Koe-kakaya informaciya po etomu voprosu est' v knige R.Keidl"Tverdye chasticy v atmosfere i v kosmose" M.: Mir, 1969. Rezyumiruya, mozhno skazat', chto v srednem potoke
chem chasticy men'she, tem ih bol'she. Pri etom meteoru nulevoi zvezdnoi velichiny sootvetstvuet primerno chastica massoi ot 10 do 1 gramma, dvizhushayasya so skorost'yu, sootvetstvenno,
ot 10 do 30 km/s. Umen'shenie massy v 100 raz daet 5 edinic vidimoi zvezdnoi velichiny. Takim obrazom, meteorov zvezdnoi velichiny 5 v potoke v 100 raz bol'she, chem meteorov
nulevoi zvezdnoi velichiny i t.d. Takovy dannye nablyudenii. A prichina, veroyatno, zaklyuchaetsya v statistikeobrazovaniya-razrusheniya chastici tel, mozhet byt', dazhe v protoplanetnom
oblake.
