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Orbital, Latitudinal, and Diurnal Variations in Meteoroid Influx, Atmospheric Ablation and Ionization, and Micrometeorite Accretion at Venus

  • Authors: Juan Diego Carrillo-Sánchez, Diego Janches, John M. C. Plane, Petr Pokorný

Juan Diego Carrillo-Sánchez et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 19.

Orbital variability of the mass fluxes, in kilograms per Earth-day. Panel (a): mass fluxes of meteoroids before atmospheric entry for the JFCs (blue line), ASTs (green line), HTCs (dark red line), OCCs (orange line), and total mass input (black line). Panel (b): mass fluxes of total MMs (gray line), total ablated (solid red line), neutral atoms (dashed light-blue line), and ionized atoms (dashed light-green line).

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