Planetary and lunar ephemeris EPM2021 and its significance for Solar system research

E. Pitjeva, D. Pavlov, D. Aksim, Margarita Kan
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引用次数: 3

Abstract

Abstract We present an updated public version of EPM (Ephemerides of Planets and the Moon). Since the last public version, EPM2017, many improvements were made in both the observational database and the mathematical model. Latest lunar laser ranging observations have been added, as well as radio ranges of Juno spacecraft and more recent ranges of Odyssey and Mars Reconnaissance Orbiter. EPM2021 uses a new improved way to calculate radio signal delays in solar plasma and has a major update in the method of determination of asteroid masses. Also, a delay-capable multistep numerical integrator was implemented for EPM in order to properly account for tide delay in the equations of the motion of the Moon. The improved processing accuracy has allowed to refine existing estimates of the mass of the Sun and its change rate, parameters of the Earth–Moon system, masses of the Main asteroid belt and the Kuiper belt; and also to raise important questions about existing numerical models of solar wind.
行星和月球星历EPM2021及其对太阳系研究的意义
摘要:我们提出了一个更新的EPM(行星和月球的星历)的公共版本。自上一个公开版本EPM2017以来,观测数据库和数学模型都进行了许多改进。新增了最新的月球激光测距观测,以及朱诺号航天器的无线电测距,以及奥德赛号和火星侦察轨道器最近的测距。EPM2021采用了一种新的改进方法来计算太阳等离子体中的无线电信号延迟,并对确定小行星质量的方法进行了重大更新。此外,为了更好地考虑月球运动方程中的潮汐延迟,在EPM中实现了具有延迟能力的多步数值积分器。处理精度的提高使现有的对太阳质量及其变化率、地月系统参数、主要小行星带和柯伊伯带质量的估计得以改进;同时也对现有的太阳风数值模型提出了重要的问题。
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