2007 FT3 live position and data

This page shows Asteroid 2007 FT3 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 2007 FT3 (less than 1.5 degrees):

StarHIP 313798.880806h 34m 44s+42° 30’ 12”
StarHIP 306438.023606h 26m 23s+40° 21’ 30”
StarHIP 304326.974406h 23m 53s+40° 48’ 31”
StarHIP 304828.651806h 24m 28s+41° 48’ 58”
StarHIP 308218.49606h 28m 29s+40° 03’ 25”
StarHIP 305268.298606h 24m 59s+42° 32’ 45”
StarHIP 310066.681806h 30m 25s+41° 24’ 06”
StarHIP 306406.962206h 26m 21s+41° 57’ 34”
StarHIP 304086.716806h 23m 38s+40° 31’ 17”
StarHIP 315148.907806h 35m 56s+41° 55’ 21”

Additional resources

Additional Resources about Asteroid 2007 FT3

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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