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Star · K7 V

Ross 176

Ross 176 is a giant star of spectral type K7 V in the constellation Cygnus, 151.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCygnus
Distance151.7 light-years (46.5 pc)
Apparent magnitudemagnitude 11.74
Absolute magnitudemagnitude 8.40
Spectral typeK7 V
Surface temperature4,040 K
Luminosity0.0778 L☉
Radius0.569 R☉
Mass0.577 M☉
Age3.0 billion years
Metallicity [Fe/H]-0.19
Right ascension (J2000)20h 22m 45.0s
Declination (J2000)+47° 18′ 26″
Space velocity (relative to the Sun)82.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.74. 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 1874. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around Ross 176, the Sun would look like a star of magnitude 8.17, in the direction where our sky has the constellation Vela. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 100341 8.07 light-years
  • HIP 99965 10.5 light-years
  • HIP 99241 14.6 light-years
  • HIP 98978 15.9 light-years
  • HIP 99680 16.0 light-years
  • Fawaris 18.5 light-years
  • HIP 98001 19.4 light-years

Open in the simulation

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