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Bird's Eye View of the Land of Lakes
PIA 17473
Avg Rating: 8.40/10
Full Size 1401x1990:
JPEG 909 KB
PNG 787 KB
TIFF 1.4 MB
PIA 17473
Avg Rating: 9.73/10
Annotated Full Size 1401x1990:
JPEG 937 KB
PNG 801 KB
TIFF 1.4 MB
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The vast hydrocarbon seas and lakes (dark shapes) near the north pole of Saturn's moon Titan sprawl out beneath the watchful eye of NASA's Cassini spacecraft. Scientists are studying images like these for clues about how Titan's hydrocarbon lakes formed. Titan is the only world other than Earth that is known to have stable bodies of liquid on its surface.
This view was made from near-infrared images of Titan obtained by Cassini's imaging science subsystem. Bright material seems to surround the lakes, which could help explain why currently almost all large bodies of liquid are found here, at Titan's north pole, rather than other parts of Titan. The imaging data suggest the surface here is unique. Explanations range from the collapse of land after a volcanic eruption to karst terrain, where liquids dissolve soluble bedrock. Karst terrains on Earth can create spectacular topography such as the Carlsbad Caverns in New Mexico
The largest of the dark shapes, at the upper right, is Kraken Mare, Titan's largest sea and about the size of the Caspian Sea and Lake Superior put together. To its left lies Ligeia Mare (which is about 300 miles or 500 kilometers across), the second largest sea. Punga Mare (about 240 miles or 380 kilometers across) is below Ligeia Mare and just above its leftmost finger is the north pole.
Other shades of grey are surface features, primarily within the bright polar surface area identified in images taken during the two previous Titan flybys (PIA17471 and PIA17472).
An annotated version is available that also labels other nearby lakes.
The near-infrared images that make up this mosaic were obtained by Cassini's imaging science subsystem on Sept. 12, 2013. They were obtained in the near infrared band of light (938 nanometers), close to the visible range of light that human eyes can see. To human eyes, the lakes would still appear darker than the surrounding terrain. To maximize signal from Titan's surface through the hazy atmosphere, 10 image footprints (and four images per footprint) were combined. The terrain visible in this image is about 1,000 miles (2,000 kilometers) from top to bottom. Image scale is 1,760 feet (536 meters) per pixel.
Until now, Cassini's imaging science subsystem has only been able to capture distant, oblique or partial views of this area (e.g., PIA08930 and PIA12812). Three recent flybys provided better viewing geometry now that sunlight has pierced the winter darkness that shrouded Titan's north pole at Cassini's arrival in the Saturn 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 Cassini's flybys this past summer.
For comparison, Cassini's visual and infrared spectrometer also obtained data on the same area around the same time: PIA17470. Other imaging camera views can be seen at PIA17471 and PIA17472.
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, 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.
For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.
Credit: NASA/JPL-Caltech/SSI
Released: October 23, 2013 (PIA 17473)
Image/Caption Information |
Alliance Member Comments
i often miss things so the obvious impact craters elude me. i do see circular structures that i presume are chryo-volcanic in origin. to my eye, they appear to resemble doughnut shaped mounds. not a central peak, a central depression. i might be perceiving them in reverse, but i don't see how an impactor could get through that much atmosphere. even if i am seeing them wrong way out, they still don't look like typical impact craters to me. is there anything in the data set that confirms they are depressions or elevations?
Very Interesting.
What is obvious are the number of impact craters, at least three with central peaks.
This area looks more like the Jupiter moon Callisto, Saturn moon Rhea or Uranus moon Umbriel, with liquid hydrocarbons filling some of the colder hollows and craters. Will be interesting to see some more recent SAR imagery of this area.
Andrew R Brown.
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