Results 181 to 190 of about 3,499 (221)

Carbon and oxygen isotope evidence for a protoplanetary disk origin of organic solids in meteorites. [PDF]

Proc Natl Acad Sci U S A
Lawrence WM, Blake GA, Eiler J.
europepmc   +1 more source

Formation of Lunar Basins from Impacts of Leftover Planetesimals

, 2022
Nesvorny D, Roig F, Vokrouhlicky D, Bottke W(, Marchi S, Morbidelli A, Deienno R.   +6 more
europepmc   +1 more source

When wet meets dry: An Ivuna-like impactor triggered volatile loss on the angrite parent body. [PDF]

Sci Adv
Zhu 朱柯 K, Chen Q, Yokoyama T, Yamaguchi A, Bouvier A, Chen L.   +5 more
europepmc   +1 more source

Magnesium phosphates experienced high-temperature transition found on the CI-like carbonaceous chondrite Yamato 980115 by Raman microspectroscopy. [PDF]

Anal Sci
Yui H, Tsychiya H, Kashima A, Urashima SH, Oguchi K, Imae N, Yamaguchi A.   +6 more
europepmc   +1 more source

Recent progress and future prospects of the early solar system chronology. [PDF]

Natl Sci Rev
Amelin Y, Yin QZ.
europepmc   +1 more source

Decoding the formation of barred olivine chondrules: Realization of numerical replication. [PDF]

Sci Adv
Miura H, Morita T, Nakamura T, Watanabe K, Tsuchiyama A, Kimura Y, Koyama C.   +6 more
europepmc   +1 more source

Planetesimals

, 2017
Processes governing the evolution of planetesimals are critical to understanding how rocky planets are formed, how water is delivered to them, the origin of planetary atmospheres, how cores and magnetic dynamos develop, and ultimately, which planets have the potential to be habitable.
core   +3 more sources

Small planetesimals in a massive disk formed Mars

Icarus, 2013
Mars is likely to be a planetary embryo formed through collisions with planetesimals, which can explain its small mass and rapid formation timescale obtained from 182Hf-182W chronometry.
Nicolas Dauphas
exaly   +2 more sources

Impact disruption of primordial planetesimals [PDF]

Planetary and Space Science, 2013
It isusually assumed that 1-10-km  sized planetesimals are formed    through coagulation processes and     continue to agglomerate via pairwise mergers.
Parisi, Mirta Gabriela
exaly   +2 more sources