File:PIA23529-Mars-DustDeposits-SyriaPlanum-20190811.jpg

页面内容不支持其他语言。
這個文件來自維基共享資源
维基百科,自由的百科全书

原始文件(2,880 × 1,800像素,文件大小:1.03 MB,MIME类型:image/jpeg


摘要

描述
English: PIA23529: Pristine Dust Deposits in Syria Planum

https://photojournal.jpl.nasa.gov/catalog/PIA23529

This image, acquired on August 11, 2019 by NASA's Mars Reconnaissance Orbiter, shows wind-blown deposits known as transverse aeolian ridges (TARs). They are frequently visible in images of the Martian tropics.

Wind-blown deposits known as transverse aeolian ridges (TARs) are frequently visible in images of the Martian tropics. They are bright ripples with heights of 2.6 meters and spacing that averages 47 meters. The TARs generally appear inactive and eroded, sometimes cratered or littered with boulders from nearby impacts and avalanches.

In Syria Planum, unusual bright deposits might be accumulations of dust blown from higher to lower elevations by nighttime slope winds, reaching speeds of up to 50 meters per second. These dust deposits resemble TARs in height and spacing but with a distinct shape from other TARs. A close up view shows that the deposits form pyramidal features with steep faces on the upwind sides (wind is blowing from the top of the picture) and tapered slopes in the downwind direction. Ridges form where the "pyramids" line up together, and the spacing of the ridges appears to be controlled by the length of the "pyramids."

These observations suggest that TARs elsewhere on Mars may have formed in a similar fashion, perhaps millions of years ago when the atmosphere was more active. They also may be forming in Syria Planum today.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. (The original image scale is 25.6 centimeters [10.1 inches] per pixel [with 1 x 1 binning]; objects on the order of 77 centimeters [30.3 inches] across are resolved.) North is up.

The University of Arizona, in Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., in Boulder, Colorado. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.
日期
来源 https://photojournal.jpl.nasa.gov/jpeg/PIA23529.jpg
作者 NASA/JPL-Caltech/University of Arizona

许可协议

Public domain 本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zhNASA版权方针页面JPL图片使用方针。)
警告:

说明

添加一行文字以描述该文件所表现的内容
Mars - Dust Deposits - Syria Planum - August 1, 2019

此文件中描述的项目

描繪內容

image/jpeg

文件历史

点击某个日期/时间查看对应时刻的文件。

日期/时间缩⁠略⁠图大小用户备注
当前2019年10月24日 (四) 13:572019年10月24日 (四) 13:57版本的缩略图2,880 × 1,800(1.03 MB)DrbogdanUser created page with UploadWizard

以下页面使用本文件:

全域文件用途

以下其他wiki使用此文件: