Mount Petras
| Mount Petras | |
|---|---|
.jpg) Map of Mount Petras | |
| Highest point | |
| Coordinates | 75°51′S 128°38′W / 75.850°S 128.633°W[1] |
| Naming | |
| Etymology | Named for Theodore Argyres Petras |
| Geography | |
  Mount Petras | |
Mount Petras is a mountain in Antarctica. It consists of volcanic rocks, most of Cretaceous age but there is also an Eocene-Oligocene volcanic system that may have been emplaced inside of thin ice. It is part of the Marie Byrd Land Volcanic Province and is its oldest volcano.
Geography and geology
Mount Petras lies in the coastal region of Marie Byrd Land, Antarctica,[1] and is located within the McCuddin Mountains together with Mount Flint[2] which lies northwest of Mount Petras.[3] The complex Mount Petras-Mount Flint-Reynolds Ridge is also known as Petras Range.[4] It lies 200–250 kilometres (120–160 mi) inland from the Amundsen Sea coast.[5]
It is an angular mountain[5] consisting of rocky spurs in an area of 5 by 8 kilometres (3.1 mi × 5.0 mi),[6] which form two ridges form a semicircular ice-filled bowl.[7] Two other summits are 2,325 metres (7,628 ft) high Putzke Peak northeast of Mount Petras, 2,716 metres (8,911 ft) high Schwob Peak south and 2,440 metres (8,010 ft) high Peter Nunatak southeast. Other outcrops occur farther southwest at Navarrette Peak, southeast at Wallace Rock[8] and northeast at Erven Nunataks.[9] The existence of an explosion crater on its northern side was inferred by González-Ferran in 1972.[10]
Both basement and volcanic rocks emerge from the West Antarctic Ice Sheet as a nunatak. The volcanic and basement rocks are separated by an unconformity at 2,700 metres (8,900 ft) elevation.[1] The highest summit of Mount Petras lies on the western ridge[7] at 2,867 metres (9,406 ft) elevation above sea level of which about 900 metres (3,000 ft) are above the West Antarctic Ice Sheet.[11] Most of the volcanic rocks are hawaiite with some mugearite,[12] while the basement is rhyodacitic[11] and mostly consists of a Cretaceous volcanic complex that makes up the bulk of Mount Petras.[5] The basement also includes schists,[13] paragneisses[14] and gneisses.[15] The mugearite occurs in the form of a lava flow, while the hawaiites form volcaniclastic deposits as tuff breccias[16] and lapilli tuffs.[17] Moraine debris and talus cover exposed rocks.[7]
Mount Petras is part of the volcanic province of Marie Byrd Land, which may be a product of a mantle plume. Other volcanoes in this province of West Antarctic volcanoes are the Ames Range, Crary Mountains, Executive Committee Range, Flood Range, Hobbs Coast nunataks, Kohler Range, Mount Murphy, Mount Siple, Mount Takahe and Mount Waesche. Some of these volcanoes are still active today.[11] Marie Byrd Land itself is a crustal dome, with its "summit" in the area of Mount Petras; the dome was probably formed by the impingement of the mantle plume under the crust[18] and volcanism may have spread outwards away from Mount Petras.[3]
Geologic history
Argon-argon dating has yielded ages of 36 and 29-27 million years for the volcanic rocks, making them the oldest in Marie Byrd Land.[19] The volcano probably formed at the surface, perhaps in contact with an early Oligocene ice sheet[1] or more likely mountain glaciers,[20] as the rocks display evidence that the volcanic eruptions took place in shallow water, most likely meltwater.[21] The basement rocks have yielded Cretaceous ages[11] and contain zircons of Devonian-Carboniferous age,[14] with some rocks reaching ages of 1364 million years.[22]
Name and research history
The volcanic history of Mount Petras is important for reconstructing the volcanic and glacial history of Marie Byrd Land.[1] During the late Cretaceous and Eocene-late Cenozoic, continental rifting occurred in the Ross Sea and West Antarctic Ice Sheet area. Beginning with the Oligocene, an ice sheet began to develop in Antarctica and acquired present-day dimensions during the Miocene or Pliocene.[11]
Mount Petras was discovered during the 1939-1941 United States Antarctic Service Expedition and named after the pilot of the expedition.[5] It was visited in 1959, 1967–1968, 1977-1978 and 1993-1994 by field expeditions.[23] During the 20th century, Mount Petras was viewed as a volcano that had formed deep under ice on a Cenozoic marine erosion surface covering West Antarctica, which had then been deformed by tectonic uplift.[1]
References
- ^ a b c d e f Wilch & McIntosh 2000, p. 477.
- ^ Wilch, McIntosh & Panter 2021, p. 519.
- ^ a b LeMasurier 1990, p. 163.
- ^ González-Ferrán & González-Bonorino 1972, p. 265.
- ^ a b c d LeMasurier 1990, p. 239.
- ^ Wilch, McIntosh & Panter 2021, p. 551.
- ^ a b c Doumani, George A.; Ehlers, Ernest G. (1 July 1962). "Petrography of Rocks from Mountains in Marie Byrd Land, West Antarctica". GSA Bulletin. 73 (7): 881. doi:10.1130/0016-7606(1962)73[877:PORFMI]2.0.CO;2. ISSN 0016-7606.
- ^ LeMasurier, McIntosh & Rex 1981, p. 20.
- ^ González-Ferrán & González-Bonorino 1972, p. 267.
- ^ González-Ferrán & González-Bonorino 1972, p. 266.
- ^ a b c d e Wilch & McIntosh 2000, p. 478.
- ^ Wilch & McIntosh 2000, p. 479.
- ^ Pankhurst 1998, p. 2537.
- ^ a b Nelson, D. A.; Cottle, J. M. (1 November 2018). "The secular development of accretionary orogens: linking the Gondwana magmatic arc record of West Antarctica, Australia and South America". Gondwana Research. 63: 9. doi:10.1016/j.gr.2018.06.002. ISSN 1342-937X.
- ^ LeMasurier, McIntosh & Rex 1981, p. 19.
- ^ Wilch & McIntosh 2000, p. 482.
- ^ Wilch & McIntosh 2000, p. 484.
- ^ Mukasa, Samuel B.; Dalziel, Ian W. D. (1 April 2000). "Marie Byrd Land, West Antarctica: Evolution of Gondwana's Pacific margin constrained by zircon U-Pb geochronology and feldspar common-Pb isotopic compositions". GSA Bulletin. 112 (4): 612. doi:10.1130/0016-7606(2000)112<611:MBLWAE>2.0.CO;2. ISSN 0016-7606.
- ^ Wilch & McIntosh 2000, p. 481.
- ^ Francis, J. E.; Marenssi, S.; Levy, R.; Hambrey, M.; Thorn, V. C.; Mohr, B.; Brinkhuis, H.; Warnaar, J.; Zachos, J.; Bohaty, S.; DeConto, R. (1 January 2008). "Chapter 8 From Greenhouse to Icehouse – The Eocene/Oligocene in Antarctica". Developments in Earth and Environmental Sciences. 8. Elsevier: 314.
- ^ Wilch & McIntosh 2000, p. 489.
- ^ Pankhurst 1998, p. 2544.
- ^ Wilch, McIntosh & Panter 2021, p. 520.
- Sources
- González-Ferrán, Oscar; González-Bonorino, Felix (1972). "The volcanic ranges of Marie Byrd Land between long. 100 and 140 W.". Antarctic Geology and Geophysics. Vol. 261. Oslo: Universitetsforlaget.
- LeMasurier, W. E.; McIntosh, W. C.; Rex, D. C. (1981). "Mid-Tertiary glacial history recorded at Mount Petras, Marie Byrd Land". Antarctic Journal of the United States. 21: 19–21.
- LeMasurier, W. E. (1990). "B. Marie Byrd Land". Volcanoes of the Antarctic Plate and Southern Oceans. Antarctic Research Series. Vol. 48. pp. 146–255. doi:10.1029/AR048. ISBN 0-87590-172-7.
- Pankhurst, R. J. (1998). "Geochronology and geochemistry of pre‐Jurassic superterranes in Marie Byrd Land, Antarctica". Journal of Geophysical Research: Solid Earth. 103 (B2): 2529–2547. doi:10.1029/97JB02605.
- Wilch, T. I.; McIntosh, W. C. (December 2000). "Eocene and Oligocene volcanism at Mount Petras, Marie Byrd Land: implications for middle Cenozoic ice sheet reconstructions in West Antarctica". Antarctic Science. 12 (4): 477–491. doi:10.1017/S0954102000000560. ISSN 1365-2079. S2CID 129298738.
- Wilch, T. I.; McIntosh, W. C.; Panter, K. S. (1 January 2021). "Chapter 5.4a Marie Byrd Land and Ellsworth Land: volcanology". Geological Society, London, Memoirs. 55 (1): 515–576. doi:10.1144/M55-2019-39. ISSN 0435-4052.