Explore
This article is from
Journal of Creation 14(1):60–74, April 2000

Browse our latest digital issue Subscribe

The pre-Flood/Flood boundary at the base of the earth’s transition zone

Max J. Hunter

The earth was created instantaneously ex nihilo by God, with a molten core, and a cool crust overlying a high-temperature sub-solidus mantle. The mantle was maintained at a ‘critical’ equilibrium pressure by gravity, the strength of which was determined by the magnitude of the created universal gravitational constant (G). The critical pressure was such that mantle melting and differentiation was inhibited.

A water vapour canopy probably surrounded the antediluvian atmosphere, which must have been essentially the same as today’s atmosphere.

As first proposed by John Woodward in 1695, God initiated the Genesis Flood by suddenly and temporarily lowering the magnitude of the gravitational constant, causing thereby an instantaneous decompression of the earth which disturbed the equilibrium of the created mantle-atmosphere-canopy system.

The decompression initiated canopy condensation and collapse (‘the windows of heaven’) and mantle melting and differentiation, including magma generation, mineralogical phase changes, crust formation and exsolution of volatiles, including copious volumes of water (‘the fountains of the great deep’). This mantle differentiation resulted in the present geophysical and geological structure and composition of the earth’s transition zone, outer mantle and lithosphere. The pre-Flood/Flood boundary is thus considered to be at the base of the transition zone, at the 660-km discontinuity.


Introduction

When young-earth creationists ascribe a pre-Flood/Flood boundary to a particular location in the geologic record, they generally use three a priori assumptions:

  1. There is an identifiable pre-Flood/Flood boundary in the observable geologic record.
  2. The first appearance of abundant fossils is one of the main characteristics marking the beginning of Flood deposited strata.
  3. The absence of fossils in lower, older strata identifies them as pre-Flood strata.

The sudden appearance of abundant fossils, and a world-wide unconformity, at the base of the Cambrian strata, or in the upper Proterozoic, Vendian strata has, in the minds of many creationist writers, identified this position as the pre-Flood/Flood boundary. They have on this basis assigned the formation of the older Precambrian strata (Archean and Proterozoic) to Creation week, usually assigning the formation of the Archean strata to Day 1 creative activity, and the Proterozoic to geological activity associated with uplift of the land on Day 3.

Few, if any, creationists seem to have considered that different criteria to those generally postulated might characterise early Flood strata. A few have proposed additional criteria, 1–3 and a few have suggested a lower, earlier, location for the boundary within the stratigraphic record. 1,3,4–7

In 1996 I summarised the trend,7 begun by Woodmorappe,4 towards consideration by creationist writers of the Precambrian as Flood rocks. I postulated that the Archean ‘basement granites’ and volcano-sedimentary strata, the Proterozoic sedimentary strata, and the waters of ‘the fountains of the great deep’ were derived by catastrophic differentiation of the earth’s mantle during the initiation and early stages of the Flood. I thus speculated that the pre-Flood/Flood boundary should lie below the base of the Archean strata, in the earth’s mantle, where these differentiation processes were thought to have initiated.

In this paper I propose that the present geophysical/geological structure of the earth’s mantle is the result of a sudden decompression of the created earth, due to a sudden, temporary reduction of the magnitude of the gravitational constant (G). I intend to document what I consider to be the evidence for a temporary reduction of G in a future article.

The outlines of the model as presented in this paper may form the basis of a comprehensive Flood geologic model.

Origin theories

Genesis 1:1

‘In the beginning God created the heaven[s] and the Earth.’

Psalm 33:6, 9

‘By the word of the Lord were the heavens made; and all the host of them by the breath of his mouth. … For he spake, and it was done; he commanded, and it stood fast [emphasis added].’

One’s conclusions regarding the structure and geological history of the earth will be strongly biased according to beliefs regarding its origin. Accordingly, a brief review of contemporary secular and creationist origin theories (cosmogenies) follows.

Regarding the origin of the Universe, Mehlert8 notes; ‘there are two primary logical foundations from which to begin [emphasis added].’ Either:

  1. ‘The universe has always existed and always will,’ (e.g. eternal or steady-state theory, as propounded by Hoyle, Gold and Bondi, in the late 1940s.) or;
  2. The universe came into being at a definite point in the past, with or without a creator being involved.’ (e.g. big-bang or standard model, first postulated by Gamow in the 1940s.)

Secular cosmogenies

Spencer9 summarises, from a creationist perspective, current views on the origin of the universe,10–17 including the solar system, and notes that the big-bang model for the origin of the universe is presently in favour with the scientific community. Spencer also notes that a Modified Nebular Hypothesis, much like the Nebular Hypothesis proposed by Pièrre Simon Laplace in 1796, is the currently accepted model for the origin of the solar system.

In the Nebular Hypothesis of solar system origin, the sun, planets, and all other solar-system bodies condense, by natural processes such as gravity, magnetic effects, and collisions, from an interstellar nebula forming first a ‘protosun’ with a surrounding disc of solid mineral grains, dust and gases. Within the disc, turbulence and random motions, it is postulated, lead to clustering so that ‘gravity begins to pull matter together by its own weight’, and over long periods of time this matter accretes as planets and moons, without layered interiors, as gravitational accretion would not produce layered objects.

Radioactive decay, and bombardment of the accreted planets and planetary satellites by meteorites, supposedly caused the newly formed planets to heat. This heating was supposedly sufficient to cause the dense material to sink toward the centre and the less dense material to move closer to the surface forming the present layered structures in the planets and moons.

Traditional creationist cosmogeny

Isaiah, 45:18

‘For thus saith the Lord that created the heavens; God himself that formed the earth and made it; he hath established it, he created it not in vain, he formed it to be inhabited …[emphasis added].’

Psalm102:25

‘Of old, thou hast laid the foundation of the earth: and the heavens are the work of thy hands.’

Whitcomb18 summarises the Traditional View involving instantaneous ex nihilo creation of the earth and the heavens about 6,000 years ago as follows:

‘The earth, like the heavens, was created without the use of pre-existent materials … which clearly implies that it was created instantaneously as a dynamic, highly complex entity. … spinning on its axis … it had a cool crust, for it was covered with water. … it did contain all of the basic elements and the foundational rocks of our present earth.
… it [the earth] is …absolutely unique in God’s eternal purposes. It was on this planet that God placed man, created in His image, to exercise dominion and to worship Him. … Because of its positional superiority in the spiritual order of things, therefore, the earth was formed first …[emphasis added].’

In this paper the traditional creationist cosmogeny, involving instantaneous ex nihilo creation (Psalm 33:9, ‘he spake, and it was done’) as outlined by Whitcomb and Morris, is assumed. The spatial relationships and relative motions of all bodies in the universe were, I believe, created fixed and functioning according to the subsequently discovered ‘Newtonian’ laws of motion19 (Psalm 33:9, ‘it stood fast’). Except for subsequent minor departures from created order, these spatial relationships and relative motions are essentially the same today as they were at creation.

Created ‘antediluvian’ earth structure

(Genesis 1:1–2, Genesis 1:6–10, Isaiah 45:18)

Figure 1.
Figure 1. A) Postulated structure of the created antediluvian earth. B) The present structure of the postdiluvian differentiated and expanded earth.
Click here for larger view

Figure 1 illustrates my conception of the created antediluvian earth structure, compared to the present postdiluvian differentiated, expanded earth. The size, total mass and density distribution of the created earth were, I believe, probably designed to impart the particular orbital and rotational dynamic characteristics required for a habitable earth (Isaiah 45:18).

Solid earth

Austin et al.20 proposed that the created pre-Flood earth was differentiated into a core, mantle, and crust and precluded a post-creation origin for this differentiation. Their conclusions would seem to be confirmed by the smoothness of the density profile through the inner and outer core and the inner mantle of today’s earth (Figure 2), the sharpness of the outer core/mantle boundary, and the magnitude of the density jump across this boundary. All these features indicate that these subdivisions of the earth’s structure may have been created that way, and did not differentiate naturally due to heating by meteorite bombardment and radioactive decay as proposed in the current modified nebular model of earth origin.

The model of Austin et al. for the created earth (Figure 1A) is used in this paper. In detail, this assumes a hot, sub-solidus mantle maintained at a critical pressure, such that a sudden significant reduction of pressure would have initiated melting and mantle differentiation, and in particular, reactions involving the formation and exsolution of water (‘the fountains of the great deep’).

Hydrosphere

Genesis 1:9,10

‘And God said, Let the waters under the heaven be gathered together unto one place …and the gathering together of the waters called he Seas …[emphasis added].’

Genesis 2:5–6

‘… for the Lord God had not caused it to rain upon the earth … But there went up a mist from the earth, and watered the whole face of the ground.’

The antediluvian hydrologic cycle may have been much different to that of today. The ‘mist’ which watered the earth (Genesis 2:6) may have resulted from slow exsolution of water from the created mantle through the cool crust. Scripture indicates that rivers existed, but due to a probable lack of storm activity, and because their source was from the ‘mist’, flow rates in these rivers would have been extremely regular. The river waters probably carried no sediment, thereby resulting in no sedimentation in the pre-Flood oceans. They may have contained dissolved salts which were derived from the mantle and were nutritional to man and beast.

Figure 2
Figure 2. The density distribution within the earth according to the Preliminary Reference Earth Model (PREM) of Dziewonski and Anderson.103 Note that a different distance scale applies to the atmosphere than applies for the solid earth.
Click here for larger view

I have suggested,7 based on the amount of water estimated to have been exsolved from the mantle during the Flood, that the volume of pre-Flood free water may have been about 10% of today’s free water. This amount of water would have been enough to provide suitable depth environments for all pre-Flood fish and sea creatures. Refinement of this figure awaits more accurate estimates of the water content of the present mantle, and calculation of the amount of water exsolved from the differentiating mantle during the Flood. Such estimates will help provide some preliminary concepts of pre-Flood geography.

Atmosphere

Many secular researchers have postulated that the earth’s atmosphere21,22 has resulted from exsolution of volatiles from the mantle early in the earth’s history,23–30some even suggesting catastrophic differentiation.31

Today’s atmosphere comprises 78.08 % nitrogen, 20.94 % oxygen, 0.93 % argon, and 0.03 % carbon dioxide.32 If we assume that the physiology of today’s air-breathing animals and mankind is similar to those of pre-Flood times, then the pre-Flood atmosphere could not have been much different compositionally from today’s.

Exsolution of significant quantities of volatiles into the earth’s atmosphere, during the Flood, or at any time during earth history, would probably have increased its toxicity, possibly to levels similar to that of the atmospheres of the gaseous planets. Thus, if significant exsolution of volatiles from the mantle did occur during the Flood, as seems likely, the volatiles most probably were precipitated and preserved in the stratigraphic record in rocks such as carbonates, nitrates, phosphates, and sulphates. The atmosphere was thus probably protected from the exsolution of volatiles from the mantle by the Flood waters, and the present atmosphere may thus be essentially the same as the antediluvian atmosphere.

Water vapour ‘canopy’

Scripture (Genesis 7 and 8) clearly records that a significant amount of rain fell, from above, to the earth, during the first forty days and nights of the Flood. Genesis 7:11–12 indicates that the water had previously been held above the earth’s surface, and was allowed to fall to the earth through ‘windows’ (KJV) or ‘floodgates’ (NIV) during the first forty days and nights of the Flood.

Prior to 1978, several creationist authors had speculated regarding the existence of a pre-Flood water vapour canopy.33–36 Dillow in 1978,37,38 modelled the canopy with its base maintained in the earth’s gravitational field at an altitude of about 9 km by a temperature inversion and Taylor stability, as the source of the Flood rain. Dillow assumed that precipitation from the canopy occurred at a global average rate of about 0.5 inches (12 mm) per hour for forty days and nights, resulting in about 40 feet (12 m) depth of precipitated water.

Dillow’s canopy model has been supported,39–44 challenged,45–48 revised and defended49 in the creationist literature. Opinion currently seems to be divided as to the validity of the canopy model. The main problems perceived with the canopy theory are the theorized high earth surface temperature under the canopy50,51 and dissipation of the latent heat of condensation during canopy collapse.52

Development of earth models

Psalm 95:4

‘In his hand are the deep places of the earth: the strength of the hills is his also [emphasis added].’

Contrary to belief among some creationists, the structure and composition of the inner earth is inferred with a large degree of confidence.53–68 Progress in the study of seismology (Figure 3) and high-pressure mineral physics now allows soundly based conclusions regarding the earth’s internal structure and composition and, to a certain extent, by inference, also its geological history (Figures 2 and 4).

Figure 3
Figure 3. Examples of raypaths through the earth following a deep focus earthquake. (P) indicates compressional waves, (S) indicates shear waves. The internal structure of the earth is inferred from earthquake recordings on a global network of seismometers, and seismogram interpretation relies on theoretical models of the earth’s interior. The predicted raypaths can be compared with what is actually recorded to provide further understanding of the internal structure of the earth.

All useful models of the density distribution inside the earth have had to satisfy estimated values for the earth’s radius, mass and moment of inertia and only became available after these parameters had been estimated to fair precision.

Bullen69 notes that the first steps toward determination of the distribution of density and other parameters within the earth were investigations by the early Greeks and Chinese (ca. 600–194 BC) concerning the earth’s shape and size. By the early 1500s, the earth had been circumnavigated and, by 1669, the dimensions of the earth were sufficiently accurately known to permit an estimation of its mean density, should evidence on its mass become available.

Newton, in 1687,70 used geophysical and planetary observations to arrive at his laws of motion, and applied these laws to investigating the earth’s shape and physical properties, laying the foundations for dynamical study of the shape and structure of the earth.

According to Newton’s Universal Theory of Gravitation the force F, between two bodies of masses m1 and m2, separated by a distance r, is given by F = Gm1m2/r2 (Newton’s ‘Inverse Square Law’ where G is the ‘universal gravitational constant’). Thus for points on the earth’s surface where r = a (earth radius), F/m(=g)=GM/a2 (where g = acceleration due to gravity, amd M is the mass of the earth).

Hence, when observational values of a (earth radius) and g (acceleration due to gravity at the earth’s surface) became available, a useful estimation of GM could be made. Once this was known, separate values of G and M could be determined by any experiment which determined either G or M alone.

Towards the close of the 18th century, Michell constructed a torsion balance to measure directly the gravitational attraction between spherical masses m1 and m2 in the laboratory,71 as suggested by Newton. This enabled the constant of gravitation G, to be determined from measurements of F, m1, m2, and d, using the relationship F = Gm1m2/d2. Cavendish71 modified Michell’s apparatus and in 1798 calculated the earth’s mean density at 5.448 g/cm3. By the early 19th century, the mean density of the earth was known to an accuracy of about 1 %.

Figure 4
Figure 4. The internal layered structure of the present earth (after Bott115).
Click here for larger view

Thompson and Tait (1879)72 proposed the first multi-layered models of the earth, with a core and an outer shell. Radau (1885)73 and Weichert (1897)74 worked out numerical details for the Thompson-Tait models using the density of surface rocks as 2.7 g/cm3, a core density of 7.47 g/cm3, and core radius of 0.844 earth radii. From Weichert’s time until about 1914 several earth models with different core densities were contemplated and in 1915 Klussmann75 constructed several models, each with three layers of constant densities and assigned thicknesses.

Haalck (1925)76 sought to allow for variation of density within layers and postulated a linear variation down to 1200 km and a different variation from there to the core boundary at 2900 km depth.

Williamson and Adams, in 1923,77 showed that compressibility alone could not raise the density in the deeper interior enough to account for the known mass of the earth. They concluded that there must be substantial changes in density, and/or chemical composition (phase changes) in the earth’s deeper interior.

Bullen (1936)78 confirmed the conclusion of Williamson and Adams (1923)77 that density increased with depth more rapidly through the transition zone than could be explained by self-compression of homogeneous material within the earth’s gravitational field. They concluded that chemical and/or phase changes must occur in this region. Birch (1958)79 inferred that phase changes in mantle mineral structure were primarily responsible for the inhomogeneity between 350 and 900 km, and that chemical changes were also possible (Figures 2 and 4). Birch’s hypothesis was verified in principle by direct laboratory experiments at very high pressures, mainly by Ringwood et al. (Canberra, Australia),80–87and Akimoto (Tokyo, Japan).88 These phase changes have now been studied in detail, in both seismic modelling and in high pressure laboratory experiments.89–92

During the early 1900s, the development of seismic theory enabled the distributions of compressional (P) wave and shear (S) wave velocities inside much of the earth to be estimated. In 1964, Birch93,94determined relationships between seismic wave velocity, density, and several other parameters, including the elastic moduli, compressibility, Poisson’s Ratio and the Seismic Parameter.95 Thus, the approximate distributions of these parameters within the earth became available.

Bullen and Haddon in 196796 produced a series of earth models, including distributions of the earth’s incompressibility, rigidity, pressure, gravitational intensity and several derived variables, including Young’s Modulus and Poisson’s Ratio. Thus, a useful first approximation of the main internal physical structure of the earth was provided.

Continued refinement of seismic techniques and laboratory mineral physics studies has allowed more accurate models of the earth’s interior to be developed,77,97–104including Model ak 135 of Kennett, Engdahl and Buland,105 used in this paper (Figure 5).

Present ‘post-Flood’ earth structure

The six main sub-divisions of the earth’s structure, from the centre out, (Figures 1 and 2) are outlined here.

Core (Depth: 2886–6371 km)

Jacobs106 noted that as early as the nineteenth century it had been suggested that the earth had a core of higher density than the surrounding mantle, and in 1906 Oldham established its existence. Birch was the first to suggest the existence of a solid inner core.

Inner core (Depth: 5156–6371 km): The inner core is thought to consist of solid iron-nickel, at a temperature of up to 7,000 °C. The prevailing secular theory regarding the inner core’s origin is that it formed by gradual solidification of the liquid core as the earth cooled.107

Outer core (Depth: 2886–5156 km): The outer core is thought to be comprised of molten iron and nickel, with some FeO, at a temperature ranging from 4,400 °C in the uppermost parts to about 6,100 °C in the deepest parts.108 The earth’s magnetic field is thought to originate in the outer core.

Inner mantle (Depth: 660–2886 km)

The inner mantle (Figure 5) extends from the outer core/inner mantle boundary, at depth 2,886 km to the 660-km seismic discontinuity at the base of the transition zone. It is considered to consist of 70 % λ-olivine ((Mg Fe Al)(Al Si) O3) with a perovskite structure, and 20 % magnesiowustite ((Mg Fe) O).109–113

The 660-km discontinuity, at the top of the inner mantle, is the most pronounced seismic discontinuity in the mantle,114,115 and is considered to be due mainly to mineral phase changes. Moving downward through the transition the γ-olivine with spinel structure transforms to λ-olivine + magnesiowustite and the garnet in the pyroxene-garnet system transforms to ilmenite, with an associated density increase of approximately 9.5 %.

Small seismic discontinuities in the outer part of the inner mantle may indicate further transitions to slightly denser states in this area.116 The minor seismic discontinuity at about 800 km for instance, may be due to the phase transition from aluminous ilmenite solid solution to orthorhombic perovskite.

Transition zone (Depth: 410–660 km)

The transition zone (Figure 5) extends from the 660-km discontinuity at its base to the 410-km discontinuity at its top.117–120 At the top of the transition zone above the discontinuity, γ-olivine ((Mg Fe)2 SiO4) is considered to transform to the higher pressure phase β-spinel (β—(MgFe)2SiO4) below the discontinuity with a 4.6 % increase in density. Aluminous pyroxene also transforms to garnet, with a 2 % increase in density.

At about 520 km, β-phase spinel is considered to transform to γ-olivine (spinel structure), and garnet to Ca-perovskite.

Outer mantle (Depth: 80–410 km)

The outer mantle (Figure 5) extends above the 410-km discontinuity.85,121–124 In the currently accepted ‘pyrolite’ mantle model, first proposed by Ringwood,80 the outer mantle consists of a pyroxene-olivine rock (peridotite) which is capable of producing basaltic magmas on partial melting. Ringwood109 proposed a detailed mineralogy for the outer mantle peridotite: 57 % olivine ((Fo89) (Mg Fe)2 SiO4), 17 % orthopyroxene ((En89) (MgFe) SiO3), 12 % omphacitic pyroxene ((Ca Mg Fe)2 Si2O6NaAlSi2O6), 14 % pyrope garnet ((MgFeCa)3 (Al Cr)2Si3O12), and minor minerals; diopside (Ca(MgFe) Si2O6) and jadeite (NaAlSi2O6).

Most researchers in high-pressure mineral physics and the seismic structure of the earth have ascribed the phase transitions in mantle minerals, including the main seismic velocity discontinuities at 410 km and 660 km depth, as occurring from the lower pressure phases to the higher pressure phases, due to increasing pressure with increasing depth. This assumption seems to be implicit in all current high-pressure mineral physics research.

Holmes,125 for instance, notes regarding phase-changes and mantle structure:

‘In the mantle continuous rise of density with depth depends on the effect of pressure in compressing the lattice structures of crystalline minerals. At certain critical depths a discontinuous jump to a higher density may occur either because the lattice has been modified into a different and tighter pattern, or because the minerals have absorbed sufficient energy to break down into their constituents ... which recrystallise in denser forms.’

More recently, Jeanloz126 stated:

‘… the rapid increases in seismic wave velocities that define the ‘transition zone’ in the mantle at depths of 410–660 km … are classically interpreted as being due to pressure-induced phase transitions in olivine. Just as graphite transforms to diamond at high pressures, olivine is known to transform to spinel and perovskite-type crystal structures at the pressures of the transition zone.’

Dearnley127 however notes that:

‘Egyed[128–130]has previously suggested Earth expansion resulting from high to low pressure phase changes accompanying the inward movement of the isobars with decrease of G.’

It is postulated here that these phase changes occurred due to the release of pressure consequent upon the postulated reduction in the magnitude of G. This caused the mantle minerals to convert to their present low-pressure structures, with consequent decrease in density and increase in volume.

The conversion of the transition zone minerals to the lower pressure, lower density phases resulted in a radial expansion of the earth of about 95–100 km. These outward redistributions of mass probably caused a decrease in the earth’s rotational velocity, which may have been partly compensated for by inward redistribution of mass involved in the differentiation of the solid inner core from a single created liquid core (Figure 1), and due to collapse of the vapour canopy.

Crust (Depth: 0–80 km)

The earth’s crust (Figure 4) is comprised of continental crust and oceanic crust.131–133 Continental crust is generally andesitic in composition, and varies in thickness from about 20 to 100 km (average 39 km). Oceanic crust is generally basaltic in composition and varies in thickness from 3 to 10 km. It is considered that the different natures of the continental and oceanic crusts reflect their different modes of origin.

Continental crust: The continental crust mass is approximately 71 % of the total crust mass and 2.1 % of the mass of the mantle.

It is generally agreed among secular researchers that the earth’s present continental crust has resulted from differentiation from the mantle, mostly during the Archean, and models for this differentiation have been constructed.134–136 Patchett134 for instance describes a plume-driven mantle differentiation model of continental crust formation, commencing in the Archean, which fits the Flood differentiation model presented here:

‘… the main advantage of a plume-driven crustal genesis model, … mantle plumes are a straightforward product of the Earth’s heat … and should have been most common in the Archaean, becoming steadily less so with time. … The intense crustal growth in the late Archaean and early Proterozoic was followed by generally smaller-scale pulses extending to the present day.’

In the Flood differentiation model presented here, the pre-Flood crust was completely destroyed and the present continental crust was formed by mantle differentiation, probably during the first forty days of the Flood.

Wedepohl137 developed a ‘standard [continental] crustal profile’ with symbolized compositions and processes, from the European Geotraverse. Wedepohl’s model comprises, from the surface down; sedimentary rocks, granite and tonalite plutons, mica schists, gneisses, amphibolites, felsic granulites, mafic granulites to the Moho, below which occur the spinel lherzolites and spinel harzburgites of the outer mantle.

Rudnick138 summarises current ideas regarding the origin of the continental crust as follows:

‘… there is considerable debate regarding how and when [the continents] formed and the processes responsible for their unique composition. Did the present mass of continents form very early in Earth’s history [supposedly 4.0 Gyr ago], with past and present growth counterbalanced by recycling of crust into the mantle? If so, what were the main processes that formed the early crust and how do they compare with those operating today?’

Maaloe and Steel131 suggest that the continental crust was formed by differentiation from the ‘primitive mantle’ and that a model composition of the primitive mantle before continent formation may be approximated by adding the composition of the crust to the average composition of the present mantle. In the creationist model this would equate to working out the composition of the created mantle.

Oceanic crust: The oceanic crust mass is approximately 29 % of the total crust mass.139

In contrast to the continental crust, the structure of the oceanic crust is fairly consistent, comprising four layers: Layer 1; approximately 300 m of semi-consolidated to unconsolidated deep-sea sediments. Layer 2; 1,000–1,500 m of basaltic pillow lavas. Layer 3; 3,000–6,500 m of sheeted dyke complex overlying a gabbroic magma chamber. Layer 4; layered peridotite overlying the Moho, below which is the peridotite and dunite of the outer mantle.140,141

It is postulated here that the basaltic oceanic crust formed due to decompression melting of peridotitic mantle material during stretching of the oceanic lithosphere due to earth expansion.

Hydrosphere

The total volume of free water at the earth’s surface142 is 1.384 x 109 km3. In an earlier paper, I postulated that 89 % of the present free water at the earth’s surface was exsolved from the mantle during the Flood as ‘the fountains of the great deep’ and 1 % was precipitated from the pre-Flood canopy.7

Atmosphere

The troposphere, the lower part of the present atmosphere, must be essentially the same composition as the antediluvian atmosphere beneath the canopy, as it supports the same air-breathing creatures, plants and mankind. The upper present atmosphere probably differentiated into the stratosphere, mesosphere and thermosphere after dissipation of the canopy, probably during the first forty days of the Flood.143–146 As previously discussed, any volatiles exsolved from the mantle during the Flood must have precipitated in sediments in the Floodwaters, otherwise they would have toxified the present atmosphere.

The Genesis Flood

Genesis 6:13

‘And God said unto Noah, The end of all flesh is come before me; for the earth is filled with violence through them; and, behold, I will destroy them with the earth [emphasis added].’

Genesis 6:17

‘And, behold, I, even I, do bring a flood of waters upon the earth, to destroy all flesh, wherein is the breath of life, from under heaven; and every thing that is in the earth shall die [emphasis added].’

Genesis 7:4

‘For yet seven days and … every living substance that I have made will I destroy from off the face of the earth.’

Genesis 7:21–23

‘And all flesh died that moved upon the earth, both of fowl, and of cattle, and of beast, and of every creeping thing that creepeth upon the earth, and every man: All in whose nostrils was the breath of life, of all that was in the dry land, died. And every living substance was destroyed which was upon the face of the ground, both man, and cattle, and the creeping things, and the fowl of the heaven; and they were destroyed from the earth … [emphasis added].’

The huge scale differentiation of the earth’s mantle from 660-km depth, and destruction of the antediluvian crust, as proposed in the Flood model presented here, would appear to be much more catastrophic than necessary to destroy mankind and air-breathing creatures.

Genesis 6:13 indicates that the destruction of ‘the earth’ was part of God’s intention for the Flood. In the process of destroying and re-making the earth, God was, in effect, setting up the geography of the earth’s surface for the next millennia, until Christ’s return and the ‘new heaven and a new earth.’ (Matthew 24:35, 2 Peter 3:13, Revelation 21:1)

The post-Flood geography, including the distribution of continents, oceans, islands, mountain ranges, rivers and lakes, and of natural resources such as fertile soils, fossil fuels, and minerals, would, by strongly influencing trade, migration and wars, etc., to a large degree influence the geo-political history of the post-Flood world.

Initiation of the Flood

Genesis 6:5–7

‘And God saw that the wickedness of man was great in the earth, and that every imagination of the thoughts of his heart was only evil continually. And it repented the Lord that he had made man on the earth, and it grieved him at his heart. And the Lord said, I will destroy man whom I have created from the face of the earth … for it repenteth me that I have made them [emphasis added].’

Genesis 6:13

‘And God said …The end of all flesh is come before me … behold, I will destroy them with the earth [emphasis added].’

Genesis 6:17.

‘And behold, I, even I, do bring a flood of waters upon the earth …’

Genesis 7:4

‘For yet seven days, and I will cause it to rain upon the earth forty days and forty nights …’

Genesis 7:10–11

‘And it came to pass after seven days, that the waters of the flood were upon the earth. In the six hundredth year of Noah’s life, in the second month, the seventeenth day of the month, the same day were all the fountains of the great deep broken up, and the windows of heaven were opened [emphasis added].’

Creationist descriptions of the Flood event must, it is suggested, explain its sudden initiation (Genesis 7:11, ‘the same day’).

Austin et al.20 have summarised the events postulated to have initiated the Flood as constituting one or a combination of the following:

a. The ‘direct hand of God’.

b. The ‘impact or near-miss’ of an astronomical object or objects.

c. Some ‘purely terrestrial event or events.’

It is here suggested that any creationist explanation of the initiation of the Flood must, ultimately, resort to the ‘direct hand of God’.

Whitcomb and Morris147 speculate concerning the initiation of the Flood as follows:

‘Great volcanic explosions and eruptions are clearly implied in the statement that “all the fountains of the great deep (were) broken up” … great quantities of liquids, perhaps liquid rocks or magmas, as well as water (probably steam) had been confined under great pressure below the surface rock structure of the earth since the time of its formation and that this mass now burst forth through great fountains … [emphasis added].’

Many creationist writers have recognised the requirement for an extremely large amount of energy to initiate the Flood process. Brown148 for instance, suggests a build-up of subterranean water pressure, culminating in the explosive failure of the crust, Baumgardner149 suggests gravitational potential energy, perhaps triggered by meteorite impact, and Auldaney,150 Fischer,151 Spencer152 and others, have suggested meteorite/asteroid impacts, and/or a close fly-by of a large planetary body.

John Woodward, a contemporary of Sir Isaac Newton, proposed in 1695153 that ‘the action and suspension of the Newtonian force of gravity’ caused the Genesis Flood. I postulate, similarly to Woodward, that the energy required to initiate the Flood constituted ‘negative gravitational potential energy’ resulting from a sudden, temporary reduction of the magnitude of the gravitational constant resulting in a sudden decompression of the earth. The duration of such a reduction of the universal gravitational constant (G) may be difficult to determine, however only a few hours may have been sufficient to initiate mantle melting and irreversible differentiation.

The Flood was thus, I postulate, and as speculated by Whitcomb and Morris, initiated by a sudden significant reduction of pressure within the interior of the earth. This initiated canopy condensation and collapse (‘the windows of heaven’) and mantle melting and differentiation, in particular, reactions involving the formation and exsolution of water (‘the fountains of the great deep’).

Canopy collapse (‘the windows of heaven’)

Genesis 7:4

‘For yet seven days, and I will cause it to rain upon the earth forty days and forty nights …’ [emphasis added].

Genesis 7:11–12

‘In the six hundredth year of Noah’s life … the same day were all the fountains of the great deep broken up, and the windows of heaven were opened. And the rain was upon the earth forty days and forty nights’ [emphasis added].

Genesis 8:2

‘The fountains …and the windows of heaven were [had been] stopped, and the rain from heaven was restrained’ [emphasis added].

An immediate effect of a sudden decompression of the earth would have been a reduction of atmospheric pressure, which would have promoted condensation of the postulated superheated steam canopy as proposed by some creationists.

One of the main objections to the canopy model, apart from the antediluvian earth surface temperature problem,154 has been the predicted large atmospheric and ocean temperature rises resulting from latent heat of condensation during canopy condensation and collapse.155,156 Morton157 recognised the heat dissipation problem and suggested that the Flood may have been initiated by a reduction of the permittivity of free space, suggesting that:

‘The permittivity hypothesis is the only creationist theory which can account for the absorption of enough heat at a rapid enough rate to allow for 40 days and nights of rain.’

Walters156 suggested that the ‘energy load’ on the atmosphere resulting primarily from ‘the energy released by the canopy when it condenses; would have caused atmospheric temperature rises much too high to sustain life’ [emphasis added].

As the Flood was specifically engineered to destroy terrestrial life on Earth, even extremely high atmospheric and oceanic temperatures, in specific areas, during canopy collapse should not have been a problem regarding the sustaining of life.

Significantly, Walters speculated that the Flood rainfall may not have covered the whole earth, but may have been ‘ concentrated near the equatorial belt, with lighter rains in the more extreme latitudes?’

In 1996 I postulated a canopy collapse scenario involving destabilisation of the canopy base by pressure perturbations caused by large Archean caldera collapse structures and associated volcanic eruptions on the earth’s surface at the initiation of the Flood.7 Depressurisation of the canopy may, I suggest, also have promoted condensation.

Some secular authors have speculated that ocean temperatures in Archean times may have been very high. Costa, et al.,158,159 for instance, note that there is evidence that; ‘ocean temperatures may have been near the boiling point in the Archaean’ [emphasis added].

Such evidence would suggest that the high temperature Flood ‘rain’ may have been concentrated, not in the equatorial areas, but in the Archean portions of the Precambrian Shields. Here canopy collapse may have been initiated by caldera collapse structures and volcanic activity associated with the rise of large ‘mantled gneiss domes’ and ‘gneiss fold ovals,’ the major tectonic structures of the Archean. The latent heat of condensation of the canopy would have been dissipated into the ‘oceanic’ Flood waters. In areas distant from the Precambrian Shields, the Flood waters, and the atmosphere, would have been cooler, allowing sea creatures, and the inhabitants of the Ark to survive. This may provide further tentative clues regarding pre-Flood geography as to the location of the construction of the Ark and its journey upon the waters.

Mantle melting and differentiation

The physico-chemical processes of mantle melting and differentiation are extremely complex.160–168 Consequently, the development of a comprehensive model of mantle melting and differentiation due to a sudden reduction in pressure is beyond the scope of this paper. Thus, only a brief outline of the envisaged scenario can be attempted.

It is proposed that the key to understanding Flood mantle melting and differentiation processes lies in determining the effect of a sudden decompression on a reconstituted pre-Flood mantle-crust-hydrosphere.131

I propose that the created mantle was maintained at a critical pressure and sub-solidus temperature by pressure determined by the magnitude of the created gravitational constant. The postulated de-compression of the earth would lower the solidus temperature causing melting of mantle minerals and initiating mantle differentiation.

Several secular authors have postulated that melting of mantle material is initiated by depressurisation. Nielson and Wilshire169 for instance suggest:

‘Melts form when a portion of the mantle exceeds the solidus temperature by progressive heating or depressurization … [emphasis added].’

McKenzie and Bickle170 note that magma is generated by decompression melting beneath mid-ocean ridges due to lithospheric extension and Asimow et al.171 discuss pressure-release melting of the earth’s mantle.

Wyllie172 examines the effect of water on the conditions for melting in the mantle, and suggests a model for magma generation involving diapiric uprise of mantle material. He proposes that uprise of magma may have begun at the base of the low velocity zone, at depths of the order of 300 km, being triggered by the outward migration of water from within the deep mantle. Interestingly Wyllie cites ‘gravitational instability’ as initiating the outward migration of water and mantle material.

Secular researchers thus recognise that depressurisation plays a vital role in mantle differentiation and melt generation.

Water exsolution (‘the fountains of the great deep’)

Genesis 7:11

‘In the six hundredth year of Noah’s life, in the second month, the seventeenth day of the month, the same day were all the fountains of the great deep broken up …[emphasis added].’

The water of the ‘fountains of the great deep’ is considered to have been derived by exsolution of water from the differentiating transition zone and outer mantle.

The significant role of water in the generation of magmas and the initiation of diapiric uprise of mantle material had been recognised by mantle researchers for many years prior to the mid 1970s.172,173–182 Researchers had speculated regarding the origin of the earth’s oceans and atmosphere by (catastrophic) ‘de-gassing’ of the mantle.183–185 Bell and Rossman186 note:

‘Determination of Earth’s water budget and the identification of suitable repositories for H [colloquially “water”] in the mantle are long-standing problems in geology with important implications for the evolution of the planet as a whole.’

Wyllie172 wrote, regarding the role of water in magma generation and initiation of diapiric uprise in the mantle:

‘… the most reasonable model for magma generation involves the diapiric uprise of mantle material …’

and proposed that:

‘… uprise may begin at the base of the low velocity zone, at depths of the order of 300 km, and … uprise may be triggered by the outward migration of water from within the deep mantle.’

In the mid to late 1970’s, researchers began to identify specific minerals as possible hosts for water in the mantle. In 1980 Akimoto et al.187 suggested hydrous magnesian silicates as hosts for water in the transition zone, and in 1985 Kato et al.188 studied the stability of phase β, a hydrous magnesium silicate, to 2300 °C at 20 GPa.

Figure 5
Figure 5. Density profile through earth’s inner mantle, transition zone and outer mantle (Model ak 135 of Kennett et al.105). The expansion of the earth’s surface due to differentiation during the Flood is indicated. Note that a different distance scale applies to the atmosphere than applies for the solid earth.
Click here for larger view

Smyth, in 1987189 cited β-Mg2SiO4 as a host for water in the mantle, and in 1994190 proposed a hypothetical ordered model for hydrous wadsleyite (Mg7Si4O14(OH)2). He predicted a maximum H2O content for the hypothetical phase of 3.3 wt%, implying that the transition zone of the mantle might contain several oceans of H2O if fully hydrated.

Finger et al.191 describe the crystal structure and crystal chemistry of phase B (Mg12Si4O19(OH)2) and suggest that the reaction B + spinel -AnhB + H2O or B + stishovite - AnhB + H2O could be a mechanism for storage and release of large volumes of water.

Thompson,192 Bell and Rossman,186 and Bai and Kohlstedt193 have reviewed the stability of various phases of hydrous magnesian silicates, and note that:

‘… of the nominally hydrous phases believed to make up the upper mantle and transition zone, none has been reported with a greater H content than wadsleyite (β-Mg2SiO4). … If the Earth’s mantle between 400 and 525 km were 60% fully hydrated wadsleyite with a density of 3.5 g/cm3, the amount of H2O incorporated in this phase would be equal to a worldwide ocean more than 8 km deep or more than four times the amount of H2O currently in the Earth’s hydrosphere.’

Thompson194 notes:

‘Since it was first reported that DHMS [Dense Hydrous Magnesian Silicates] were found when the simple system MgO–SiO2–H2O was subjected to high pressure and temperature there have been repeated suggestions that such minerals might be able to store water deep in the mantle. … most of the nominally anhydrous minerals (NAMS) in the mantle contain structurally bound OH. Pyroxenes contain 200–500 ppm water, and β-Mg2SiO4 has been found to contain up to 4,000 ppm (0.4 wt%) water.’
These findings may be highly significant for a catastrophic Flood mantle differentiation model.

The pre-Flood/Flood boundary

In the Flood geological model presented in this paper, the only ‘rocks’ which can be considered to retain their pre-flood characteristics are those of the inner mantle, and the core, below the 660-km discontinuity. Seismic evidence suggests that even the rocks of the inner mantle may have changed their characteristics slightly due to the reduction of hydrostatic pressure throughout the earth due to the postulated decompression although the effects of the pressure reduction should diminish with depth.

The pre-Flood/Flood boundary is thus considered to occur at the base of the earth’s transition zone, at the 660-km discontinuity.

Above the 660-km discontinuity, the rocks of the transition zone and outer mantle would have suffered progressively more complete disintegration of their created perfection towards the earth’s surface. The reduction of confining pressure towards the earth’ surface would have allowed progressively more magma differentiation, mixing of mineral components, and disintegration of the mantle structure.

This decompression model explains the progressive change in the composition of rocks from deep in the mantle towards the surface. The deeper rocks such as dunites, peridotites, pyroxenites are almost monomineralic (90+% olivine) while the shallower rocks such as granites are polymineralic. This variation perhaps reflects progressively more mixing of components in the shallower, lower-pressure outer mantle during the Flood catastrophe.

The mineralogical phase changes principally at the 660 and 410-km discontinuities, resulted from a sudden decrease of confining pressure. This is contrary to the general conception of cause by increase of confining pressure with depth.

The consistent reduction in the density of the crustal sedimentary pile towards the earth’s surface probably reflects the progressive reduction with time, of the energy, and thus the load-carrying capacity, of the Flood waters as they waned toward the end of the Flood. This is contrary to the common interpretation, that density increases downward due to the weight of overlying sediment.

Acknowledgements

The helpful advice given by Marcus Coleman, in particular with regard to the relationship of gravity to other forces, and alternative theories of gravitation is gratefully acknowledged, as are the comments of two anonymous reviewers and the editorial advice of Dr Tas Walker.

Posted on homepage: 12 April 2007

References

  1. Snelling, A.A., Creationist geology: Where do the Precambrian strata fit? Journal of Creation 5(2):154–175, 1991. Return to text.
  2. Austin, S.A. and Wise, K.P., The pre-Flood/Flood boundary as defined in Grand Canyon, Arizona and Eastern Mojave Desert, California; in: Walsh R.E. (ed.), Proceedings of the Third International Conference on Creationism, Creation Science Fellowship, Pittsburgh, Pennsylvania, pp. 37–47, 1994. Return to text.
  3. Davison, G.E., The importance of unconformity-bounded sequences in Flood stratigraphy, Journal of Creation 9(2):223–243, 1995. Return to text.
  4. Woodmorappe, J., A diluviological treatise on the stratigraphic separation of fossils, Creation Res. Soc. Quart. 20(3):133–185, 1983. Return to text.
  5. Snelling, A.A., Creationist geology— the Precambrian, Creation 6(1):42–46, 1983. Return to text.
  6. Hunter, M.J., Archean rock strata: Flood deposits— the first forty days; in: Proceedings of the 1992 Twin-Cities Creation Conference, Twin-Cities Creation Science Association, Northwestern College, Genesis Institute, Roseville, Minnesota, pp. 153–161, 1992. Return to text.
  7. Hunter, M.J., Is the pre-Flood/Flood boundary in the earth’s mantle? Journal of Creation 10(3):344–357, 1996. Return to text.
  8. Mehlert, A.W., The origin of the universe: a creationist evaluation of current scientific theories, Journal of Creation 8(2):238–245, 1994. Return to text.
  9. Spencer, W.R., The origin and history of the solar system; in: Walsh, R.E. (ed.), The Proceedings of the Third International Conference on Creationism, Creation Science Fellowship Inc., Pittsburgh, Pennsylvania, pp. 513–524, 1994. Return to text.
  10. Carey, S.W., Evolution of beliefs on the nature and origin of the earth; in: Carey, S.W. (ed.), The Expanding Earth: A Symposium, Hobart University, Tasmania, 1981. Return to text.
  11. McCall, G.J.H. Progress in research into the early history of the earth: a review, 1970–1980, Spec. Pub. Geol. Soc. Aust. 7:3–18, 1981. Return to text.
  12. Weaver, H. and Danly, L. (eds), The Formation and Evolution of Planetary Systems, Cambridge University Press, 1989. Return to text.
  13. DeYoung, D.B., The big bang: a reality check, Bible Science News 33(4):1–5, May 1995. Return to text.
  14. Taylor, S.R., Destiny or Chance: Our Solar System and its Place in the Cosmos, Cambridge University Press, 1998. Return to text.
  15. Saari, D.G., Celestial mechanics: orbits of all sorts, Nature 395:19, 1998. Return to text.
  16. Hamilton, D.P., Solar system: circular problems, Nature 396:413, 1998. Return to text.
  17. Gladman, B., Twenty eight ways to build a solar system, Nature 396:513–514, 1998. Return to text.
  18. Whitcomb, J.C., The creation of the heavens and the earth, Creation Res. Soc. Quart. 4(2): 69–74, 1967. Return to text.
  19. Stump, M.E.W. and Rowlands, R.G., Leaving Physics, F.W. Cheshire Pty Ltd, 1963. Return to text.
  20. Austin, S.A., Baumgardner, J.R., Russell Humphreys, D., Snelling, A.A., Vardiman, L. and Wise, K.P., Catastrophic plate tectonics: a global Flood model of earth history; in: Proceedings of the Third International Conference on Creationism, Creation Science Fellowship Inc., Pittsburgh, Pennsylvania, pp. 609–621, 1994. Return to text.
  21. Holland, H.D., The Chemistry of the Atmosphere and Oceans, John Wiley and Sons, 1978. Return to text.
  22. Meadows, A.J., Surface temperature of the early earth and the nature of the terrestrial atmosphere, Nature 226:927–928, 1970. Return to text.
  23. Houghton, J.T., The Physics of Atmospheres, Columb. University Press, 1977. Return to text.
  24. Holland, H.D., Model for the evolution of the earth’s atmosphere, Publ. Petrologic Studies: A Volume to Honour A. F. Buddington, pp. 447–477, 1962. Return to text.
  25. Walker, J.C.G., Evolution of the Atmosphere, McMillan Publ. Co., 1977. Return to text.
  26. Walker, J.C.G., The earliest atmosphere of the earth, Precambrian Research 17:147–171, 1982. Return to text.
  27. Hart, R., Dymond, J. and Hogan, L., Preferential formation of the atmosphere-sialic crust system from the upper mantle, Nature 278:156–159, 1979. Return to text.
  28. Pollack, J.B. and Yung, Y.L., Origin and evolution of planetary atmospheres, Ann. Rev. Earth Planet. Sci. 8: 425–487, 1980. Return to text.
  29. Holland, Degassing of the earth; in: Holland, H.D. and Trendall, A.F. (eds), Patterns of Change in Earth Evolution, Dahlem Konferenzen, Berlin, Heidelberg, New York, 1984. Return to text.
  30. Holland, H.D., Origins of breathable air, Nature 347:17, 1990. Return to text.
  31. Fanale, F.P., A case for catastrophic early degassing of the earth, Chem. Geol. 8:79–105, 1971. Return to text.
  32. Ronan, C. (ed.), Amateur Astronomy, Hamlyn, 1989. Return to text.
  33. Vail, I.N., The Deluge and its Cause, Suggestion Publishing, p. 91, 1905. Return to text.
  34. Udd, S.V., The canopy and Genesis 1:6–8, Creation Res. Soc. Quart. 12:90–93, 1975. Return to text.
  35. Strickling, J.E., The waters above the firmament, Creation Res. Soc. Quart 12(4):221, 1976. Return to text.
  36. Kofahl, R.E., Could the Flood waters have come from a canopy or extraterrestrial source? Creation Res. Soc. Quart. 13:202–206, 1977. Return to text.
  37. Dillow, J.C., Mechanics and thermodynamics of the pre-Flood vapour canopy, Creation Res. Soc. Quart. 15:148–159, 1978. Return to text.
  38. Dillow, J.C., The Waters Above: The Earth’s Pre-Flood Canopy, Moody Press, Chicago, 1981. Return to text.
  39. Akridge, G.R., Venusian canopy, Creation Res. Soc. Quart. 16(3):188–189, 1979. Return to text.
  40. Cyr, D.L., Global precipitation under a canopy, Creation Res. Soc. Quart. 15:184–211, 1979. Return to text.
  41. Bixler, R.R., Does the Bible speak of a vapour canopy? In: The Proceedings of the First International Conference on Creationism 1:19–21, 1986. Return to text.
  42. Rush, D.E. and Vardiman, L., Pre-Flood vapor canopy radiative temperature profiles; in: Walsh, R.E. and Brooks, C.L. (eds), The Proceedings of the Second International Conference on Creationism 2:231–245, Technical Symposium Sessions, Creation Science Fellowship, Pittsburgh, Pennsylvania. Return to text.
  43. Jorgensen, G.S., Fundamental physics of a water vapour canopy atmosphere; in: Proceedings of the 1992 Twin-Cities Creation Conf., 1992. Return to text.
  44. Jorgensen, G.S., The canopy, the Moon, the Earth’s tilt, and pre-Flood ice age; in: Proceedings of the Third International Conference on Creationism 2:287–303, Technical Symposium Sessions, Creation Science Fellowship, Pittsburgh, Pennsylvania, 1994. Return to text.
  45. Morton, G.R., Can the canopy hold water? Creation Res. Soc. Quart 16, 1979. Return to text.
  46. Morton, G.R., The warm earth fallacy, Creation Res. Soc. Quart. 17:40–41, 1980. Return to text.
  47. Morton, G.R., Reply to Dillow, Creation Res. Soc. Quart. 17:229–230, 1981. Return to text.
  48. Walters, T.W., Thermodynamic analysis of a condensing vapour canopy, Creation Res. Soc. Quart. 28:122–131, 1991. Return to text.
  49. Dillow, J.C., Reply to Morton: the canopy can hold water, Creation Res. Soc. Quart. 17:229, 1981. Return to text.
  50. Johnson, G.L., Global heat balance with a liquid water and ice canopy, Creation Res. Soc. Quart. 23:54–61. Return to text.
  51. Morton, G.R., Can the canopy hold water? Creation Res. Soc. Quart 16, 1979. Return to text.
  52. Johnson, G.L., Global heat balance with a liquid water and ice canopy, Creation Res. Soc. Quart. 23:54–61, 1980. Return to text.
  53. McElhinny, M.W. (ed.), The Earth: Its Origin, Structure and Evolution, Academic Press Inc. London, 1979. Return to text.
  54. Brown, G.C. and Musset, A.E., The Inaccessible Earth, George Allen and Unwin, London, 1981. Return to text.
  55. Nakiboglu, S.M., Hydrostatic theory of the earth and its mechanical implications, Phys. Earth Planet. Int. 28:302–311, 1982. Return to text.
  56. Bott, M.H.P., The Interior of the Earth: Its Structure, Constitution and Evolution, Edward Arnold, 1982. Return to text.
  57. Kopystynski, J.L. and Teisseyre, R., Constitution of the Earth’s Interior, Elsevier, 1984. Return to text.
  58. Wood, B. and Helffrich, G., Internal structure of the earth, Nature 344:1061, 1990. Return to text.
  59. Poirier, J.P., Introduction to the Physics of the Earth’s Interior, Cambridge University Press., 1991. Return to text.
  60. Jacobs, J.A., Deep Interior of the Earth, Chapman Hall, 1992. Return to text.
  61. Green, D.H. and Ringwood, A.E., Mineral assemblages in a model mantle composition, Jour. Geophys. Res. 68:937–945, 1963. Return to text.
  62. Menzies, M.A. (ed.), Continental Mantle, Clarendon Press, Oxford, 1990. Return to text.
  63. Birch, F., Differentiation of the mantle, Bull. Geol. Soc. Amer. 69:483–486, 1958. Return to text.
  64. Bullen, K.E., The Earth’s Density, Chapman and Hall, London, 1975. Return to text.
  65. Green, D.H. and Ringwood, A.E., Mineral assemblages in a model mantle composition, Jour. Geophys. Res. 68:937–945, 1963. Return to text.
  66. Hofmann, A.W., Chemical differentiation of the earth: the relationship between mantle, continental crust, and oceanic crust, Earth Planet. Sci. Lett. 90:297–314, 1988. Return to text.
  67. Bullen, K.E., The variation of density and the ellipticities of strata of equal density within the earth, Mon. Not. Roy. Astron. Soc., Geophys. Suppl. 3:395–401, 1936. Return to text.
  68. Birch, F., Differentiation of the mantle, Bull. Geol. Soc. Amer. 69:483–486, 1958. Return to text.
  69. Bullen, K.E., The Earth’s Density, University of Sydney, London, Chapman and Hall, 1975. Return to text.
  70. Newton, I., Philosophiae Naturalis Principia Mathematica, Roy. Soc. London, 1687. Return to text.
  71. Poirier, J.P., On Poisson’s ratio and composition of the earth’s lower mantle, Phys. Earth Planet. Int. 46:357–368, 1987. Return to text.
  72. Thompson, Sir W. (later Lord Kelvin) and Tait, P.G., Treatise on Natural Philosophy, Cambridge University Press, 1879. Return to text.
  73. Tisserand, F., Traité dé Mecanique Céleste. 2, Paris, 1891. Return to text.
  74. Weichert, E., Über die massenverteilung; in: Innern der Erde. Nachr. Ges. Wiss. Göttingen, Math. Phys. Klasse. pp. 221–243. Return to text.
  75. Klussmann, W., Über das Innere der Erde. Gerl. Beitr. Geophys. 14:1–38, 1915. Return to text.
  76. Haalk, H., Über die lagerung der massen in: Innern der Erde und deren elastizitatskonstanten auf grund der neuesten ergebnisse. Z. angew. Geophys. 1:257–280, 1925. Return to text.
  77. Williamson, E.D. and Adams, L.H., Density distribution in the earth, Jour. Wash. Acad. Sci. 13:413–428, 1923. Return to text.
  78. Bullen, K.E., The variation of density and the ellipticities of strata of equal density within the earth, Mon. Not. Roy. Astron. Soc., Geophys. Suppl. 3:395–401, 1936. Return to text.
  79. Birch, F., Differentiation of the mantle, Bull. Geol. Soc. Amer. 69:483–486, 1958. Return to text.
  80. Ringwood, A.E., A model for the upper mantle, 2, Jour. Geophys. Res. 67:4473–4477, 1962. Return to text.
  81. Ringwood, A.E., Mac Gregor, I.D. and Boyd, F.R., Petrological constitution of the upper mantle, Carnegie Inst. Washington Yearbook 63:147–152, 1964. Return to text.
  82. Ringwood, A.E., Mineralogy of the mantle; in: Hurley, P.M. (ed.), Advances in Earth Science, MIT Press, Cambridge, Massachusetts, pp. 357–399, 1966. Return to text.
  83. Ringwood, A.E. and Major, A., Some high-pressure transformations of geophysical significance, Earth Planet. Sci. Lett. 2:106–110, 1967. Return to text.
  84. Ringwood, A.E., Phase transformations in the mantle, Earth Planet. Sci. Lett. 5:401, 1969. Return to text.
  85. Ringwood, A.E., Composition and evolution of the upper mantle; in: Hart, P.J. (ed.), The earth’s crust and upper mantle, Amer. Geophys. Union, Geophys. Monograph 13:1–17, 1969. Return to text.
  86. Ringwood, A.E. and Green, D.H., Phase transformations and the earth’s interior, Physics of Earth and Planetary Interiors, Special Volume, Symposium, Canberra, Int. Upper Mantle Committee and Aust. Academy of Sci., Upper Mantle Project Sci. Report, no. 26, 6–10 January, 1969. Return to text.
  87. Ringwood, A.E., Composition and Petrology of the Earth’s Mantle, McGraw-Hill Inc., 1975. Return to text.
  88. Akimoto, S., High-pressure research in geophysics: past, present and future; in: Manghnani, M.H. and Sono, Y. (eds), High Pressure Research in Mineral Physics, Washington, D.C., American Geophysical Union, pp. 1–13, 1987. Return to text.
  89. Liebermann, R.C. and Ringwood, A.E., Birch’s law and polymorphic phase transformations, Jour. Geophys. Res. 78:6926–6932, 1973. Return to text.
  90. Rubie, D.C., Mechanisms of phase changes. Nature 338:703-704, 1989. Return to text.
  91. Brearley, A.J., Rubie, D.C. and Ito, E., Mechanism of the transformations between the α, β, and γ polymorphs of Mg2SiO4 at 15 GPa, Phys. Chem. Minerals 18:343–358, 1992. Return to text.
  92. Rubie, D.C. and Brearley, A.J., Phase transitions between β and γ (Mg2Fe)2SiO4 in the earth’s mantle: mechanisms and rheological implications, Science 264:1445-1448, 1994. Return to text.
  93. Birch, F., Density and composition of mantle and core, J. Geophys. Res. 69:4377, 1964. Return to text.
  94. Chung, D.H., Birch’s law: why is it so good? Science 177:261–263, 1972. Return to text.
  95. The Seismic Parameter is defined by Poirier, Ref. 59, p. 14. Return to text.
  96. Bullen, K.E. and Haddon, R.A.W., Earth models based on compressibility theory, Phys. Earth Planet. Int. 1:1–13, 1967. Return to text.
  97. Bullen, K.E., An earth model based on a compressibility-pressure hypothesis, Mon. Not. Roy. Astr. Soc., Geophys. Suppl. 6:50–59, 1950. Return to text.
  98. Clark, S.P. and Ringwood, A.E., Density distribution and constitution of the mantle, Rev. Geophys. 2:35, (Models I and II (? pyrolite and eclogite models), 1964. Return to text.
  99. Press, F., The earth’s interior as inferred from a family of models; in: Robertson, E.C. (ed.), The Nature of the Solid Earth, Symposium held at Harvard University, Cambridge, Massachusetts, 16–18, April, 1970. Return to text.
  100. Haddon, R.A.W. and Bullen, K. E., An earth model incorporating free earth oscillation data, Phys. Earth Planet. Int. 2:35–49, 1969. Return to text.
  101. Wang, C.Y., Density and constitution of the mantle, Jour. Geophys. Res. 75(17), 1970. Return to text.
  102. Wang, C.Y., A simple earth model, Jour. Geophys. Res. 77:4318–4329, 1972. Return to text.
  103. Dziewonski, A.M. and Anderson, D.L., Preliminary earth reference model, Phys., Earth Planet Int., 25:297–356, 1981. Return to text.
  104. Kennett, B.L.N. and Engdahl, E.R., Traveltimes for global earthquake location and phase identification, Geophys. Jour. Int. 105:429–465, 1991. Return to text.
  105. Kennet, B.L.N., Engdahl, E.R. and Buland, R., Constraints on seismic velocities in the earth from traveltimes, Geophys. Jour. Int. 122:108–124, 1995. Return to text.
  106. Jacobs, J.A., The earth’s core in a nutshell, Nature 356:329–331, 1992. Return to text.
  107. Buffett, B.A., Huppert, H.E., Lister, J.R. and Woods, A.W., Analytical model for solidification of the earth’s core, Nature 356, 26 March, 1992. Return to text.
  108. Bassett, W.A., What is in the earth’s core besides iron? Science 266:1662–1663, 1994. Return to text.
  109. Ringwood, A.E., Composition and Petrology of the Earth’s Mantle, McGraw-Hill Inc., 1975. Return to text.
  110. Ito, E. and Yamada, H., Stability relations of silicate spinel, ilmenite and perovskite; in: Akimoto, S. and Manghanni, M.H. (eds), High Pressure Research in Geophysics, Reidel, Dordrecht, pp. 405–419, 1982. Return to text.
  111. Anderson, D.L. and Jordan, T., The composition of the lower mantle, Phys. Earth Planet. Int. 3:23–35, 1970. Return to text.
  112. Liu, L., Phase transformations and the constitution of the upper mantle; in: McElhinny, M.W. (ed.), The Earth: Its Origin, Structure and Evolution, pp. 177–202, 1979. Return to text.
  113. Knittle, E.R., and Jeanloz, R., Synthesis and equation of state of (Mg Fe) SiO3 Perovskite to over 100 GPa, Science 235:668–670, 1987. Return to text.
  114. Anderson, D.L. and Bass, J.D., Transition region of the earth’s upper mantle, Nature 320:322–328, 1986. Return to text.
  115. Bott, M.H.P., The Interior of the Earth: Its Structure, Constitution and Evolution, Edward Arnold, 1982. Return to text.
  116. Ringwood, A.E., Composition and origin of the earth; in: McElhinny, M.W. (ed.), The Earth: Its Origin, Structure and Evolution, Academic Press, London, New York, San Francisco, pp. 1–58, 1979. Return to text.
  117. Ita, J., and Stixrude, L., Petrology, elasticity, and composition of the mantle transition zone, Jour. Geophys. Res. 97:6849–6866, 1992. Return to text.
  118. Gasparik, T., The role of volatiles in the transition zone, Jour. Geophys. Res. 98:4287–4299, 1993. Return to text.
  119. Anderson D.L. and Bass, J.D., Transition region of the earth’s upper mantle, Nature 320:321–327, 1986. Return to text.
  120. Jeanloz, R. and Thompson, A.B., Phase transitions and mantle discontinuities, Rev. Geophys. Space Phys. 21:51–74, 1983. Return to text.
  121. Ringwood, A.E., Mac Gregor, I.D. and Boyd, F.R., Petrological constitution of the upper mantle, Carnegie Inst. Washington Yearbook 63:147–152, 1964. Return to text.
  122. Liu, L., Phase transformations and the constitution of the upper mantle; in: McElhinny, M.W. (ed.), The Earth: Its Origin, Structure and Evolution, pp. 177–202, 1979. Return to text.
  123. Bass, J.D. and Anderson, D.L., Composition of the upper mantle: geophysical tests of two petrological models, Geophys. Res. Lett. 11:237–240, 1984. Return to text.
  124. Duffy, T.S. and Anderson, D.L., Seismic velocities in mantle minerals and the mineralogy of the upper mantle, Jour. Geophys. Res. B94:1895–1912, 1989. Return to text.
  125. Holmes, A., Principles of Physical Geology, Thomas Nelson and Sons, London, 532, 1944. Return to text.
  126. Jeanloz, R., Earth dons a different mantle, Nature 378:130–131, 1995. Return to text.
  127. Dearnley, R., Orogenic fold belts and a hypothesis of earth evolution; in: Ahrens, L.H., Press, F., Runcorn, S.K. and Urey, H.C. (eds), Physics and Chemistry of the Earth, Pergamon Press, 1966. Return to text.
  128. Egyed, L., Determinations of changes in the dimensions of the earth from palaeogeographical data, Nature 178:534, 1956. Return to text.
  129. Egyed, L., A new dynamic conception of the internal constitution of the earth, Geol. Rundsch. 46:101, 1957. Return to text.
  130. Egyed, L. and Stegena, L., Physical background of a dynamic earth model, Z. fur. Geophysik. 24:260, 1958. Return to text.
  131. Maaloe, S. and Steel, R., Mantle composition derived from the composition of lherzolites, Nature 285:321–322, 1980. Return to text.
  132. Hofmann, A.W., Chemical differentiation of the earth: the relationship between mantle, continental crust, and oceanic crust, Earth Planet. Sci. Lett. 90:297–314, 1988. Return to text.
  133. Baer, A.J., Speculations on the evolution of the lithosphere, Precambrian Research 5:249–260, 1977. Return to text.
  134. Taylor, S.R., Not mere scum of the earth, Nature 346:608–609, 1990. Return to text.
  135. Patchett, P.J., Scum of the earth after all, Nature 382:758, 1996. Return to text.
  136. Christensen, N.I. and Mooney, W.D., Seismic velocity structure and composition of the continental crust: a global view, Jour. Geophys. Res. 100(B7)9761–9788, 1995. Return to text.
  137. Wedepohl, K.H., The composition of the continental crust, Geochimica et Cosmochimica Acta, 59(7):1217–1232, 1995. Return to text.
  138. Rudnick, R.L., Making continental crust, Nature 378:571–578, Maaloe and Steel, Ref. 160, 1995. Return to text.
  139. Brown, G.C. and Mussett, A.E., The Inaccessible Earth, George Allen and Unwin, 1981. Return to text.
  140. Cann, J.R., A model for oceanic crustal structure developed, Geophys. J. R. Astr. Soc. 39:169–187, 1974. Return to text.
  141. Emillani, C. (ed.), The Sea 7: The Ocean Lithosphere, Wiley, New York, 1980. Return to text.
  142. Baumgartner, A. and Reichel, E., The World Water Balance, Elsevier Scientific Publishing Co., Amsterdam, 1975. Return to text.
  143. Walker, J.C.G., The earliest atmosphere of the earth, Precambrian Research 17:147–171, 1981. Return to text.
  144. Pollack, J.B. and Yung, Y.K., Origin and evolution of planetary atmospheres, Ann. Rev. Earth Planet. Sci. 8:425–487, 1980. Return to text.
  145. Holland, H.D., Model for the evolution of the earth’s atmosphere, Petrological Studies: A Volume to Honor A. F. Buddington, pp. 447–477, 1962. Return to text.
  146. Hart, R., Dymond, J. and Hogan, L., Preferential formation of the atmosphere-sialic crust system from the upper mantle, Nature 278:156–159, 1979. Return to text.
  147. Whitcomb, J.C. and Morris, H.M., The Genesis Flood, The Presbyterian and Reformed Publishing Co., Philadelphia, Pennsylvania, 1969. Return to text.
  148. Brown (Jr), W.T., In the Beginning, Center for Scientific Creation, 1989. Return to text.
  149. Baumgardner, J.R., Runaway subduction as the driving mechanism for the Genesis Flood; in: The Proceedings of the Third International Conference on Creationism, Creation Science Fellowship Inc., Pittsburgh, Pennsylvania, 1994. Return to text.
  150. Auldaney, Asteroids and their connection to the Flood; in: Proceedings of the Twin-Cities Creation Conference, Northwestern College, Roseville, Minnesota, Twin-Cities Creation Science Association, Northwestern College, Genesis Institute, 1992. Return to text.
  151. Fischer, A giant meteorite impact and rapid continental drift; in: The Proceedings of the Third International Conference on Creationism, Creation Science Fellowship Inc., Pittsburgh, Pennsylvania, 1994. Return to text.
  152. Spencer, Catastrophic impact bombardment surrounding the Genesis Flood; in: The Proceedings of the Third International Conference on Creationism, Creation Science Fellowship Inc., Pittsburgh, Pennsylvania, 1998. Return to text.
  153. Woodward, J., An essay toward a natural history of the earth: and terrestrial bodies, especially minerals: as also of the sea, rivers, and springs, with an account of the universal deluge: and of the effects that it had upon the earth, British Museum Photo Services, (originally published: London, printed for R. Wilkin, 1695), 1972. Return to text.
  154. Morton, G.R., Can the canopy hold water? Creation Res. Soc. Quart 16:164–169, 1979. Return to text.
  155. Johnson, G.L., Global heat balance with a liquid water and ice canopy, Creation Res. Soc. Quart. 23:54–61, 1986. Return to text.
  156. Walters, T.W., Thermodynamic analysis of a condensing vapour canopy, Creation Res. Soc. Quart. 28:122–130, 1991. Return to text.
  157. Morton, G.R., The Flood on an expanding earth, Creation Res. Soc. Quart. 19:219–224, 1983. Return to text.
  158. Costa, U.R., Fyfe, W.S., Kerrich, R. and Nesbitt, H.W., Archaean hydrothermal talc and evidence for high ocean temperatures, Chem. Geol. 30:341–349, 1980. Return to text.
  159. Costa, U.R., Fyfe, W.S., Kerrich, R. and Nesbitt, H.W., Is ocean formation synchronous with the first preservation of crust? Spec. Publs. Geol. Soc. Aust. 7:453–456, 1981. Return to text.
  160. Hanks, T.J. and Anderson, D.L., The early thermal history of the earth, Phys. Earth Planet. Int. 2:19–29, 1969. Return to text.
  161. Green, D.H., Magmatic activity as the major process in chemical evolution of the earth’s crust and upper mantle, Tectonophysics 13:47–71, 1972. Return to text.
  162. Hargraves, R.B. (ed.), Physics of Magmatic Processes, Princeton University Press, New Jersey, 1980. Return to text.
  163. Hofmeisner, A.M., Effect of a hadean terrestrial magma ocean on crust and mantle evolution, Jour. Geophys. Res. 88:4963–4983, 1983. Return to text.
  164. Ohtani, E., Generation of komatiite magma angravitational differentiation in the deep upper mantle, Earth Planet. Sci. Lett. 67:261–272, 1984. Return to text.
  165. Ohtani, E., The primordial magma ocean and it’s implication for stratification of the mantle, Phys. Earth Planet. Int. 38:70–80, 1985. Return to text.
  166. Carmichael, I.S.E. and Eugster, H.P. (eds), Rev. Mineral. 17:467–499. Return to text.
  167. Stevenson, D.J., Stalking the magma ocean, Nature 355:301, 23 1992. Return to text.
  168. Xie, Q. and Kerrich, R., Silicate-perovskite and majorite signature komatiites from the archean abitibi greenstone belt: implications for early mantle differentiation and stratification, Jour. Geophys. Res. 99(B8):15,799–15,812, 1994. Return to text.
  169. Nielson, J.E., and Wilshire, H.G., Magma transport and metasomatism in the mantle: a critical review of current geochemical models, Amer. Mineral. 78:1117–1134, 1993. Return to text.
  170. McKenzie and Bickle, The volume and composition of melt generated by extension of the lithosphere, Journal of Petrology 29(3):625–679, 1988. Return to text.
  171. Asimow, P.D., Hirschmann, M.M., Ghiorso, M.S., O’Hara, M.J., and Stolper, E.M., The effect of pressure-induced solid-solid phase transitions on decompression melting of the mantle, Geochimica et Cosmochimica Acta. 59(21):4489–4506, 1995. Return to text.
  172. Wyllie, P.J., The role of water in magma generation and initiation of diapiric uprise in the mantle, Jour. Geophys. Res. 76:1328–1338, 1971. Return to text.
  173. Gilluly, J., The water content of magmas, Am. Jour. Sci., Fifth Series, Vol. XXXIII (198) pp. 430–441, 1937. Return to text.
  174. Hamilton, D.L., Burnham, C.W. and Osborn, E.F., Solubility of water and effects of oxygen fugacity and water content of crystallisation in mafic magmas, Jour. Petrol. 5:21–39, 1964. Return to text.
  175. Burnham, C.W., Hydrothermal fluids at the magmatic stage; in: Barnes, H.L. (ed.), Geochemistry of Hydrothermal Ore Deposits, New York, Holt, Rinehart and Winston, pp. 34–76, 1967. Return to text.
  176. Hill, R.E.T. and Boettcher, A.L., water in the earth’s mantle: melting curves of basalt-water and basalt-water-carbon dioxide, Science 167:980–981, 1970. Return to text.
  177. Kushiro, I., Effect of water on the composition of magmas formed at high pressures, Jour. Petrol. 13(2):311–334, 1972. Return to text.
  178. Wyllie, P.J., Magmas and volatile components, Amer. Mineral. 64:469–500, 1979. Return to text.
  179. Ahrens, T.J., Water storage in the mantle, Nature 342:122–123, 1989. Return to text.
  180. Persikov. E.S., Zharikov, V.A., Bukhtiyarov, P.G. and Pol’skoy, S.F., The effect of volatiles on the proprerties of magmatic melts, Eur. Jour. Mineral. 2:621–642, 1990. Return to text.
  181. Candela. P.A., Physics of aqueous phase evolution in plutonic environments, Amer. Mineral. 76:1081–1091, 1991. Return to text.
  182. Gallagher, K. and Hawkesworth, C., Dehydration melting and the generation of continental Flood basalts, Nature 358:57–59, 1992. Return to text.
  183. Fanale, F.P., A case for catastrophic early degassing of the earth, Chem. Geol. 8:79–105, 1971. Return to text.
  184. Rubey, W.W., Geologic history of sea water, Bull. Geol. Soc. Amer. 62:1111–1147, 1951. Return to text.
  185. Holland, H.D., Origins of breathable air, Nature 347:17, 1990. Return to text.
  186. Bell, D.R. and Rossman, G.R., Water in earth’s mantle: the role of nominally anhydrous minerals, Science 255:1391–1397, 1992. Return to text.
  187. Akimoto, S. and Akaogi, M., The system Mg2SiO2-MgO-H2O at high pressures and temperatures— possible hydrous magnesian silicates in the mantle transition zone, Physics Earth Planet. Int. 23:268–275, 1980. Return to text.
  188. Kato, T., and Kumazaw, M., Stability of phase B, a hydrous magnesium silicate, to 2300oC at 20 GPA, Geophys. Res. Lett. 12(8):534–535, 1985. Return to text.
  189. Smyth, J.R., B-Mg2SiO4—A potential host for water in the mantle? Amer. Mineral. 72:1051–1055, 1987. Return to text.
  190. Smyth, J.R., A crystallographic model for hydrous wadsleyite (B-Mg2SiO4): an ocean in the earth’s interior? Amer. Mineral. 79: 1021–1024, 1994. Return to text.
  191. Finger, L.W., Ko, J., Hazen, R.M., Gasparik, T., Hemley, R.J., Prewitt, C.T. and Weidner, D.J., Crystal chemistry of phase B and an anhydrous analogue: implications for water storage in the upper mantle, Nature 341:140–142, 1989. Return to text.
  192. Thompson, A.B., Water in the earth’s upper mantle, Nature 358:295–302, 1992. Return to text.
  193. Bai, Q. and Kohlstedt, D.L., Substantial hydrogen solubility in olivine and implications for water storage in the mantle, Nature 357:672–674, 1992. Return to text.
  194. Hemley, R.J., Turning off the water, Nature 378:14–15, 1995. Return to text.