HD 196067

Planetary system · 130.3 light-years away · also HD 196067, HIP 102125

HD 196067 is 130 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this G0 V star; the first was found in 2012 by radial velocity (La Silla Observatory).

Fly there in 3D

Worth knowing

HD 196067 c goes round its star every 4.60 days, 19 times as often as Mercury goes round the Sun.

HD 196067 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.

Where the archive gives only a period or only an orbit size, the other is worked out from Kepler’s third law with the star’s mass.

The star

Spectral typeG0 V
Surface temperature6,072 K
Mass1.16 solar masses
Radius1.71 solar radii
Luminosity3.54 times the Sun
Apparent magnitude6.51
Ageabout 4.2 billion years
Distance from the Sun130.3 light-years (39.9 parsecs)
Position (J2000)RA 310.4364°, Dec -75.3515°
ConstellationOctans

The other star

HD 196067 B has no spectral type listed of magnitude 7.07, moving through space with it. In 2023 it was 16.7″ from HD 196067, at position angle 20° (Washington Double Star Catalog, 20417-7521 DUN 232): 667 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.

Planets (2)

PlanetYearOrbitRadiusMassFound
HD 196067 c4.60 days0.0569 AU from Kepler’s law3.21 R⊕ estimated10.4 M⊕ minimumRadial Velocity, 2025
HD 196067 b9.3 years4.710 AU12.4 R⊕ estimated3623.2 M⊕Radial Velocity, 2012

Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.

The planets, compared

For a star of 6,072 K, 3.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.76 to 3.08 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.

The light you see left 130 years ago, around 1900.

Nearest systems to it

Also found by La Silla Observatory

Sources

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