Eyre Lacuna (Titan)

Intermittent lake in Australia.

Eyre Lacuna is a feature on Saturn's largest moon, Titan, believed to be a currently dry bed of an intermittent hydrocarbon lake. When full, the lake would be composed of liquid methane and ethane. It was detected in 2007 by the Cassini–Huygens space probe. (wikipedia entry)

A lacuna is an irregularly shaped depression having the appearance of a dry lake bed. On Titan they are named after lakes on Earth, preferably with a shape similar to the lacus or lacuna on Titan.

Image Source. Marker locations are approximate and may not always appear to align with image on map.

NW 359 km

Rombaken Sinus

MRV
5 Hours 37 Minutes
Walking
7 Days 10 Hours

N 146 km

Patos Sinus(next)

MRV
2 Hours 17 Minutes
Walking
3 Days 1 Hour

NE 4044 km

Mývatn Lacus

MRV
2 Days 15 Hours
Walking
83 Days 21 Hours

W 771 km

Vid Flumina

MRV
12 Hours 2 Minutes
Walking
15 Days 23 Hours

Eyre Lacuna

72.6° N 134.9° E

E 630 km

Freeman Lacus

MRV
9 Hours 51 Minutes
Walking
13 Days 1 Hour

SW 236 km

Cayuga Lacus

MRV
3 Hours 41 Minutes
Walking
4 Days 21 Hours

S 114 km

Vänern Lacus(last)

MRV
1 Hour 47 Minutes
Walking
2 Days 9 Hours

SE 146 km

Ohrid Lacus

MRV
2 Hours 17 Minutes
Walking
3 Days

Tour so far: Visited 108 locations over 1,286 km. Next: Patos Sinus
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