@InProceedings{Martini:2019:CuEsAl,
author = "Martini, Paulo Roberto",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Curvas espectrais de alguns condritos brasileiros",
booktitle = "Anais...",
year = "2019",
editor = "Gherardi, Douglas Francisco Marcolino and Sanches, Ieda DelArco
and Arag{\~a}o, Luiz Eduardo Oliveira e Cruz de",
pages = "463--466",
organization = "Simp{\'o}sio Brasileiro de Sensoriamento Remoto, 19. (SBSR)",
publisher = "Instituto Nacional de Pesquisas Espaciais (INPE)",
address = "S{\~a}o Jos{\'e} dos Campos",
keywords = "Curvas Espectrais, Condritos, Spectral Signatures-Chondrites.",
abstract = "Neste trabalho se apresentam as curvas espectrais de quatro
meteoritos brasileiros do tipo conhecidos como condritos
ordin{\'a}rios. Uma pequena s{\'{\i}}ntese bibliogr{\'a}fica
sobre o tema tamb{\'e}m {\'e} mostrada assim como
descri{\c{c}}{\~o}es sucintas referentes {\`a}s amostras e suas
descobertas. Os picos e as selas das curvas combinam com
assinaturas observadas na literatura consultada para meteoritos
condr{\'{\i}}ticos tipo L e H. Ao final se faz tentativamente
uma an{\'a}lise sobre poss{\'{\i}}veis corpos parentais destes
quatro meteoritos rochosos. Esta tentativa parte de medidas
espectrais tomadas por telesc{\'o}pios e por sondas espaciais
sobre asteroides silicosos Tipo S situados no {\^a}mago do
Cintur{\~a}o. As curvas de laborat{\'o}rio e as tomadas
remotamente n{\~a}o convergem fruto talvez dos regolitos gerados
pelo intemperismo solar. Sugere-se ao final que os procedimentos
de an{\'a}lise descritos neste artigo sejam estendidos para o
conjunto de 71 meteoritos brasileiros cadastrados at{\'e} 2017.
ABSTRACT: The article presents spectral curves of four Brazilian
meteorites known as ordinary chondrites. A small bibliographic
review about spectral signatures of meteorites is also presented
with brief descriptions about the samples and their discoveries.
The designs of the curves match very well with the signatures
observed in the reviewed literature about chondrite meteorites of
types L and H. At the end a tentative anlysis about parental
bodies of the four rocky meteorites is done. This tentative is
based on the spectral measurements obtained through telescopes and
space probes over silicate asteroids of Type S located at the very
center of the Belt. It was observed that S curves measured in the
labs and by remote devices such as telescope and probes do not fit
well with the curves of chondrites recovered on Earth. The cause
maybe is the solar weathering that somehow changes the surface
signatures of the S-asteroids. As a conclusion it is suggested
that procedures described within this article could be extended to
the others 71 known Brazilian metorites recovered up to 2017.",
conference-location = "Santos",
conference-year = "14-17 abril 2019",
isbn = "978-85-17-00097-3",
language = "pt",
organisation = "Instituto Nacional de Pesquisas Espaciais (INPE)",
ibi = "8JMKD3MGP6W34M/3U2HDEP",
url = "http://urlib.net/ibi/8JMKD3MGP6W34M/3U2HDEP",
targetfile = "97388.pdf",
type = "Geologia",
urlaccessdate = "23 maio 2024"
}