跳至內容

File:Copland crater.png

頁面內容不支援其他語言。
這個檔案來自維基共享資源
維基百科,自由的百科全書

原始檔案 (2,272 × 1,884 像素,檔案大小:2.5 MB,MIME 類型:image/png


摘要

描述
English: *Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
  • Scale: Copland crater has a diameter of 208 kilometers (129 miles)
  • Projection: This image is a portion of the NAC approach mosaic from Mercury flyby 3. It is shown in a simple cylindrical map projection with a resolution of 500 meters/pixel (0.31 miles/pixel).
Of Interest: Visible in the center of this image is the crater Copland, recently named in honor of the American composer and pianist Aaron Copland. Aaron Copland and this crater are both unquestionably worthy candidates for named features on Mercury, but how this specific crater came to be known as Copland has an interesting back-story. Amateur astronomer Ronald Dantowitz and his colleagues Scott Teare and Marek Kozubal used the Mt. Wilson 60-inch telescope in 1998 to observe a very bright feature on this portion of Mercury's surface, and they assumed that the bright feature was an impact crater. Mr. Dantowitz expressed his wish that the crater be named "Copland" once better images of the area were obtained from spacecraft. Surprisingly, MESSENGER images from Mercury flyby 3 revealed that the small bright feature, seen at the left edge of this image, is not an impact crater but more closely resembles a volcanic vent! No convention for naming volcanic vents on Mercury has yet been adopted, because none were identified prior to MESSENGER's first Mercury flyby. However, even if a convention for naming volcanic features on Mercury is adopted in the future, the naming rules will likely differ from those for impact craters, and thus "Copland" would probably not be an acceptable name for the bright volcanic feature. A MESSENGER team member corresponded with Mr. Dantowitz and suggested that the name Copland be proposed instead for a large crater nearby. He agreed, and the International Astronomical Union (IAU) approved the name Copland on March 3, 2010. Copland crater is flooded with volcanic smooth plains material that could be related to the activity that formed the bright vent.
日期
來源 http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/Copland.png
作者 NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

授權條款

Public domain 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/zhNASA版權政策JPL圖像使用政策
警告:

說明

添加單行說明來描述出檔案所代表的內容

在此檔案描寫的項目

描繪內容

著作權狀態 繁體中文 (已轉換拼寫)

斷定方法:​美國聯邦政府的作品 繁體中文 (已轉換拼寫)

多媒體型式 繁體中文 (已轉換拼寫)

image/png

校驗和 繁體中文 (已轉換拼寫)

ea00f692e53dfa30995501d03a9ec9aaffccdfad

斷定方法:​SHA-1 中文 (已轉換拼寫)

2,616,420 位元組

1,884 像素

2,272 像素

檔案歷史

點選日期/時間以檢視該時間的檔案版本。

日期/時間縮⁠圖尺寸用戶備⁠註
目前2010年12月17日 (五) 18:40於 2010年12月17日 (五) 18:40 版本的縮圖2,272 × 1,884(2.5 MB)LobStoRreduced palette from 24-bit RGB to 8-bit greyscale
2010年4月30日 (五) 07:44於 2010年4月30日 (五) 07:44 版本的縮圖2,272 × 1,884(4.6 MB)Bryan Derksen{{Information |Description={{en|1=Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS) Scale: Copland crater has a diameter of 208 kilometers (129 miles) Projection: This image is a portion of the NAC approach mosaic from Mercur

下列頁面有用到此檔案:

全域檔案使用狀況

以下其他 wiki 使用了這個檔案: