Density, porosity and magnetic susceptibility of the Kosice meteorite shower and homogeneity of its parent meteoroid

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F14%3A00107122" target="_blank" >RIV/00216224:14310/14:00107122 - isvavai.cz</a>

Nalezeny alternativní kódy

RIV/67985815:_____/14:00427677 RIV/67985831:_____/14:00427677

Výsledek na webu

<a href="https://www.sciencedirect.com/science/article/pii/S0032063314000373" target="_blank" >https://www.sciencedirect.com/science/article/pii/S0032063314000373</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1016/j.pss.2014.02.003" target="_blank" >10.1016/j.pss.2014.02.003</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Density, porosity and magnetic susceptibility of the Kosice meteorite shower and homogeneity of its parent meteoroid

Popis výsledku v původním jazyce

Bulk and grain densities, porosities, and magnetic susceptibilities of 67 individuals of Kosice H chondrite fall were measured. The mean bulk and grain densities were determined to be 3.43 g/cm(3) with standard deviation (s.d.) of 0.11 g/cm(3) and 3.79 g/cm(3) with s.d. 0.07 g/cm(3), respectively. Porosity is in the range from 4.2% to 16.1%. The logarithm of the apparent magnetic susceptibility (in 10(-9) m(3)/kg) shows narrow distribution from 5.17 to 5.49 with mean value at 5.35 with s.d. 0.08. These results indicate that all studied Make meteorites are of the same composition down to g scale without the presence of foreign (non-H) clasts and are similar to other H chondrites. Kosice is thus a homogeneous meteorite fall derived from a homogeneous meteoroid.

Název v anglickém jazyce

Density, porosity and magnetic susceptibility of the Kosice meteorite shower and homogeneity of its parent meteoroid

Popis výsledku anglicky

Bulk and grain densities, porosities, and magnetic susceptibilities of 67 individuals of Kosice H chondrite fall were measured. The mean bulk and grain densities were determined to be 3.43 g/cm(3) with standard deviation (s.d.) of 0.11 g/cm(3) and 3.79 g/cm(3) with s.d. 0.07 g/cm(3), respectively. Porosity is in the range from 4.2% to 16.1%. The logarithm of the apparent magnetic susceptibility (in 10(-9) m(3)/kg) shows narrow distribution from 5.17 to 5.49 with mean value at 5.35 with s.d. 0.08. These results indicate that all studied Make meteorites are of the same composition down to g scale without the presence of foreign (non-H) clasts and are similar to other H chondrites. Kosice is thus a homogeneous meteorite fall derived from a homogeneous meteoroid.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2014

Kód důvěrnosti údajů

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

Název periodika

PLANETARY AND SPACE SCIENCE

ISSN

0032-0633

e-ISSN

—

Svazek periodika

93-94

Číslo periodika v rámci svazku

5

Stát vydavatele periodika

GB - Spojené království Velké Británie a Severního Irska

Počet stran výsledku

5

Strana od-do

96-100

Kód UT WoS článku

000335278000010

EID výsledku v databázi Scopus

2-s2.0-84898436735