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Understanding Apoapsis and Periapsis: The Extremes of an Orbital Journey

Jenny Bose


 Orbiting celestial bodies follow a continuous path around their parent objects, be it planets around stars or satellites around planets. This orbital journey is characterized by two critical points: the apoapsis and periapsis. Understanding these extremes of an orbital trajectory is fundamental to comprehending the mechanics and dynamics of celestial motion. In this article, we delve into the concepts of apoapsis and periapsis, exploring their significance in the fascinating world of orbits.


索引于

  • 中国社会科学院
  • 谷歌学术
  • 打开 J 门
  • 中国知网(CNKI)
  • 引用因子
  • 宇宙IF
  • 电子期刊图书馆
  • 研究期刊索引目录 (DRJI)
  • 秘密搜索引擎实验室
  • ICMJE

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