Rigil Kentaurus or Toliman - α1 Centauri (alpha1 Centauri)
Rigil Kentaurus or Toliman, also designated as α1 Centauri (alpha1 Centauri), is a multiple main-sequence star in the constellation of Centaurus.
Rigil Kentaurus or Toliman visual magnitude is -0.01. Thanks to its high brightness, Rigil Kentaurus or Toliman is clearly visible when observed from locations with dark skyes, and should be also quite easily visible from light polluted areas.
The table below summarizes the key facts about Rigil Kentaurus or Toliman:
Rigil Kentaurus or Toliman - α1 Centauri (alpha1 Centauri) is below the horizon from Greenwich, United Kingdom .
Altitude: -43.1°
Azimuth: 138.1°
Direction: South-East
Celestial coordinates and finder chart of Rigil Kentaurus or Toliman
Rigil Kentaurus or Toliman is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of Rigil Kentaurus or Toliman are provided in the following table:
The simplified sky map below shows the position of Rigil Kentaurus or Toliman in the sky:

Visibility of Rigil Kentaurus or Toliman from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Rigil Kentaurus or Toliman - α1 Centauri (alpha1 Centauri) is currently not visible from Greenwich, United Kingdom
Digitized Sky Survey image of Rigil Kentaurus or Toliman
The image below is a photograph of Rigil Kentaurus or Toliman from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of Rigil Kentaurus or Toliman is -3.642 arcsec per year in Right Ascension and 0.699 arcsec per year in Declination and the associated displacement for the next 100 years is represented with the red arrow.

Distance of Rigil Kentaurus or Toliman from the Sun and relative movement
Rigil Kentaurus or Toliman is distant 4.39 light years from the Sun and it is moving towards the Sun at the speed of 22 kilometers per second.
Spectral properties of Rigil Kentaurus or Toliman
Rigil Kentaurus or Toliman belongs to spectral class G2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where Rigil Kentaurus or Toliman is situated in the Hertzsprung–Russell diagram.

Rigil Kentaurus or Toliman star system properties
Rigil Kentaurus or Toliman is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the Rigil Kentaurus or Toliman double sysyem: