Results 51 to 60 of about 42,149 (288)
Collisions in the solar system - I. Impacts of the Apollo-Amor-Aten asteroids upon the terrestrial planets [PDF]
Monthly Notices of the Royal Astronomical Society, 1985 On determine, a l'aide d'une nouvelle technique, la probabilite de collision entre chacun des asteroides de population connue (4 Aten, 34 Apollo et 38 Amor) et chacune des planetes ...
D. I. Steel, W. J. Baggaley
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Advanced Science, EarlyView.Sodium ion capacitor (SIC) is currently constrained by the low discharge capacity of commercial activated carbon as positive electrode material. This review provides a holistic summary of research efforts on alternative porous carbon materials for SIC. Image created by the authors with www.biorender.com.
Ademola Adeniji +2 more
wiley +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.
doaj +1 more source
Stochasticity & Predictability in Terrestrial Planet Formation [PDF]
, 2016 Terrestrial planets are thought to be the result of a vast number of gravitational interactions and collisions between smaller bodies. We use numerical simulations to show that practically identical initial conditions result in a wide array of final ...
Grimm, Simon L. +3 more
core +2 more sources
Advanced Science, EarlyView.2D ferroelectrics materials enabling non‐volatile polarization memory, optical excitability, and neuromorphic processing within a unified material and provides a mechanistic analysis of polarization‐induced band modulation, including photon‐assisted domain reorientation, switching kinetics, and interfacial dipole coupling that governs resistive ...
Parthasarathi Pal +3 more
wiley +1 more source
Formation of the terrestrial planets in the solar system around 1 au via radial concentration of planetesimals [PDF]
Astronomy & Astrophysics, 2018 Context. No planets exist inside the orbit of Mercury and the terrestrial planets of the solar system exhibit a localized configuration. According to thermal structure calculation of protoplanetary disks, a silicate condensation line (~1300 K) is located around 0.1 au from the Sun except for the early phase of disk evolution, and planetesimals could ...
Ogihara, Masahiro +3 more
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Advanced Electronic Materials, EarlyView.This tutorial introduces a practical framework for implementing early‐stage Life‐Cycle Assessment (LCA) in flexible and printed electronics. Using organic electrochemical transistors (OECTs) as a case study, the modular Process‐of‐Record and open‐access inventory provides a rich resource adaptable to a plethora of technologies in printed electronics ...
Laura Teuerle +6 more
wiley +1 more source
The Astrophysical Journal, 2023 We introduce a mathematical framework for statistical exoplanet population and astrobiology studies that may help direct future observational efforts and experiments.
Piero Madau
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Atmospheric Circulation of Exoplanets [PDF]
, 2009 We survey the basic principles of atmospheric dynamics relevant to explaining existing and future observations of exoplanets, both gas giant and terrestrial.
Cho, James Y-K. +2 more
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Formation of the Terrestrial Planets from a Narrow Annulus
, 2009 We show that the assembly of the Solar System terrestrial planets can be successfully modelled with all of the mass initially confined to a narrow annulus between 0.7 and 1.0 AU.
Brad M. S. Hansen +20 more
core +1 more source