Results 21 to 30 of about 838,568 (119)
Frontiers in Chemistry, 2021 The occurrence of hydrogen atom-ordered form of ice Ih, ice XI, in the outer Solar System has been discussed based on laboratory experiments because its ferroelectricity influences the physical processes in the outer Solar System.
Akira Kouchi +12 more
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Vesta and Ceres: crossing the history of the Solar System [PDF]
Space Science Reviews, 2011, Volume 163, Issue 1-4, pp. 25-40, 2011 The evolution of the Solar System can be schematically divided into three different phases: the Solar Nebula, the Primordial Solar System and the Modern Solar System. These three periods were characterized by very different conditions, both from the point of view of the physical conditions and from that of the processes there were acting through them ...
arxiv +1 more source
Evolution of Stars on The Establishment of The Solar System and Planetary System
Jurnal Ilmiah Pendidikan Fisika Al-Biruni, 2016 This research is the literature studies that provide an introduction to the theory of the formation and early evolution of solar system and planetary systems.
Khilyatul Khoiriyah
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On the Solar System-Debris Disk Connecction [PDF]
, 2007 This paper emphasizes the connection between solar and extra-solar debris disks: how models and observations of the Solar System are helping us understand the debris disk phenomenon, and vice versa, how debris disks are helping us place our Solar System into context.
arxiv +1 more source
Market Formation in Turkish Solar Electricity Generation: Technology Innovation System Approach
İzmir İktisat Dergisi, 2023 The Technological Innovation System (TIS) is a theoretical approach to the analysis of a new technology's diffusion dynamics. The development and establishment of market-related structures are essential for maturing a TIS and its long-term success ...
Erkan Erdil, Yelda Erden Topal
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Protracted Timescales for Nebular Processing of First-formed Solids in the Solar System
The Astrophysical Journal, 2023 The calcium–aluminum-rich inclusions (CAIs) from chondritic meteorites are the first solids formed in the solar system. Rim formation around CAIs marks a time period in early solar system history when CAIs existed as free-floating objects and had not yet
Prajkta Mane +3 more
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The Eons of Chaos and Hades [PDF]
Solid Earth, 2010 We propose the <i>Chaotian Eon</i> to demarcate geologic time from the origin of the Solar System to the Moon-forming impact on Earth. This separates the solar system wide processes of planet formation from the subsequent divergent evolution ...
C. Goldblatt +3 more
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Refractory Metal Nuggets -- Formation of the First Condensates in the Solar Nebula [PDF]
, 2012 As gas flowed from the solar accretion disk or solar nebula onto the proto-Sun, magnetic pressure gradients in the solar magnetosphere and the inner solar nebula provided an environment where some of this infalling flow was diverted to produce a low pressure, high temperature, gaseous, "infall" atmosphere around the inner solar nebula.
arxiv +1 more source
Constraining the parameter space for the Solar Nebula [PDF]
, 2020 If we want to understand planetesimal formation, the only data set we have is our own Solar System. It is particularly interesting as it is so far the only planetary system we know of that developed life. Understanding the conditions under which the Solar Nebula evolved is crucial in order to understand the different processes in the disk and the ...
arxiv +1 more source
EPJ Web of Conferences, 2009 The outer solar system extends beyond a heliocentric distance of 5 AU. It contains the giant planets and their systems (rings and satellites), the Kuiper belt, the comets (except those which approach episodically the inner solar system) and, at its outer
Encrenaz T.
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