499 Venusia

Main-belt asteroid

499 Venusia is an asteroid in the outer asteroid belt, discovered by Max Wolf in 1902.[3] Its diameter is 81 km (50.6 miles).[4] It is a dark P-type asteroid. It has an average distance from the Sun of 4 AU (600 million km).[2]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ a b "499 Venusia (1902 KX)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
  3. ^ Lutz D. Schmadel (9 March 2013). Dictionary of Minor Planet Names. Springer Science & Business Media. pp. 84–. ISBN 978-3-662-02804-9.
  4. ^ Thomas Wm Hamilton (15 April 2014). Dwarf Planets and Asteroids: Minor Bodies of the Solar System. Strategic Book Publishing Rights Agency. pp. 27–. ISBN 978-1-62857-728-0.
  • 499 Venusia at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 499 Venusia at the JPL Small-Body Database Edit this at Wikidata
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters
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  • 498 Tokio
  • 499 Venusia
  • 500 Selinur
Authority control databases Edit this at Wikidata
  • JPL SBDB
  • MPC


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