499 Venusia
A three-dimensional model of 499 Venusia based on its light curve. | |
Discovery | |
---|---|
Discovered by | Max Wolf |
Discovery site | Heidelberg |
Discovery date | 24 December 1902 |
Designations | |
1902 KX | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 113.31 yr (41388 d) |
Aphelion | 4.8693 AU (728.44 Gm) |
Perihelion | 3.1479 AU (470.92 Gm) |
4.0086 AU (599.68 Gm) | |
Eccentricity | 0.21471 |
8.03 yr (2931.4 d) | |
149.18° | |
0° 7m 22.116s / day | |
Inclination | 2.0907° |
256.245° | |
174.952° | |
Earth MOID | 2.16081 AU (323.253 Gm) |
Jupiter MOID | 0.446284 AU (66.7631 Gm) |
Jupiter Tisserand parameter | 3.011 |
Physical characteristics | |
Mean radius | ±1.65 40.69km |
13.48 h (0.562 d) | |
±0.004 0.0468 | |
9.39 | |
|
499 Venusia is a minor planet orbiting the Sun, discovered by Max Wolf in 1902.[2] Its diameter is 81 km (50.6 miles).[3] It is a dark P-type asteroid.
References
- ↑ "499 Venusia (1902 KX)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 6 May 2016.
- ↑ Lutz D. Schmadel (9 March 2013). Dictionary of Minor Planet Names. Springer Science & Business Media. pp. 84–. ISBN 978-3-662-02804-9.
- ↑ 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.
External links
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