Meteorites: samples of NEOs in the laboratory

被引:2
|
作者
Perron, C [1 ]
Zanda, B [1 ]
机构
[1] Museum Natl Hist Nat, Lab Etud Mat Extraterrestre, F-75005 Paris, France
关键词
NEO; meteorites; reflectance spectroscopy;
D O I
10.1016/j.crhy.2005.01.005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Meteorites can be considered as samples of near-Earth objects (NEOs), and as such they may be useful for inferring the properties of the latter, including those that may encounter the Earth in the future. This article reviews the main properties of meteorites which can be of interest in NEO research. We first briefly recall the characteristics of a meteorite fall and the biases it introduces in the passage from the near Earth meteoroid population to the meteorite population. We then describe in more detail the mineralogical and chemical composition of the various classes of meteorites. The relations between meteorites and asteroids that can be inferred from reflectance spectroscopy, and the porosity of meteorites are treated in Sections 4 and 5, respectively. The last section deals with meteorite ages, with emphasis on the cosmic ray exposure age. To cite this article: (c) 2005 Academie des sciences. Published by Elsevier SAS. All rights reserved.
引用
收藏
页码:345 / 360
页数:16
相关论文
共 50 条
  • [1] Photomosaics of the cathodoluminescence of 60 sections of meteorites and lunar samples
    Akridge, DG
    Akridge, JMC
    Batchelor, JD
    Benoit, PH
    Brewer, J
    DeHart, JM
    Keck, BD
    Jie, L
    Meier, A
    Penrose, M
    Schneider, DM
    Sears, DWG
    Symes, SJK
    Zhang, YH
    JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2004, 109 (E7) : E07S031 - 10
  • [2] Micro-elemental analysis of some Transylvanian meteorites and lunar samples
    Vasilescu, Angela
    Constantinescu, B.
    Bugoi, Roxana
    Ceccato, D.
    Grambole, D.
    Herrmann, F.
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION B-BEAM INTERACTIONS WITH MATERIALS AND ATOMS, 2009, 267 (12-13): : 2233 - 2235
  • [3] Surface compositions of NEOs
    Dotto, E
    Barucci, MA
    Binzel, RP
    Debló, M
    COMPTES RENDUS PHYSIQUE, 2005, 6 (03) : 303 - 312
  • [4] Fundamental constraints and questions from the study of martian meteorites and the need for returned samples
    Udry, Arya
    Ostwald, Amanda M.
    Day, James M. D.
    Hallis, Lydia J.
    PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2025, 122 (02)
  • [5] Spectroscopic investigations of meteorites
    Pentikainen, Hanna
    Penttila, Antti
    Muinonen, Karri
    Peltoniemi, Jouni
    JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 2014, 146 : 391 - 401
  • [6] Laboratory experiments on the impact disruption of iron meteorites at temperature of near-Earth space
    Katsura, Takekuni
    Nakamura, Akiko M.
    Takabe, Ayana
    Okamoto, Takaya
    Sangen, Kazuyoshi
    Hasegawa, Sunao
    Liu, Xun
    Mashimo, Tsutomu
    ICARUS, 2014, 241 : 1 - 12
  • [7] Numerical determination of visible/NIR optical constants from laboratory spectra of HED meteorites
    Davalos, Jorge A. G.
    Carvano, Jorge Marcio
    Blanco, Julio
    ICARUS, 2017, 285 : 275 - 290
  • [8] Optimal options for rendezvous and impact missions to neos
    De Pascale, Paolo
    Vasile, Massimiliano
    Casotto, Stefano
    JBIS-JOURNAL OF THE BRITISH INTERPLANETARY SOCIETY, 2006, 59 (11): : 386 - 394
  • [9] Central Force Optimization and NEOs - First Cousins?
    Formato, Richard A.
    JOURNAL OF MULTIPLE-VALUED LOGIC AND SOFT COMPUTING, 2010, 16 (06) : 547 - 565
  • [10] Tungsten stable isotope compositions of terrestrial samples and meteorites determined by double spike MC-ICPMS
    Krabbe, Nadine
    Kruijer, Thomas S.
    Kleine, Thorsten
    CHEMICAL GEOLOGY, 2017, 450 : 135 - 144