The seamount appears to be part of a long geological lineament with the neighbouring Henderson and Ducie islands, as well as the southern Tuamotus and Line Islands. Such a lineament may have been generated by a hotspot; the nearby Easter hotspot is a candidate hotspot.
There is a topographic swell that connects the two islands and continues eastward towards Sala y Gomez. The origin of this swell and the various volcanoes and seamounts associated with it has been variously explained as either being due to a mantle plume which forms volcanoes that are then carried away through plate motion or by a "hot line" where a number of simultaneously active volcanic centres develop.[4] This geological lineament may extend all the way to Tonga.[6]
Crough seamount was probably formed by the Easter hotspot that also generated Easter Island[7] albeit with the participation of a nearby fracture zone[8] that modified the trend of the hotspot path.[9] In this case the Easter Island-Sala y Gomez ridge and the Crough Seamount would be conjugate volcanic ridges paired across the East Pacific Rise.[10] although it is possible that two separate hotspots were active on the eastern and western side of the East Pacific Rise.[11][12] Another theory postulates that Crough was formed by its own hotspot, the Crough hotspot.[13]
Together with Ducie and Henderson Crough forms a 1,300 kilometres (810 mi) long westward trending lineament[14] with each volcano becoming older the farther west it lies,[15] and which may be a prolongation of the southern Tuamotus[16] which were generated by the same hotspot.[10] Even farther west the hotspot track may include Oeno, Minerve Reef, Marutea, Acton, Rangiroa, the Line Islands and the Mid-Pacific Mountains, although a continuation through the Line Islands is problematic if it is assumed that the Easter hotspot generated this track.[13][17] A different theory has Crough seamount as its own hotspot, that formed the seamounts and islands together with another hotspot ("Larson"),[18] and lesser contributions of the Society and Marquesas hotspot.[19] East of Crough, a series of even younger volcanic ridges continues until the East Pacific Rise[20] where the hotspot may be located.[13] The Crough hotspot may be a conjugate of the Easter hotspot,[21] and sourced from the middle mantle.[18]
Crough is an east-west trending seamount[5] which rises over 2 kilometres (1.2 mi) from the seafloor to a depth of less than 722 metres (2,369 ft)[22] at 650 metres (2,130 ft).[23] It has a flat top and the presence of coral sands indicates that Crough once emerged above sea level before subsiding to its present depth,[22] having formerly hosted corals[24] and pteropods. Wave erosion that took place when Crough emerged above sea level truncated the seamount, turning it into a flat guyot.[25]Pillow lavas crop out between 1,400–950 metres (4,590–3,120 ft).[26] Crough Seamount has a volume of 660 cubic kilometres (160 cu mi), comparable to that of other submarine volcanoes such as Macdonald seamount, Mehetia and Moua Pihaa.[23]
A second seamount lies nearby and partly overlaps with Crough,[1] it is named Thomas Seamount[27] in honour of a geophysicist.[28] This seamount is even shallower than Crough as it reaches a depth of 600 metres (2,000 ft) but has a smaller volume of 600 cubic kilometres (140 cu mi).[23]
Argon-argon dating has yielded ages of 8.4 to 7.6 million years ago for samples dredged from Crough,[31] while other geological indicators suggest an age of between 7 and 10 million years ago.[32] Other estimates of its age are 4[15]-3 million years.[33]
In 1955, a strong earthquake was recorded on the northern flank of Crough Seamount;[34] the characteristics of the earthquake resemble these of volcanic processes and it is thus possible that Crough Seamount is still active. Such activity may constitute a post-shield stage of volcanism.[33] The earthquake has also been interpreted as a normal fault earthquake[2] which sometimes occur in young oceanic crust, but the 1955 Crough event was considerably stronger than other earthquakes of this type.[35]
^Irving, Robert.; Dawson, Terence P. (2012). The marine environment of the Pitcairn Islands. Dundee: The Pew Environment Group. ISBN9781845861612. OCLC896746178.
^ abStoffers, P.; Glasby, G. P.; Stuben, D.; Renner, R. M.; Pierre, T. G.; Webb, J.; Cardile, C. M. (1993). "Comparative mineralogy and geochemistry of hydrothermal iron-rich crusts from the Pitcairn, Teahitia-mehetia, and Macdonald hot spot areas of the S. W. Pacific". Marine Georesources & Geotechnology. 11 (1): 47. doi:10.1080/10641199309379905.
Binard, N.; Stoffers, P.; Hékinian, R.; Searle, R.C. (October 1996). "Intraplate en echelon volcanic ridges in the South Pacific west of the Easter microplate". Tectonophysics. 263 (1–4): 23–37. doi:10.1016/S0040-1951(96)00036-4. ISSN0040-1951.
Hekinian, Roger; Stoffers, Peter; Akermand, Dietrich; Binard, Nicolas; Francheteau, Jean; Devey, Colin; Garbe-Schönberg, Dieter (August 1995). "Magmatic evolution of the Easter microplate-Crough Seamount region (South East Pacific)". Marine Geophysical Researches. 17 (4): 375–397. doi:10.1007/bf01227041. ISSN0025-3235. S2CID129757272.
Okal, Emile A.; Cazenave, Anny (January 1985). "A model for the plate tectonic evolution of the east-central Pacific based on SEASAT investigations". Earth and Planetary Science Letters. 72 (1): 99–116. doi:10.1016/0012-821X(85)90120-7. ISSN0012-821X.
Searle, R.C.; Francheteau, J.; Cornaglia, B. (April 1995). "New observations on mid-plate volcanism and the tectonic history of the Pacific plate, Tahiti to Easter microplate". Earth and Planetary Science Letters. 131 (3–4): 395–421. doi:10.1016/0012-821X(95)00018-8. ISSN0012-821X.
Spencer, T. (1989). "Tectonic and environmental histories in the Pitcairn Group, Palaeogene to present: reconstructions and speculations". Atoll Research Bulletin. 322: 1–22. doi:10.5479/si.00775630.322.1. hdl:10088/5906.
Talandier, Jacques; Okal, Emile A. (1987). "Seismic detection of underwater volcanism: The example of French Polynesia". Pure and Applied Geophysics. 125 (6): 919–950. doi:10.1007/bf00879361. ISSN0033-4553. S2CID128415828.