Erratum to "Petrographic criteria for fluid mobility of graphitic carbon in terrestrial and extraterrestrial samples" [J. Geochemical Exploration 89(2006) 235-238]

Paula Lindgren, John Parnell

Research output: Contribution to journalArticle

Abstract

Graphitic carbon is a widespread precipitate in terrestrial and extraterrestrial samples. However it has a range of possible origins, which can be difficult to distinguish, including the in situ alteration of organic matter, thermal alteration of hydrocarbons, and precipitation from C-O-H fluids. Petrographic characteristics help to understand the origin of the graphite, including relationships with rock fabric, paragenetic sequences and evidence for fluid mobility. Characterization of a range of terrestrial samples will allow better interpretation of the petrography of carbon in extraterrestrial samples. In particular, improved petrographic data from carbonaceous chondrites and ureilite meteorites should help to distinguish the origin of carbon in their parent bodies. (c) 2006 Elsevier B.V. All rights reserved.

Original languageEnglish
Pages (from-to)125
Number of pages1
JournalJournal of Geochemical Exploration
Volume91
Issue number1-3
DOIs
Publication statusPublished - Oct 2006

Keywords

  • INTERPLANETARY DUST PARTICLES
  • ISOTOPIC COMPOSITION
  • UREILITES
  • NITROGEN
  • CHONDRITES
  • HYDROGEN
  • GENESIS

Cite this

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title = "Erratum to {"}Petrographic criteria for fluid mobility of graphitic carbon in terrestrial and extraterrestrial samples{"} [J. Geochemical Exploration 89(2006) 235-238]",
abstract = "Graphitic carbon is a widespread precipitate in terrestrial and extraterrestrial samples. However it has a range of possible origins, which can be difficult to distinguish, including the in situ alteration of organic matter, thermal alteration of hydrocarbons, and precipitation from C-O-H fluids. Petrographic characteristics help to understand the origin of the graphite, including relationships with rock fabric, paragenetic sequences and evidence for fluid mobility. Characterization of a range of terrestrial samples will allow better interpretation of the petrography of carbon in extraterrestrial samples. In particular, improved petrographic data from carbonaceous chondrites and ureilite meteorites should help to distinguish the origin of carbon in their parent bodies. (c) 2006 Elsevier B.V. All rights reserved.",
keywords = "INTERPLANETARY DUST PARTICLES, ISOTOPIC COMPOSITION, UREILITES, NITROGEN, CHONDRITES, HYDROGEN, GENESIS",
author = "Paula Lindgren and John Parnell",
year = "2006",
month = "10",
doi = "10.1016/j.gexplo.2006.05.004",
language = "English",
volume = "91",
pages = "125",
journal = "Journal of Geochemical Exploration",
issn = "0375-6742",
publisher = "Elsevier",
number = "1-3",

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TY - JOUR

T1 - Erratum to "Petrographic criteria for fluid mobility of graphitic carbon in terrestrial and extraterrestrial samples" [J. Geochemical Exploration 89(2006) 235-238]

AU - Lindgren, Paula

AU - Parnell, John

PY - 2006/10

Y1 - 2006/10

N2 - Graphitic carbon is a widespread precipitate in terrestrial and extraterrestrial samples. However it has a range of possible origins, which can be difficult to distinguish, including the in situ alteration of organic matter, thermal alteration of hydrocarbons, and precipitation from C-O-H fluids. Petrographic characteristics help to understand the origin of the graphite, including relationships with rock fabric, paragenetic sequences and evidence for fluid mobility. Characterization of a range of terrestrial samples will allow better interpretation of the petrography of carbon in extraterrestrial samples. In particular, improved petrographic data from carbonaceous chondrites and ureilite meteorites should help to distinguish the origin of carbon in their parent bodies. (c) 2006 Elsevier B.V. All rights reserved.

AB - Graphitic carbon is a widespread precipitate in terrestrial and extraterrestrial samples. However it has a range of possible origins, which can be difficult to distinguish, including the in situ alteration of organic matter, thermal alteration of hydrocarbons, and precipitation from C-O-H fluids. Petrographic characteristics help to understand the origin of the graphite, including relationships with rock fabric, paragenetic sequences and evidence for fluid mobility. Characterization of a range of terrestrial samples will allow better interpretation of the petrography of carbon in extraterrestrial samples. In particular, improved petrographic data from carbonaceous chondrites and ureilite meteorites should help to distinguish the origin of carbon in their parent bodies. (c) 2006 Elsevier B.V. All rights reserved.

KW - INTERPLANETARY DUST PARTICLES

KW - ISOTOPIC COMPOSITION

KW - UREILITES

KW - NITROGEN

KW - CHONDRITES

KW - HYDROGEN

KW - GENESIS

U2 - 10.1016/j.gexplo.2006.05.004

DO - 10.1016/j.gexplo.2006.05.004

M3 - Article

VL - 91

SP - 125

JO - Journal of Geochemical Exploration

JF - Journal of Geochemical Exploration

SN - 0375-6742

IS - 1-3

ER -