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. 2.

Variation in the eccentricity with the relative (to Jupiter) apsidal longitude, ϖ − ϖ₅. Top panel: Results for the control orbit of Miorita with state vectors separated −3σ from the nominal ones. Middle panel: Results for 504181 (2006 TC). Bottom panel: Results for 482798 (2013 QK₄₈). The source of the input data is JPL’s Horizons.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.