Unusual sources of fossil micrometeorites deduced from relict chromite in the small size fraction in ~467 Ma old limestoneOPEN ACCESS
Philipp R. Heck, Birger Schmitz, Xenia Ritter, Surya S. Rout, Noriko T. Kita, Céline Defouilloy, Katarina Keating, Kevin Eisenstein, Fredrik Terfelt MAPS, Version of Record online: 02 February 2024 LINK (OPEN ACCESS)PDF (OPEN ACCESS) “Extraterrestrial…
Atmospheric CO2 levels from 2.7 billion years ago inferred from micrometeorite oxidationOPEN ACCESS
O. R. Lehmer, D. C. Catling, R. Buick, D. E. Brownlee and S. Newport Science Advances 22 Jan 2020: Vol. 6, no. 4, eaay4644 DOI: 10.1126/sciadv.aay4644 LINK (OPEN ACCESS) PDF (OPEN ACCESS) “Earth’s atmospheric composition…
The micrometeorite flux to Earth during the Frasnian–Famennian transition reconstructed in the Coumiac GSSP section, France
Birger Schmitz, Raimund Feist, Matthias M.M. Meier, Ellinor Martin, Philipp R. Heck, Davide Lenaz, Dan Topa, Henner Busemann, Colin Maden, Amy A. Plant, Fredrik Terfelt Earth and Planetary Science Letters Volume 522, 15 September 2019,…
The Meteorite from Steinheim, SW Germany: Probably a Pallasite
Buchner E. *, Hölzel M., Schmieder M., Ferrière L., Koeberl C., Rasser M., Fietzke J., Frische M., Meier M. M. M., Busemann H., Maden C., Kutterolf S. 81st Annual Meeting of The Meteoritical Society 2018…
Rare meteorites common in the Ordovician periodOPEN ACCESS
Philipp R. Heck, Birger Schmitz, William F. Bottke, Surya S. Rout, Noriko T. Kita, Anders Cronholm, Céline Defouilloy, Andrei Dronov & Fredrik Terfelt Nature Astronomy 1 Article number: 0035 (2017) doi:10.1038/s41550-016-0035 Published online: 23 January…
A new type of solar-system material recovered from Ordovician marine limestoneOPEN ACCESS
B. Schmitz, Q. -Z. Yin, M. E. Sanborn,M. Tassinari,C. E. Caplan & G. R. Huss Nature Communications 7, Article number:ncomms11851 doi:10.1038/ncomms11851 Published 14 June 2016 LINK (OPEN ACCESS) PDF (OPEN ACCESS) “From mid-Ordovician ~470 Myr-old limestone…
The Composition of the Flux of Micrometeorites after the L-Chondrite Parent Body Breakup ~470 Ma Ago: ≤1% H Chondritic, ≥99% L Chondritic
P. R. Heck, B. Schmitz, S. S. Rout, T. Tenner, K. Villalon, A. Cronholm, F. Terfelt, N. T. Kita 47th Lunar and Planetary Science Conference (2016), Abstract #1191 PDF
