Results 141 to 150 of about 3,808 (207)

Chondrules in the wind [PDF]

, 2012
Tamara Goldin
openalex   +1 more source

Erratum: “Compound Chondrule Formation in Optically Thin Shock Waves” (2019, ApJ, 877, 84)

, 2022
Sota Arakawa, T. Nakamoto
openalex   +1 more source

Low-Temperature Aqueous Alteration of Chondrites. [PDF]

Space Sci Rev
Lee MR, Alexander CMO, Bischoff A, Brearley AJ, Dobrică E, Fujiya W, Le Guillou C, King AJ, van Kooten E, Krot AN, Leitner J, Marrocchi Y, Patzek M, Petaev MI, Piani L, Pravdivtseva O, Remusat L, Telus M, Tsuchiyama A, Vacher LG.   +19 more
europepmc   +1 more source

Experimental chondrules by melting samples of olivine, clays and carbon with a CO2 laser

, 2015
K. E. Cervantes-de la Cruz, Fernando Ortega‐Gutiérrez, Jesús Solé Viñas, Antígona Segura Peralta, Margarita Adela Margarita Adela, Blanca Sonia Ángeles García, María del Consuelo Macías Romo, Carlos Linares López   +7 more
openalex   +1 more source

Secondary Ion Mass Spectrometry for Mg Isotope Ratio Measurements: Application to Meteoritic Chondrules and Cometary Particles [PDF]

, 2020
N. T. Kita, Kohei Fukuda, Guillaume Siron   +2 more
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Cross-Scale Multimodal Imaging for Organic Matter in Extraterrestrial Samples. [PDF]

Anal Chem
Dong M, Yang W, Hao J, Jia X, Yang O, Lo MKF, Cao B, Hu S, Lin Y.   +8 more
europepmc   +1 more source

Chondrule age distribution and rate of heating events for chondrule formation

Chondrule age distribution and rate of heating events for chondrule formation
Chondrules are considered to be formed by flash heating events in the protoplanetary disk. In order to evaluate some basic factors in the heating mechanism, we examined the rate of heating events that explains the abundance and the observed age distribution of chondrules in unequilibrated ordinary chondrites. First, we compiled the literature data of ^(
openaire   +1 more source

The Ni isotopic composition of Ryugu reveals a common accretion region for carbonaceous chondrites. [PDF]

Sci Adv
Spitzer F, Kleine T, Burkhardt C, Hopp T, Yokoyama T, Abe Y, Aléon J, O'D Alexander CM, Amari S, Amelin Y, Bajo KI, Bizzarro M, Bouvier A, Carlson RW, Chaussidon M, Choi BG, Dauphas N, Davis AM, Di Rocco T, Fujiya W, Fukai R, Gautam I, Haba MK, Hibiya Y, Hidaka H, Homma H, Hoppe P, Huss GR, Ichida K, Iizuka T, Ireland TR, Ishikawa A, Itoh S, Kawasaki N, Kita NT, Kitajima K, Komatani S, Krot AN, Liu MC, Masuda Y, Morita M, Moynier F, Motomura K, Nakai I, Nagashima K, Nguyen A, Nittler L, Onose M, Pack A, Park C, Piani L, Qin L, Russell SS, Sakamoto N, Schönbächler M, Tafla L, Tang H, Terada K, Terada Y, Usui T, Wada S, Wadhwa M, Walker RJ, Yamashita K, Yin QZ, Yoneda S, Young ED, Yui H, Zhang AC, Nakamura T, Naraoka H, Noguchi T, Okazaki R, Sakamoto K, Yabuta H, Abe M, Miyazaki A, Nakato A, Nishimura M, Okada T, Yada T, Yogata K, Nakazawa S, Saiki T, Tanaka S, Terui F, Tsuda Y, Watanabe SI, Yoshikawa M, Tachibana S, Yurimoto H.   +90 more
europepmc   +1 more source

Reply to: The breakup of a long-period comet is not a likely match to the Chicxulub impactor. [PDF]

Sci Rep, 2022
Siraj A, Loeb A.
europepmc   +1 more source

Impact-induced sublimation drives volatile depletion in carbonaceous meteorites. [PDF]

Nat Commun
Long ZY, Moynier F, Bögels TFJ, Fang L, Caracas R, Paquet M, Jourdan F, Luu TH, Rigoussen D, Qiu KF, Deng J, Day JMD.   +11 more
europepmc   +1 more source