首页> 外文期刊>Journal of Astrophysics & Aerospace Technology >Energy Dissipated by an Aster Accelerated in a Gravitational Field: Estimation of the Lifetime of a Planet or a Star Being Destroyed
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Energy Dissipated by an Aster Accelerated in a Gravitational Field: Estimation of the Lifetime of a Planet or a Star Being Destroyed

机译:在引力场中加速的紫ster耗散的能量:估计被毁行星或恒星的寿命

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An equation giving the Energy Dissipated by an aster accelerated in a Gravitational Field (EDGF) is presented. EDGF is applied in the present work to express the Schwarzschild radius and to calculate the total evaporation time of the Sun, of the nucleus of our Galaxy and of any star being collapsing gravitationally. Evaporation times of the planets of the Solar system is tabulated in a model where they are swallowed by the Sun collapsing gravitationally from its stage of red giant up to that of white dwarf. In addition, EDGF is used to estimate the scale of the Solar system (limit of the Solar system) which is an important criterion for the identification of a planet or a celestial object as belonging to the Solar system or not. In this work, the limit of the Solar system is estimated at about 160 AU. All our results are compared with available astronomical previsions.
机译:提出了一个方程,给出了在引力场(EDGF)中加速的翠菊耗散的能量。 EDGF用于当前工作中,以表示Schwarzschild半径,并计算太阳,银河系原子核以及万有引力塌陷的任何恒星的总蒸发时间。在一个模型中,将太阳系行星的蒸发时间列表化为一个模型,在该模型中,太阳在重力作用下从红色巨人阶段到白矮星阶段被吞噬。此外,EDGF用于估算太阳系的规模(太阳系的极限),这是识别行星或天体是否属于太阳系的重要标准。在这项工作中,估计太阳系的极限约为160 AU。我们将所有结果与可用的天文预报进行了比较。

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