Physical and Chemical Properties of Meteoroids

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520240" target="_blank" >RIV/67985815:_____/19:00520240 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/67985831:_____/19:00520240

Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

Physical and Chemical Properties of Meteoroids

Popis výsledku v původním jazyce

The chapter provides a comprehensive and up to date review of physical properties (structure, strength, porosity etc.) and chemical composition of small solar system bodies with sizes ranging from several micrometers to several meters. Experts from different fields of research, using different methods, joined their efforts to present and compare results of laboratory investigation of meteorites, interplanetary dust particles (IDPs), and micrometeorites, studies of cometary and asteroidal dust by remote sensing, in-situ investigation or sample-return missions, and properties of meteoroids derived from observations of meteors. Meteors sample the whole population of meteoroids in the vicinity of the Earth and provide data of their orbits. The best currently available methods and models of inferring physical properties of meteoroids from their behavior during the atmospheric entry, in particular fragmentation, are discussed. Chemical compositions are extracted from meteor spectra. Perfectly designed figures and tables convey the information clearly and concisely to the reader. The data are relevant for understanding other solar system objects, especially comets and asteroids.

Název v anglickém jazyce

Physical and Chemical Properties of Meteoroids

Popis výsledku anglicky

The chapter provides a comprehensive and up to date review of physical properties (structure, strength, porosity etc.) and chemical composition of small solar system bodies with sizes ranging from several micrometers to several meters. Experts from different fields of research, using different methods, joined their efforts to present and compare results of laboratory investigation of meteorites, interplanetary dust particles (IDPs), and micrometeorites, studies of cometary and asteroidal dust by remote sensing, in-situ investigation or sample-return missions, and properties of meteoroids derived from observations of meteors. Meteors sample the whole population of meteoroids in the vicinity of the Earth and provide data of their orbits. The best currently available methods and models of inferring physical properties of meteoroids from their behavior during the atmospheric entry, in particular fragmentation, are discussed. Chemical compositions are extracted from meteor spectra. Perfectly designed figures and tables convey the information clearly and concisely to the reader. The data are relevant for understanding other solar system objects, especially comets and asteroids.

Druh

C - Kapitola v odborné knize

CEP obor

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OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

<a href="/cs/project/GA16-00761S" target="_blank" >GA16-00761S: Rozpady meteoroidů a malých asteroidů v zemské atmosféře</a><br>

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2019

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název knihy nebo sborníku

Meteoroids: Sources of Meteors on Earth and Beyond

ISBN

9781108426718

Počet stran výsledku

26

Strana od-do

37-62

Počet stran knihy

306

Název nakladatele

University Press

Místo vydání

Cambridge

Kód UT WoS kapitoly

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