RA: 
Dec: 

Position of Rosetta in the Sky

The current position of Rosetta is computed using high quality data sets provided by the JPL Horizons ephemeris service (see acknowledgements). It is important to be aware that for objects like comets there might be large discrepancies between the predicted magnitude and the real one. This happens because comets magnitude is highly influenced by physical phenomena which can be hardly modelled and calculated in advance.

Current close conjunctions

List of bright objects (stars brighter than magnitude 9.0 and galaxies brighter than magmitude 14.0) close to Rosetta (less than 1.5 degrees):

TypeNameMagnitudeArDec
StarHIP 38492007h 52m 59s+22° 33’ 23”
StarHIP 386038.670407h 54m 14s+23° 30’ 14”
StarHIP 387118.509407h 55m 31s+24° 21’ 47”
StarHIP 387527.59307h 56m 01s+24° 39’ 56”
StarHIP 387557.235807h 56m 02s+23° 41’ 35”
StarHIP 387616.796207h 56m 06s+23° 37’ 25”
StarHIP 387857.496807h 56m 19s+22° 34’ 19”
StarHIP 390776.81407h 59m 42s+23° 10’ 58”
StarHIP 390878.054407h 59m 46s+23° 05’ 13”
StarHIP 391946.259408h 01m 00s+23° 34’ 59”
StarHIP 392238.860808h 01m 22s+22° 21’ 30”
StarHIP 392357.1408h 01m 30s+23° 54’ 45”
StarHIP 394658.581808h 03m 58s+23° 24’ 20”
GalaxyNGC 248113.607h 57m 13s+23° 46’ 00”
GalaxyNGC 251213.908h 03m 07s+23° 23’ 32”

Additional resources

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:  ()
Follow theskylive.com on Facebook Follow theskylive.com on Twitter Follow theskylive.com on Google+ Share on Facebook Share on Twitter Share on Google+