Results 141 to 150 of about 5,656 (205)

Triple oxygen isotopes of lunar water unveil indigenous and cometary heritage. [PDF]

Proc Natl Acad Sci U S A
Thiemens MM, Martinez MHN, Thiemens MH.
europepmc   +1 more source

The role of Bells in the continuous accretion between the CM and CR chondrite reservoirs. [PDF]

Meteorit Planet Sci, 2020
van Kooten E, van Kooten E, Cavalcante L, Wielandt D, Bizzarro M.   +4 more
europepmc   +1 more source

A 4,565-My-old record of the solar nebula field. [PDF]

Proc Natl Acad Sci U S A
Maurel C, Gattacceca J.
europepmc   +1 more source

The late formation of chondrites as a consequence of Jupiter-induced gaps and rings. [PDF]

Sci Adv
Srivastava B, Izidoro A.
europepmc   +1 more source

Meteoritic Evidence for a Ceres-sized Water-rich Carbonaceous Chondrite Parent Asteroid. [PDF]

Nat Astron, 2020
Hamilton VE, Goodrich CA, Treiman AH, Connolly HC, Zolensky ME, Shaddad MH.   +5 more
europepmc   +1 more source

Interstellar ices as carriers of supernova material to the early solar system. [PDF]

Nat Commun
Bizzarro M, Schiller M, Holst J, Bouvier L, Groen M, Moynier F, van Kooten EMME, Schönbächler M, Haugbølle T, Watson D, Johansen A, Connelly JN, Bizzarro E.   +12 more
europepmc   +1 more source

Oxygen isotope characteristics of chondrules from the Yamato‐82094 ungrouped carbonaceous chondrite: Further evidence for common O‐isotope environments sampled among carbonaceous chondrites

, 2017
T. Tenner, M. Kimura, N. Kita
semanticscholar   +1 more source

The nucleosynthetic fingerprint of the outermost protoplanetary disk and early Solar System dynamics. [PDF]

Sci Adv
van Kooten E, Zhao X, Franchi I, Tung PY, Fairclough S, Walmsley J, Onyett I, Schiller M, Bizzarro M.   +8 more
europepmc   +1 more source

Early silica crust formation in planetesimals by metastable silica-rich liquid immiscibility or cristobalite crystallisation: the possible origin of silica-rich chondrules. [PDF]

Sci Rep, 2020
Faure F.
europepmc   +1 more source

History of chondrule forming heating events inferred from chondrule age distribution

History of chondrule forming heating events inferred from chondrule age distribution
Chondrules are major components in primitive meteorites and consist of 70 percent by volume in ordinary chondrites. They are considered to be formed by a flash heating of dusts in the protoplanetary disk, though the nature of the heating mechanism is not yet well understood.
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