Mount Hampton

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Template:Short description Template:Infobox mountain

Mount HamptonTemplate:Efn is a shield volcano with a circular ice-filled caldera. It is a twin volcano with Whitney Peak to the northwest and has erupted phonolite rocks. It is the northernmost of the volcanoes which comprise the Executive Committee Range in Marie Byrd Land, Antarctica and was active during the Miocene.

Geography and geology

File:HamptonMap.jpg
Topographic map of Mount Hampton (1:250,000 scale) from USGS Mount Hampton

Mount Hampton is the northernmost volcano of the Executive Committee Range in Marie Byrd Land, Antarctica. It has the form of a symmetrical uneroded shield volcano[1] with an "impressive" appearance and an ice-filled[2] Script error: No such module "convert". wide caldera.[3] Like other volcanoes in the Executive Committee Range, it is a paired volcano[4] with the northwesterly Script error: No such module "convert". high Whitney Peak and the southeasterly Script error: No such module "convert". high Marks Peak, which is the main summit of Mount Hampton.[5]Template:Efn The northwesterly summit is associated with its own caldera, which is partly cut by the Mount Hampton caldera on the southeastern flank and buried by the lava flows from the latter.[6] The centres of the two calderas are about Script error: No such module "convert". apart.[7] Based on outcrops, it appears that most of the volcano is formed by flow rocks[8] but cinder and lava bombs occur at parasitic vents.[9]

The mountain rises about Script error: No such module "convert". above the surface of the West Antarctic Ice Sheet[10] which buries most of the edifice, and moraine ridges are found at its base on the ice sheet.[11] Owing to climate conditions, the persistence of permanent ice atop of the mountain is unlikely over the long term;[12] erosion there appears to have been episodic[13] with maxima during interglacials[14] and there is no evidence of cirque formation.[15] Lichens have been found on the mountain.[16]

Composition

The volcano is formed by phonolite rocks, but parasitic vents have also erupted basanite[17] and Whitney Peak also erupted trachyte and benmoreite.[18] Hawaiite has been reported as well.[19] The volcanic rocks contain augite and feldspar; further, spinel-containing lherzolite xenoliths have been found.[20] In general, composition is unique for each volcano in the Executive Committee Range.[21]

Eruption history

Mount Hampton is one of the oldest volcanoes of Antarctica and was active during the Miocene.[22] Despite this, it is less eroded than some younger volcanoes in the region;[23] in general, the ages of the Marie Byrd Land volcanoes are not correlated to their erosion status.[24] It appears that Whitney Peak is the older half of the edifice and that volcanic activity then migrated to Mount Hampton.[25] More generally, volcanism in the Executive Committee Range migrated southwards over time at an average rate of Script error: No such module "convert"., although Mount Hampton and its southern neighbour Mount Cumming were simultaneously active 10 million years ago.[26]

Last parasitic eruptions took place around 11.4 million years ago[27] and the youngest radiometric dates are 8.3 million years.[28] As at other volcanoes of Marie Byrd Land, the parasitic activity at Mount Hampton occurred after a long period of dormancy.[29] However, the presence around the caldera rim of snow-covered[30] inactive Script error: No such module "convert". high ice towersTemplate:Efn indicate that the mountain is geothermally active[31] and may have erupted during the Holocene.[32] Later research suggested that the ice towers were actually formed by wind-driven erosion of snow and ice. There is no evidence of geothermal processes[33] and seismic activity recorded at the volcano may be due to volcano-tectonic processes or due to ice movement.[34]

See also

Notes

Template:Notelist

Sources

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  1. Carracedo et al. 2019, p.439
  2. GNIS
  3. Wilch, McIntosh and Panter 2021, p.546
  4. LeMasurier and Rex, 1989, p.7225
  5. LeMasurier and Thompson, 1990, p.194
  6. LeMasurier and Thompson, 1990, p.189
  7. Rocchi, LeMasurier and Vincenzo 2006, p.1001
  8. Rocchi, LeMasurier and Vincenzo 2006, p.997
  9. LeMasurier and Thompson, 1990, p.190
  10. Carracedo et al. 2019, p.439
  11. LeMasurier and Thompson, 1990, p.190
  12. Carracedo et al. 2019, p.442
  13. Carracedo et al. 2019, p.444
  14. Carracedo et al. 2016
  15. Lemasurier and Rocchi 2005, p.57
  16. Scharon and Early, p.91
  17. Carracedo et al. 2019, p.439
  18. LeMasurier and Rex, 1989, p.7228
  19. Panter et al. 2021, p.580
  20. Carracedo et al. 2019, p.439
  21. LeMasurier and Rex, 1989, p.7229
  22. Carracedo et al. 2019, p.439
  23. Rocchi, LeMasurier and Vincenzo 2006, p.997
  24. LeMasurier and Thompson, 1990, p.158
  25. LeMasurier and Thompson, 1990, p.189
  26. LeMasurier and Rex, 1989, p.7227
  27. Carracedo et al. 2019, p.439
  28. Carracedo et al. 2019, p.442
  29. LeMasurier and Thompson, 1990, p.197
  30. LeMasurier p.91
  31. LeMasurier and Wade, 1968
  32. LeMasurier and Thompson, 1990, p.193
  33. Wilch, McIntosh and Panter 2021, p.547
  34. Lough et al. 2012

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