Earth-grazing meteoroid of 13 October 1990

Расчёт масс метеорных тел путём приближения траекторий

Saturn's Meteoroid Crash

Question 1: The dinosaur meteoroid and the day; Question 2: School guards

Lunar meteoroid impacts and how to observe them

Conference summary: Meteoroids

Conference on Meteoroids 1994 August 28–31 Bratislava, Slovakia

Etude des forces perturbatrices agissant sur les meteorites du faisceau Geminid, causees par le champ radiatif solaire

The available observational data for the beginning and end heights of meteors in the Perseid, Southern Taurid and Geminid meteor streams is compared to the quantitative theory of dustball meteor ablation due to Hawkes & Jones. A reasonable agreement between model predictions and observations is found. Following the analysis of Hapgood, Rothwell & Royrvik the amount of energy required to fragment unit mass of meteoroid material is calculated, with the result that meteors are possibly more fragile than assumed in theory.

Meteoroid swarms colliding with the Moon

As a logical extension from previous papers by the authors, a general method is derived for calculation of the meteoroid flux at any finite point, for an arbitrary spectrum of broad meteoroid streams at infinity. This formalism is explicitly applied, obtaining plots of relative flux versus angle for a set of examples dealing with monoenergetic isotropic distributions, and limited monoenergetic isotropic distributions.

Dust wall helps shield spacecraft from meteoroids

Meteoroids' effect studied

Rockets vs. Meteoroids