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Star · G5

HIP 9618

HIP 9618 is a main-sequence star of spectral type G5 in the constellation Aries, 219.5 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

ConstellationAries
Distance219.5 light-years (67.3 pc)
Apparent magnitudemagnitude 9.20
Absolute magnitudemagnitude 5.06
Spectral typeG5
Surface temperature5,650 K
Luminosity0.848 L☉
Radius0.959 R☉
Mass0.942 M☉
Age5.6 billion years
Metallicity [Fe/H]-0.02
Right ascension (J2000)2h 03m 37.0s
Declination (J2000)+21° 16′ 51″
Space velocity (relative to the Sun)63.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.20. Visible from the whole Northern Hemisphere and south to latitude 69° S. North of latitude 69° N it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1807. 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 HIP 9618, the Sun would look like a star of magnitude 8.97, in the direction where our sky has the constellation Virgo. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 9452 8.75 light-years
  • HIP 10710 14.8 light-years
  • HIP 8221 16.6 light-years
  • HIP 9434 18.2 light-years
  • HIP 10351 18.6 light-years
  • HIP 10652 18.9 light-years

Open in the simulation

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