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192 Nausikaa live position and data

This page shows Asteroid 192 Nausikaa 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 Asteroid 192 Nausikaa (less than 1.5 degrees):

TypeNameMagnitudeArDec
StarHIP 673287.842213h 47m 58s-16° 03’ 53”
StarHIP 674458.167613h 49m 20s-14° 45’ 42”
StarHIP 677087.284413h 52m 15s-14° 40’ 35”
StarHIP 677847.948213h 53m 11s-15° 59’ 53”
StarHIP 678507.401613h 53m 51s-14° 39’ 50”
StarHIP 678966.441213h 54m 21s-17° 10’ 48”
StarHIP 679618.522213h 55m 03s-15° 31’ 27”
StarHIP 680077.63613h 55m 36s-16° 08’ 40”
StarHIP 680258.8113h 55m 48s-14° 47’ 37”
StarHIP 682938.789213h 58m 46s-15° 54’ 18”

Additional resources

Additional Resources about Asteroid 192 Nausikaa

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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