{{Short description|Lake on Titan}} {{Infobox feature on celestial object |name = Eyre Lacuna |image = PIA17655 crop Titan north polar seas and lakes.jpg |caption = [[Synthetic aperture radar]] mosaic of Titan's north polar region, showing hydrocarbon seas and lakes |type = Lacus |coordinates = {{coord|72.6|N|225.1|W|globe:titan_type:landmark|display=inline,title}} |diameter = 25.4 km <ref name = "USGS">{{cite web | title = Eyre Lacuna | work = planetarynames.wr.usgs.gov| publisher = [[United States Geological Survey|USGS]] | url = https://planetarynames.wr.usgs.gov/Feature/14786| access-date = 2013-12-28}}</ref> It is named after [[Lake Eyre]], an [[intermittent lake]] in [[Australia]].<ref name = "USGS"/> |eponym = [[Lake Abaya]] }}
'''Eyre Lacuna''' is a feature on Saturn's largest moon, [[Titan (moon)|Titan]], believed to be a currently dry bed of an intermittent [[Lakes of Titan|hydrocarbon lake]].
When full, the lake would be composed of [[liquid]] [[methane]] and [[ethane]].<ref name="Coustenis2008">{{cite book|last1=Coustenis | first1 = A. | last2 = Taylor |first2 = F. W.|title=Titan: Exploring an Earthlike World|url=https://books.google.com/books?id=j3O47dxrDAQC&pg=PA154|date=21 July 2008|publisher=[[World Scientific]]|pages= 154–155|isbn= 978-981-281-161-5}}</ref> It was detected in 2007 by the ''[[Cassini–Huygens]]'' [[space craft|space probe]].
==References== {{reflist}}
{{Titan}}
[[Category:Lakes of Titan (moon)]]
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