Results 151 to 160 of about 5,656 (205)

In situ 60 Fe- 60 Ni systematics of chondrules from unequilibrated ordinary chondrites

, 2018
M. Telus, G. Huss, K. Nagashima, R. Ogliore, S. Tachibana   +4 more
semanticscholar   +1 more source

Tungsten isotopic constraints on the age and origin of chondrules

Proceedings of the National Academy of Sciences of the United States of America, 2016
G. Budde, T. Kleine, T. Kruijer, C. Burkhardt, K. Metzler   +4 more
semanticscholar   +1 more source

Phase-specific nanoscale mechanics of anhydrous astromaterials and implications for larger-scale strength. [PDF]

npj Space Explor
Davis TP, Garvie LAJ, Hoover CG.
europepmc   +1 more source

Physicochemical Controls on the Compositions of the Earth and Planets. [PDF]

Space Sci Rev
Sossi PA, Hin RC, Kleine T, Morbidelli A, Nimmo F.   +4 more
europepmc   +1 more source

The fall, recovery, classification, and initial characterization of the Hamburg, Michigan H4 chondrite. [PDF]

Meteorit Planet Sci, 2020
Heck PR, Greer J, Boesenberg JS, Bouvier A, Caffee MW, Cassata WS, Corrigan C, Davis AM, Davis DW, Fries M, Hankey M, Jenniskens P, Schmitt-Kopplin P, Sheu S, Trappitsch R, Velbel M, Weller B, Welten K, Yin QZ, Sanborn ME, Ziegler K, Rowland D, Verosub KL, Zhou Q, Liu Y, Tang G, Li Q, Li X, Zajacz Z.   +28 more
europepmc   +1 more source

In Situ Helium Isotope Microimaging of Meteorites. [PDF]

Anal Chem
Bajo KI, Kawasaki N, Sakaguchi I, Suzuki TT, Itose S, Matsuya M, Ishihara M, Uchino K, Yurimoto H.   +8 more
europepmc   +1 more source

Hourglass chondrules

, 2011
Warin, Roger, Hatert, Frédéric, Kashuba, John   +2 more
openaire   +1 more source

Relict chondrules in primitive achondrites: Remnants from their precursor parent bodies

, 2017
D. Schrader, T. Mccoy, K. Gardner-Vandy
semanticscholar   +1 more source

I-Xe systematics of the impact plume produced chondrules from the CB carbonaceous chondrites: Implications for the half-life value of 129I and absolute age normalization of 129I-129Xe chronometer.

Geochimica et Cosmochimica Acta, 2017
O. Pravdivtseva, A. Meshik, C. Hohenberg, A. Krot   +3 more
semanticscholar   +1 more source

Shock-wave heating model for chondrule formation: Formation of prolate chondrules

Shock-wave heating model for chondrule formation: Formation of prolate chondrules
Millimeter-sized, spherical silicate grains abundant in chondritic meteorites, which are called as chondrules, are considered to be a strong evidence of the melting event of the dust particles in the protoplanetary disk. One of the most plausible scenarios is that the chondrule precursor dust particles are heated and melt in the high-velocity rarefied ...
openaire