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Loki Patera

Coordinates: 13°00′N 308°48′W / 13°N 308.8°W / 13; -308.8[7]
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Voyager 1 observation of Loki Patera and nearby lava flows and volcanic pits.
Loki Patera on moon Io
(artist's concept; 0:18).[1]
Map of temperature and crust age of Loki Patera obtained by the Large Binocular Telescope.

Loki Patera /ˈloʊki ˈpætərə/ is the largest volcanic depression on Jupiter's moon Io, 202 kilometres (126 mi) in diameter.[2] It contains an active lava lake, with an episodically overturning crust.[3] The level of activity seen is similar to a superfast spreading mid-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 by Voyager 1's Infrared Interferometer Spectrometer and Radiometer (IRIS) instrument were consistent with sulfur volcanism.[6]

Loki Patera is located at 13°00′N 308°48′W / 13°N 308.8°W / 13; -308.8[7]. It is named after the Norse god Loki.[7] Amaterasu Patera is located to the north and Manua Patera to the northwest.[citation needed]

Geology

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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 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]

History

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On 8 March 2015 (9 years ago) (2015-03-08), a rare orbital alignment occurred between Io and Europa, two of the moons 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 the Large Binocular Telescope Observatory in southeast Arizona. The observation also revealed that there is a difference in the magma supply of the two halves of Loki.[11]

In December 2023 and February 2024, the Juno 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]

See also

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Wikimedia Commons has media related to Loki Patera.

References

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  1. ^ "Looking Into Io's Loki Patera (Artist's Concept)". NASA/JPL. 2024-04-18. Retrieved 2024-04-25.
  2. ^ Radebaugh, J.; et al. (2001). "Paterae on Io: A new type of volcanic caldera?". J. Geophys. Res. 106 (E12): 33005–33020. Bibcode:2001JGR...10633005R. doi:10.1029/2000JE001406.
  3. ^ a b Howell, R. R.; R. M. C. Lopes (2007). "The nature of the volcanic activity at Loki: Insights from Galileo NIMS and PPR data". Icarus. 186 (2): 448–461. Bibcode:2007Icar..186..448H. doi:10.1016/j.icarus.2006.09.022.
  4. ^ "iavcei2004". Archived from the original on 9 October 2007. Retrieved 2 September 2024.
  5. ^ Lopes, Rosaly; de Kleer, Katherine; Keane, James Tuttle (2023). Io: A New View of Jupiter’s Moon (2nd ed.). Springer Nature. p. 192. ISBN 978-3-031-25669-1.
  6. ^ Hanel, R.; et al. (1979). "Infrared Observations of the Jovian System from Voyager 1". Science. 204 (4396): 972–76. doi:10.1126/science.204.4396.972-a. PMID 17800431. S2CID 43050333.
  7. ^ a b "Loki Patera". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  8. ^ Davies, A. (2007). "Effusive activity: landforms and thermal emission evolution". Volcanism on Io: A Comparison with Earth. Cambridge University Press. pp. 142–52. ISBN 978-0-521-85003-2.
  9. ^ Matson, D. L.; et al. (2006). "Io: Loki Patera as a magma sea". J. Geophys. Res. 111 (E9): E09002. Bibcode:2006JGRE..111.9002M. doi:10.1029/2006JE002703.
  10. ^ Rathbun, J. A.; J. R. Spencer (2006). "Loki, Io: New ground-based observations and a model describing the change from periodic overturn". Geophysical Research Letters. 33 (17): L17201. arXiv:astro-ph/0605240. Bibcode:2006GeoRL..3317201R. doi:10.1029/2006GL026844. S2CID 29626659.
  11. ^ University of California, Berkeley (2017-05-10). "Waves of lava seen in Jupiter's moon Io's largest volcanic crater". Retrieved 2017-10-11.
  12. ^ "NASA's Juno Gives Aerial Views of Mountain, Lava Lake on Io - NASA". 2024-04-18. Retrieved 2024-04-27.

Bibliography

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