Titan M30590 TITANLUX Synthetic Paint, 375 ml, Colour: Vermillion

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In March 2009, structures resembling lava flows were announced in a region of Titan called Hotei Arcus, which appears to fluctuate in brightness over several months. Though many phenomena were suggested to explain this fluctuation, the lava flows were found to rise 200 meters (660ft) above Titan's surface, consistent with it having erupted from beneath the surface. [132] Titanian". Oxford English Dictionary (Onlineed.). Oxford University Press. (Subscription or participating institution membership required.)a b c Stofan, E. R.; Elachi, C.; Lunine, Jonathan I.; Lorenz, R. D.; Stiles, B.; Mitchell, K. L.; Ostro, S.; Soderblom, L.; etal. (2007). "The lakes of Titan". Nature. 445 (1): 61–64. Bibcode: 2007Natur.445...61S. doi: 10.1038/nature05438. PMID 17203056. S2CID 4370622.

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AVIATR: An Airplane Mission for Titan". Universetoday.com. January 2, 2012. Archived from the original on March 28, 2013 . Retrieved February 26, 2013. On April 3, 2013, NASA reported that complex organic chemicals could arise on Titan based on studies simulating the atmosphere of Titan. [59] Strobel, Darrell F. (2010). "Molecular hydrogen in Titan's atmosphere: Implications of the measured tropospheric and thermospheric mole fractions" (PDF). Icarus. 208 (2): 878–886. Bibcode: 2010Icar..208..878S. doi: 10.1016/j.icarus.2010.03.003. Archived from the original (PDF) on August 24, 2012.

Cassini Sees the Two Faces of Titan's Dunes". JPL, NASA. Archived from the original on May 2, 2013. Wye, L. C.; Zebker, H. A.; Lorenz, R. D. (2009). "Smoothness of Titan's Ontario Lacus: Constraints from Cassini RADAR specular reflection data". Geophysical Research Letters. 36 (16): L16201. Bibcode: 2009GeoRL..3616201W. doi: 10.1029/2009GL039588. Earth could seed Titan with life". BBC News. March 18, 2006. Archived from the original on October 31, 2012 . Retrieved March 10, 2007.