Last Updated:2025/11/22

By measuring the pulsation periods of cepheid variables, astronomers can determine distances to nearby galaxies.

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By measuring the pulsation periods of cepheid variables, astronomers can determine distances to nearby galaxies.

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ケフェイド型変光星の脈動周期を測定することで、天文学者は近くの銀河までの距離を測定できます。

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