Last Updated:2025/11/30

The astronomers closely monitored the Mira variable as its brightness declined over a 330-day cycle.

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The astronomers closely monitored the Mira variable as its brightness declined over a 330-day cycle.

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天文学者たちは、光度が約330日周期で低下するミラ型変光星(周期が100日以上で非常に赤く、赤外線で1等以上、可視光で2.5等以上の振幅を示す脈動変光星)を注意深く観測した。

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