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File:PIA10008 Seas and Lakes on Titan.jpg

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摘要

描述

This Cassini false-color mosaic shows all synthetic-aperture radar images to date of Titan's north polar region. Approximately 60 percent of Titan's north polar region, above 60 degrees north latitude, is now mapped with radar. About 14 percent of the mapped region is covered by what is interpreted as liquid hydrocarbon lakes.

Features thought to be liquid are shown in blue and black, and the areas likely to be solid surface are tinted brown. The terrain in the upper left of this mosaic is imaged at lower resolution than the remainder of the image

Most of the many lakes and seas seen so far are contained in this image, including the largest known body of liquid on Titan. These seas are most likely filled with liquid ethane, methane and dissolved nitrogen.

Many bays, islands and presumed tributary networks are associated with the seas. The large feature in the upper right center of this image is at least 100,000 square kilometers (40,000 square miles) in area, greater in extent than Lake Superior (82,000 square kilometers or 32,000 square miles), one of Earth's largest lakes. This Titan feature covers a greater fraction of the surface, at least 0.12 percent, than the Black Sea, Earth's largest terrestrial inland sea, at 0.085 percent. Larger seas may exist, as it is probable that some of these bodies are connected, either in areas unmapped by radar or under the surface (see PIA08365).

Of the 400 observed lakes and seas, 70 percent of their area is taken up by large "seas" greater than 26,000 square kilometers (10,000 square miles).

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the United States and several European countries.

For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov/home/index.cfm.

The original NASA image has been modified by rotating 90 degrees clockwise, cropping and reduction in size (the linear pixel density was reduced 50%).

Some of the features in this image have been annotated in Wikimedia Commons.
日期
來源 http://photojournal.jpl.nasa.gov/catalog/?IDNumber=PIA10008
作者 NASA / JPL-Caltech / USGS
其他版本

PIA10008 Seas and Lakes on Titan full size.jpg - larger, higher resolution version (4696 × 4696 pixels, 10.4 MB)

PIA17655 crop Titan north polar seas and lakes.jpg - slightly lower resolution version with most complete coverage (3000 × 3000 pixels, 3.68 MB)
本圖像或影音收錄於美國國家航空暨太空總署 (NASA)噴射推進實驗室(Jet Propulsion Laboratory),其照片編號為: PIA10008

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Methane lakes in Titan

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日期/時間縮⁠圖尺寸用戶備⁠註
目前2013年11月12日 (二) 03:01於 2013年11月12日 (二) 03:01 版本的縮圖2,348 × 1,900(2.62 MB)WolfmanSFSlightly wider view on top and right
2012年4月8日 (日) 09:44於 2012年4月8日 (日) 09:44 版本的縮圖2,280 × 1,840(2.1 MB)WolfmanSFTweak cropping; add 40 pixels at upper margin to fully display several lakes
2007年12月16日 (日) 00:18於 2007年12月16日 (日) 00:18 版本的縮圖2,280 × 1,800(2.05 MB)WolfmanSF{{Information |Description=This Cassini false-color mosaic shows all synthetic-aperture radar images to date of Titan's north polar region. Approximately 60 percent of Titan's north polar region, above 60 degrees north latitude, is now mapped with radar.

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