LokiPatera/ˈloʊkiˈpætərə/ is the largest volcanic depression onJupiter's moonIo, 202 kilometres (126 mi) in diameter.[2] It contains an activelava lake, with an episodically overturning crust.[3] The level of activity seen is similar to a superfast spreadingmid-ocean ridge on Earth.[4] It is the largest volcano on Io, producing about 10% of Io’s total thermal emission.[5] Temperature measurements of thermal emission at Loki Patera taken byVoyager 1's Infrared Interferometer Spectrometer and Radiometer (IRIS) instrument were consistent with sulfur volcanism.[6]
Loki Patera is located at13°00′N308°48′W / 13°N 308.8°W /13; -308.8[7]. It is named after theNorse godLoki.[7]Amaterasu Patera is located to the north andManua Patera to the northwest.[citation needed]
Io's lava lakes such as Loki Patera are depressions partially filled with molten lava covered by a thin solidified crust. These lava lakes are directly connected to a magma reservoir below.[8] Observations of thermal emission at several of Io's lava lakes reveal glowing molten rock along Loki Patera's margin, caused by the lake's crust breaking up along the edge of the patera. Over time, because the solidified lava is denser than the still-molten magma below, this crust can founder, exposing fresh, hot molten rock.[9] At sites such as Loki Patera, this can occur episodically. During an overturning episode, Loki can emit up to ten times more heat than when its crust is stable.[3]
During an eruption, a wave of foundering crust has been observed to spread out across the patera at the rate of about 1 km (3,300 ft) per day, until the crust of the lake has been resurfaced. Another eruption then begins once the new crust has cooled and thickened enough for it to no longer be buoyant over the molten lava.[10]
On 8 March 2015 (10 years ago) (2015-03-08), a rare orbital alignment occurred between Io andEuropa, two of themoons of Jupiter, that allowed researchers to distinguish heat being emitted from Loki Patera. They were able to accomplish this because Europa's surface is coated in water ice which reflects small amounts of sunlight at infrared wavelengths. Scientists were able to determine that there were two waves of resurfacing lava, which explains the change in brightness on Loki Patera every 400–600 days. The images that helped researchers discover this were captured by theLarge Binocular Telescope Observatory in southeastArizona. The observation also revealed that there is a difference in themagma supply of the two halves of Loki.[11]
In December 2023 and February 2024, theJuno spacecraft completed extremely close flybys of Io, including the first closeup images of the northern latitudes, showing the islands within Loki Patera surrounded by a reflective glassy black surface.[12]
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