Results 131 to 140 of about 3,558 (195)

The variety and origin of materials accreted by Bennu's parent asteroid. [PDF]

Nat Astron
Barnes JJ, Nguyen AN, Abernethy FAJ, Bajo K, Bekaert DV, Bloch E, Brennecka GA, Busemann H, Cowpe JS, Crowther SA, Ek M, Fawcett LJ, Fehr MA, Franchi IA, Füri E, Gilmour JD, Grady MM, Greenwood RC, Haenecour P, Kawasaki N, Koefoed P, Krietsch D, Le L, Liszewska KM, Maden C, Malley J, Marrocchi Y, Marty B, Meyer LAE, Peretyazhko TS, Piani L, Render J, Russell SS, Rüfenacht M, Sakamoto N, Schönbächler M, Shollenberger QR, Smith L, Thomas-Keprta K, Verchovsky AB, Villeneuve J, Wang K, Welten KC, Wimpenny J, Worsham EA, Yurimoto H, Zimmermann L, Zhao X, Alexander CMO, Amini M, Baczynski A, Bland P, Borg LE, Burgess R, Caffee MW, Chaves LC, Clay PL, Dworkin JP, Foustoukos DI, Glavin DP, Hamilton VE, Hill D, House CH, Huss GR, Ireland T, Jilly CE, Jourdan F, Keller LP, Kruijer TS, Lai V, McCoy TJ, Nagashima K, Nishiizumi K, Ogliore R, Ong IJ, Reddy SM, Rickard WDA, Sandford S, Saxey DW, Timms N, Weis D, Wilbur ZE, Zega TJ, DellaGiustina DN, Wolner CWV, Connolly HC, Lauretta DS.   +86 more
europepmc   +1 more source

The ²⁶Al-²⁶Mg systematics of FeO-rich chondrules from Acfer 094: two chondrule generations distinct in age and oxygen isotope ratios. [PDF]

Geochim Cosmochim Acta, 2019
Hertwig AT, Makoto K, Ushikubo T, Defouilloy C, Kita NT.   +4 more
europepmc   +1 more source

Hourglass chondrules

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

Are CK chondrites really a distinct group or just equilibrated CVs? [PDF]

, 2003
Franchi, I.A., Greenwood, R.G., Kearsley, A.T.   +2 more
core  

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  

The initial solar system abundance of ⁶⁰Fe and early core formation of the first asteroids. [PDF]

Sci Adv
Fang L, Moynier F, Chaussidon M, Limare A, Makhatadze GV, Villeneuve J.   +5 more
europepmc   +1 more source

The great isotopic dichotomy of the early Solar System. [PDF]

Nat Astron, 2019
Kruijer TS, Kleine T, Borg LE.
europepmc   +1 more source

The background temperature of the protoplanetary disk within the first four million years of the Solar System. [PDF]

Earth Planet Sci Lett, 2018
Schrader DL, Fu RR, Desch SJ, Davidson J.   +3 more
europepmc   +1 more source

Evidence for oxygen isotopic exchange in chondrules from Kaba (CV3.1) carbonaceous chondrite during aqueous fluid-rock interaction on the CV parent asteroid. [PDF]

Acta Geogr Geol Meteorol Debr Geol Gemorfol Termeszfoldr Sor, 2019
Krot AN, Nagashima K, Fintor K, Pál-Molnár E.   +3 more
europepmc   +1 more source

Chondrules as direct thermochemical sensors of solar protoplanetary disk gas. [PDF]

Sci Adv, 2018
Libourel G, Portail M.
europepmc   +1 more source