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Lithospheric necking - A dynamic model for rift morphologyRifting is examined as the growth of a necking instability. A rift is nucleated by means of a small thickness perturbation imposed at the base of a strong layer which overlies a weaker substrate. The conditions for which the initial disturbance will amplify as the lithosphere extends are evaluated for a range of rheological parameters, and the associated pattern of near-surface deformation is determined. It was found that this unstable lithospheric extension results in a pattern of deformation that is consistent with the major morphological characteristics of rift zones. For an initial perturbation narrower than the dominant wavelength, deformation concentrates in a zone of width comparable to the dominant wavelength; for an initial thickness perturbation wider than the dominant wavelength, deformation develops periodically at the dominant wavelength in the region above the perturbation. It is noted that the width of a rift is essentially independent of the layer/substrate strength ratio. For a power law viscous surface layer (n = 3), the dominant wavelength varies with the layer/substrate strength ratio to the one-third power and is always larger than for a plastic surface layer of the same thickness. The unstable extension of a strong viscous surface layer may be responsible for the great width of rift zones on Venus.
Document ID
19860053225
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Zuber, M. T.
(NASA Goddard Space Flight Center Greenbelt, MD; Brown University, Providence, RI, United States)
Parmentier, E. M.
(Brown University Providence, RI, United States)
Date Acquired
August 12, 2013
Publication Date
April 1, 1986
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 77
Issue: 3-4
ISSN: 0012-821X
Subject Category
Geophysics
Accession Number
86A37963
Funding Number(s)
CONTRACT_GRANT: NSG-7605
Distribution Limits
Public
Copyright
Other

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