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pro vyhledávání: '"V.I. Musiy"'
Publikováno v:
Symposium - International Astronomical Union. 90:199-204
The radius for gravitational capture of meteoroids by the Earth is where R is the Earth's radius, h is the height where marked deceleration of meteor bodies begins, α0 is the average distance of the Earth from the Sun, v∞ and vg are preatmospheric