New augite geothermometer for nakhlites

Introduction: nakhlites, together with shergottites and chassinites constitute the “SNC” group of Martian meteorites. MIL 03346 is a nakhlite, that was found at Miller Range, in Antarctica and is mainly composed of clinopyroxene (79%), with minor olivine (1%), and 20% vitrophyric intercumulus materi...

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Main Authors: A. M. Fioretti, M. C. Domeneghetti, M. Alvaro, L. Marinangeli, F. Camara
Other Authors: A.M. Fioretti, M.C. Domeneghetti
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2014
Subjects:
Online Access:http://hdl.handle.net/2434/478115
http://www.hou.usra.edu/meetings/metsoc2014/pdf/5013.pdf
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spelling ftunivmilanoair:oai:air.unimi.it:2434/478115 2024-04-21T07:48:00+00:00 New augite geothermometer for nakhlites A. M. Fioretti M. C. Domeneghetti M. Alvaro L. Marinangeli F. Camara A.M. Fioretti M.C. Domeneghetti M. Alvaro F. Camara L. Marinangeli 2014-09 http://hdl.handle.net/2434/478115 http://www.hou.usra.edu/meetings/metsoc2014/pdf/5013.pdf eng eng Wiley info:eu-repo/semantics/altIdentifier/wos/WOS:000341914200115 Annual meeting of the meteoritical-society volume:49 issue:supplement 1 firstpage:A118 lastpage:A118 numberofpages:1 journal:METEORITICS & PLANETARY SCIENCE http://hdl.handle.net/2434/478115 http://www.hou.usra.edu/meetings/metsoc2014/pdf/5013.pdf info:eu-repo/semantics/closedAccess nakhlite Martian meteorite geothermometer calibration MIL 03346 single crystal X-ray diffraction electron microporobe Settore GEO/06 - Mineralogia info:eu-repo/semantics/article 2014 ftunivmilanoair 2024-03-27T16:39:24Z Introduction: nakhlites, together with shergottites and chassinites constitute the “SNC” group of Martian meteorites. MIL 03346 is a nakhlite, that was found at Miller Range, in Antarctica and is mainly composed of clinopyroxene (79%), with minor olivine (1%), and 20% vitrophyric intercumulus material [1,2]. The clinopyroxene is augite with a homogeneous core (En36Fs24Wo40) and an iron enriched rim (En8Fs64Wo28). Since the first modern petrologic studies of Nakhla, the nakhlite group of meteorites has been interpreted as augite-rich cumulate igneous rocks, derived from basaltic magma, that erupted onto the surface of Mars [3,4]. The relative low closure temperature (Tc) of ca. 500 (±100)°C calculated for MIL 03346 by [5] with the available geothermometer [6] would correspond to a slow cooling rate that is in disagreement with the petrologic evidence for an origin from a fast cooled lava flow. Geothermometer calibration: ex-situ annealing experiments combined with high-resolution single-crystal X-ray diffraction (HR-SC-XRD) on crystals from MIL 03346 clearly showed that the degree of order remained unchanged at 600°C thus suggesting that the actual Tc is close to this temperature. We then undertook an ex situ annealing experiments combined with HR-SC-XRD at 600, 700, 800 and 900 °C until the equilibrium in the Fe2+-Mg exchange on two crystals from exactly the same fragment of MIL 03346 sample in order to obtain a new geothermometer for augites from Martian nakhlites: lnkD = -4421(±561)/T(K) + 1.46(±0.52) (R2=0.988) where kD = [(Fe2+M1)(MgM2) / (Fe2+M2)(MgM1)] Results: applying this new equation to MIL 03346 the closure temperature resulted to be 605(84)°C about 100°C higher than that calculated with previously available calibration (i.e. Brizi et al. 2000). However, this closure temperature of 605°C is still lower than expected based on petrologic evidences and suggests that MIL 03346 clinopyroxene bears record of a thermal event that postdates, or is superimposed on, the natural cooling path of the host lava ... Article in Journal/Newspaper Antarc* Antarctica The University of Milan: Archivio Istituzionale della Ricerca (AIR)
institution Open Polar
collection The University of Milan: Archivio Istituzionale della Ricerca (AIR)
op_collection_id ftunivmilanoair
language English
topic nakhlite
Martian meteorite
geothermometer calibration
MIL 03346
single crystal X-ray diffraction
electron microporobe
Settore GEO/06 - Mineralogia
spellingShingle nakhlite
Martian meteorite
geothermometer calibration
MIL 03346
single crystal X-ray diffraction
electron microporobe
Settore GEO/06 - Mineralogia
A. M. Fioretti
M. C. Domeneghetti
M. Alvaro
L. Marinangeli
F. Camara
New augite geothermometer for nakhlites
topic_facet nakhlite
Martian meteorite
geothermometer calibration
MIL 03346
single crystal X-ray diffraction
electron microporobe
Settore GEO/06 - Mineralogia
description Introduction: nakhlites, together with shergottites and chassinites constitute the “SNC” group of Martian meteorites. MIL 03346 is a nakhlite, that was found at Miller Range, in Antarctica and is mainly composed of clinopyroxene (79%), with minor olivine (1%), and 20% vitrophyric intercumulus material [1,2]. The clinopyroxene is augite with a homogeneous core (En36Fs24Wo40) and an iron enriched rim (En8Fs64Wo28). Since the first modern petrologic studies of Nakhla, the nakhlite group of meteorites has been interpreted as augite-rich cumulate igneous rocks, derived from basaltic magma, that erupted onto the surface of Mars [3,4]. The relative low closure temperature (Tc) of ca. 500 (±100)°C calculated for MIL 03346 by [5] with the available geothermometer [6] would correspond to a slow cooling rate that is in disagreement with the petrologic evidence for an origin from a fast cooled lava flow. Geothermometer calibration: ex-situ annealing experiments combined with high-resolution single-crystal X-ray diffraction (HR-SC-XRD) on crystals from MIL 03346 clearly showed that the degree of order remained unchanged at 600°C thus suggesting that the actual Tc is close to this temperature. We then undertook an ex situ annealing experiments combined with HR-SC-XRD at 600, 700, 800 and 900 °C until the equilibrium in the Fe2+-Mg exchange on two crystals from exactly the same fragment of MIL 03346 sample in order to obtain a new geothermometer for augites from Martian nakhlites: lnkD = -4421(±561)/T(K) + 1.46(±0.52) (R2=0.988) where kD = [(Fe2+M1)(MgM2) / (Fe2+M2)(MgM1)] Results: applying this new equation to MIL 03346 the closure temperature resulted to be 605(84)°C about 100°C higher than that calculated with previously available calibration (i.e. Brizi et al. 2000). However, this closure temperature of 605°C is still lower than expected based on petrologic evidences and suggests that MIL 03346 clinopyroxene bears record of a thermal event that postdates, or is superimposed on, the natural cooling path of the host lava ...
author2 A.M. Fioretti
M.C. Domeneghetti
M. Alvaro
F. Camara
L. Marinangeli
format Article in Journal/Newspaper
author A. M. Fioretti
M. C. Domeneghetti
M. Alvaro
L. Marinangeli
F. Camara
author_facet A. M. Fioretti
M. C. Domeneghetti
M. Alvaro
L. Marinangeli
F. Camara
author_sort A. M. Fioretti
title New augite geothermometer for nakhlites
title_short New augite geothermometer for nakhlites
title_full New augite geothermometer for nakhlites
title_fullStr New augite geothermometer for nakhlites
title_full_unstemmed New augite geothermometer for nakhlites
title_sort new augite geothermometer for nakhlites
publisher Wiley
publishDate 2014
url http://hdl.handle.net/2434/478115
http://www.hou.usra.edu/meetings/metsoc2014/pdf/5013.pdf
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation info:eu-repo/semantics/altIdentifier/wos/WOS:000341914200115
Annual meeting of the meteoritical-society
volume:49
issue:supplement 1
firstpage:A118
lastpage:A118
numberofpages:1
journal:METEORITICS & PLANETARY SCIENCE
http://hdl.handle.net/2434/478115
http://www.hou.usra.edu/meetings/metsoc2014/pdf/5013.pdf
op_rights info:eu-repo/semantics/closedAccess
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