पृथ्वी और अंतरिक्ष विज्ञान · Book 4 · स्नातक वर्ष 2

University Earth and Space Sciences — Year 2

University Earth and Space Sciences — Year 2 · स्नातक वर्ष 2

16Sedimentary Basins Compared

Off the coast of the eastern United States, beneath the continental shelf, the Baltimore Canyon Trough holds at least 14 km14\,\mathrm{km} of sedimentary rock. A borehole drilled into such a pile reads its history backwards: each unit it crosses was once the sea floor, at a depth that fossils and sediments record, and has since been buried and squeezed. The depth of every dated surface is a point on a curve of sinking. Yet most of the sinking was caused by the weight of the sediment itself. To learn what made the basin, that weight has to be taken off, layer by layer. This chapter shows how, and what the result says about the lithosphere.

You already know

From the Year 1 volume: sedimentary basin, subsidence and tectonic subsidence, accommodation, eustasy; compaction, decompaction and Athy’s law, the solid thickness of a layer; the sediment load, which amplifies subsidence by (ρm−ρw)/(ρm−ρs)(\rho_m - \rho_w)/(\rho_m - \rho_s); Airy isostasy; the lithosphere and its geotherm; continental rifts and passive margins. From the physics volumes: the heat equation and its Fourier solutions. From Chapter 13: the foreland basin, flysch and molasse.

A semi-submersible drilling rig in the North Sea. The boreholes drilled from such rigs give the thicknesses, ages and rock types from which the subsidence of a basin is reconstructed. Photograph Erik Christensen, 2005, CC BY-SA 3.0.
A semi-submersible drilling rig in the North Sea. The boreholes drilled from such rigs give the thicknesses, ages and rock types from which the subsidence of a basin is reconstructed. Photograph Erik Christensen, 2005, CC BY-SA 3.0.

16.1 Basins and what makes them sink

The Year 1 volume told basins apart by where they lie. Here they are told apart by what drives their subsidence.

Definition 16.1 (Intracratonic, rift and passive-margin basins)

An intracratonic basin is a broad, round or oval basin in the interior of a continent, far from plate boundaries, that subsides slowly over very long times without major faulting. A rift basin is a basin bounded by normal faults in a continental lithosphere being stretched; its subsidence follows the stretching and then the cooling of the lithosphere. A passive-margin basin is the wedge of sediment, thickening oceanwards, that accumulates on a continental margin after break-up, over the thinned crust of the old rift.

The foreland basin of Chapter 13 completes the list, and the basins that open along strike-slip faults are left to the Year 3 volume. Three mechanisms make the floor of a basin sink:

  • mechanical thinning: when the crust is stretched and thinned by faults, light crust is replaced by denser mantle and the surface goes down to restore isostasy;
  • thermal contraction: a lithosphere that has been heated, by stretching or from below, cools afterwards, grows denser and sinks, slowly, over tens of millions of years;
  • loading: the weight of a thrust belt, or of the sediment itself, bends the lithosphere down; that flexure belongs to the Year 3 volume, and the local, Airy form of the sediment load is enough here.

Rift basins combine the first two, passive margins inherit the second from their rift stage, foreland basins are made by the third. Intracratonic basins are the least understood.

Four families of basins in schematic sections across the lithosphere (not to scale; sediment in yellow, continental crust in orange, oceanic crust in grey). The vertical exaggeration is large: real basins are hundreds of kilometres wide and a few to fifteen kilometres deep.
Four families of basins in schematic sections across the lithosphere (not to scale; sediment in yellow, continental crust in orange, oceanic crust in grey). The vertical exaggeration is large: real basins are hundreds of kilometres wide and a few to fifteen kilometres deep.

The rift basins of the North Sea are the classic case of the first two mechanisms. Grabens formed there from the Triassic, and the last major stretching lasted from the Middle Jurassic to the mid-Cretaceous; the faults then fell quiet, and the middle of the basin went on sinking as a broad saucer, filled by chalks, sandstones and, through most of the Tertiary, shales and mudstones. Loaded by water alone, its basement would have sunk a further 1100 to 1400 m1400\,\mathrm{m} in the middle and 600 to 700 m700\,\mathrm{m} on the flanks after the faulting had stopped.

The passive margin of the eastern United States shows the same sinking on a larger scale. Seismic profiles across the shelf show more than 14 km14\,\mathrm{km} of Mesozoic and younger rock in the Baltimore Canyon Trough and 8 km8\,\mathrm{km} in the Georges Bank basin, in units that thicken oceanwards. Its Jurassic depocentres follow the structures of the rift and the zones of its later thermal subsidence.

The Michigan basin is the type of the intracratonic basins. Ovate, some hundreds of thousands of square kilometres in area, it holds more than 4 km4\,\mathrm{km} of Phanerozoic sediment laid down in distinct episodes over some 500 million years, with little faulting. Its episodes of faster subsidence coincide with those of other basins in the interiors of North America and other continents, which suggests a cause larger than one basin. Backstripping more than 57 000 well logs shows a long-lived, nearly circular pattern of subsidence, which the authors suggest mantle downwelling could explain, interrupted at the times of two orogenies on the distant margin of the continent. Why intracratonic basins sink is still debated.

16.2 Subsidence curves

A well, or a measured section, gives for each unit its present depth, its rock type and its age, read from fossils or from correlation. With the depth of water in which each unit was laid down, read from its fossils and sedimentary structures, it gives the history of the basin.

Definition 16.2 (Subsidence curve)

A subsidence curve of a basin at a site is the graph of the depth of a reference surface, usually the basement or the base of the oldest unit, below sea level, against time. The total subsidence curve uses the sediment thickness as it was at each time, plus the water depth; the tectonic subsidence curve replaces the sediment by water and removes its isostatic effect.

A unit is never as thick in the past as it is today. Buried, it lost porosity; its grains have not changed, but its water has been squeezed out. The Year 1 volume wrote the porosity at depth zz as Athy’s law, ϕ(z)=ϕ0 e−z/c\phi(z) = \phi_0\,e^{-z/c}, and found the solid thickness of a layer between z1z_1 and z2z_2,

Ts=(z2−z1)−ϕ0c(e−z1/c−e−z2/c),T_s = (z_2 - z_1) - \phi_0 c\left(e^{-z_1/c} - e^{-z_2/c}\right),

which stays the same when the layer moves. To decompact a unit to a shallower position, with its top now at z1′z_1', one looks for the base z2′z_2' that holds the same solid thickness. The equation has no closed solution, but the fixed-point iteration

z2′←z1′+Ts+ϕ0c(e−z1′/c−e−z2′/c)z_2' \leftarrow z_1' + T_s + \phi_0 c\left(e^{-z_1'/c} - e^{-z_2'/c}\right)

starting from z2′=z1′+Tsz_2' = z_1' + T_s converges in a few steps. The mass per unit area of the layer is that of its grains plus that of its pore water,

m=ρgTs+ρw (z2−z1−Ts),m = \rho_g T_s + \rho_w\,(z_2 - z_1 - T_s),

with ρg\rho_g the density of the grains; dividing the mass of a column by its thickness gives its mean density ρˉs\bar\rho_s.

For the lithologies used in this chapter, sand, shale, chalk and shaly sand, the table below gives the constants of Sclater and Christie (1980), as bundled in an open-source program. Sand keeps its porosity deepest, chalk loses it fastest.

lithologygrain density (kg m−3\mathrm{kg}\,\mathrm{m}^{-3})surface porosity ϕ0\phi_0decay length cc (m\mathrm{m})
sand26500.493704
shale27000.631960
chalk27100.701408
shaly sand26800.562564

16.3 Backstripping

A total subsidence curve mixes two causes: whatever made the basin, and the weight of what filled it. Separating them is the purpose of the next procedure, the central tool of basin analysis.

Definition 16.3 (Backstripping)

Backstripping is the reconstruction of the tectonic subsidence of a basin through time: the units of a well are removed one by one, from the youngest, the remaining ones are decompacted at each step, and the isostatic effect of the sediment and water load is removed to give the depth at which the basement would have stood under water alone.

The last step is an isostatic balance. The Year 1 volume made it for a basin filled to sea level; the general case adds the depth of water and the level of the sea.

Proposition 16.4 (Airy backstripping)

Let a basin hold, at some time, a sediment column of thickness SS and mean density ρˉs\bar\rho_s, under a water depth WdW_d, while the sea stood ΔSL\Delta_{SL} above its present level. In local isostasy over a mantle of density ρm\rho_m, with water of density ρw\rho_w, the tectonic subsidence at that time, measured from present sea level, is

Y=S ρm−ρˉsρm−ρw+Wd−ΔSL ρmρm−ρw.Y = S\,\frac{\rho_m - \bar\rho_s}{\rho_m - \rho_w} + W_d - \Delta_{SL}\,\frac{\rho_m}{\rho_m - \rho_w}.

Proof. Compare two columns over the same lithosphere, down to a depth of compensation below both. In the first, water of depth WdW_d lies over the sediment of thickness SS; in the second, water alone fills a basin of depth Y′Y' below the same sea surface. Their masses are equal:

ρwWd+ρˉsS+ρm (d−Wd−S)=ρwY′+ρm (d−Y′),\rho_w W_d + \bar\rho_s S + \rho_m\,(d - W_d - S) = \rho_w Y' + \rho_m\,(d - Y'),

with dd the common depth of the compensation level below the sea surface. Hence Y′(ρm−ρw)=S(ρm−ρˉs)+Wd(ρm−ρw)Y'(\rho_m - \rho_w) = S(\rho_m - \bar\rho_s) + W_d(\rho_m - \rho_w), which is the first two terms. If the sea stood ΔSL\Delta_{SL} higher than today, that extra water is no part of the basin’s own subsidence: removing it, the water-loaded basement rises by ΔSLρw/(ρm−ρw)\Delta_{SL}\rho_w/(\rho_m - \rho_w), and its depth below today’s sea level is smaller again by ΔSL\Delta_{SL}; together, ΔSL ρm/(ρm−ρw)\Delta_{SL}\,\rho_m/(\rho_m - \rho_w). ∎

With ρm=3330 kg m−3\rho_m = 3330\,\mathrm{kg}\,\mathrm{m}^{-3} and ρw=1030 kg m−3\rho_w = 1030\,\mathrm{kg}\,\mathrm{m}^{-3}, a column of sediment of mean density 2300 kg m−32300\,\mathrm{kg}\,\mathrm{m}^{-3} counts for 1030/2300=0.451030/2300 = 0.45 of its thickness in tectonic subsidence: more than half of the thickness of a basin’s fill is made room for by its own weight. A sea 100 m100\,\mathrm{m} higher than today lowers the result by 145 m145\,\mathrm{m}. The water depth and the past sea level are the weakest data: fossils give a range of water depths, often hundreds of metres wide on the slope, and the tectonic subsidence inherits that range.

Method 16.5 (Backstripping a well)

  1. List the units from the base, with the present depths of their tops and bases, their lithology constants (ρg,ϕ0,c)(\rho_g, \phi_0, c), the ages of their tops, and the water depth at each of those ages.
  2. Compute the solid thickness TsT_s of each unit from its present depths.
  3. For the age of the top of unit kk, remove all the younger units. Put the top of unit kk at depth zero and decompact it; put each older unit, in turn, under the one above it and decompact it.
  4. Add up the thicknesses to give SS, and the masses to give the mean density ρˉs=∑m/S\bar\rho_s = \sum m / S.
  5. Apply Proposition 16.4 to obtain YY; the total subsidence is S+WdS + W_d.
  6. Repeat for each age, from the oldest to the present; plot YY and S+WdS + W_d against age.

The figure below shows the result for an invented well in a rift basin. Four units were cored: a syn-rift sand laid down while faults were active, between 165 and 150 Ma150\,\mathrm{Ma}; then a shale, a chalk and a shaly sand. Today, no decompaction is needed: the basement lies at 6030 m6030\,\mathrm{m} and the column has a mean density of 2358 kg m−32358\,\mathrm{kg}\,\mathrm{m}^{-3}, so that Y=2648 mY = 2648\,\mathrm{m} under 100 m100\,\mathrm{m} of water. At 150 Ma150\,\mathrm{Ma}, the sand alone, decompacted at the surface, was 2239 m2239\,\mathrm{m} thick, with a mean density of 2055 kg m−32055\,\mathrm{kg}\,\mathrm{m}^{-3}: under 200 m200\,\mathrm{m} of water, Y=1441 mY = 1441\,\mathrm{m}. The total subsidence is more than twice the tectonic one, and the tectonic curve shows a fast first stage, then a slowing sinking: the shape of a rift.

Backstripping of an invented well with four units (data in the weekend problem): basement depth with the sediment as it was at each time, and tectonic subsidence, with the curve of the stretching model fitted to the subsidence at the end of rifting ().
Backstripping of an invented well with four units (data in the weekend problem): basement depth with the sediment as it was at each time, and tectonic subsidence, with the curve of the stretching model fitted to the subsidence at the end of rifting (Section 16.4).
Backstripping the invented well at 150\, Ma (depths to scale): the four units today; the sand alone at the end of rifting, decompacted at the surface under 200\, m of water; the same lithosphere loaded by water alone, whose basement stands higher because water is lighter than sediment.
Backstripping the invented well at 150 Ma150\,\mathrm{Ma} (depths to scale): the four units today; the sand alone at the end of rifting, decompacted at the surface under 200 m200\,\mathrm{m} of water; the same lithosphere loaded by water alone, whose basement stands higher because water is lighter than sediment.

16.4 The stretching model

Why does a rift basin sink first fast and then slowly? In 1978 D. McKenzie proposed a model so simple that its parameters can be fitted to a single well.

Definition 16.6 (Stretching model; stretching factor; syn-rift and post-rift subsidence)

The stretching model of a basin represents rifting as an instantaneous, uniform stretching of the whole lithosphere by pure shear: crust and mantle lithosphere are thinned by the same factor, and hot asthenosphere rises passively to fill the space, after which the lithosphere cools. The stretching factor β\beta is the ratio of the width of the stretched region after stretching to its width before, equal to the ratio of the initial to the final thickness of the crust. The subsidence produced during stretching is the syn-rift subsidence; that produced afterwards by the cooling of the lithosphere is the post-rift subsidence, or thermal subsidence.

Stretching in nature takes a finite time, millions of years. Later versions of the model let it last, but as long as it is not too slow the simple instantaneous version gives the subsidence roughly but correctly, since after the stretching the cooling proceeds in much the same way.

The stretching model (not to scale): a lithosphere of thickness a with a crust t_c is stretched to  times its width; crust and mantle lithosphere thin by , the asthenosphere rises, and the surface sinks by the syn-rift subsidence S_i under water. Here = 2.
The stretching model (not to scale): a lithosphere of thickness aa with a crust tct_c is stretched to β\beta times its width; crust and mantle lithosphere thin by β\beta, the asthenosphere rises, and the surface sinks by the syn-rift subsidence SiS_i under water. Here β=2\beta = 2.

Proposition 16.7 (Subsidence in the stretching model)

Let a lithosphere of thickness aa, with a crust of thickness tct_c, have a linear geotherm from 00 at the surface to the temperature T1T_1 of the asthenosphere at its base; let crust and mantle have densities ρc(1−αT)\rho_c(1 - \alpha T) and ρm(1−αT)\rho_m(1 - \alpha T), with α\alpha the thermal expansion coefficient. If it is stretched instantaneously by β\beta and the basin filled with water of density ρw\rho_w:

  1. the syn-rift subsidence is

    Si=a(1−1β)[(ρm−ρc)tca(1−αT1tc2a)−αT1ρm2]ρm(1−αT1)−ρw;S_i = \frac{a\left(1 - \dfrac{1}{\beta}\right)\left[(\rho_m - \rho_c)\dfrac{t_c}{a} \left(1 - \dfrac{\alpha T_1 t_c}{2a}\right) - \dfrac{\alpha T_1 \rho_m}{2}\right]} {\rho_m(1 - \alpha T_1) - \rho_w};
  2. the post-rift subsidence, a time tt after stretching, is, to the first term of a series,

    St=E0 βπsin⁡πβ(1−e−t/τ),E0=4aρmαT1π2(ρm−ρw),τ=a2π2κ,S_t = E_0\,\frac{\beta}{\pi}\sin\frac{\pi}{\beta}\left(1 - e^{-t/\tau}\right),\qquad E_0 = \frac{4a\rho_m\alpha T_1}{\pi^2(\rho_m - \rho_w)},\qquad \tau = \frac{a^2}{\pi^2\kappa},

    where κ\kappa is the thermal diffusivity and τ\tau is the thermal time constant of the lithosphere.

Proof. (1) Compare the column before stretching with the column just after, down to the old base of the lithosphere, at depth aa below the surface before stretching. Before, the crust of thickness tct_c and the mantle lithosphere are at temperatures T=T1z/aT = T_1 z/a; after, both are thinner by β\beta and their temperatures run from 00 to T1T_1 over a/βa/\beta, so that a point at depth z′z' below the base of the water has T=T1βz′/aT = T_1\beta z'/a; beneath, the asthenosphere at T1T_1 has density ρm(1−αT1)\rho_m(1 - \alpha T_1); above, water fills the depth SiS_i. The mass of a layer of density ρ(1−αT)\rho(1 - \alpha T) in which TT grows linearly from TaT_a to TbT_b is ρ h (1−α(Ta+Tb)/2)\rho\,h\,(1 - \alpha(T_a + T_b)/2). Before, the column holds

ρctc(1−αT1tc2a)+ρm(a−tc)(1−αT1(a+tc)2a);\rho_c t_c\left(1 - \frac{\alpha T_1 t_c}{2a}\right) + \rho_m (a - t_c)\left(1 - \frac{\alpha T_1 (a + t_c)}{2a}\right);

after, it holds the water, the thinned crust and mantle lithosphere, and the asthenosphere that fills the rest of the depth aa:

ρwSi+ρctcβ(1−αT1tc2a)+ρm(a−tc)β(1−αT1(a+tc)2a)+ρm(1−αT1)(a−Si−aβ).\rho_w S_i + \frac{\rho_c t_c}{\beta}\left(1 - \frac{\alpha T_1 t_c}{2a}\right) + \frac{\rho_m (a - t_c)}{\beta}\left(1 - \frac{\alpha T_1 (a + t_c)}{2a}\right) + \rho_m(1 - \alpha T_1)\left(a - S_i - \frac{a}{\beta}\right).

Isostasy makes the two equal. Collecting the terms in SiS_i on one side and the factor (1−1/β)(1 - 1/\beta) on the other, and expanding, gives the formula; the algebra is Exercise 16.11.

(2) After stretching, the plate cools by conduction between a surface held at 00 and a base held at T1T_1, towards the linear profile it started from. The excess temperature solves the heat equation with zero values at top and base, and so is a sum of terms bnsin⁡(nπz/a) e−n2κπ2t/a2b_n\sin(n\pi z/a)\,e^{-n^2\kappa\pi^2 t/a^2}; each cools with its own time, τ/n2\tau/n^2. The heat lost makes the column contract by α∫ΔT dz\alpha\int \Delta T\,\mathrm{d}z, and the extra water that fills the space sinks it further by the factor ρm/(ρm−ρw)\rho_m/(\rho_m - \rho_w). Only odd terms contribute; keeping the first one, whose coefficient is computed from the initial profile, gives the expression. The others cool nine or more times faster, and after about ten million years they shift the subsidence by a nearly constant amount, less than 100 m100\,\mathrm{m} for β\beta from 1.2 to 4 with the values below. ∎

The parameters of McKenzie’s paper are a=125 kma = 125\,\mathrm{km}, T1=1333 ∘CT_1 = 1333\,{}^{\circ}\mathrm{C}, α=3.28×10−5 K−1\alpha = 3.28 \times 10^{-5}\,\mathrm{K}^{-1}, κ=8×10−7 m2 s−1\kappa = 8 \times 10^{-7}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}, ρm=3330 kg m−3\rho_m = 3330\,\mathrm{kg}\,\mathrm{m}^{-3} (at 0 ∘C0\,{}^{\circ}\mathrm{C}), ρc=2800 kg m−3\rho_c = 2800\,\mathrm{kg}\,\mathrm{m}^{-3}; with sea water at 1030 kg m−31030\,\mathrm{kg}\,\mathrm{m}^{-3} they give τ=62.7 Myr\tau = 62.7\,\mathrm{Myr} and E0=3207 mE_0 = 3207\,\mathrm{m}. With a crust of 35 km35\,\mathrm{km}, the syn-rift subsidence is Si=4334 m×(1−1/β)S_i = 4334\,\mathrm{m} \times (1 - 1/\beta).

Water-loaded subsidence of the stretching model for four stretching factors, with a 35\, km crust and the parameters of the text: the syn-rift step at t = 0, then the post-rift curve, which has reached 63\,\% of its final value at t =.
Water-loaded subsidence of the stretching model for four stretching factors, with a 35 km35\,\mathrm{km} crust and the parameters of the text: the syn-rift step at t=0t = 0, then the post-rift curve, which has reached 63 %63\,\% of its final value at t=τt = \tau.

Three features of the model carry to real basins.

  • The syn-rift step grows with β\beta, and so does the post-rift subsidence; but their ratio changes little, so that both parts point to the same β\beta if the model holds.
  • The time scale of the post-rift subsidence does not depend on β\beta: it is set by the thickness of the lithosphere alone. After τ\tau, 63 %63\,\% of the thermal subsidence is done; after 3τ3\tau, about 95 %95\,\%. A rift that stopped two hundred million years ago hardly sinks any more.
  • The syn-rift term is a competition between the light crust thinned, which makes the surface sink, and the hot asthenosphere risen, which buoys it up. With a thin crust the second wins and stretching raises the surface (Exercise 16.10).

To fit a well, the tectonic subsidence at the end of rifting gives SiS_i, hence β=1/(1−Si/4334 m)\beta = 1/(1 - S_i/4334\,\mathrm{m}) for a 35 km35\,\mathrm{km} crust; the post-rift curve is then predicted and compared with the rest of the backstripped points. In the invented well, Si=1441 mS_i = 1441\,\mathrm{m} gives β=1.50\beta = 1.50, and the curve passes within a few metres of the later points (figure in Section 16.3). Real basins are rarely so obliging. In the central North Sea, stretching of 50 to 100 %100\,\% in the middle, β\beta from 1.5 to 2, reproduces the amplitude and rate of the post-rift subsidence. On the margin of the eastern United States, only one segment, the Long Island Platform, has an early post-rift fill as thick as uniform stretching predicts; in the Georges Bank Basin and the Baltimore Canyon Trough the fill is 1.5 to 3 times thicker, and other causes must be at work.

16.5 Basins compared

The table below gathers the four families. The curves differ in shape and in time scale, and a subsidence curve is often the first clue to the nature of a basin buried under younger rocks.

basinexamplethickness and durationshape of the tectonic subsidence curve
riftcentral North Seagrabens from the Triassic; last stretching Middle Jurassic to mid-Cretaceous; 1.1 to 1.4 km1.4\,\mathrm{km} of water-loaded post-rift sinkinga fast syn-rift step, then an exponential slowing with τ\tau of tens of Myr
passive marginBaltimore Canyon Troughmore than 14 km14\,\mathrm{km} since the Jurassicas a rift, with a large post-rift part; the fill thickens oceanwards
forelandNorth Alpine Molassemore than 4 km4\,\mathrm{km} at the thrust front, late Eocene to late Miocenedeepest against the belt and migrating with it; its inner part finally overridden by the thrusts
intracratonicMichiganmore than 4 km4\,\mathrm{km} in episodes over some 500 Myrslow, with episodes of faster sinking shared by distant basins

A foreland basin sinks under a load that moves towards it: the basin migrates with the belt, the Alpine one by at least 210 km210\,\mathrm{km} over the European craton, and its inner part is finally overridden and carried by the thrusts, as the Subalpine Molasse was in Chapter 13. A rift slows down as it cools, whatever its stretching. An intracratonic basin sinks slowly and long, in pulses; neither stretching nor a load explains it well, which is why it remains a research question.

In the lab — Subsidence analysis

Basin analysts do the work of the method box with programs. One open-source program, for instance, reads a drill site as a list of units with their ages, depths and lithologies, and a table of lithologies with their grain density, surface porosity and decay length. Its backstripping module decompacts the units and returns the tectonic subsidence at each age; since a palaeo water depth is known only as a range, the user gives a minimum and a maximum and the program returns the two subsidences and their mean. A second module works the other way: from a model of tectonic subsidence it predicts the water depths of the past, which can be checked against the fossils. Analysts then fit stretching factors, test sea-level curves, and map the subsidence of a whole basin from hundreds or thousands of wells.

Exercises

Data for the exercises, unless stated otherwise: ρm=3330 kg m−3\rho_m = 3330\,\mathrm{kg}\,\mathrm{m}^{-3}, ρc=2800 kg m−3\rho_c = 2800\,\mathrm{kg}\,\mathrm{m}^{-3}, ρw=1030 kg m−3\rho_w = 1030\,\mathrm{kg}\,\mathrm{m}^{-3}; stretching model with a=125 kma = 125\,\mathrm{km}, T1=1333 ∘CT_1 = 1333\,{}^{\circ}\mathrm{C}, α=3.28×10−5 K−1\alpha = 3.28 \times 10^{-5}\,\mathrm{K}^{-1}, κ=8×10−7 m2 s−1\kappa = 8 \times 10^{-7}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}, τ=62.7 Myr\tau = 62.7\,\mathrm{Myr}, E0=3207 mE_0 = 3207\,\mathrm{m}; a 35 km35\,\mathrm{km} crust gives Si=4334 m×(1−1/β)S_i = 4334\,\mathrm{m}\times(1 - 1/\beta); lithology constants in the table of Section 16.2.

Exercise 16.1 ★

Name the family of each basin and the main cause of its subsidence: (a) the Michigan basin; (b) the central North Sea; (c) the Baltimore Canyon Trough; (d) the North Alpine Molasse; (e) the Indo-Gangetic plain in front of the Himalaya.

Solution

Solution of Exercise 16.1.

(a) Intracratonic: slow subsidence in pulses over hundreds of millions of years, without major faulting; its cause is debated. (b) Rift: mechanical thinning of the crust during stretching, then thermal contraction as the lithosphere cools. (c) Passive margin: the thermal subsidence inherited from the rift stage, amplified by the load of a thick sediment wedge. (d) and (e) Foreland: the lithosphere bent down by the load of the thrust belt, the Alps and the Himalaya.

Exercise 16.2 ★

A basin holds 3.0 km3.0\,\mathrm{km} of sediment of mean density 2300 kg m−32300\,\mathrm{kg}\,\mathrm{m}^{-3}. (a) Find its tectonic subsidence if the sediment reaches sea level. (b) And if 200 m200\,\mathrm{m} of water lie on top? (c) What fraction of the thickness of the fill is due to the load of the fill itself?

Solution

Solution of Exercise 16.2.

(a) Y=3000×(3330−2300)/(3330−1030)=3000×1030/2300=1343 mY = 3000\times(3330 - 2300)/(3330 - 1030) = 3000\times1030/2300 = 1343\,\mathrm{m}. (b) 1343+200=1543 m1343 + 200 = 1543\,\mathrm{m}. (c) Without its load, the basement would lie at 1343 m1343\,\mathrm{m}: 1−1343/3000=55 %1 - 1343/3000 = 55\,\% of the thickness is made room for by the load.

Exercise 16.3 ★

Seismic refraction shows that a 35 km35\,\mathrm{km} crust has been thinned to 25 km25\,\mathrm{km} in a rift. (a) What is β\beta? (b) How thick is the lithosphere just after stretching? (c) What is the syn-rift subsidence under water?

Solution

Solution of Exercise 16.3.

(a) β=35/25=1.4\beta = 35/25 = 1.4. (b) 125/1.4=89.3 km125/1.4 = 89.3\,\mathrm{km}. (c) Si=4334×(1−1/1.4)=1238 mS_i = 4334\times(1 - 1/1.4) = 1238\,\mathrm{m}.

Exercise 16.4 ★

(a) Check that τ=62.7 Myr\tau = 62.7\,\mathrm{Myr} (1 Myr=3.156×1013 s1~\text{Myr} = 3.156 \times 10^{13}\,\mathrm{s}). (b) Some programs use κ=1×10−6 m2 s−1\kappa = 1 \times 10^{-6}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}: what is τ\tau then? (c) What would it be for a lithosphere 100 km100\,\mathrm{km} thick, with κ=8×10−7 m2 s−1\kappa = 8 \times 10^{-7}\,\mathrm{m}^{2}\,\mathrm{s}^{-1}? (d) What fraction of the post-rift subsidence is done after τ\tau, and after 3τ3\tau?

Solution

Solution of Exercise 16.4.

(a) τ=(1.25×105)2/(π2×8×10−7)=1.979×1015 s\tau = (1.25\times10^{5})^2/(\pi^2\times8\times10^{-7}) = 1.979 \times 10^{15}\,\mathrm{s}, that is 1.979×1015/3.156×1013=62.7 Myr1.979\times10^{15}/3.156\times10^{13} = 62.7\,\mathrm{Myr}. (b) 62.7×0.8=50.2 Myr62.7\times0.8 = 50.2\,\mathrm{Myr}. (c) 62.7×(100/125)2=40.1 Myr62.7\times(100/125)^2 = 40.1\,\mathrm{Myr}. (d) 1−e−1=63 %1 - e^{-1} = 63\,\%; 1−e−3=95 %1 - e^{-3} = 95\,\%.

Exercise 16.5 ★★

A shale unit lies today between 1000 m1000\,\mathrm{m} and 2000 m2000\,\mathrm{m}. (a) Find its porosity at the top and at the base. (b) Find its solid thickness. (c) Find its mass per unit area and its mean density, the pores being full of water.

Solution

Solution of Exercise 16.5.

(a) 0.63 e−1000/1960=0.3780.63\,e^{-1000/1960} = 0.378; 0.63 e−2000/1960=0.2270.63\,e^{-2000/1960} = 0.227. (b) Ts=1000−0.63×1960×(0.6004−0.3605)=704 mT_s = 1000 - 0.63\times1960\times(0.6004 - 0.3605) = 704\,\mathrm{m}. (c) m=2700×704+1030×296=2.206×106 kg m−2m = 2700\times704 + 1030\times296 = 2.206 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}; ρˉ=2206 kg m−3\bar\rho = 2206\,\mathrm{kg}\,\mathrm{m}^{-3}.

Exercise 16.6 ★★

The shale of Exercise 16.5 is brought back to the surface. (a) Iterate the decompaction formula from z2′=Tsz_2' = T_s until it changes by less than 1 m1\,\mathrm{m}. (b) What is its mean density at the surface? (c) By how much was it thicker?

Solution

Solution of Exercise 16.6.

(a) z2′←704+1234.8 (1−e−z2′/1960)z_2' \leftarrow 704 + 1234.8\,(1 - e^{-z_2'/1960}): 1077, 1226, 1278, 1296, 1301, 1303, 1304; the layer is 1304 m1304\,\mathrm{m} thick. (b) (2700×704+1030×600)/1304=1932 kg m−3(2700\times704 + 1030\times600)/1304 = 1932\,\mathrm{kg}\,\mathrm{m}^{-3}. (c) By 304 m304\,\mathrm{m}, or 30 %30\,\%: the water that compaction has squeezed out.

Exercise 16.7 ★★

In the central North Sea, the water-loaded basement sank 1100 to 1400 m1400\,\mathrm{m} after the stretching that ended in the mid-Cretaceous, about 100 Myr100\,\mathrm{Myr} ago. (a) What post-rift subsidence does the model give after 100 Myr100\,\mathrm{Myr} for β=1.5\beta = 1.5 and β=2\beta = 2? (b) Do those values bracket the observation? (c) For which β\beta does the model give 1250 m1250\,\mathrm{m}? Use βπsin⁡πβ=0.4705\frac{\beta}{\pi}\sin\frac{\pi}{\beta} = 0.4705 for β=1.6\beta = 1.6 and 0.52040.5204 for β=1.7\beta = 1.7 and interpolate.

Solution

Solution of Exercise 16.7.

(a) 1−e−100/62.7=0.79711 - e^{-100/62.7} = 0.7971. For β=1.5\beta = 1.5: 3207×0.4135×0.7971=1057 m3207\times0.4135\times0.7971 = 1057\,\mathrm{m}; for β=2\beta = 2: 3207×0.6366×0.7971=1627 m3207\times0.6366\times0.7971 = 1627\,\mathrm{m}. (b) Yes: 1100 to 1400 m1400\,\mathrm{m} lies between. (c) βπsin⁡πβ=1250/(3207×0.7971)=0.4890\frac{\beta}{\pi}\sin\frac{\pi}{\beta} = 1250/(3207\times0.7971) = 0.4890, so β=1.6+0.1×(0.4890−0.4705)/(0.5204−0.4705)=1.64\beta = 1.6 + 0.1\times(0.4890 - 0.4705)/(0.5204 - 0.4705) = 1.64, within the 50 to 100 %100\,\% of stretching inferred for the basin.

Exercise 16.8 ★★

The syn-rift basin of a stretching model is filled not with water but with sediment of density 2300 kg m−32300\,\mathrm{kg}\,\mathrm{m}^{-3}. (a) In the formula for SiS_i, what changes? (b) Compute the sediment-loaded SiS_i for β=1.5\beta = 1.5 with a 35 km35\,\mathrm{km} crust, given that the numerator of the formula is a(1−1/β)×74.69 kg m−3a(1 - 1/\beta)\times74.69\,\mathrm{kg}\,\mathrm{m}^{-3} and that ρm(1−αT1)=3184.4 kg m−3\rho_m(1 - \alpha T_1) = 3184.4\,\mathrm{kg}\,\mathrm{m}^{-3}. (c) Compare with the water-loaded value.

Solution

Solution of Exercise 16.8.

(a) The density of the fill replaces ρw\rho_w in the denominator. (b) The numerator is 125 000×(1/3)×74.69=3.112×106125\,000\times(1/3)\times74.69 = 3.112 \times 10^{6}; Si=3.112×106/(3184.4−2300)=3519 mS_i = 3.112\times10^{6}/(3184.4 - 2300) = 3519\,\mathrm{m}. (c) Under water, 3.112×106/2154.4=1445 m3.112\times10^{6}/2154.4 = 1445\,\mathrm{m}: the sediment-filled basin is 2.44 times deeper.

Exercise 16.9 ★★

A backstripped well gives Y=2171 mY = 2171\,\mathrm{m} at 100 Ma100\,\mathrm{Ma}, assuming today’s sea level. (a) If the sea then stood 100 m100\,\mathrm{m} higher, what is YY? (b) If the fossils give a water depth between 100 and 500 m500\,\mathrm{m} instead of 300 m300\,\mathrm{m}, what range of YY follows? (c) Which of the two uncertainties is the larger?

Solution

Solution of Exercise 16.9.

(a) 2171−100×3330/2300=2171−145=2026 m2171 - 100\times3330/2300 = 2171 - 145 = 2026\,\mathrm{m}. (b) YY changes metre for metre with WdW_d: from 1971 to 2371 m2371\,\mathrm{m}. (c) The water depth, ±200 m\pm200\,\mathrm{m}, against 145 m145\,\mathrm{m} for the sea level.

Exercise 16.10 ★★★

(a) Show from Proposition 16.7 that stretching makes the surface rise instead of sink when (ρm−ρc)tca(1−αT1tc2a)<αT1ρm2(\rho_m - \rho_c)\frac{t_c}{a}\left(1 - \frac{\alpha T_1 t_c}{2a}\right) < \frac{\alpha T_1\rho_m}{2}. (b) Neglecting the small term αT1tc/(2a)\alpha T_1 t_c/(2a), find the critical crustal thickness. (c) Refine it with one iteration. (d) Where on Earth would you look for rifts that rise as they open?

Solution

Solution of Exercise 16.10.

(a) SiS_i has the sign of the bracket in its numerator, since the denominator, 3184.4−10303184.4 - 1030, is positive; it is negative, an uplift, when the bracket is. (b) (ρm−ρc)tc/a=αT1ρm/2(\rho_m - \rho_c)t_c/a = \alpha T_1\rho_m/2 gives tc=a αT1ρm/(2(ρm−ρc))=125×0.04372×3330/1060=17.17 kmt_c = a\,\alpha T_1\rho_m/(2(\rho_m - \rho_c)) = 125\times0.04372\times 3330/1060 = 17.17\,\mathrm{km}. (c) tc=17.17/(1−0.04372×17.17/250)=17.22 kmt_c = 17.17/(1 - 0.04372\times17.17/250) = 17.22\,\mathrm{km}. (d) Where the crust is thinner than about 17 km17\,\mathrm{km} before stretching: in oceanic lithosphere, or in a continental crust already thinned by an earlier rifting.

Exercise 16.11 ★★★

(a) Write the isostatic balance of the proof of Proposition 16.7, part (1), and derive the formula for SiS_i. (b) Show that the exact final post-rift subsidence, when the plate has returned to its linear geotherm, is αρmT1a(1−1/β)/(2(ρm−ρw))\alpha\rho_m T_1 a(1 - 1/\beta)/(2(\rho_m - \rho_w)). (c) Compute it for β=2\beta = 2 and compare it with the final value of the first-term formula.

Solution

Solution of Exercise 16.11.

(a) Before stretching, the column holds the lithosphere of mass M=ρctc(1−αT1tc/(2a))+ρm(a−tc)(1−αT1(a+tc)/(2a))M = \rho_c t_c(1 - \alpha T_1 t_c/(2a)) + \rho_m(a - t_c)(1 - \alpha T_1(a + t_c)/(2a)); after, ρwSi+M/β+ρm(1−αT1)(a−Si−a/β)\rho_w S_i + M/\beta + \rho_m(1 - \alpha T_1)(a - S_i - a/\beta). Equating them, Si[ρm(1−αT1)−ρw]=(1−1/β)[ρm(1−αT1)a−M]S_i[\rho_m(1 - \alpha T_1) - \rho_w] = (1 - 1/\beta)[\rho_m(1 - \alpha T_1)a - M], and expanding MM, ρm(1−αT1)a−M=(ρm−ρc)tc(1−αT1tc/(2a))−ρmαT1a/2\rho_m(1 - \alpha T_1)a - M = (\rho_m - \rho_c)t_c(1 - \alpha T_1 t_c/(2a)) - \rho_m\alpha T_1 a/2: the formula. (b) The final profile is T1z/aT_1 z/a; the initial one exceeds it by T1z(β−1)/aT_1 z(\beta - 1)/a above a/βa/\beta and by T1(1−z/a)T_1(1 - z/a) below. The integrals are T1a(β−1)/(2β2)T_1 a(\beta - 1)/(2\beta^2) and T1a(β−1)2/(2β2)T_1 a(\beta - 1)^2/(2\beta^2), whose sum is T1a(1−1/β)/2T_1 a(1 - 1/\beta)/2. The contraction α\alpha times this, loaded by water, gives the expression. (c) 3.28×10−5×3330×1333×125 000×0.5/(2×2300)=1978 m3.28\times10^{-5} \times3330\times1333\times125\,000\times0.5/(2\times2300) = 1978\,\mathrm{m}, against 3207×2/π=2042 m3207\times 2/\pi = 2042\,\mathrm{m}: the first term overstates the final subsidence by 64 m64\,\mathrm{m}, 3 %3\,\%.

Exercise 16.12 ★★★

A passive margin was stretched by β=2\beta = 2 and has been cooling for 150 Myr150\,\mathrm{Myr}; the basin has stayed full of sediment of mean density 2400 kg m−32400\,\mathrm{kg}\,\mathrm{m}^{-3} up to sea level. (a) Find the water-loaded post-rift subsidence. (b) How thick is the post-rift sediment? (c) In the Baltimore Canyon Trough the early post-rift fill is 1.5 to 3 times thicker than uniform stretching predicts: what thickness would that mean here? (d) Suggest causes.

Solution

Solution of Exercise 16.12.

(a) 3207×0.6366×(1−e−150/62.7)=2042×0.9086=1855 m3207\times0.6366\times(1 - e^{-150/62.7}) = 2042\times0.9086 = 1855\,\mathrm{m}. (b) 1855×2300/(3330−2400)=4588 m1855\times 2300/(3330 - 2400) = 4588\,\mathrm{m}. (c) 6.9 to 13.8 km13.8\,\mathrm{km}. (d) The model leaves out several things that could deepen the basin: a mantle lithosphere stretched more than the crust, a regional (flexural) response to the load of the sediment, a transient uplift of the margin during rifting followed by sinking, or a supply of sediment so large that the basin was overfilled and loaded beyond sea level on the shelf.

Problem 16.1

Weekend problem — Backstripping a well

In the invented Kestrel Basin, a well cored four units. From the base: a sand laid down during rifting, from 165 to 150 Ma150\,\mathrm{Ma}, today between 4420 m4420\,\mathrm{m} and 6030 m6030\,\mathrm{m}; a shale, 150 to 100 Ma100\,\mathrm{Ma}, between 3310 m3310\,\mathrm{m} and 4420 m4420\,\mathrm{m}; a chalk, 100 to 60 Ma60\,\mathrm{Ma}, between 1700 m1700\,\mathrm{m} and 3310 m3310\,\mathrm{m}; a shaly sand, 60 Ma60\,\mathrm{Ma} to today, between 0 m0\,\mathrm{m} and 1700 m1700\,\mathrm{m} below the sea floor. Fossils give the water depth at the top of each unit when it was laid down: 200 m200\,\mathrm{m} at 150 Ma150\,\mathrm{Ma}, 300 m300\,\mathrm{m} at 100 Ma100\,\mathrm{Ma}, 150 m150\,\mathrm{m} at 60 Ma60\,\mathrm{Ma}; today it is 100 m100\,\mathrm{m}. Use the lithology table of the chapter, ρm=3330 kg m−3\rho_m = 3330\,\mathrm{kg}\,\mathrm{m}^{-3} and ρw=1030 kg m−3\rho_w = 1030\,\mathrm{kg}\,\mathrm{m}^{-3} for both sea and pore water, sea level as today, and the stretching model of the chapter with a 35 km35\,\mathrm{km} crust. Depths are rounded to the metre.

Part I — Compaction.

  1. Find the porosity of the sand at its top and at its base today.
  2. Find the solid thickness of the sand.
  3. The solid thicknesses of the shale, chalk and shaly sand are 1011 m1011\,\mathrm{m}, 1409 m1409\,\mathrm{m} and 1004 m1004\,\mathrm{m}. Check one of them.
  4. Find the mass per unit area of each unit today, then the mean density of the whole column.
  5. At 150 Ma150\,\mathrm{Ma} the sand lay at the sea floor. Decompact it: iterate from z2′=Tsz_2' = T_s until the change is less than 1 m1\,\mathrm{m}.
  6. Find the mean density of the decompacted sand.

Part II — Backstripping.

  1. Find the tectonic subsidence YY at 150 Ma150\,\mathrm{Ma}.
  2. Find the tectonic subsidence today. Why is no decompaction needed?
  3. A program gives Y=2171 mY = 2171\,\mathrm{m} at 100 Ma100\,\mathrm{Ma} and Y=2453 mY = 2453\,\mathrm{m} at 60 Ma60\,\mathrm{Ma}. Compute the mean rate of tectonic subsidence in each of the three intervals since 150 Ma150\,\mathrm{Ma}.
  4. Find the total subsidence today and compare it with the tectonic subsidence.
  5. What fraction of the depth of the basement today is due to the load of the sediment?
  6. If the sea at 100 Ma100\,\mathrm{Ma} had stood 100 m100\,\mathrm{m} higher than today, what would YY have been then?

Part III — Fitting the stretching model. Rifting is taken as instantaneous and ending at 150 Ma150\,\mathrm{Ma}.

  1. Which point of the curve gives the syn-rift subsidence?
  2. Find the stretching factor β\beta, to two decimals.
  3. How thick were the crust and the lithosphere just after stretching?
  4. With β\beta rounded, compute βπsin⁡πβ\frac{\beta}{\pi}\sin\frac{\pi}{\beta} and the final post-rift subsidence.
  5. Predict YY at 100, 60 and 0 Ma0\,\mathrm{Ma}.
  6. Compare with the backstripped values.
  7. The fit is close because the well is invented. Give three reasons why a real well would not fit so well.

Part IV — The next 50 million years.

  1. How much more tectonic subsidence will occur in the next 50 Myr50\,\mathrm{Myr}?
  2. If the water depth stays at 100 m100\,\mathrm{m}, how much sediment of density 2400 kg m−32400\,\mathrm{kg}\,\mathrm{m}^{-3} can accumulate in that time?
  3. What fraction of its final post-rift subsidence has the basin already done?
  4. When was half of it done?
  5. To sum up: what stretching factor does the well record?
Solution

Solution of Problem 16.1.

1. 0.49 e−4420/3704=0.1490.49\,e^{-4420/3704} = 0.149 at the top; 0.49 e−6030/3704=0.0960.49\,e^{-6030/3704} = 0.096 at the base. 2. Ts=1610−0.49×3704×(0.3032−0.1963)=1416 mT_s = 1610 - 0.49\times3704\times(0.3032 - 0.1963) = 1416\,\mathrm{m}. 3. Shale: 1110−0.63×1960×(e−3310/1960−e−4420/1960)=1110−1234.8×(0.1847−0.1049)=1011 m1110 - 0.63\times1960\times(e^{-3310/1960} - e^{-4420/1960}) = 1110 - 1234.8 \times(0.1847 - 0.1049) = 1011\,\mathrm{m}. 4. Shaly sand: 2680×1004+1030×696=3.408×106 kg m−22680\times1004 + 1030\times696 = 3.408 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}; chalk: 2710×1409+1030×201=4.025×106 kg m−22710\times1409 + 1030\times201 = 4.025 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}; shale: 2700×1011+1030×99=2.832×106 kg m−22700\times1011 + 1030\times99 = 2.832 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}; sand: 2650×1416+1030×194=3.952×106 kg m−22650\times1416 + 1030\times194 = 3.952 \times 10^{6}\,\mathrm{kg}\,\mathrm{m}^{-2}. Total 1.4217×107 kg m−21.4217 \times 10^{7}\,\mathrm{kg}\,\mathrm{m}^{-2}, ρˉs=14 216 910/6030=2358 kg m−3\bar\rho_s = 14\,216\,910/6030 = 2358\,\mathrm{kg}\,\mathrm{m}^{-3}. 5. z2′←1416+1815 (1−e−z2′/3704)z_2' \leftarrow 1416 + 1815\,(1 - e^{-z_2'/3704}): 1993, 2171, 2221, 2235, 2238, 2239, 2239: 2239 m2239\,\mathrm{m}. 6. (2650×1416+1030×823)/2239=2055 kg m−3(2650\times1416 + 1030\times823)/2239 = 2055\,\mathrm{kg}\,\mathrm{m}^{-3}. 7. Y=2239×(3330−2055)/2300+200=1241+200=1441 mY = 2239\times(3330 - 2055)/2300 + 200 = 1241 + 200 = 1441\,\mathrm{m}. 8. Y=6030×(3330−2358)/2300+100=2548+100=2648 mY = 6030\times(3330 - 2358)/2300 + 100 = 2548 + 100 = 2648\,\mathrm{m}. The units are measured at their present depths: they are already as compacted as they are today. 9. (2171−1441)/50=14.6 m(2171 - 1441)/50 = 14.6\,\mathrm{m} per million years from 150 to 100 Ma100\,\mathrm{Ma}; (2453−2171)/40=7.05 m(2453 - 2171)/40 = 7.05\,\mathrm{m} from 100 to 60 Ma60\,\mathrm{Ma}; (2648−2453)/60=3.25 m(2648 - 2453)/60 = 3.25\,\mathrm{m} since: the sinking slows down. 10. 6030+100=6130 m6030 + 100 = 6130\,\mathrm{m}, 2.31 times the tectonic subsidence. 11. (6130−2648)/6130=57 %(6130 - 2648)/6130 = 57\,\%. 12. 2171−100×3330/2300=2026 m2171 - 100\times3330/2300 = 2026\,\mathrm{m}. 13. The point at the end of rifting, 150 Ma150\,\mathrm{Ma}: Si=1441 mS_i = 1441\,\mathrm{m}, if no thermal subsidence took place during the 15 Myr15\,\mathrm{Myr} of rifting. 14. β=1/(1−1441/4334)=1/0.6675=1.50\beta = 1/(1 - 1441/4334) = 1/0.6675 = 1.50. 15. 35/1.50=23.3 km35/1.50 = 23.3\,\mathrm{km} of crust and 125/1.50=83.3 km125/1.50 = 83.3\,\mathrm{km} of lithosphere. 16. (1.50/π)sin⁡(π/1.50)=0.4775×0.8660=0.4135(1.50/\pi)\sin(\pi/1.50) = 0.4775\times0.8660 = 0.4135; 3207×0.4135=1326 m3207\times0.4135 = 1326\,\mathrm{m}. 17. Si=4334/3=1445 mS_i = 4334/3 = 1445\,\mathrm{m}. At 100 Ma100\,\mathrm{Ma}, t=50 Myrt = 50\,\mathrm{Myr}: 1326×(1−e−50/62.7)=729 m1326\times(1 - e^{-50/62.7}) = 729\,\mathrm{m}, Y=2173 mY = 2173\,\mathrm{m}; at 60 Ma60\,\mathrm{Ma}: 1326×0.7620=1010 m1326\times0.7620 = 1010\,\mathrm{m}, Y=2455 mY = 2455\,\mathrm{m}; today: 1326×0.9086=1205 m1326\times0.9086 = 1205\,\mathrm{m}, Y=2650 mY = 2650\,\mathrm{m}. 18. The model is 2 m2\,\mathrm{m} deeper at each point: 2173 against 2171, 2455 against 2453, 2650 against 2648. 19. Palaeo water depths known only to within a hundred metres or more; past sea levels different from today’s; a rifting that lasted 15 Myr15\,\mathrm{Myr}, during which part of the heat was already lost; flexure rather than local isostasy; a mantle stretched more or less than the crust; a crust not 35 km35\,\mathrm{km} thick before rifting. 20. 1326×(e−150/62.7−e−200/62.7)=67 m1326\times(e^{-150/62.7} - e^{-200/62.7}) = 67\,\mathrm{m}. 21. 66.6×2300/(3330−2400)=165 m66.6\times2300/(3330 - 2400) = 165\,\mathrm{m}. 22. 1−e−150/62.7=91 %1 - e^{-150/62.7} = 91\,\%. 23. τln⁡2=43.5 Myr\tau\ln2 = 43.5\,\mathrm{Myr} after the end of rifting: at 106.5 Ma106.5\,\mathrm{Ma}. 24. β=1.50\beta = \textbf{1.50}: the crust was stretched to one and a half times its width.

Terms defined in this chapter

See all 957 terms in the glossary