2015 RR245 live position and data

This page shows Asteroid 2015 RR245 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 2015 RR245 (less than 1.5 degrees):

Type	Name	Magnitude	Ar	Dec
Star	HIP 1771	0	00h 22m 25s	+06° 40’ 05”
Star	HIP 2025	6.6392	00h 25m 41s	+07° 41’ 28”
Star	HIP 2083	7.8226	00h 26m 18s	+06° 05’ 39”
Star	HIP 2181	8.783	00h 27m 34s	+07° 14’ 04”
Star	HIP 2244	8.597	00h 28m 30s	+07° 05’ 24”
Star	HIP 2369	8.988	00h 30m 14s	+05° 21’ 44”
Star	HIP 2548	5.7036	00h 32m 23s	+06° 57’ 19”

Additional resources

Additional Resources about Asteroid 2015 RR245

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

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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