Karavannoe: Mineralogy, trace element geochemistry, and origin of Eagle Station group pallasites. (20th April 2022)
- Record Type:
- Journal Article
- Title:
- Karavannoe: Mineralogy, trace element geochemistry, and origin of Eagle Station group pallasites. (20th April 2022)
- Main Title:
- Karavannoe: Mineralogy, trace element geochemistry, and origin of Eagle Station group pallasites
- Authors:
- Teplyakova, Svetlana N.
Lorenz, Cyril A.
Ivanova, Marina A.
Humayun, Munir
Kononkova, Nataliya N.
Borisovsky, Sergey E.
Korochantsev, Alexander V.
Franchi, Ian A.
Zinovieva, Nina G. - Abstract:
- ABSTRACT: Karavannoe is a pallasite found in Russia in 2010. The mineralogy, chemistry, and oxygen isotopic composition indicate that Karavannoe is a member of the Eagle Station Pallasite (ESP) group. Karavannoe contains mostly olivine and subdued interstitial Fe, Ni‐metal. Zoned distribution of FeO in small, rounded grains of olivine and FeO and Al2 O3 in chromite shows that the cooling rate of the melt was fast during the crystallization of the round olivine grains. Siderophile element distribution and correlations of Au‐As and Os‐Ir concentrations in Karavannoe and the other ESP metal record its magmatic origin. FeO‐rich composition of olivine, low W and Ga, and high Ni abundances in the Karavannoe metal indicate the formation of the metal from an oxidized chondrite precursor. Model calculations demonstrate that the ESPs' metal compositions correspond to the solids of the fractional crystallization of CV‐ or CO‐chondrite‐derived metallic liquids. The Karavannoe metal composition corresponds to the solid fraction crystallized after ~40% fractional crystallization. The Mg/(Mg+Fe) atom ratio of complementary silicate liquid corresponds to Fo70, possibly indicating that the olivine is not in equilibrium with the metal and could have been a product of the late evolutionary processes in the Karavannoe parent body mantle. In any ESP genesis Karavannoe was not in equilibrium with its metal and is a product of mantle differentiation processes. Olivine of Karavannoe and ESPs isABSTRACT: Karavannoe is a pallasite found in Russia in 2010. The mineralogy, chemistry, and oxygen isotopic composition indicate that Karavannoe is a member of the Eagle Station Pallasite (ESP) group. Karavannoe contains mostly olivine and subdued interstitial Fe, Ni‐metal. Zoned distribution of FeO in small, rounded grains of olivine and FeO and Al2 O3 in chromite shows that the cooling rate of the melt was fast during the crystallization of the round olivine grains. Siderophile element distribution and correlations of Au‐As and Os‐Ir concentrations in Karavannoe and the other ESP metal record its magmatic origin. FeO‐rich composition of olivine, low W and Ga, and high Ni abundances in the Karavannoe metal indicate the formation of the metal from an oxidized chondrite precursor. Model calculations demonstrate that the ESPs' metal compositions correspond to the solids of the fractional crystallization of CV‐ or CO‐chondrite‐derived metallic liquids. The Karavannoe metal composition corresponds to the solid fraction crystallized after ~40% fractional crystallization. The Mg/(Mg+Fe) atom ratio of complementary silicate liquid corresponds to Fo70, possibly indicating that the olivine is not in equilibrium with the metal and could have been a product of the late evolutionary processes in the Karavannoe parent body mantle. In any ESP genesis Karavannoe was not in equilibrium with its metal and is a product of mantle differentiation processes. Olivine of Karavannoe and ESPs is similar in composition, while the metal is different. We propose a model of ESP formation involving an impact‐induced intrusion of liquid core metal into a basal mantle layer, followed by fractional crystallization of the metal. The metal textures and chemical zoning of Karavannoe minerals point to remelting and rapid cooling due to a later impact event. … (more)
- Is Part Of:
- Meteoritics & planetary science. Volume 57:Number 6(2022)
- Journal:
- Meteoritics & planetary science
- Issue:
- Volume 57:Number 6(2022)
- Issue Display:
- Volume 57, Issue 6 (2022)
- Year:
- 2022
- Volume:
- 57
- Issue:
- 6
- Issue Sort Value:
- 2022-0057-0006-0000
- Page Start:
- 1158
- Page End:
- 1173
- Publication Date:
- 2022-04-20
- Subjects:
- Meteorites -- Periodicals
Planetology -- Periodicals
523.4 - Journal URLs:
- http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1945-5100 ↗
http://www.uark.edu/%7Emeteor/ ↗
http://www.uark.edu/meteor/ ↗
http://adsabs.harvard.edu/tocservice.html ↗
http://onlinelibrary.wiley.com/ ↗ - DOI:
- 10.1111/maps.13814 ↗
- Languages:
- English
- ISSNs:
- 1086-9379
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5703.350000
British Library DSC - BLDSS-3PM
British Library STI - ELD Digital store - Ingest File:
- 21827.xml