Lord Howe seamount chain

The Lord Howe seamount chain is the seamount chain that includes Lord Howe Island. [1] It is one of the two parallel seamount chains alongside the east coast of Australia; the Lord Howe and Tasmantid seamount chains both run north-south through parts of the Coral sea and Tasman sea.[1] These chains have longitudes of approximately 159°E and 156°E respectively.[1]

The Lord Howe seamount chain is on the western slope of Lord Howe Rise, a deep-sea elevated plateau which is a submerged part of Zealandia.[1] The Tasmantid and Lord Howe seamount chains are both broadly within the Tasman basin (the abyssal plain between Lord Howe Rise and the Australian continental shelf), and lie on opposite sides of Dampier Ridge (a submerged continental fragment).[1][2]

The Lord Howe seamount chain extends from the Chesterfield group (20°S) to Flinder's seamount (34.7°S).[3] It includes Nova bank, Argo and Kelso seamounts, Capel and Gifford guyots, Middleton and Elizabeth reefs, Lord Howe Island and Balls Pyramid.[1]

The Lord Howe and Tasmantid chains each resulted from the Indo-Australian Plate moving northward over a stationary hotspot; the hotspot for the Lord Howe chain is expected to presently be beneath Flinder's seamount.[4] On the Australian mainland, a third north-south sequence of extinct volcanoes (which includes the Glasshouse mountains) is likely to have the same origin.[4]

The chain formed during the Miocene. It features many coral-capped guyots.

References

  1. 1 2 3 4 5 6 Willem J. M. van der Linden, Morphology of the Tasman sea floor. New Zealand Journal of Geology and Geophysics. Vol.13 (1970) 282-291.
  2. ↑ McDougall et al, Dampier Ridge, Tasman Sea, as a stranded continental fragment. Australian Journal of Earth Sciences 41 (1994). 395-406.
  3. ↑ Przeslawski et al. Biogeography of the Lord Howe Rise region, Tasman Sea. Deep-Sea Research Part II 58 (2011) 959–969.
  4. 1 2 W. J. Morgan and J. P. Morgan. Plate velocities in hotspot reference frame: electronic supplement.


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