Data Structure ?
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Data Structure ?
*The above analysis is the result extracted and analyzed by the system, and the specific actual data shall prevail.
README.md
# 背景
日食は、新月の時期に月がその2つの軌道交点のいずれかの近くにあるときにのみ起こります。そのとき、月の半影、本影、または偽本影が地球の表面を横切り、日食を引き起こすことができます。日食には4種類あります。部分日食は、月の半影が地球を横切り、本影と偽本影が地球を完全に外れるときに起こります。環状日食は、月の偽本影が地球を横切るが太陽を完全に覆わないときに起こります。全食は、月の本影が地球を横切り、太陽を完全に覆うときに起こります。また、ハイブリッド日食は、月の本影と偽本影が地球を横切り、環状日食と全食が異なる場所で見られるときに起こります。地球は、紀元前2000年から西暦3000年までの5000年間に11898回の日食を経験します。
月食は、満月の時期に月がその2つの軌道交点のいずれかの近くにあるときに起こります。そのとき、月が地球の半影または本影を通過し、月食を引き起こすことができます。月食には3種類あります。半影月食は、月が地球の半影を横切るが本影を外れるときに起こります。部分月食は、月が地球の半影と本影を横切るときに起こります。全食は、月が地球の半影と本影を横切り、完全に地球の本影に入るときに起こります。地球は、紀元前2000年から西暦3000年までの5000年間に12064回の月食を経験します。
# 謝辞
月食の予測は、NASAのゴダード宇宙飛行センターのフレッド・エスペナックによって行われました。
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