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Star · F8

Kepler-408

Kepler-408 is a main-sequence star of spectral type F8 in the constellation Draco, 290.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationDraco
Distance290.8 light-years (89.1 pc)
Apparent magnitudemagnitude 8.89
Absolute magnitudemagnitude 4.14
Spectral typeF8
Surface temperature6,100 K
Luminosity1.92 L☉
Radius1.23 R☉
Mass1.08 M☉
Age6.7 billion years
Metallicity [Fe/H]-0.20
Right ascension (J2000)18h 59m 08.7s
Declination (J2000)+48° 25′ 24″
Space velocity (relative to the Sun)54.9 km/s

In the sky

Too faint for the naked eye (magnitude 8.89); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 42° S. North of latitude 42° 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 1735. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.2 million years.

The Sun seen from there

From a planet around Kepler-408, the Sun would look like a star of magnitude 9.58, 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 92467 11.3 light-years
  • HIP 92689 12.6 light-years
  • HIP 93320 17.0 light-years

Open in the simulation

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