A Venus trojan is an asteroid that orbits the Sun in the vicinity of Venus. Trojans travel in Venus-Sun Lagrangian points L4, leading 60°, or L5, trailing 60°. 2013 ND15 is the only known trojan of Venus, and is located near Venus's Lagrangian point L4. While 524522 Zoozve is currently a quasi-satellite of Venus, it is expected to be ejected from that configuration and become a Venus trojan orbiting at Venus' L5 point in about 500 years.
Exploration
The only known temporary trojan of Venus is 2013 ND15. It orbits Venus in a tadpole orbit around Venus's Lagrangian point L4. The asteroid was discovered in July 2013 by N. Primak, A. Schultz, T. Goggia and K. Chambers, observing for the Pan-STARRS project. As of September 2014, the asteroid had been observed 21 times over a data-arc span of 26 days. It is classified as an Aten asteroid, and its semi-major axis is 0.7235 astronomical units (AU) closely matches that of Venus. However, it has a high eccentricity of 0.6115 and a low orbital inclination of 4.794°. With an absolute magnitude of 24.1, its estimated diameter ranges between 40 and 100 meters, based on an assumed albedo range of 0.04 to 0.20. In addition to being a Venus co-orbital, the asteroid is also a Mercury-crosser and Earth-crosser. 2013 ND15 shows resonant or near-resonant orbital behavior with Mercury, Venus, and Earth. Its short-term orbital behavior differs from the other three known Venus co-orbitals: (322756) 2001 CK32, 524522 Zoozve, and 2012 XE133. According to a Minor Planet Center list, it does not list 2013 ND15 as a potentially hazardous asteroid (PHA), as it has only passed 0.077 AU from Earth on 21 June 2016.
See also Trojan (celestial body) Earth trojan Mars trojan Jupiter trojan Uranus trojan Neptune trojan
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