116P/Wild 4 live position and data

This page shows Comet 116P/Wild 4 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 116P/Wild 4 (less than 1.5 degrees):

StarHIP 491987.976610h 02m 29s+14° 33’ 27”
StarHIP 493818.82610h 04m 54s+12° 50’ 51”
StarHIP 491688.482810h 02m 03s+15° 21’ 38”
StarHIP 493957.85410h 05m 03s+15° 08’ 04”
StarHIP 492078.452410h 02m 35s+14° 20’ 22”
StarHIP 488558.122209h 57m 52s+13° 36’ 25”
StarHIP 495518.802810h 07m 02s+14° 09’ 28”
StarHIP 493487.647810h 04m 26s+13° 35’ 42”
StarHIP 490108.85909h 59m 53s+14° 52’ 39”
GalaxyNGC 310713.810h 04m 21s+13° 37’ 17”
GalaxyNGC 312113.910h 06m 52s+14° 22’ 21”

Additional resources

Additional Resources about Comet 116P/Wild 4

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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