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142 G. Scorpii

Gliese 667, HR 6426, HD 156384
LHS 442 (AB components), LHS 443 (C component)

Proper NameNone
Bayer DesignationNone
Gould Number142 G. Scorpii
HR (BSC)6426
HD156384
Other DesignationsGliese 667, LHS 442 (AB), LHS 443 (AB)
ConstellationScorpius
Right Ascension17h 18m 56s (AB)
17h 18m 59s (C)
Declination-34° 59' 22" (AB)
-34° 59' 49" (C)
Distance24 light years
7 parsecs
MagnitudeApparent: +6.37 (A), +7.38 (B), +10.22 (C)
Absolute: +7.20 (A), +8.21 (B), +10.92 (C)
Spectral ClassK3V orange dwarf (A)
K4V orange dwarf (B)
M1.5V red dwarf (C)
Planets in this system Gliese 667 C b (HD 156384 C b), super Earth
Gliese 667 C c (HD 156384 C c), super Earth
Gliese 667 C d (HD 156384 C d), unconfirmed exoplanet
Gliese 667 C e (HD 156384 C e), unconfirmed exoplanet
Gliese 667 C f (HD 156384 C f), unconfirmed exoplanet
Gliese 667 C g (HD 156384 C g), unconfirmed exoplanet

Gliese 667 C b and c are confirmed exoplanets, but the proposed planets d, e, f and g of this system are now thought unlikely to exist
Optimum VisibilityJune / July

The A and B components of 142 G. Scorpii (or Gliese 667) are not distinguishable in this image (the apparent doubling of the central star in orange and blue reflects its proper motion, rather than two separate component stars of the system). The C star, in a more distant orbit around the AB binary pair, can be seen very close to the marked star, to the southeast (lower left). Imagery provided by Aladin sky atlas

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