In the Vinony graph
Vinony's link graph records 326 inbound references to Gliese 667, and connects out to list of stars in Scorpius, stellar classification and star catalogue.
Vinony files it under Gliese 667, Gliese and GJ objects and Gould objects.
Vinony links it to 31 Wikipedia language editions.
Key facts
- Constellation
- Scorpius
- Right ascension
- 17 18 57.16483
- Declination
- −34 ° 59 ′ 23.1416 ″
- Apparent magnitude v
- 5.91/7.20
- Spectral type
- K3V + K5V
- Evolutionary stage
- main sequence
via Wikipedia infobox
Wikidata facts
- Instance of
- star
- Has part
- Gliese 667 C
- Constellation
- Scorpius
- Distance from Earth
- 23.2
- Radius
- 0.76
- Mass
- 0.73
- Variable-star type
- flare star
- Image
- Scorpius constellation map.svg
Show 19 more facts
- right ascension component of proper motion
- 1168
- luminosity
- 0.13
- Commons category
- Gliese 667
- spectral class
- K4- V
- catalog code
- WEB 14302
- topic has template
- Template:Gliese 667
- topic's main category
- Category:Gliese 667
- apparent magnitude
- 3.12
- parallax
- 143.45
- right ascension
- 259.738186800
- declination
- -34.989761545
- effective temperature
- 4646
- radial velocity
- -4.0
- epoch
- J2000.0
- metallicity
- -0.43
- surface gravity
- 46000
- color index
- 1.031
- absolute magnitude
- 7.078
- declination component of proper motion
- -170
Sources (2)
via Wikidata · CC0
~9 min read
Encyclopedic overview
Gliese 667 (142 G. Scorpii) is a triple-star system in the constellation Scorpius lying at a distance of about 7.2 parsecs (23 light-years) from Earth. All three of the stars have masses smaller than the Sun. To the naked eye, the system appears to be a single faint star of magnitude 5.89. The system has a relatively high proper motion, exceeding 1 second of arc per year.
There is a 12th-magnitude star visually close to the other three, but it is a distant background star not gravitationally bound to the system.
Excerpted from Wikipedia’s “Gliese 667” article, available under the CC BY-SA 4.0 licence.