HD 34445

Planetary system · 150.3 light-years away · also HD 34445, HIP 24681

HD 34445 is 150 light-years from the Sun. The NASA Exoplanet Archive lists 6 planets around this G0 V star; the first was found in 2009 by radial velocity (W. M. Keck Observatory).

Fly there in 3D

Worth knowing

HD 34445 e goes round its star every 49.2 days, 1.8 times as often as Mercury goes round the Sun.

The star

Spectral typeG0 V
Surface temperature5,879 K
Mass1.14 solar masses
Radius1.38 solar radii
Luminosity2.01 times the Sun
Apparent magnitude7.31
Ageabout 8.5 billion years
Distance from the Sun150.3 light-years (46.1 parsecs)
Position (J2000)RA 79.4207°, Dec 7.3527°
ConstellationOrion

Planets (6)

PlanetYearOrbitRadiusMassFound
HD 34445 e49.2 days0.269 AU4.26 R⊕ estimated16.8 M⊕ minimumRadial Velocity, 2017
HD 34445 d117.9 days0.482 AU6.07 R⊕ estimated30.7 M⊕ minimumRadial Velocity, 2017
HD 34445 c214.7 days0.718 AU8.42 R⊕ estimated53.5 M⊕ minimumRadial Velocity, 2017
HD 34445 f676.8 days1.543 AU6.88 R⊕ estimated37.9 M⊕ minimumRadial Velocity, 2017
HD 34445 b2.9 years2.070 AU13.9 R⊕ estimated260.62 M⊕ minimumRadial Velocity, 2009
HD 34445 g15.6 years6.360 AU13.6 R⊕ estimated120.6 M⊕ minimumRadial Velocity, 2017

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 5,879 K, 2.0 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.34 to 2.36 AU. 2 of its 6 known planets orbit 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 150 years ago, around 1880.

Nearest systems to it

Also found by W. M. Keck Observatory

Sources

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