Fig. 1.
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Orbital evolution of 622577 Miorita (2014 LU14). Left panels: Results of a simulation of the nominal orbit and the full physical model (in black), after removing the Earth–Moon system (in blue), and after removing Jupiter (in brown). Central panels: Short-term results of the full physical model and the 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. Right panels: Integrations in the central panels but over a longer time span. Time evolution of the value of the semimajor axis, a (top panels), eccentricity, e (second to top), inclination, i (middle), the longitude of the ascending node, Ω (second to bottom), and the argument of perihelion, ω (bottom). The origin of time is the epoch 2460800.5 JD barycentric dynamical time and the output cadence is 36.525 d for the left and central panels, and 25 yr for the right panels. The source of the input data is JPL’s Horizons.
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