On the dynamical evolution of 2002 VE68
C. de la Fuente Marcos, R. de la Fuente Marcos

TL;DR
This study investigates the long-term orbital dynamics of minor planet 2002 VE68, confirming its status as a Venus quasi-satellite, analyzing its past and future evolution, and highlighting its interactions with Earth, Mercury, and the Moon.
Contribution
The paper provides a detailed dynamical analysis of 2002 VE68's orbital history and future, including the influence of multiple planets and the identification of its quasi-satellite status over thousands of years.
Findings
2002 VE68 is confirmed as a Venus quasi-satellite for at least 7,000 years.
Close Earth encounters within 0.002 AU are possible at aphelion.
The object will remain a Venus quasi-satellite for about 500 more years.
Abstract
Minor planet 2002 VE68 was identified as a quasi-satellite of Venus shortly after its discovery. At that time its data-arc span was only 24 days, now it is 2,947 days. Here we revisit the topic of the dynamical status of this remarkable object as well as look into its dynamical past and explore its future orbital evolution which is driven by close encounters with both the Earth-Moon system and Mercury. In our calculations we use a Hermite integration scheme, the most updated ephemerides and include the perturbations by the eight major planets, the Moon and the three largest asteroids. We confirm that 2002 VE68 currently is a quasi-satellite of Venus and it has remained as such for at least 7,000 yr after a close fly-by with the Earth. Prior to that encounter the object may have already been co-orbital with Venus or moving in a classical, non-resonant Near-Earth Object (NEO) orbit. The…
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