File:057Tyrrhena Patera.png

原始文件 (3,947 × 2,964像素,文件大小:6.85 MB,MIME类型:image/png


摘要

描述
English: Tyrrhenus Mons lies on the northeast edge of the Hellas impact basin. It numbers among a handful of similar low volcanic structures (originally called paterae, after the Latin word for dish) in the cratered highlands next to Hellas. The others are Hadriaca (also on the northeast) and Amphitrites, Peneus, and Pityusa (all on the southwest of Hellas). Tyrrhenus and its neighbors also show a different volcanic style than later volcanos such as Olympus Mons and the others in Tharsis and Elysium. Tyrrhenus's low slopes, wide structure, and heavily scored flanks suggest that it is made of easily eroded materials. Scientists call such volcanic debris "pyroclastic," from the Greek meaning fire-broken. The image is a mosaic of infrared frames taken during daytime by the Thermal Emission Imaging System (THEMIS) on NASA's Mars Odyssey orbiter. Circling Mars every two hours, THEMIS scans the surface in five visible and 10 infrared bands. The smallest details it can record at infrared wavelengths are 100 meters (330 feet) wide; at visible wavelengths, THEMIS has imaged selected regions at 18-meter (59 feet) resolution.

Location: 21.4°S, 106.6°E
Instrument: IR
Image Size: 395 x 296 km, 245 x 184 mi, 3947 x 2964 pixels

Resolution: 100m (330 ft)
日期 在2011年之前
date QS:P,+2011-00-00T00:00:00Z/7,P1326,+2011-00-00T00:00:00Z/9
-05-18
来源 http://themis.asu.edu/node/5427
作者 NASA / JPL-Caltech / Arizona State University

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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。)
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