A microchondrule‐bearing micrometeorite and comparison with microchondrules in CM chondrites

Author:

Suttle M. D.123ORCID,Genge M. J.23ORCID,Salge T.4ORCID,Lee M. R.5ORCID,Folco L.1,Góral T.4,Russell S. S.3,Lindgren P.6ORCID

Affiliation:

1. Dipartimento di Scienze della Terra Università di Pisa 56126 Pisa Italy

2. Department of Earth Science and Engineering Imperial College London South Kensington London SW7 2AZ UK

3. Mineral and Planetary Sciences The Natural History Museum Cromwell Rd London SW7 5BD UK

4. Imaging and Analysis Centre Core Research Laboratories The Natural History Museum Cromwell Rd London SW7 5BDUK

5. School of Geographical and Earth Sciences University of Glasgow Glasgow G12 8QQ UK

6. Earth Science and Physical Geography Lund University 221 00 Lund Sweden

Funder

Ministero dell’Istruzione, dell’Università e della Ricerca

Science and Technology Facilities Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference100 articles.

1. The Formation Conditions of Chondrules and Chondrites

2. BigolskiJ. N. WeisbergM. K. EbelD. S. andConnollyH. C.2014.Microchondrules: Records of multiple heating events in the solar nebula and implications for type II chondrule formation (abstract). 45th Lunar and Planetary Science Conference. p. 1879.

3. Microchondrules in three unequilibrated ordinary chondrites

4. Maximum pixel spectrum: a new tool for detecting and recovering rare, unanticipated features from spectrum image data cubes

5. Chromite composition in relation to chemistry and texture of ordinary chondrites

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