日本地球惑星科学連合2016年大会

講演情報

ポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS13] 月の科学と探査

2016年5月22日(日) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*長岡 央(早稲田大学先進理工学部)、諸田 智克(名古屋大学大学院環境学研究科)、本田 親寿(会津大学)、西野 真木(名古屋大学宇宙地球環境研究所)

17:15 〜 18:30

[PPS13-P05] 月クレーター崩壊度地質ユニット年代測定法の適用評価

*坪内 彩音1春山 純一2三宅 亙1 (1.東海大学 工学研究科、2.宇宙航空研究開発機構 宇宙科学研究所)

キーワード:年代学、月面クレーター、クレーター崩壊度

The age of the moon is an important clue in understanding the former state of igneous activity of the moon. To explore the time course of the scale and the eruption of the magma leads to pursue the internal evolution of the moon. Generally, exploring crater size frequency distribution is used to determine the model ages of lunar geological units. However, this age determination is susceptible to the influence of secondary craters, and an error is likely to occur in the measured age. Therefore, by using another age determination, it is necessary to confirm whether the measurement age by the age determination that is free from influence of the secondary crater should be investigated. The way based on the status of crater collapse is another expected method for age determination of lunar geological units. In order to establish this method, it is needed to investigate the correlation between the age of the geological units and a parameter value expressed by F which is corresponding to the total amount of impacted objects disrupting the craters. Since the F value is a numerical value determined by the most collapsed crater in a geological unit, it does not include the effects of secondary craters probably occurring after the formation of the oldest most collapsed craters. Here, we explore the correlation relationship between the F values and the model ages based on crater size frequency distribution for several lunar geological units, and discuss the possibility of the way based on crater collapse as an age determination of lunar geological units.