213P/Van Ness live position and data

This page shows Comet 213P/Van Ness 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 213P/Van Ness (less than 1.5 degrees):

Type	Name	Magnitude	Ar	Dec
Star	HIP 50203	7.9064	10h 14m 57s	+09° 12’ 40”
Star	HIP 49766	6.9326	10h 09m 31s	+09° 35’ 35”
Star	HIP 49637	4.2286	10h 07m 54s	+09° 59’ 51”
Star	HIP 50081	7.3366	10h 13m 30s	+09° 11’ 09”
Star	HIP 50353	8.7012	10h 16m 55s	+08° 14’ 42”
Star	HIP 50470	8.4558	10h 18m 19s	+08° 40’ 56”
Star	HIP 50370	8.375	10h 17m 02s	+10° 06’ 51”

Additional resources

Additional Resources about Comet 213P/Van Ness

• 15 Days Ephemerides
• Interactive Sky Map (Planetarium)
• Rise & Set Times
• Distance from Earth
• Light Curve

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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