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Planetary system · 5 known planets · Scorpius

Gliese 667 C

GJ 667 C
Its star: not above the horizon after darkRises 15:22 · not up after dark
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Gliese 667 CN ↑ E ← · 36° FIELD

Where is Gliese 667 C?

Times for LondonChange city

Below the horizon after dark tonight in Scorpius. Rises 15:22.

Rises
15:22
Highest
17:23
Sets
19:25
Best after dark
—

Can I see Gliese 667 C?

No. The planets of Gliese 667 C can’t be seen with the eye, binoculars or any amateur telescope: they are lost in their star’s light. What you can do is point toward the star.

From London tonight, the star Gliese 667 C isn’t above the horizon while the sky is dark. It rises at 15:22 and sets at 19:25, in daylight or twilight.

Why is Gliese 667 C interesting?

Gliese 667 C has 5 known planets, discovered between 2009 and 2013 by the radial velocity method.

2 of them are close to Earth’s size or mass, based on the catalog values.

What can you see?

Eyes

Direction only

Gliese 667 C is not visible to the eye. The combined light of its two brighter companions is around magnitude 6, at the naked-eye limit.

Binoculars

The bright pair shows as one star; the red dwarf is too faint and close to separate.

Telescope

Around magnitude 10, near the brighter pair; a telescope and chart help. The planets themselves can’t be seen with any backyard telescope.

What you’re likely to see, not what a space telescope photographs.

About

Gliese 667 C is a red dwarf about 22 light-years away in Scorpius. It belongs to a triple star system, orbiting a pair of orange stars, Gliese 667 A and B.

Several planets have been reported around it, including Gliese 667 Cc, a super-Earth in the habitable zone. How many planets the star has is debated, as some signals may come from the star’s own activity.

From one of its planets, the other two stars of the system would shine brightly in the sky.

Gliese 667 A and B, the two orange stars, orbit each other every few decades. The red dwarf C lies much farther out.

Red dwarfs are the most common stars in our galaxy, and many of them have small planets. Planets close enough to a dim red dwarf to be warm are often tidally locked, with one side always facing the star.

The planets were found from the tiny wobble they cause in the star’s motion, a method that can confuse planets with starspots and other stellar activity.

The Gliese 667 C system

Known planets of Gliese 667 C (catalog values from exoplanet.eu)
PlanetMassRadiusOrbitFrom starFoundMethod
GJ 667 Cb5.59 M⊕—7.20 days0.0505 AU2009Radial Velocity
GJ 667 Cc3.81 M⊕—28.1 days0.125 AU2011Radial Velocity
GJ 667 Cf2.70 M⊕—39.0 days0.156 AU2013Radial Velocity
GJ 667 Ce2.70 M⊕—62.2 days0.213 AU2013Radial Velocity
GJ 667 Cg4.61 M⊕—256.2 days0.549 AU2013Radial Velocity

M⊕ / R⊕ = Earth masses / radii; M♃ / R♃ = Jupiter. Masses from radial velocity are often minimum masses. Data: The Extrasolar Planets Encyclopaedia, exoplanet.eu (CC BY 4.0).

Questions

How many planets does Gliese 667 C have?
At least two are widely accepted. Others have been proposed but are debated.

Sources: The Extrasolar Planets Encyclopaedia (CC BY 4.0); star chart: Wikidata (CC0). Positions computed for your place and time with astronomy-engine. Data & Licences