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499 Venusia





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Venusia (minor planet designation: 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]

499 Venusia
A three-dimensional model of 499 Venusia based on its light curve
Discovery
Discovered byMax Wolf
Discovery siteHeidelberg
Discovery date24 December 1902
Designations

MPC designation

(499) Venusia
Pronunciationvɪˈnjʃiə[1]

Alternative designations

1902 KX
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.31 yr (41388 d)
Aphelion4.8693 AU (728.44 Gm)
Perihelion3.1479 AU (470.92 Gm)

Semi-major axis

4.0086 AU (599.68 Gm)
Eccentricity0.21471

Orbital period (sidereal)

8.03 yr (2931.4 d)

Mean anomaly

149.18°

Mean motion

0° 7m 22.116s / day
Inclination2.0907°

Longitude of ascending node

256.245°

Argument of perihelion

174.952°
Physical characteristics

Mean radius

40.69±1.65 km

Synodic rotation period

13.48 h (0.562 d)

Geometric albedo

0.0468±0.004

Absolute magnitude (H)

9.39

References

edit
  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  • ^ a b "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.
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    Last edited on 14 January 2024, at 20:37  





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    This page was last edited on 14 January 2024, at 20:37 (UTC).

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