Ontario Lacus
| Ontario Lacus | |
|---|---|
 RADAR-image of Ontario Lacus taken by Cassini on January 12, 2010. | |
| Feature type | Lacus |
| Coordinates | 72°S 183°W / 72°S 183°WCoordinates: 72°S 183°W / 72°S 183°W |
| Diameter | 235 km[note 1] |
| Eponym | Lake Ontario |
Ontario Lacus is a lake composed of methane, ethane and propane near the south pole of Saturn's moon Titan. Its character as a hydrocarbon lake was confirmed[1] by observations from the Cassini spacecraft, published in the 31 July 2008 edition of Nature. Ontario Lacus has a surface area of about 15,000 square kilometers (5,800 sq mi), about 20% smaller than its terrestrial namesake, Lake Ontario in North America. In April 2012, it was announced that it may be more like a mudflat or salt pan.[2]
Shorelines
On January 12, 2010, Cassini took a more detailed radar-image of Ontario Lacus showing numerous remarkable features. The northern shoreline features low hills, probably about 1 kilometer (3,000 feet) in altitude, and flooded river valleys. A smooth, wave-sculpted shoreline, like that seen on the southeastern side of Lake Michigan, can be seen at the northeastern part of the lake. Smooth lines parallel to the current shoreline could be formed by low waves over time, which were likely driven by winds sweeping in from the west or southwest. The southeast shore features a round-headed bay intruding into the shore.
The middle part of the western shoreline shows the first well-developed river delta observed on Titan, showing that liquid hydrocarbons flowing down from a higher plain have switched channels on their way into the lake, forming at least two lobes. Examples of this kind of channel switching and wave-modified deltas can be found on Earth at the southern end of Lake Albert between Uganda and the Democratic Republic of Congo in Africa and in the remains of an ancient lake known as Megachad in the African country Chad.[3]
Shore recession
Infrared observations indicate that the southwestern shoreline of the lake receded 9–11 km over a four-year period (2005-2009), evidently due to evaporation during the dry southern hemisphere fall.[4] Over the same interval, no change was observed in the southern or southeastern shorelines, indicative of steeper slopes in those regions. The sizes of northern hemisphere lakes and maria, in contrast, have been much more stable.[4]
Depth
By terrestrial standards, the lake appears to be extremely shallow. Radar measurements made in July 2009 and January 2010 indicate an average depth of 0.4 – 3.2 m, and a maximum depth of 2.9 – 7.4 m.[5] This gives the lake an estimated volume of 7 to 50 km3, less than one thirtieth the volume of Earth's Lake Ontario. The notoriously shallow Lake Okeechobee in Florida has a similar depth.
Waves
Any waves present on the lake are also far smaller than those that would be present on a sizable body of liquid water on Earth; their estimated maximum height was less than 3 mm during observations of a radar specular reflection during Cassini's T49 flyover of July 2009.[6] On Titan, waves can be generated at lower wind speeds than on Earth, due to the four times greater atmospheric density, and should be seven times higher at a given wind speed, due to Titan's surface gravity being one seventh as strong.[6] The lack of waves could indicate either wind speed less than 0.5 m/s, or an unexpectedly viscous composition of the hydrocarbon fluid.[5][6] However, the apparent presence of a wave-generated beach on the lake's northeast shore suggests that at times considerably higher waves form.[6]
Notes
- ↑ The USGS web site gives the size as a "diameter", but it is actually the length in the longest dimension.
References
- ↑ "NASA Confirms Liquid Lake On Saturn Moon". NASA. 2007-07-30. Retrieved 2007-07-30.
- ↑ Cassini Finds Titan Lake is Like a Namibia Mudflat - NASA
- ↑ http://photojournal.jpl.nasa.gov/catalog/PIA13172
- ↑ 4.0 4.1 Turtle, E. P.; Perry, J. E.; Hayes, A. G.; McEwen, A. S. (2011-02-15). "Shoreline retreat at Titan’s Ontario Lacus and Arrakis Planitia from Cassini Imaging Science Subsystem observations". Icarus 212 (2): 957–959. Bibcode:2011Icar..212..957T. doi:10.1016/j.icarus.2011.02.005. Retrieved 2012-03-25.
- ↑ 5.0 5.1 Wall, Mike (2010-12-17). "Saturn Moon's 'Lake Ontario': Shallow and Virtually Wave-free". Space.Com web site. Retrieved 2010-12-19.
- ↑ 6.0 6.1 6.2 6.3 Wye, Lauren; Zebker, Howard (2009-12-02). "Titan's Ontario Lacus: Smoothness Constraints from Cassini RADAR (video)" (slide set). SETI Institute Colloquium Series. Cosmo Learning. Retrieved 2010-12-21.
External links
- NASA/JPL videos describing recent discoveries about Ontario Lacus
- Staff (2008-08-03). "Titan's Ethane Lake". Astrobiology Magazine. Retrieved 2008-08-05.
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