Results 21 to 30 of about 312,228 (284)
Probing Massive Star Nucleosynthesis with Data on Metal-Poor Stars and the Solar System [PDF]
Metal-poor stars were formed during the early epochs when only massive stars had time to evolve and contribute to the chemical enrichment. Low-mass metal-poor stars survive until the present and provide fossil records of the nucleosynthesis of early ...
Qian Yong-Zhong
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THE PHYSICAL MEANING OF THE TITIUS-BODE FORMULA
It is proposed an special hypothesis of the formation of symmetric objects in space with the help of the interference of standing waves which act in the process of evolution of the primordial gas-dust cloud including the formation of the Solar system ...
V. A. Smirnov
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The dynamics of Wolf numbers based on nonlinear dynamo with magnetic helicity: comparisons with observations [PDF]
We investigate the dynamics of solar activity using a nonlinear one-dimensional dynamo model and a phenomenological equation for the evolution of Wolf numbers. This system of equations is solved numerically. We take into account the algebraic and dynamic
Kleeorin, N. +5 more
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EUV imaging and spectroscopy for improved space weather forecasting
Accurate predictions of harmful space weather effects are mandatory for the protection of astronauts and other assets in space, whether in Earth or lunar orbit, in transit between solar system objects, or on the surface of other planetary bodies. Because
Golub Leon +8 more
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Organic Matter in the Asteroid Ryugu: What We Know So Far
The Hayabusa2 mission was tasked with returning samples from the C-complex asteroid Ryugu (1999 JU3), in order to shed light on the formation, evolution and composition of such asteroids.
Christian Potiszil +8 more
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The formation of the solar system
The solar system started to form about 4.56 Gyr ago and despite the long intervening time span, there still exist several clues about its formation. The three major sources for this information are meteorites, the present solar system structure and the ...
Davies, M. B. +9 more
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Vesta and Ceres: crossing the history of the Solar System
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.
Coradini, Angioletta +3 more
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Asteroids and comets, which have long been of interest to astronomers, are important components of the solar system. They contain rich primitive information about the early solar system, which provide a unique pathway for studying the formation and ...
ShiBang Du +12 more
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Control of Magnetopause Flux Rope Topology by Non-local Reconnection
Dayside magnetic reconnection between the interplanetary magnetic field and the Earth’s magnetic field is the primary mechanism enabling mass and energy entry into the magnetosphere.
Lars Mejnertsen +2 more
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Planetary Engulfment Prognosis within the ρ CrB System
Exoplanets have been detected around stars at various stages of their lives, ranging from young stars emerging from formation to the latter stages of evolution, including white dwarfs and neutron stars.
Stephen R. Kane
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