51′ 10″
Space velocity (relative to the Sun)28.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.72. Visible from the whole Northern Hemisphere and south to latitude 43° S. North of latitude 43° N 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 1804. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.9 million years.

The Sun seen from there

From a planet around Kepler-409, the Sun would look like a star of magnitude 9.00, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • HIP 95631 12.9 light-years
  • HIP 97700 14.2 light-years
  • HIP 94922 16.6 light-years
  • Kepler-138 16.7 light-years

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.