N-body simulations of main-belt asteroidal dust yield fluxes at inner planets that match scaled Grün and Müller models after calibration, with low-eccentricity grains dominating flux and high-eccentricity grains driving the high-velocity impact tail.
year = 1918, month = oct, volume =
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
A review summarizing dynamical and physical evolution of Solar System comets and exocomets, highlighting large gaps in exocomet physics due to lack of direct probes.
citing papers explorer
-
Modeling and Analysis of Main-Belt Asteroidal Dust Flux and Velocity Distribution at Inner Planets
N-body simulations of main-belt asteroidal dust yield fluxes at inner planets that match scaled Grün and Müller models after calibration, with low-eccentricity grains dominating flux and high-eccentricity grains driving the high-velocity impact tail.
-
The evolution of exocomets and their source populations
A review summarizing dynamical and physical evolution of Solar System comets and exocomets, highlighting large gaps in exocomet physics due to lack of direct probes.