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       #Post#: 84--------------------------------------------------
       NCGT SEA LEVELS
       By: Admin Date: January 29, 2017, 8:31 pm
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       New Concepts in Global Tectonics Journal, V. 4, No. 4, December
       2016. www.ncgt.org
       A History of the Earth’s Seawater:
       Transgressions and Regressions
       Karsten M. Storetvedt
       Institute of Geophysics, University of Bergen, Bergen, Norway
       karsten.storetvedt@uib.no
       Problem outline
       o a large extent, the history of the Earth’s dynamo-tectonic
       development is related to the origin of the oceanic water masses
       and their surface oscillations – characterized by the advances
       and retreats of epicontinental oceans. During major parts of
       post-Precambrian time, the present land surface was extensively
       covered by shallow seas, while today the continents are dryer
       than at any time during the last 570 million years
       (Phanerozoic). During the late Mesozoic, the continental
       flooding was nearly as widespread as that of the Lower-Middle
       Palaeozoic, though the highest sea-level may not have been
       higher than 200-400 metres above the present shore line (cf.
       Miller et al., 2005). “Today, a similar rise would inundate less
       than half the area that was flooded in the Cretaceous, because
       our continents stand high above the sea, whereas the Mesozoic
       lands were low and flat” (van Andel, 1985). The same low and
       flat continents were apparently the norm during the Palaeozoic
       as well as in Precambrian time; the elevation of our continents
       and continental mountain chains, as well as the mid-ocean
       ridges, seems to have a quite recent origin – having basically
       occurred during the last 5 million years of Earth history (cf.
       Storetvedt, 2015 for references and a compilation of evidence).
       ...
       It is natural to think that seawater is intimately associated
       with the Earth’s internal chemical reconstitution and degassing,
       but when did the bulk of surface water accumulate? During
       Precambrian times, there is no factual evidence for the
       existence of deep sea basins, and the volume of surface water
       was apparently modest – but there is ample evidence of
       deposition in shallow marine waters within greenstone belts
       (Figure 1) along with indications of fluvial activity (cf.
       Windley, 1977). Perhaps an appropriate description of the
       surface conditions in the late Precambrian can be unveiled by
       the Grand Canyon sedimentary system – as described by Dunbar
       (1949, p. 93-94):
       “The Grand Canyon system is essentially unmetamorphosed, thus
       contrasting in the most striking manner with the underlying
       schists, which must be vastly older. The system begins with a
       basal conglomerate resting on a peneplaned surface of the Vishnu
       schists. Following this come limestone and then limy shale and
       sandy shale and quartzites. The limestones, and probably a
       larger part of the shales and quartzites, were deposited in
       shallow marine water, but parts of the sandy shale and sandstone
       are bright red and are so commonly mud **** as to suggest
       deposition on a broad floodplain. The region was probably part
       of a great delta plain in which submarine and subaerial
       deposition alternated. And since these strata were formed near
       sea-level, the region obviously subsided slowly [...] while
       deposition was in progress.”
       The Archaean aeon, which was characterized by features such as
       the relative abundance of komatiite extrusions and a relative
       scarcity of redbeds and carbonates, was succeeded by the much
       more diversified geological record of the Proterozoic –
       progressively distinguished by large sedimentary basins with
       primitive living forms more abundantly recorded in surface
       carbonates. Contrasting strongly with the Proterozoic situation,
       the Cambrian experienced a general “transgression onto cratons,
       with a classic orthoquartzite-to-shale sequence resting
       unconformably on Precambrian and overlain by carbonates” (Hallam
       1992). And suddenly, a diversity of complex life forms,
       dominated by trilobites and brachiopods, appear in abundance at
       the base of the Cambrian; this remarkable biological explosion
       was probably a direct consequence of the rapidly increasing
       volume of surface water. Thus began a major Lower-Middle
       Palaeozoic submergence of the apparently flat and low-lying
       continental masses that was accompanied by a rapid development
       of sea-living creatures. According to Dunbar (1949, p. 155),
       “the Early Cambrian oceans seem to have been somewhat openly
       connected, so that intermigration was easy and the leading types
       of life are much alike in various parts of the world”. Thus, the
       Cambrian eustatic transgression probably represents the first
       major supply of water to the Earth’s surface – degassed from the
       interior of the Earth; the explosive prevalence of marine fauna
       at that time is likely to have been a consequence.
       Figure 1. Depiction of a transect across a block of late
       Archaean greenstone belts – subsiding rift basins developing
       along one of the pre-existing orthogonal fracture systems, with
       associated volcanism and shallow water sedimentation. Diagram is
       based on Cloos (1939).
       For post-Precambrian time – ranging from 570 My to the Present,
       the stratigraphic record is generally well exposed due to the
       fact that epicontinental seas repeatedly covered substantial
       parts of the present land surface.
       ...
       It can be envisaged that continuous planetary degassing and
       related reorganization of the Earth’s interior mass has modified
       both the internal and the outer regions of the Earth
       progressively since early Archaean time – transforming an
       initially thick proto-crust as well as progressively, and
       episodically, increasing the volume of surface water (cf.
       Storetvedt, 2003 and 2011). The gradual accumulation of fluids
       and gases in the upper mantle and lower crust must have led to a
       considerable increase in the confining pressure at these levels.
       At each depth level, rocks and fluids would naturally be subject
       to a common pressure – producing a kind of high pressure vessel
       situation – with fractures being kept open just like those in
       near-surface rocks at low pressures (Gold’s pore theory, see
       Hoyle, 1955; Gold, 1999). This principle is well demonstrated in
       the Kola and KTB (S. Germany) deep continental boreholes (which
       reached maximum depths of 12 and 9 km, respectively) where open
       fractures filled with hydrous fluids were found throughout the
       entire sections drilled (e.g., Möller et al., 1997; Smithson et
       al., 2000); brines were seen to coexist with crustal rocks and,
       in the KTB site, the salinity of the formation water turned out
       to be about twice that of present-day normal sea water (Möller
       et al., 2005). In both drill sites, a variety of dissolved gases
       and fluids was found; primitive helium was observed at different
       depth levels indicating that the fluids were of deep interior
       origin (Smithson et al., 2000). As there is no observational
       evidence that deep oceanic depressions existed prior to the
       middle-late Mesozoic (see below), the bulk of present-day
       surface water must, in fact, have been exhaled from the deep
       interior during later stages of the Earth’s history.
       Nevertheless, there are reasons for believing that most of the
       planet’s water is still residing in the deep interior.
       ...
       It has been demonstrated that natural occurrences of the
       granulite-to-eclogite transition are strongly impeded when
       hydrous fluids are absent (e.g., Austrheim, 1987 and 1990;
       Walther, 1994; Leech, 2001; Austrheim et al., 1997). Thus,
       Austrheim (1998) argues that hydrous fluids are much more
       important than either temperature or pressure, and Leech (2001)
       concluded that gravity-driven sub-crustal delamination (through
       eclogite formation) is strongly controlled by the availability
       of water. According to Austrheim et al. (1997), the
       eclogitization process brings about material weakening which
       make eclogites deform more easily than their protoliths – the
       degree of deformability being further increased in the presence
       of water. Thus, the large density increase consequent upon
       eclogitization destabilizes the lower crust and makes it detach
       from the relatively unaffected crust above (Leech, 2001). Figure
       4 gives an illustration of this sub-crustal thinning process –
       advancing upward and eventually forming deep sea basins.
       ...
       As a consequence of the Earth’s degassing and associated
       internal mass reorganization, changes of its moment of inertia
       would be a natural consequence – producing secular changes of
       the globe’s rate of rotation as well as episodic, but generally
       progressive, changes of its spatial orientation (true polar
       wander). A method for studying the Earth’s spin rate (length of
       day, L.O.D.) for the geological past was introduced by Wells
       (1963 and 1970): by counting presumed growth increments in
       recent and fossil corals, he estimated the number of days per
       year back to the Lower Palaeozoic. A famous result from this
       study was that Middle Devonian corals gave some 400 daily growth
       lines per year – suggesting a pronounced slowing of the Earth’s
       spin rate over the past 380 million years. Subsequent studies of
       skeletal increments in marine fossils back to the Ordovician
       were generally consistent with a higher rotation rate also in
       the Lower Palaeozoic (Pannella et al., 1968). Creer (1975) and
       Whyte (1977) summarized the palaeontological length of day data
       available by the mid-1970. Figure 5 shows the graph of presumed
       number of days during post-Precambrian time given by Creer. A
       subsequent compilatory L.O.D. study by Williams (1989) gave
       closely similar results – in addition to presenting fossil clock
       data for the Mesozoic. More recently, a study by Rosenberg
       (1997) concluded that at Grenville time (some 900 million years
       ago) the year had 440 days.
       ...
       Concluding summary
       In this paper, the focus has been on the origin of Earth’s
       surface water and the cause of sea-level changes for which the
       crustal product is a continuing, albeit jerky, loss of
       eclogitized gravity-driven continental material to the mantle –
       eventually leading to formation of the present-day thin oceanic
       crust and deep sea basins. As a result of the actual degassing
       Earth model, today’s continents have, during the Phanerozoic,
       been repeatedly flooded by slowly rising seas which after
       sea-level high stands have subsequently retreated to form
       distinct sea-level lows. It is an observation of paramount
       importance, long noted by many authors, that the most marked
       regressive events occur at times of principal geological time
       boundaries – representing revolutionary episodes in Earth
       history – in terms of tectonic, magmatic, biological and
       environmental happenings. In this way, sea-level changes became
       intimately linked to the rest of the planet’s first-order
       geological manifestations.
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