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110P/Hartley 3 live position and data

This page shows Comet 110P/Hartley 3 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 110P/Hartley 3 (less than 1.5 degrees):

TypeNameMagnitudeArDec
StarHIP 145547.940603h 07m 52s+23° 41’ 16”
StarHIP 148478.8203h 11m 44s+23° 59’ 13”
StarHIP 146217.760803h 08m 51s+25° 22’ 06”
StarHIP 140807.954403h 01m 28s+25° 07’ 35”
StarHIP 146108.137803h 08m 40s+25° 35’ 30”
StarHIP 144518.596803h 06m 32s+24° 13’ 17”
StarHIP 145488.226603h 07m 50s+25° 33’ 07”
StarHIP 147188.602603h 10m 08s+24° 39’ 48”
StarHIP 143765.467203h 05m 26s+25° 15’ 18”
StarHIP 143798.619803h 05m 30s+25° 52’ 07”

Additional resources

Additional Resources about Comet 110P/Hartley 3

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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