The Evolution of the Indian Ocean since the Late Cretaceous

All available ship and aeroplane tracks across the Indian Ocean were searched for identifiable magnetic anomalies and transform faults, and hence the age and direction of motion at the time of formation of about two-thirds of the floor of the ocean established. The magnetic lineations show that Indi...

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Published in:Geophysical Journal International
Main Authors: McKenzie, Dan, Sclater, John G.
Format: Text
Language:English
Published: Oxford University Press 1971
Subjects:
Online Access:http://gji.oxfordjournals.org/cgi/content/short/24/5/437
https://doi.org/10.1111/j.1365-246X.1971.tb02190.x
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spelling fthighwire:oai:open-archive.highwire.org:gji:24/5/437 2023-05-15T13:56:55+02:00 The Evolution of the Indian Ocean since the Late Cretaceous McKenzie, Dan Sclater, John G. 1971-12-01 00:00:00.0 text/html http://gji.oxfordjournals.org/cgi/content/short/24/5/437 https://doi.org/10.1111/j.1365-246X.1971.tb02190.x en eng Oxford University Press http://gji.oxfordjournals.org/cgi/content/short/24/5/437 http://dx.doi.org/10.1111/j.1365-246X.1971.tb02190.x Copyright (C) 1971, Oxford University Press Articles TEXT 1971 fthighwire https://doi.org/10.1111/j.1365-246X.1971.tb02190.x 2012-11-23T22:14:16Z All available ship and aeroplane tracks across the Indian Ocean were searched for identifiable magnetic anomalies and transform faults, and hence the age and direction of motion at the time of formation of about two-thirds of the floor of the ocean established. The magnetic lineations show that India moved away from Antarctica at about 18 cm/y for 20 My in the Early Tertiary. This rapid motion ceased in the Eocene and was followed by a period in which little or no spreading took place west of the Ninety East Ridge. Australia separated from Antarctica during this period. The present spreading episode began about 36 My ago. This detailed study has permitted instantaneous poles of rotation to be obtained, and has established that Africa is now moving northward at 2cm/y relative to Antarctica in the South West Indian Ocean. The evolution of the triple junction between the South East, South West and Central Indian Ridges is clearly reflected in the topography and magnetic lineations. The depth of parts of the ocean formed since the Late Cretaceous increases with age in the manner expected from the temperature structure of a cooling plate, and supports the evolution determined from the magnetic lineations in a most remarkable way. Heat flow observations are more scattered but also consistent with the same thermal model. The proposed evolution agrees with the distribution of known continental fragments and with the Late Cretaceous palaeomagnetic poles from surrounding continents and one obtained from the shape of the magnetic lineations south of India. It is, however, not yet clear how to reconstruct Gondwanaland from the Late Cretaceous reconstructions. Text Antarc* Antarctica HighWire Press (Stanford University) East Ridge ENVELOPE(-136.671,-136.671,63.833,63.833) Indian Geophysical Journal International 24 5 437 528
institution Open Polar
collection HighWire Press (Stanford University)
op_collection_id fthighwire
language English
topic Articles
spellingShingle Articles
McKenzie, Dan
Sclater, John G.
The Evolution of the Indian Ocean since the Late Cretaceous
topic_facet Articles
description All available ship and aeroplane tracks across the Indian Ocean were searched for identifiable magnetic anomalies and transform faults, and hence the age and direction of motion at the time of formation of about two-thirds of the floor of the ocean established. The magnetic lineations show that India moved away from Antarctica at about 18 cm/y for 20 My in the Early Tertiary. This rapid motion ceased in the Eocene and was followed by a period in which little or no spreading took place west of the Ninety East Ridge. Australia separated from Antarctica during this period. The present spreading episode began about 36 My ago. This detailed study has permitted instantaneous poles of rotation to be obtained, and has established that Africa is now moving northward at 2cm/y relative to Antarctica in the South West Indian Ocean. The evolution of the triple junction between the South East, South West and Central Indian Ridges is clearly reflected in the topography and magnetic lineations. The depth of parts of the ocean formed since the Late Cretaceous increases with age in the manner expected from the temperature structure of a cooling plate, and supports the evolution determined from the magnetic lineations in a most remarkable way. Heat flow observations are more scattered but also consistent with the same thermal model. The proposed evolution agrees with the distribution of known continental fragments and with the Late Cretaceous palaeomagnetic poles from surrounding continents and one obtained from the shape of the magnetic lineations south of India. It is, however, not yet clear how to reconstruct Gondwanaland from the Late Cretaceous reconstructions.
format Text
author McKenzie, Dan
Sclater, John G.
author_facet McKenzie, Dan
Sclater, John G.
author_sort McKenzie, Dan
title The Evolution of the Indian Ocean since the Late Cretaceous
title_short The Evolution of the Indian Ocean since the Late Cretaceous
title_full The Evolution of the Indian Ocean since the Late Cretaceous
title_fullStr The Evolution of the Indian Ocean since the Late Cretaceous
title_full_unstemmed The Evolution of the Indian Ocean since the Late Cretaceous
title_sort evolution of the indian ocean since the late cretaceous
publisher Oxford University Press
publishDate 1971
url http://gji.oxfordjournals.org/cgi/content/short/24/5/437
https://doi.org/10.1111/j.1365-246X.1971.tb02190.x
long_lat ENVELOPE(-136.671,-136.671,63.833,63.833)
geographic East Ridge
Indian
geographic_facet East Ridge
Indian
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_relation http://gji.oxfordjournals.org/cgi/content/short/24/5/437
http://dx.doi.org/10.1111/j.1365-246X.1971.tb02190.x
op_rights Copyright (C) 1971, Oxford University Press
op_doi https://doi.org/10.1111/j.1365-246X.1971.tb02190.x
container_title Geophysical Journal International
container_volume 24
container_issue 5
container_start_page 437
op_container_end_page 528
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