File:Bashō crater EN0244751374M.png
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說明
摘要
[編輯]描述Bashō crater EN0244751374M.png |
English: Date acquired: May 07, 2012
Image Mission Elapsed Time (MET): 244751374 Image ID: 1771144 Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS) Center Latitude: -31.66° Center Longitude: 189.89° E Resolution: 169 meters/pixel Scale: The diameter of Basho (the crater featured in this image) is approx. 80 km (50 mi.) Incidence Angle: 34.8° Emission Angle: 63.2° Phase Angle: 79.5° Of Interest: This striking, oblique image of Bashō shows the distinctive dark halo that encircles the crater. The halo is composed of "Low Reflectance Material" (LRM), which was excavated from depth when the crater was formed. Bashō is also renowned for its bright ray craters, which render the crater easily visible even from very far away. This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week. |
日期 | |
來源 | BASHED BASHO |
作者 | NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington |
授權條款
[編輯]Public domainPublic domainfalsefalse |
本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zh,NASA版權政策或JPL圖像使用政策) | ||
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日期/時間 | 縮圖 | 尺寸 | 用戶 | 備註 | |
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目前 | 2020年8月1日 (六) 17:38 | 1,020 × 1,024(857 KB) | Jstuby(對話 | 貢獻) | crop black line | |
2020年7月27日 (一) 05:03 | 1,024 × 1,024(862 KB) | Jstuby(對話 | 貢獻) | Uploaded a work by NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington from [https://messenger.jhuapl.edu/Explore/Science-Images-Database/gallery-image-865.html BASHED BASHO] with UploadWizard |
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水平解析度 | 28.34 dpc |
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垂直解析度 | 28.34 dpc |
檔案修改日期時間 | 2020年8月1日 (六) 17:37 |