Vine–Matthews–Morley hypothesis

The Vine–Matthews–Morley hypothesis, also known as the Morley–Vine–Matthews hypothesis, was the first key scientific test of the seafloor spreading theory of continental drift and plate tectonics. Its key impact was that it allowed the rates of plate motions at mid-ocean ridges to be computed. It states that the Earth's oceanic crust acts as a recorder of reversals in the geomagnetic field direction as seafloor spreading takes place.


Harry Hess proposed the seafloor spreading hypothesis in 1960 (published in 1962 [1]); the term "spreading of the seafloor" was introduced by geophysicist Robert S. Dietz in 1961.[2] According to Hess, seafloor was created at mid-oceanic ridges by the convection of the earth's mantle, pushing and spreading the older crust away from the ridge.[3] Geophysicist Frederick John Vine and the Canadian geologist Lawrence W. Morley independently realized that if Hess's seafloor spreading theory was correct, then the rocks surrounding the mid-oceanic ridges should show symmetric patterns of magnetization reversals using newly collected magnetic surveys.[4] Both of Morley's letters to Nature (February 1963) and Journal of Geophysical Research (April 1963) were rejected, hence Vine and his PhD adviser at Cambridge University, Drummond Hoyle Matthews, were first to publish the theory in September 1963.[5][6] Some colleagues were skeptical of the hypothesis because of the numerous assumptions made—seafloor spreading, geomagnetic reversals, and remanent magnetism—all hypotheses that were still not widely accepted.[7] The Vine–Matthews–Morley hypothesis describes the magnetic reversals of oceanic crust. Further evidence for this hypothesis came from Cox and colleagues (1964) when they measured the remanent magnetization of lavas from land sites.[8][9] Walter C. Pitman and J.R. Heirtzler offered further evidence with a remarkably symmetric magnetic anomaly profile from the Pacific-Antarctic Ridge.[10]

Marine magnetic anomalies

The Vine–Matthews-Morley hypothesis correlates the symmetric magnetic patterns seen on the seafloor with geomagnetic field reversals. At mid-ocean ridges, new crust is created by the injection, extrusion, and solidification of magma. After the magma has cooled through the Curie point, ferromagnetism becomes possible and the magnetization direction of magnetic minerals in the newly formed crust orients parallel to the current background geomagnetic field vector. Once fully cooled, these directions are locked into the crust and it becomes permanently magnetized.[9] Lithospheric creation at the ridge is considered continuous and symmetrical as the new crust intrudes into the diverging plate boundary. The old crust moves laterally and equally on either side of the ridge. Therefore, as geomagnetic reversals occur, the crust on either side of the ridge will contain a record of remanent normal (parallel) or reversed (antiparallel) magnetizations in comparison to the current geomagnetic field. A magnetometer towed above (near bottom, sea surface, or airborne) the seafloor will record positive (high) or negative (low) magnetic anomalies when over crust magnetized in the normal or reversed direction. The ridge crest is analogous to “twin-headed tape recorder”, recording the Earth's magnetic history.[11]

Typically there are positive magnetic anomalies over normally magnetized crust and negative anomalies over reversed crust.[9] Local anomalies with a short wavelength also exist, but are considered to be correlated with bathymetry.[6] Magnetic anomalies over mid-ocean ridges are most apparent at high magnetic latitudes, over north-south trending ridges at all latitudes away from the magnetic equator, and east-west trending spreading ridges at the magnetic equator.[6]

The intensity of the remanent magnetization in the crust is greater than the induced magnetization. Consequently, the shape and amplitude of the magnetic anomaly is controlled predominately by the primary remanent vector in the crust. In addition, where the anomaly is measured on Earth affects its shape when measured with a magnetometer. This is because the field vector generated by the magnetized crust and the direction of the Earth's magnetic field vector are both measured by the magnetometers used in marine surveys. Because the Earth's field vector is much stronger than the anomaly field, a modern magnetometer measures the sum of the Earth's field and the component of the anomaly field in the direction of the Earth's field.

Sections of crust magnetized at high latitudes have magnetic vectors that dip steeply downward in a normal geomagnetic field. However, close to the magnetic south pole, magnetic vectors are inclined steeply upwards in a normal geomagnetic field. Therefore, in both these cases the anomalies are positive. At the equator the Earth's field vector is horizontal so that crust magnetized there will also align horizontal. Here, the orientation of the spreading ridge affects the anomaly shape and amplitude. The component of the vector that effects the anomaly is at a maximum when the ridge is aligned east-west and the magnetic profile crossing is north-south.[9]


The hypothesis links seafloor spreading and geomagnetic reversals in a powerful manner, with each expanding knowledge of the other. Early in the history of investigating the hypothesis only a short record of geomagnetic field reversals was available for studies of rocks on land.[8] This was sufficient to allow computing of spreading rates over the last 700,000 years on many mid-ocean ridges by locating the closest reversed crust boundary to the crest of a mid-ocean ridge.[11] Marine magnetic anomalies were found later to span the vast flanks of the ridges.[9] Drillcores into the crust on these ridge flanks allowed dating of the early and of the older anomalies. This in turn allowed design of a predicted geomagnetic time scale.[9] With time, investigations married land and marine data to produce an accurate geomagnetic reversal time scale for almost 200 million years.[12]

See also


  1. Hess, H. H. (November 1, 1962). "History of Ocean Basins". In A. E. J. Engel; Harold L. James; B. F. Leonard (eds.). Petrologic Studies: A volume in honor of A. F. Buddington. Boulder, CO: Geological Society of America. pp. 599–620. OCLC 499940734.CS1 maint: uses editors parameter (link)
  2. Dietz, Robert S. (1961). "Continent and Ocean Basin Evolution by Spreading of the Sea Floor". Nature. 190 (4779): 854–857. Bibcode:1961Natur.190..854D. doi:10.1038/190854a0.
  3. Iseda, Tetsuji. "Philosophical interpretations of the plate tectonics revolution". Retrieved 27 February 2011.
  4. Morley, L.W. and Larochelle, A., 1964. Paleomagnetism as a means of dating geological events. Geochronology in Canada, 8, pp.39-51. page 50.
  5. "Frederick Vine and Drummond Matthews, pioneers of plate tectonics". The Geological Society. Retrieved 19 Mar 2014.
  6. Vine, F. J; Matthews, D. H. (1963). "Magnetic Anomalies Over Oceanic Ridges". Nature. 199 (4897): 947–949. Bibcode:1963Natur.199..947V. doi:10.1038/199947a0.
  7. Frankel, Henry (1982). "The development, reception, and acceptance of the Vine-Matthews-Morley hypothesis". Historical Studies in the Physical Sciences. Baltimore, Maryland. 13 (1): 1–39. doi:10.2307/27757504. JSTOR 27757504.
  8. Cox, Allan; Doell, Richard R.; Dalrymple, G. Brent (1964). "Reversals of the Earth's magnetic field". Science. 144 (3626): 1537–1543. ISSN 0036-8075.
  9. Kearey, Philip; Klepeis, Keith A.; Vine, Frederick J. (2009). Global tectonics (3rd ed.). Chichester: Wiley-Blackwell. ISBN 9781444303223.
  10. Pitman, W. C.; Heirtzler, J. R. (1966-12-02). "Magnetic anomalies over the Pacific-Antarctic ridge". Science. 154 (3753): 1164–1171. doi:10.1126/science.154.3753.1164. ISSN 0036-8075.
  11. Vine, F.J. (1966). "Spreading of the ocean floor: new evidence". Science. 154 (3755): 1405–1415. Bibcode:1966Sci...154.1405V. doi:10.1126/science.154.3755.1405. PMID 17821553.
  12. Ogg, J. G. (2012). "Geomagnetic polarity time scale". In Gradstein, F. M.; Ogg, J. G.; Schmitz, Mark; Ogg, Gabi (eds.). The geologic time scale 2012. Volume 2 (1st ed.). Elsevier. pp. 85–114. ISBN 9780444594259.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.