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Washington, D.C. The imaging team consists of scientists from the US, England, France, and
Germany. The visual and infrared mapping spectrometer team is based at the University of Arizona. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.
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In this mosaic, Kraken Mare, which is Titan's largest sea and covers about the same area as Earth's
Caspian Sea and Lake Superior combined, can be seen spreading out with many tendrils on the upper right,. The big dark zone up and left of Kraken is Ligeia Mare, the second largest sea. Below Ligeia,
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This false-color mosaic, made from infrared data collected by NASA's
Cassini spacecraft, reveals the differences in the composition of surface materials around hydrocarbon lakes at Titan, Saturn's largest moon. Titan is the only other place in the solar system that we know has stable liquid on its
174:
Until now, the spectrometer has only been able to capture distant, oblique or partial views of this area until now. The Sept. 12, 2013 flyby provided better viewing geometry. And sunlight has begun to pierce the winter darkness that shrouded Titan's north pole at
Cassini's arrival in the Saturn
160:
The orange areas are thought to be evaporite -- the Titan equivalent of salt flats on Earth. The evaporated material is thought to be organic chemicals originally from Titan's haze particles that once dissolved in liquid methane. They appear orange in this image against the greenish backdrop of
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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 Cassini-Huygens mission for NASA\'s Science Mission Directorate,
156:
Scientists mapped near-infrared colors onto the visible color spectrum. Red in this image was assigned a wavelength of 5 microns (10 times longer than visible light), green 2.0 microns (four times longer than visible light), and blue 1.3 microns (2.6 times longer than visible light).
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shaped similar to a sports fan's foam finger that points just up from left, is Punga Mare, the third Titan Sea. Numerous other smaller lakes dot the area. Titan's north pole is located in the geographic location just above the end of the "finger" of Punga Mare.
154:
surface, though its lakes are made of liquid ethane and methane rather than liquid water. While there is one large lake and a few smaller ones near Titan's south pole, almost all of Titan's lakes appear near the moon's north pole.
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system nine years ago. A thick cap of haze that once hung over the north pole has also dissipated as northern summer approaches. And, thankfully, Titan's beautiful, almost cloudless, rain-free weather continued during this flyby.
181:
Views of this area by other
Cassini instruments include PIA17471, PIA17472, PIA17473 and PIA14584 from the imaging science subsystem; and PIA10008 and PIA17031 from the radar mapper. An earlier VIMS view can be seen at PIA16845.
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An annotated version of this image, with a high-resolution strip highlighted, is also available. In this version, the north pole is marked with a red cross and other smaller lakes are also labeled.
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The resolution varies across this composite view depending on when each cube of data was acquired, but the best surface sampling is 2 miles (3 kilometers) per pixel.
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The original NASA image has been cropped, and borders were added. Some of the features in this image have been annotated in
Wikimedia Commons.
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joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use.
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The data shown here were obtained by
Cassini's visual and infrared mapping spectrometer during a close flyby of Titan on Sept. 12, 2013.
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This file contains additional information, probably added from the digital camera or scanner used to create or digitize it.
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If the file has been modified from its original state, some details may not fully reflect the modified file.
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The following pages on the
English Knowledge (XXG) use this file (pages on other projects are not listed):
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states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."
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Click on a date/time to view the file as it appeared at that time.
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data may be copyrighted if they are not explicitly produced by the
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http://www.ciclops.org/view/7733/Titans-Northern-Lakes-Salt-Flats
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For more information about the
Cassini-Huygens mission, visit
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The NASA website hosts a large number of images from the
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Add a one-line explanation of what this file represents
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in the United States because it was solely created by
83:(2,120 × 1,600 pixels, file size: 1.02 MB, MIME type:
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Commons is a freely licensed media file repository.
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work of the federal government of the United States
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334:, insignia and emblems is restricted per U.S. law
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228:NASA / JPL-Caltech / Space Science Institute
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1111:The following other wikis use this file:
1362:xmp.did:08BDF193F43DE311AA40D10252EEB0F1
193:and the Cassini imaging team home page,
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143:PIA17470 Titan northern hemisphere.jpg
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862:Items portrayed in this file
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1155:Usage on id.wikipedia.org
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1135:Usage on bn.wikipedia.org
1115:Usage on ar.wikipedia.org
291:NASA copyright policy page
191:http://saturn.jpl.nasa.gov
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358:Hubble Space Telescope
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111:description page there
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384:SOHO (ESA & NASA)
353:in the public domain.
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347:Russian space agency
295:JPL Image Use Policy
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32:Global file usage
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1199:சோட்டோனெரா லாகசு
1096:Sionascaig Lacus
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1139:লাডোগা ল্যাকাস
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1119:سوتونيرا لاكوس
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1076:Lakes of Titan
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781:Mayda Insula
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1189:கட்ச் லாகுனா
1179:Hammar Lacus
1159:Ngami Lacuna
1149:دریاوار حمار
1129:ألبانو لاكوس
1124:بحيرات تيتان
1110:
1091:Ngami Lacuna
1081:Müggel Lacus
1071:Ladoga Lacus
1066:Kutch Lacuna
1061:Hammar Lacus
1056:Albano Lacus
990:
987:File history
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624:Ladoga Lacus
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597:Mackay Lacus
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491:Jingpo Lacus
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283:unless noted
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119:You can help
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1327:Image width
1318:Color space
1275:Orientation
1234:辛纳赛格湖 (土卫六)
1219:索托内拉湖 (土卫六)
1209:阿尔巴诺湖 (土卫六)
651:Neagh Lacus
571:Kivu Lacus
518:Ligeia Mare
464:Kraken Mare
426:Annotations
336:14 CFR 1221
141:Description
1224:拉多加湖 (土卫六)
1214:哈马尔湖 (土卫六)
1047:File usage
1004:Dimensions
545:Punga Mare
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85:image/jpeg
27:File usage
1229:慕格湖 (土卫六)
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1030:(1.02 MB)
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998:Date/Time
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428:InfoField
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323:Warnings:
236:Licensing
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1330:2,120 px
1262:Metadata
843:Captions
285:". (See
37:Metadata
1015:current
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867:depicts
847:English
330:Use of
133:Summary
81:
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1286:72 dpi
1278:Normal
410:. Its
343:Soviet
225:Author
215:Source
1254:土卫六湖泊
1249:纳库鲁干湖
1239:恩加米乾湖
362:STScI
253:false
250:false
1322:sRGB
1244:卡奇干湖
1007:User
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824:2120
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402:The
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205:Date
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293:or
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297:.)
289:,
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