Cooling rates and parent bodies of iron meteorites from group IIICD, IAB, and IVB
Author:
Publisher
IOP Publishing
Subject
Condensed Matter Physics,Mathematical Physics,Atomic and Molecular Physics, and Optics
Link
http://stacks.iop.org/1402-4896/39/i=3/a=031/pdf
Reference41 articles.
1. Origin of Iron Meteorite Groups IAB and IIICD
2. Classification and properties of iron meteorites
3. Chemical fractionation in iron meteorites and its interpretation
4. The cooling rates and parent planets of several iron meteorites
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1. Cooling rates and impact histories of group IAB and other IAB complex iron meteorites inferred from zoned taenite and the cloudy zone;Meteoritics & Planetary Science;2021-10-18
2. An evolutionary system of mineralogy, Part IV: Planetesimal differentiation and impact mineralization (4566 to 4560 Ma);American Mineralogist;2021-05-01
3. Noble gases and nitrogen in Raghunathpura (IIAB) and Nyaung (IIIAB) iron meteorites;Meteoritics & Planetary Science;2018-09-23
4. Microstructural and paleomagnetic insight into the cooling history of the IAB parent body;Geochimica et Cosmochimica Acta;2018-05
5. Siderophile element systematics of IAB complex iron meteorites: New insights into the formation of an enigmatic group;Geochimica et Cosmochimica Acta;2016-09
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