Shepherding Miorita and its flock: A group of near-Earth asteroids driven by apsidal and von Zeipel-Lidov-Kozai secular resonances - A source of low-perihelion asteroids

Open Access

Fig. C.1.

Time evolution of the apsidal longitude ϖ − ϖ₅ of 622577 Miorita (2014 LU₁₄). Results from the calculations displayed in the central panels of Fig. 1. Nominal orbit in black, those of control orbits with state vectors separated ±3σ from the nominal ones in lime and green, respectively, and ±9σ in orange and red, respectively. The source of the input data is JPL’s Horizons.

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