Zobrazeno 1 - 10
of 38
pro vyhledávání: '"J. Roszjar"'
Publikováno v:
Meteoritics & Planetary Science. 55:558-574
We report on the petrography and mineralogy of five Yamato polymict eucrites to better constrain the formation and alteration of crustal material on differentiated asteroids. Each sample consists of different lithic clasts that altogether form four d
Autor:
Joerg Fritz, N Chutimun Chanmuang, J. Roszjar, Lidia Pittarello, Christoph Lenz, Christian Koeberl
Publikováno v:
Meteoritics & Planetary Science. 55:669-678
Decline of giant impacts on Mars by 4.48 billion years ago and an early opportunity for habitability
Autor:
Desmond E. Moser, Axel Wittmann, Francis M. McCubbin, David J. Larson, Anthony J. Irving, L. F. White, G. Arcuri, David A. Reinhard, Kimberly T. Tait, I. Barker, J. Roszjar, Connor Davis, James Darling
Publikováno v:
Moser, D E, Arcuri, G A, Reinhard, D, White, L F, Darling, J, Barker, I R, Larson, D J, Irving, A J, McCubbin, F M, Tait, K, Roszjar, J, Wittmann, A & Davis, C 2019, ' Decline of giant impacts on Mars by 4.48 billion years ago and an early opportunity for habitability ', Nature Geoscience, vol. 12, no. 7, pp. 522–527 . https://doi.org/10.1038/s41561-019-0380-0
The timing of the wane in heavy meteorite bombardment of the inner planets is debated. Its timing determines the onset of crustal conditions consistently below the thermal and shock pressure limits for microbiota survival, and so bounds the occurrenc
Autor:
Martin J. Whitehouse, Hajime Hiyagon, J. Roszjar, Timm John, Kentaro Terada, Addi Bischoff, Kohei Fukuda, Yuichi Morishita
Publikováno v:
Geochimica et Cosmochimica Acta. 245:385-405
The enriched basaltic (martian) shergottite Ksar Ghilane (KG) 002, discovered in 2010, is exceptionally rich in coexisting but discrete apatite and merrillite crystals. It has been selected to better constrain the formation conditions and post-crysta
Publikováno v:
Earth and Planetary Science Letters. 459:311-319
The hydrophilic nature of halogens makes these elements ideal for probing potential hydrous geologic processes. Generally, in magmatic settings the stable isotopes of Cl may fractionate when H is in low concentrations and little fractionation occurs
Autor:
Chutimun Chanmuang, Martin Lee, Ludovic Ferrière, Luke Daly, Jörg Fritz, Christoph Lenz, Christian Koeberl, J. Roszjar, Lidia Pittarello
Publikováno v:
Geological Society of America Abstracts with Programs.
Autor:
J. Van Orman, Addi Bischoff, Klaus Mezger, Martin J. Whitehouse, J. Roszjar, G. Srinivasan, Erik E. Scherer
Publikováno v:
Earth and Planetary Science Letters. 452:216-226
The asteroid 4 Vesta is the second most massive planetesimal in the Solar System and a rare example of a planetary object that possibly can be linked to a specific group of differentiated meteorites, the howardite–eucrite–diogenite suite. The 182
Autor:
Akira Yamaguchi, Vinciane Debaille, J. Roszjar, Lidia Pittarello, Philippe Claeys, Christian Koeberl
Publikováno v:
Meteoritics & Planetary Science
Meteoritics & planetary science, 2019
Meteoritics & planetary science, 2019
Meteorite fusion crusts are quenched melt layers formed during meteoroid atmospheric entry, mostly preserved as coating on the meteorite surface. Antarctic ureilite Asuka (A) 09368 and H chondrites A 09004 and A 09502 exhibit well preserved thick fus
Autor:
Joshua F. Snape, Jeremy J. Bellucci, Alexander A. Nemchin, J. Roszjar, Martin J. Whitehouse, Phil A. Bland, Gretchen Benedix
The initial Pb compositions of one enriched shergottite, one intermediate shergottite, two depleted shergottites, and Nakhla have been measured by Secondary Ion Mass Spectrometry (SIMS). These values, in addition to data from previous studies using a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6286d533abe1fed2f3bc4179916ef303
http://urn.kb.se/resolve?urn=urn:nbn:se:nrm:diva-2992
http://urn.kb.se/resolve?urn=urn:nbn:se:nrm:diva-2992
Publikováno v:
Microstructural Geochronology
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3154fa00dd5b173adc5dcd575c2a12ad
https://doi.org/10.1002/9781119227250.ch5
https://doi.org/10.1002/9781119227250.ch5