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Kraken Mare

Coordinates: 68°N 310°W / 68°N 310°W / 68; -310
From Wikipedia, the free encyclopedia

Kraken Mare
False-color mosaic of synthetic aperture radar images showing all of Kraken Mare. The large island Mayda Insula is left of top center, and Jingpo Lacus is at upper left. A portion of Ligeia Mare enters the view at top right.
Feature typeMare
Coordinates68°N 310°W / 68°N 310°W / 68; -310
Diameter1,170 km[note 1]
EponymKraken

Kraken Mare /ˈkrɑːkən ˈmɑːreɪ/ is the largest known hydrocarbon sea on the surface of Saturn's moon Titan. It was discovered by the space probe Cassini in 2006, and was named in 2008 after the Kraken, a legendary sea monster.[1] It covers an area slightly bigger than the Caspian Sea on Earth, making it the largest known lake in the Solar System.

Description

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At 500,000 km2,[2] Kraken Mare is thought to be the largest body of liquid on Titan. It lies in the moon's northern polar region and is thought to be larger than the Caspian Sea on Earth.[1][3] Its status as a sea of hydrocarbons (mainly liquid methane) was identified by radar imagery. Analyses of the Cassini radar altimeter data used as a sounder have shown that the main body of Kraken Mare is at least 100 metres (330 ft) deep and likely deeper than 300 metres (980 ft).[4] One of its northernmost bays (Moray Sinus) has a depth of 85 metres (279 ft) at its center and shows an attenuation of the signal in the liquid that is compatible with a composition of 70% methane, 16% nitrogen and 14% ethane (assuming ideal mixing).[4] Shallow capillary waves 1.5 centimetres (0.59 in) high moving at 0.7 metres per second (2.3 ft/s; 1.6 mph; 2.5 km/h) have been detected on the surface of Kraken Mare.[5]

An island in the sea is named Mayda Insula. Kraken Mare may be hydrologically connected to the second-largest sea on Titan, Ligeia Mare.[6] This connection has been suggested for the difference in sea composition, as certain compounds flow into Kraken Mare from Ligeia Mare. In addition, Kraken Mare has a lower methane concentration than Ligeia Mare.[7]

The narrow constriction in the sea at 317°W, 67°N, about 17 kilometres (11 mi) wide and similar in size to the Strait of Gibraltar, officially named Seldon Fretum,[8] has been termed the 'Throat of Kraken' and suggested to be a location of significant currents.[9] Titan's orbital eccentricity may lead to tides of 1 metre (3.3 ft) in Kraken Mare, generating currents here of 0.5 metres per second (1.6 ft/s; 1.1 mph; 1.8 km/h) and possibly whirlpools.[6] Other calculations estimate tides as high as 5 metres (16 ft).[2]

Changing features known as "Magic Islands" are observed in Kraken Mare. These features, which are further indications of an active hydrocarbon cycle on Titan, are possibly rising bubbles due to nitrogen exsolution.[10][11]

Observation and exploration

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Kraken Mare, along with other Lakes of Titan, was first discovered by the Cassini–Huygens space probe on July 22, 2006. This was accomplished by noticing that certain dark regions, especially near the poles, had low radar reflectivity, as well as similar morphological features to that of terrestrial lakes.[12] Many observations since have confirmed these findings.[13][2][14] In addition to the radar images, the Cassini instrument VIMS (Visible and Infrared Mapping Spectrometer) has surveyed Kraken Mare and its surroundings.[13]

There have been multiple proposals and ideas to explore the depths of Kraken Mare via probes and submarines. One such submarine has gone through a phase one NASA study, complete with submarine design and schematics.[15] Another proposal, the Titan Mare Explorer was a finalist to explore another lake Ligeia Mare, with Kraken Mare as a secondary target, but InSight, a Mars lander, was ultimately approved instead.[16] The Titan Mare Explorer was also suggested for inclusion on the unprogressed Titan Saturn System Mission.

While a mission to Titan has been approved, the drone Dragonfly, there are no current missions to explore Kraken Mare or other lakes on Titan.[17]

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  • Synthetic aperture radar image (top) overlaid onto a visible light/infrared image of Titan's north polar region, showing the full extent of Kraken Mare.
    Synthetic aperture radar image (top) overlaid onto a visible light/infrared image of Titan's north polar region, showing the full extent of Kraken Mare.
  • Radar image showing the northern portion of Kraken Mare, including the large island Mayda Insula.
    Radar image showing the northern portion of Kraken Mare, including the large island Mayda Insula.
  • Radar image of a portion of Kraken Mare with a rugged coastline and numerous islands.
    Radar image of a portion of Kraken Mare with a rugged coastline and numerous islands.
  • Specular reflection off Jingpo Lacus in the Kraken Mare region, observed by Cassini on July 8, 2009.
    Specular reflection off Jingpo Lacus in the Kraken Mare region, observed by Cassini on July 8, 2009.

See also

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Notes

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  1. ^ The USGS web site gives the size as a "diameter", but it is actually the length in the longest dimension.

References

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  1. ^ a b "Kraken Mare". Gazetteer of Planetary Nomenclature. USGS Astrogeology Science Center. Archived from the original on August 8, 2018. Retrieved March 16, 2012.
  2. ^ a b c Hayes, Alexander G. (June 29, 2016). "The Lakes and Seas of Titan". Annual Review of Earth and Planetary Sciences. 44 (1): 57–83. Bibcode:2016AREPS..44...57H. doi:10.1146/annurev-earth-060115-012247. ISSN 0084-6597. Archived from the original on January 20, 2021. Retrieved September 14, 2020.
  3. ^ "Kraken Mare: The Largest Methane Sea Known To Humankind". WorldAtlas. April 25, 2017. Retrieved October 13, 2023.
  4. ^ a b Poggiali, V.; Hayes, A. G.; Mastrogiuseppe, M.; Le Gall, A.; Lalich, D.; Gomez-Leal, I.; Lunine, Jonathan I. (2020). "The bathymetry of Moray Sinus at Titan's Kraken Mare". Journal of Geophysical Research: Planets. 125 (12). Bibcode:2020JGRE..12506558P. doi:10.1029/2020JE006558.
  5. ^ Hand, Eric (December 16, 2014). "Spacecraft spots probable waves on Titan's seas". Science. Archived from the original on January 4, 2015. Retrieved January 14, 2015.
  6. ^ a b Lorenz, R. D. (2014). The Throat of Kraken : Tidal Dissipation and Mixing Timescales in Titan's Largest Sea (PDF). 45th Lunar and Planetary Science Conference (2014). The Woodlands, Texas. p. 1476. Archived (PDF) from the original on March 4, 2016. Retrieved June 9, 2014.
  7. ^ Lorenz, Ralph D. (2014). "The flushing of Ligeia: Composition variations across Titan's seas in a simple hydrological model". Geophysical Research Letters. 41 (16): 5764–5770. Bibcode:2014GeoRL..41.5764L. doi:10.1002/2014GL061133. ISSN 1944-8007. S2CID 129370565. Archived from the original on January 25, 2022. Retrieved April 1, 2021.
  8. ^ "Seldon Fretum". USGS planetary nomenclature page. USGS. Archived from the original on April 27, 2015. Retrieved May 23, 2015.
  9. ^ Rincon, P. (March 18, 2014). "'Waves' detected on Titan moon's lakes". BBC web site. BBC. Archived from the original on May 31, 2014. Retrieved June 9, 2014.
  10. ^ Farnsworth, Kendra K.; Chevrier, Vincent F.; Steckloff, Jordan K.; Laxton, Dustin; Singh, Sandeep; Soto, Alejandro; Soderblom, Jason M. (2019). "Nitrogen Exsolution and Bubble Formation in Titan's Lakes". Geophysical Research Letters. 46 (23): 13658–13667. Bibcode:2019GeoRL..4613658F. doi:10.1029/2019GL084792. ISSN 1944-8007. S2CID 213542086. Archived from the original on August 3, 2020. Retrieved April 1, 2021.
  11. ^ Hofgartner, J. D.; Hayes, A. G.; Lunine, Jonathan I.; Zebker, H.; Stiles, B. W.; Sotin, C.; Barnes, J. W.; Turtle, E. P.; Baines, K. H.; Brown, R. H.; Buratti, B. J. (2014). "Transient features in a Titan sea". Nature Geoscience. 7 (7): 493–496. Bibcode:2014NatGe...7..493H. doi:10.1038/ngeo2190. ISSN 1752-0908. Archived from the original on March 10, 2021. Retrieved April 1, 2021.
  12. ^ Stofan, E. R.; Elachi, C.; Lunine, Jonathan I.; Lorenz, R. D.; Stiles, B.; Mitchell, K. L.; Ostro, S.; Soderblom, L.; Wood, C.; Zebker, H.; Wall, S. (2007). "The lakes of Titan". Nature. 445 (7123): 61–64. Bibcode:2007Natur.445...61S. doi:10.1038/nature05438. ISSN 1476-4687. PMID 17203056. S2CID 4370622. Archived from the original on March 9, 2021. Retrieved April 1, 2021.
  13. ^ a b Stephan, Katrin; Jaumann, Ralf; Brown, Robert H.; Soderblom, Jason M.; Soderblom, Laurence A.; Barnes, Jason W.; Sotin, Christophe; Griffith, Caitlin A.; Kirk, Randolph L.; Baines, Kevin H.; Buratti, Bonnie J. (2010). "Specular reflection on Titan: Liquids in Kraken Mare". Geophysical Research Letters. 37 (7): n/a. Bibcode:2010GeoRL..37.7104S. doi:10.1029/2009GL042312. ISSN 1944-8007.
  14. ^ Hayes, A.; Aharonson, O.; Callahan, P.; Elachi, C.; Gim, Y.; Kirk, R.; Lewis, K.; Lopes, R.; Lorenz, R.; Lunine, Jonathan I.; Mitchell, K. (2008). "Hydrocarbon lakes on Titan: Distribution and interaction with a porous regolith". Geophysical Research Letters. 35 (9). Bibcode:2008GeoRL..35.9204H. doi:10.1029/2008GL033409. ISSN 1944-8007.
  15. ^ Hartwig, J. W.; Colozza, A.; Lorenz, R. D.; Oleson, S.; Landis, G.; Schmitz, P.; Paul, M.; Walsh, J. (March 1, 2016). "Exploring the depths of Kraken Mare – Power, thermal analysis, and ballast control for the Saturn Titan submarine". Cryogenics. 2015 Space Cryogenics Workshop, June 24–26, 2015, Phoenix, AZ Hosted by NASA Glenn Research Center, Cleveland, OH, USA. 74: 31–46. Bibcode:2016Cryo...74...31H. doi:10.1016/j.cryogenics.2015.09.009. ISSN 0011-2275. Archived from the original on May 29, 2017. Retrieved April 1, 2021.
  16. ^ Stofan, E.; Lorenz, R.; Lunine, Jonathan I.; Bierhaus, E. B.; Clark, B.; Mahaffy, P. R.; Ravine, M. (2013). "TiME - the Titan Mare Explorer". 2013 IEEE Aerospace Conference. p. 211. Bibcode:2013aero.confE.211S. doi:10.1109/AERO.2013.6497165. ISBN 978-1-4673-1813-6. S2CID 17290531. Archived from the original on January 21, 2022. Retrieved April 1, 2021.
  17. ^ "NASA selects Titan drone for next New Frontiers mission". SpaceNews. June 28, 2019. Archived from the original on January 25, 2022. Retrieved April 1, 2021.
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