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DETERMINATION OF PARAMETERS OF SMALL METEOROID BODIES: THE INFLUENCE OF THE HEAT OF ABLATION

https://doi.org/10.26006/29490995_2024_16_4_75

Abstract

The ablation model is used to estimate the physical parameters of millimeter-sized meteoroids. In the ablation model used, the energy of the incident flow is spent only on the loss of mass of the meteoroid. The selection of parameters (size and density) of meteoroids for the reproduction of light curves is carried out using an automated approach. The influence of ablation heat on the mass, density and size of meteoroids was investigated. The estimates of meteoroid parameters obtained within the framework of this model are compared with estimates based on empirical relationships and with estimates based on another ablation model.

About the Authors

A. I. Bushmanova
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation


V. V. Efremov
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation


O. P. Popova
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation


D. O. Glazachev
Sadovsky Institute of Geospheres Dynamics of Russian Academy of Sciences
Russian Federation


A. P. Kartashova
Institute of Astronomy of the Russian Academy of Sciences
Russian Federation


Review

For citations:


Bushmanova A.I., Efremov V.V., Popova O.P., Glazachev D.O., Kartashova A.P. DETERMINATION OF PARAMETERS OF SMALL METEOROID BODIES: THE INFLUENCE OF THE HEAT OF ABLATION. Dynamic Processes in Geospheres. 2024;16(4):74-81. (In Russ.) https://doi.org/10.26006/29490995_2024_16_4_75

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ISSN 2222-8535 (Print)
ISSN 2949-0995 (Online)