297P/Beshore (2008 J2) live position and data

This page shows Comet 297P/Beshore (2008 J2) 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 297P/Beshore (2008 J2) (less than 1.5 degrees):

StarHIP 250688.770205h 21m 58s+22° 57’ 13”
StarHIP 248224.863805h 19m 16s+22° 05’ 48”
StarHIP 252748.769205h 24m 19s+22° 18’ 20”
StarHIP 256217.093405h 28m 25s+22° 44’ 33”
StarHIP 255394.878805h 27m 38s+21° 56’ 13”
StarHIP 246688.6105h 17m 32s+22° 49’ 45”
StarHIP 255868.60505h 28m 06s+22° 55’ 50”
StarHIP 255728.238605h 27m 55s+23° 17’ 35”
StarHIP 253908.559405h 25m 53s+21° 47’ 09”
StarHIP 253068.864405h 24m 48s+24° 06’ 23”

Additional resources

Additional Resources about Comet 297P/Beshore (2008 J2)

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.

RA:  ()
Dec:  ()