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单词 aphelion
释义

Definition of aphelion in English:

aphelion

nounPlural aphelia apˈhiːlɪənəˈfiliən
Astronomy
  • The point in the orbit of a planet, asteroid, or comet at which it is furthest from the sun.

    〔天文〕远日点

    Mars is at aphelion

    火星处在远日点。PERIHELION 的反义词。

    The opposite of perihelion
    Example sentencesExamples
    • Variations in the timing of perihelion and aphelion are caused by a ‘wobbling’ in the Earth's axis of rotation as it rotates around the Sun.
    • There are small cyclic variations in those apparent sizes because the Earth-Moon distance changes as the latter moves between perigee and apogee, and the Earth-Sun separation alters as the former moves between perihelion and aphelion.
    • Furthermore, any resonance with the Earth is illusory in that Mercury is not well placed for observations except during its brief greatest elongations near its aphelion.
    • This is because at aphelion the planet is moving slowest, and consequently it is less likely to pass across the Sun during the critical window.
    • This affects the climate because the influx of solar energy to our planet would then vary between perihelion and aphelion by a larger proportion than at present.

Origin

Mid 17th century: alteration of modern Latin aphelium (by substitution of the Greek inflection -on), from Greek aph' hēlion 'from the sun'.

Definition of aphelion in US English:

aphelion

nounəˈfēlēənəˈfiliən
Astronomy
  • The point in the orbit of a planet, asteroid, or comet at which it is furthest from the sun.

    〔天文〕远日点

    Mars is at aphelion

    火星处在远日点。PERIHELION 的反义词。

    The opposite of perihelion
    Example sentencesExamples
    • Variations in the timing of perihelion and aphelion are caused by a ‘wobbling’ in the Earth's axis of rotation as it rotates around the Sun.
    • This is because at aphelion the planet is moving slowest, and consequently it is less likely to pass across the Sun during the critical window.
    • This affects the climate because the influx of solar energy to our planet would then vary between perihelion and aphelion by a larger proportion than at present.
    • There are small cyclic variations in those apparent sizes because the Earth-Moon distance changes as the latter moves between perigee and apogee, and the Earth-Sun separation alters as the former moves between perihelion and aphelion.
    • Furthermore, any resonance with the Earth is illusory in that Mercury is not well placed for observations except during its brief greatest elongations near its aphelion.

Origin

Mid 17th century: alteration of modern Latin aphelium (by substitution of the Greek inflection -on), from Greek aph' hēlion ‘from the sun’.

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更新时间:2024/11/8 23:24:58