聂鲁达四边形的地质(H13)，水星

IF 1.9 4区地球科学 Q2 GEOGRAPHY

Journal of Maps Pub Date : 2023-09-14 DOI:10.1080/17445647.2023.2256353

Benjamin Man, David A. Rothery, Matthew R. Balme, Susan J. Conway, Jack Wright, David L. Pegg, Annie R. Lennox, Salvatore Buoninfante

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引用次数: 0

摘要

我们展示了水星聂鲁达四边形(H13)的第一张地质图。H13位于水星的南半球，在纬度22.5°S - 65°S，经度90°E-180°之间，总面积不到500万平方公里，相当于水星表面的6.5%。地图数字化以1:30万至1:70万的比例进行，最终以1:30万的比例呈现，这些数据来自美国宇航局信使号任务的任务结束数据产品。我们区分了三个主要的光地质平原单位:火山口间平原、中间平原和平滑平原。我们还根据陨石坑的降解状态来区分直径≥20 km的陨石坑及其材料。我们已经完成了两个版本的地图，一个使用三级火山口降解方案，另一个使用五级火山口降解方案。此外，还绘制了伦勃朗撞击盆地的具体地质单元图。这张地图为ESA-JAXA的BepiColombo水星任务提供了背景和目标。

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Geology of the Neruda quadrangle (H13), Mercury

We present the first geological map of the Neruda Quadrangle (H13), Mercury. H13 is in Mercury’s southern hemisphere between latitudes 22.5°S–65°S, and longitudes 90°E–180° covering a total area of just under 5 million km², equivalent to 6.5% of the planet’s surface. Map digitisation was carried out at scales between 1:300,000 and 1:700,000 for final presentation at 1:3,000,0000, from end-of-mission data products from NASA’s MESSENGER mission. We distinguish three main photogeologic plains units: intercrater, intermediate, and smooth plains. We also distinguish all craters and their materials ≥ 20 km in diameter based on their degradation state. We have completed two versions of the map, one using a three-class crater degradation scheme and one using a five-class crater degradation scheme. In addition, specific geological units were charted for the Rembrandt impact basin. This map has been constructed to provide context and targets for the ESA-JAXA BepiColombo mission to Mercury.

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来源期刊

Journal of Maps 地学-自然地理

CiteScore

4.30

自引率

9.10%

发文量

审稿时长

6-12 weeks

期刊介绍： The Journal of Maps is a peer-reviewed, inter-disciplinary, online journal that aims to provide a forum for researchers to publish maps and spatial diagrams.