As stated earlier in this Section, in 1985 the writer (NMS) initiated a research project while still at NASA's Goddard Space Flight Center, on which I continued to work until retiring from there in September, 1988. The supporting field effort was conducted while on sabbatical from Goddard between June and September of 1985. Although presented as a paper twice at professional meetings, this work remains unpublished because it is incomplete, with some open questions that would benefit from more research (unlikely, as funding is no longer accessible). However, the study did produce enough valid and meaningful results to justify putting forth the main data displays and analytical inferences as a model for the role of space imagery in a basic geoscience investigation.
The title of one of the presented papers, "Terranes as Terrains," aptly summarizes the essence of the study. Freely translated, this refers to an attempt to determine whether certain kinds of geo-structural units (terranes) have distinctive and diagnostic landscape features (terrains) that make them easy to identify and that help us understand their origin, significance, and history. Three goals prompted this investigation:
The study applies morphometry to conventional and digital topographic databases and, wherever useful, Landsat/SPOT imagery.
The word "terrane" originally referred to "a crustal block, usually bounded by faults, with a geologic history distinct from histories of juxtaposed blocks of differing characteristics." With the advent and acceptance of plate tectonic theory, users modified this concept with new insights into certain crustal blocks that they called "tectonostratigraphic", "accreted", or "suspect" terranes. In this view, they consider terranes to be diverse segments of crust that originated and developed often far from their present locations and over time traveled on a moving plate that converged with another plate, eventually colliding with a continental margin (along or within this second plate). There, they obducted (shoved onto) against the margin, rather than incompletely subducting (diving under) the second plate, thereby becoming accreted to that plate. A brief overview of terranes is given on this Wikipedia website.
To give a pictorial example: Here are two stages of the growth of the Himalayas. Individual land masses (these can be large, hundreds to thousands of kilometers on a side) riding on an oceanic plate that is subducting into southern Asia are in succession added to the Asian continent. Eventually in Cenozoic time the entire subcontinent of India will be welded against the Asian plate:
Thus, masses such as microcontinents embedded in oceanic crust moving to a subduction zone may be unable to follow that crust downward and will be "scraped off" along thrust faults to emplace along the growing edge of the continental crust on the other plate. Or, a variant: if an island arc complex (e.g., Java, page 17-2) on the upper plate, above a subduction zone gets squeezed between two converging plates as a continent on the lower plate eventually reached the zone, much of the arc would be caught "in the crunch" to be driven on and welded to (accreted) the encroaching continent. The usual criteria for terrane recognition come from stratigraphic, structural, and paleomagnetic discontinuities between adjacent terranes. (For a quick review of relevant concepts, read pages 507 and following, and other parts of Chapter 18 in the introductory text: Physical Geology by B.J. Skinner and S.C. Porter, 1994, J. Wiley & Sons, Inc.)
Whereas in the thinking about growth of continents prior to the accreted terrane concepts, scientists explained complex geo-crustal units in the continents as the consequence of fold-squeezing and fault transport during mountain building at geosynclinal sites, without much geographic displacement. Now, the new view recognizes distant site origins and relocations because of long movements on the "conveyor belts" of diverging plates. Continents thus grow by progressive accretion of numerous plates over time onto early cratonic nuclei. Since this concept first gained favor in the 1970s, geoscientists have recognized hundreds of terranes on all continents, in the sense that we re-interpreted older ideas about mapped geologic units to fit the terrane model. As an illustration of the terrane addition/continental growth version, consider this map that portrays a collage of the major terranes emplaced along the western margin of North America.
The Klamath Mountains of northwestern California-Southwestern Oregon were the type of locality for developing the concept of accreted terranes, because of the pioneering mapping and interpreting by Irwin, Blake, and others. Early, somewhat generalized, maps of the two adjacent areas display the first interpretations of these groups of terranes (the upper map that follows shows the terranes in northern California and part of the Oregon Klamaths, and the lower map continues coverage in Oregon to the north and west) :
Each of the named terranes is a unit which, after travelling some distance, "docked" against the paleo-North American continent, during some specific period. Most of the inner (continentward) units are progressively older than those outside, although thrust faulting can sometimes carry a younger unit over part of older ones. Each terrane maintains some internal structural integrity and consists of a series of stratigraphic units (formations), many not having counterparts in other nearby terranes. Those that do were likely deposited across boundaries after terrane emplacements.