Tissemouminites: A new group of primitive achondrites spanning the transition between acapulcoites and winonaites

Author:

Stephant A.12ORCID,Carli C.1ORCID,Anand M.2,Néri A.3,Davidson J.4ORCID,Pratesi G.15ORCID,Cuppone T.5,Greenwood R. C.2,Franchi I. A.2ORCID

Affiliation:

1. Istituto di Astrofisica e Planetologia Spaziali – INAF Rome 00133 Italy

2. School of Physical Sciences The Open University Milton Keynes MK7 6AA UK

3. Bayerisches Geoinstitut University of Bayreuth Bayreuth 95447 Germany

4. Buseck Center for Meteorite Studies, School of Earth and Space Exploration Arizona State University Tempe Arizona 85287 USA

5. Dipartimento di Scienze della Terra Università degli Studi di Firenze Firenze 50121 Italy

Funder

Agenzia Spaziale Italiana

H2020 Marie Skłodowska-Curie Actions

Science and Technology Facilities Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference75 articles.

1. Benedix G. K. andLauretta D. S.2006.Thermodynamic Constraints on the Formation History of Acapulcoites (Abstract #2129). 37th Lunar and Planetary Science Conference. CD‐ROM.

2. Thermodynamic constraints on the formation conditions of winonaites and silicate-bearing IAB irons

3. A petrologic study of the IAB iron meteorites: Constraints on the formation of the IAB-Winonaite parent body

4. Benedix G. K. McCoy T. J. andLauretta D. S.2003.Is NWA 1463 the Most Primitive Winonaite?66th Annual Meteoritical Society Meeting abstract 5125.

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