関連する実験動画
Updated: Jul 12, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
まとめ
月面のクレーターであるタイコは,月面の夜の間,周囲よりも暖かいままです. 97時間まで検出されたこの熱異常は,クレーター壁に吸収された太陽熱によるもので,月の内部熱によるものではありません.
科学分野:
- 月面地質学 月面地質学
- 惑星科学は惑星科学である.
- 熱画像は,熱画像によるものです.
背景:
- 月のクレーターティコは,月の夜間に顕著な熱異常を呈しています.
- 以前の研究では,クレーターとその周辺の間のこの温度差を観測しました.
研究 の 目的:
- 月面のクレーターTychoに関連した熱異常の原因を調査するために.
- 異常が太陽の熱か月の内部熱によるものかどうかを判断する.
主な方法:
- 月の夜間のタイコクレーターの赤外線画像の取得.
- 太陽光照明の停止後,最大97時間,熱異常をモニタリングします.
主要な成果:
- ティコクレーターは,月の夜間に周囲よりも暖かいことが観察されました.
- 熱異常の温度は,時間とともに徐々に低下した.
- 異常は,新月期以降には検出できなくなった.
- 日没前の太陽に向いているより急なクレーターの壁は,冷却期中により暖かかった.
結論:
- 月のクレーターTychoの熱異常は,主にその壁によって吸収された太陽熱によって引き起こされます.
- 観測された現象は,月の内部熱源に起因するものではありません.
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