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67P/Churyumov-Gerasimenko live position and data

This page shows Comet 67P/Churyumov-Gerasimenko location and other relevant astronomical data in real time. The celestial coordinates, magnitude, distances and speed are updated in real time and are computed using high quality data sets provided by the JPL Horizons ephemeris service (see acknowledgements for details). The sky map shown below represents a rectangular portion of the sky 60x40 arcminutes wide. By comparison the diameter of the full Moon is about 30 arcmins, so the full horizontal extent of the map is approximately 2 full Moons wide. Depending on the device you are using, the map can be dragged horizondally or vertically using the mouse or touchscreen. The deep sky image in the background is provided by the Digitized Sky Survey (acknowledgements).

Current close conjunctions

List of bright objects (stars brighter than magnitude 9.0 and galaxies brighter than magmitude 14.0) close to Comet 67P/Churyumov-Gerasimenko (less than 1.5 degrees):

TypeNameMagnitudeArDec
StarHIP 824278.14916h 50m 43s-25° 25’ 39”
StarHIP 819508.484216h 44m 21s-26° 19’ 29”
StarHIP 817138.236416h 41m 26s-24° 24’ 08”
StarHIP 822456.93116h 48m 13s-24° 31’ 35”
StarHIP 817738.368216h 42m 09s-24° 49’ 08”
StarHIP 817286.04516h 41m 36s-24° 28’ 04”
StarHIP 821406.605216h 46m 51s-25° 31’ 42”
StarHIP 822177.90816h 47m 46s-23° 58’ 27”
StarHIP 824747.646416h 51m 21s-24° 50’ 02”

Additional resources

Additional Resources about Comet 67P/Churyumov-Gerasimenko

Astronomy databases

This online sky chart is created using the following astronomy databases and services:

  1. The Digitized Sky Survey, a photographic survey of the whole sky created using images from different telescopes, including the Oschin Schmidt Telescope on Palomar Mountain
  2. The Hipparcos Star Catalogue, containing more than 100.000 bright stars
  3. The PGC 2003 Catalogue, containing information about 1 million galaxies
  4. The GSC 2.3 Catalogue, containing information about more than 2 billion stars and galaxies
Please see the acknowledgements section.

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