Results 61 to 70 of about 838,568 (119)

Evidence for Magnetically‐Driven Accretion in the Distal Solar System

AGU Advances
Paleomagnetic measurements of meteorites indicate that magnetic fields existed in the inner solar nebula capable of driving accretion at rates similar to those observed for young stellar objects with protoplanetary disks.
Elias N. Mansbach, Benjamin P. Weiss, Eduardo A. Lima, Michael Sowell, Joseph L. Kirschvink, Roger R. Fu, Saverio Cambioni, Xue‐Ning Bai, Jodie B. Ream, Chisato Anai, Atsuko Kobayashi, Hironori Hidaka   +11 more
doaj   +1 more source

Ejection of Bodies from the Solar System in the Course of the Accumulation of the Giant Planets and the Formation of the Cometary Cloud [PDF]

, 1972
V. S. Safronov
openalex   +1 more source

Planetary Formation Constrained by Collisions between Millimeter-sized Lunar Particles and Lunar Surface from Chang’E-4 Mission

The Astrophysical Journal
Exploring low-velocity collisions is crucial for unraveling intricate processes in planetary formation, particularly the bouncing barrier that impedes the aggregation of dust into sizable planetesimals.
Lei Lei, Xiaoping Zhang, Pengwei Luo, Guozheng Zhang, Jilin You, Jiahui Liu, Yanyan Xu, Shuai Fu, Xiongyao Li, Zhiguo Meng, Cunhui Li, Haiyan Zhang, Yunzhao Wu   +12 more
doaj   +1 more source

The Formation of Disks by Inelastic Collisions of Gravitating Particles. Applications to the Dynamics of the Saturn's Ring and to the Formation of the Solar System [PDF]

, 1974
A. Brahic
openalex   +1 more source

Presolar grains [PDF]

The chemical makeup of our solar system is a reflection of Galactic chemical evolution in the local interstellar medium (ISM) over the past ~9 Ga before the formation of the solar system. Although the incorporated ISM dust was mostly destroyed during the solar system formation, a small fraction of the ISM dust, known as presolar grains, is preserved in
arxiv   +1 more source

Early Solar System Turbulence Constrained by High Oxidation States in the Oldest Noncarbonaceous Planetesimals

The Planetary Science Journal
Early solar system (SS) planetesimals constitute the parent bodies of most meteorites investigated today. Nucleosynthetic isotope anomalies of bulk meteorites have revealed a dichotomy between noncarbonaceous (NC) and carbonaceous (CC) groups ...
Teng Ee Yap, Konstantin Batygin, François L. H. Tissot   +2 more
doaj   +1 more source

Structure of Self-Gravitating Discs and Solar System Formation [PDF]

, 1980
J.B.C. Davies
openalex   +1 more source

Volatile-rich comets ejected early on during Solar System formation [PDF]

, 2022
Sarah Anderson, Jean-Marc Petit, Benoît Noyelles, O. Mousis, P. Rousselot   +4 more
openalex   +3 more sources

Massive Supernovae, Orion Gamma Rays, and the Formation of the Solar System [PDF]

, 1995
A. G. W. Cameron, Peter Höflich, Philip C. Myers, Donald D. Clayton   +3 more
openalex   +1 more source

Meteoritic Evidence for the Infall of Large Interstellar Dust Aggregates during the Formation of the Solar System [PDF]

, 1998
John A. Wood
openalex   +1 more source