Fig. 6: An example of a Kamo’oalewa-like outcome of a lunar ejecta particle.
From: Lunar ejecta origin of near-Earth asteroid Kamo’oalewa is compatible with rare orbital pathways
a Evolution of the semi-major axis and b relative mean longitude for the KL1 trajectory (vL = 5.1 km s−1). HS motion is shown in blue, while QS motion is shown in yellow. The HS-QS oscillations persist for up to 4500 years (not shown).
