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SEDIMENTARY ROCKS
Evaporites & Coal
Md. Asif Hasan
EVAPORITES
Enormous volumes of sediment in the ancient sedimentary record are composed
mainly or entirely of what are called evaporite minerals: minerals precipitated from a
saline solution that has been concentrated by evaporation. Most evaporites in the
sedimentary record are marine evaporites (solutions derived from normal sea water by
evaporation are said to be hypersaline), but there are also non-marine evaporites. There
are a great many evaporite minerals, but only a few are common. It’s been estimated that
something like one percent of Phanerozoic rocks are evaporites, and that a quarter to a
third of the area of the continents is underlain by evaporite deposits in the subsurface,
with thicknesses ranging from a few meters to hundreds of meters. (Think “salt mines”:
there really are such things)
 The Permian Period was the time of greatest evaporite deposition—
presumably because much of the great supercontinent of Pangea lay in a low-
latitude belt of continental aridity in what we call, in the present time, the
“horse latitudes”, where the troposphere experiences widespread subsidence in
the downgoing leg of the low-latitude Hadley cell of the general circulation of
the atmosphere.
 If you leave dolomite out of consideration (and some nearly primary dolomite
must have been associated with hypersaline conditions), the three most
common evaporite minerals are gypsum (a hydrated calcium sulfate mineral),
anhydrite (an anhydrous calcium sulfate mineral), and halite, NaCl. But the only
evaporite you as field geologists are likely to see is gypsum, because halite
dissolves so readily in surface waters except in the most arid regions, and
anhydrite, being the high-pressure anhydrous form of calcium sulfate, is mostly
restricted to depths greater than tens to hundreds of meters.
 Are you likely to see evaporites in outcrop? The answer is yes, for gypsum,
but no, for halite (the two most voluminous evaporite deposits). Only in the
driest of climates—in the interior of Iran, for example—is rock salt exposed at
the Earth’s surface.
 Evaporites are excellent indicators of paleoclimate: it takes a hot and arid
climate for major evaporite deposits to form. As you will see in a later chapter
on economic sedimentology, evaporites can form seals for the accumulation of
petroleum hydrocarbons in reservoir rocks. On a more prosaic note, gypsum is
the mineral that’s used to make plaster and “drywall” (gypsum wallboard).
 Evaporite deposits are known from all the continents, with ages ranging from
Precambrian to Late Cenozoic (although Precambrian evaporites are scarce,
either because they were not deposited or because they have been dissolved
away during diagenesis through geologic time). Unfortunately, however, there
are no modern evaporite depositional environments representative of the
extensive areas of evaporite deposition that existed at various times and places
in the geologic past. As with dolostones, this has led to great difficulties and a
diversity of competing theories in interpreting the depositional environments
of evaporites.
Evaporite Minerals
anhydrite CaSO4
calcite CaCO3
carnallite KMgCl3
.6H2
O)
dolomite CaMg(CO3
)2
gypsum CaSO4
.2H2
O
halite NaCl
kainite KMg(SO4
)2
.H2
O
kieserite Mg SO4
.H2
O
langbeinite K2
Mg2
(SO4
)3
magnesite MgCO3
polyhalite K2
Ca2
Mg(SO4
)4
.2H2
O
sylvite KCl
More than eighty naturally occurring evaporite minerals have been identified. The
intricate equilibrium relationships among these minerals have been the subject of many
studies over the years. But there are only about a dozen major evaporite minerals. But of
the above minerals, only three are of paramount importance: gypsum, anhydrite, and
halite.
 Gypsum is a calcium sulfate mineral containing water of hydration. It’s
monoclinic with one perfect cleavage, and usually white or colorless but
sometimes gray or reddish. It’s one of the softest of common minerals: you can
scratch it with your fingernail. Its specific gravity is relatively low, 2.32.
Although phase equilibria in the CaSO4–H2O system are far from clear, because
of the difficulty of studying equilibrium precipitation and dissolution in the
laboratory, it seems clear that gypsum is the mineral that is stable at surface
conditions and is virtually always the primary evaporite precipitation product.
 Anhydrite is an anhydrous calcium sulfate mineral. It’s orthorhombic, has one
perfect cleavage and two other good cleavages, and is usually white to colorless
but sometimes gray. Its specific gravity is relatively high, 2.93. It is usually seen
as massive granular aggregates rather as well formed crystals. It’s stable at
higher pressures and temperatures than is gypsum, so gypsum is converted to
anhydrite when the evaporite deposit is buried. The deepest reported
occurrence of gypsum is about 1300 m.
 Halite is a cubic mineral with a perfect cubic cleavage. It’s colorless when pure
but can be reddish from iron and various other colors as well. It’s easy to
identify by its salty taste. It forms surface outcrops only in the most arid
regions. It’s also a relatively low-density mineral: the specific gravity is 2.16.
Not all evaporites are marine deposits. Nonmarine evaporites are common,
although the volume of nonmarine evaporites is not nearly as great as that of
marine evaporites. Nonmarine evaporites are common in continental extensional
basins. There is a great variety of nonmarine evaporite minerals.
Chemistry of Evaporites
You know, of course, that the oceans are salty. The salinity of sea water is close to 35
parts per thousand, ppt (parts dissolved materials, by mass, per thousand parts of bulk sea
water, by mass). Generally the salinity varies only slightly from place to place in the
oceans, because of dilution and evaporation, although these slight differences are of
extreme importance in controlling the circulation and also the biology of the oceans. But
in certain unusual situations, the salinity can rise to much higher values, giving rise to
evaporite precipitation.
Almost all of the salt in sea water is accounted for by seven ions. Here’s a table that
lists these ions and their concentration in percent by weight. These seven ions account for
99.7% by weight of all the dissolved salts in sea water.
Cl
-
55
Na
+
31
SO4
2-
7.7
Mg
2+
3.7
Ca
2+
1.16
K
+
1.10
HCO3
-
0.41
Of these, the last is controlled by the equilibrium between sea water and the CO2
of the
atmosphere. The dominant control on the rest is the dissolved-salt content of river runoff.
Back in 1849 an Italian chemist named Usiglio made a classic, widely cited, but
somewhat misleading experiment on evaporite deposition. He took a volume of normal
sea water and slowly evaporated it, and kept track of the composition and mass of
precipitated salts as a function of extent of evaporation. He found that when the water is
reduced in volume to about 50% of the original volume, a little iron oxide and some
aragonite are precipitated, but precipitation of the major evaporite minerals doesn’t begin
until the volume is reduced to about 20%, when gypsum is precipitated. Then when the
volume is reduced to about 10%, halite begins to be precipitated. Further reduction in
volume then leads to the precipitation of various magnesium sulfates and chlorides, and
finally to NaBr and KCl.
In terms of volumes of precipitated salts, experiments like that of Usiglio show that if
a column of sea water 1000 m thick is evaporated to dryness, the precipitated salt deposit
would be about 15 m thick. Of this, 0.5 m would be gypsum, 11.8 m would be halite, and
the rest, 2.7 m, would be mainly salts of potassium and magnesium. But is this how most
evaporite deposits are formed? No; read on.
Kinds of Evaporite Deposits
 Gypsum rock is usually finely granular but sometimes coarsely crystalline. The
mode of occurrence of gypsum is rather variable, because, as you will see
presently, diagenetic changes are usually far-reaching. Details of bedding are
usually not well preserved. Gypsum is also common as nodules in a matrix of
carbonate or shale.
 Anhydrite rock is usually bedded, often with delicate lamination that’s
continuous for long distances. It’s usually fine grained. You seldom see
anhydrite in outcrop, however, for reasons that will become apparent soon.
 Rock salt is a massive, coarsely crystalline, and nonjointed rock. It sometimes
shows bedding, especially by alternation of beds with greater or lesser
concentration of nonhalite impurities (gypsum, anhydrite, carbonates, and
siliciclastics).
Diagenesis of Evaporites
Changes in evaporites during burial and unroofing are usually substantial, for three
reasons:
Evaporite minerals in general are very susceptible to solution and reprecipitation.
• Gypsum is converted to anhydrite upon burial, and then the anhydrite is usually
reconverted to gypsum as it makes it way to the surface again. When gypsum is
replaced by anhydrite, there is a 38% loss in volume, because of the great
difference in density between the two minerals. So there’s great extra
compaction on the way down (which, incidentally, is conducive to nontectonic
deformation, because if the pore water, preexisting and newly released, can’t
drain away fast enough, the reduction in solids volume tends to cause a liquefied
state in which the pore-water pressure can approach the lithostatic pressure).
Conversely, on the way up the anhydrite is reconverted to gypsum, provided that
extra water is available. This expansion tends to cause even more local
deformation of the deposit. The change from anhydrite to gypsum on the way up
is usually delayed until the near-surface zone of influence of surface groundwater
is reached. This gypsum–anhydrite diagenetic cycle is shown in
Figure : The gypsum-anhydrite diagenetic cycle
• Halite tends to flow plastically on a large scale, because it’s relatively weak and
because its deposits have a substantially lower bulk density than the “normal”
rocks (carbonates and siliciclastics) with which it’s interstratified on a large
scale. A horizontal layer of halite lying between layers of denser rock represents
a gravitationally unstable situation, and even slight preexisting nonplanarity of
the layer leads to uprise of columns or domes of salt, called diapirs, typically on
scales of several kilometers. Hence the term salt tectonics.
Sedimentary Structures in Evaporites
 Do evaporites precipitate as bottom growths or as discrete mineral
particles? The former is demonstrable in some cases, but the widespread
existence of primary sedimentary structures, like lamination, cross
stratification, ripple marks, and graded bedding—just as in siliciclastic
sediments and rocks— gives good evidence that the latter is the more
important mode of deposition. It’s clear that once evaporite crystals are
precipitated they are susceptible to reworking and transportation before final
deposition.
 Evaporites are highly susceptible to early and significant diagenesis, owing to
the extreme solubility of the evaporite minerals. Most of the sedimentary
structures in evaporites are diagenetic. Various kinds of postdepositional folds
and veins are common. Veins of gypsum cutting fine siliciclastic rocks
(mudrocks and fine sandstones), both parallel and oblique to stratification, are
c presumably the largely siliciclastic sediment contained an admixture of
gypsum, which was remobilized upon shallow burial.
 A striking and common diagenetic structure in calcium sulfate evaporites
is nodular anhydrite
Theories of Evaporite Deposition
 The great thickness of some evaporite deposits, as well as the common
dominance of gypsum in the deposit, argue against simple evaporation of a
body of sea water to dryness. One has to appeal to a continuous evaporation
process whereby a water body partially isolated from the open ocean is
subjected to net evaporation (evaporation is greater than fresh-water runoff
into the basin).
 If in such a continuous-evaporation basin there is no outflow of water, only
inflow, then all of the dissolved salts must be precipitated somehow, whatever
the ratio of sea-water inflow and fresh-water runoff. The common dominance of
one or another evaporite mineral suggests, however, that some percentage of
the concentrated brine flows out of the basin, somehow, during the evaporation
process. Presumably the outflow would contain a disproportionate
concentration of the harder-to-precipitate salts. The outflow could be as an
outgoing underflow of denser, more saline water beneath an inflowing surface
current of normal sea water (Figure A). Or it could be as a gravity-driven diffuse
flow through a permeable barrier (Figure B).
 If a greater percentage of the water is returned to the open ocean by reflux, then
gypsum would be the dominant evaporite, whereas if a lesser percentage of the
water is returned by reflux, then halite would be the dominant evaporite. In the
least common situation, where an even smaller percentage of the basin water is
returned by reflux, the more exotic evaporites would be formed.
 Shallow ocean-margin continuous-evaporation basins of the kind described above
are a natural way of accounting for the thick and extensive deposits of evaporites
seen in the sedimentary record, but keep in mind that no good examples are known
from the modern, so it’s all a matter of deduction rather than of observation.
 Many evaporite deposits are relatively thin and intimately associated with
sediments of other compositions, and show excellent evidence of very shallow-
water conditions, like desiccation cracks. An appealing way of accounting for such
evaporites is to assume that they are sabkha deposits. A sabkha is a low-lying but
supratidal surface along a coast with net evaporating conditions and little supply of
siliciclastic sediment. (The adjective supratidal refers to elevations just above the
high-tide level.) Most of the time the sabkha surface is emergent, but occasional
storms cover the surface with sea water. That water tends to seep down into the
sabkha surface, and during later evaporation the water rises again by capillary
action, and the dissolved salt is precipitated as evaporite minerals. If the shoreline is
prograding, a layer of evaporites some meters thick may be deposited in that way.
Figure: Major evaporite deposits of the world
Prepared By Md. Asif Hasan
47th Batch
CHERT
Introduction
 Chert is the general term for very fine-grained and nonporous sedimentary
rocks that consist mostly or entirely of silica, in the form of either amorphous
silica or microcrystalline quartz presumably derived from recrystallization of
amorphous silica. The non-scientific equivalent term is flint.
 Cherts are fairly easy to identify, even though you can’t see the constituents
with your unaided eye, because of the way they fracture and the way they look
on fracture surfaces. Cherts are widespread (they are the last of the rocks we’ll
consider in this course that you are likely to see commonly), but their total
contribution to the sedimentary record is probably not much more than a
percent or two.
 The crystal size of quartz in recrystallized chert is usually in the range 5–20 μm.
Electron microscopy of fractured surfaces shows the quartz to be polyhedral,
equant to elongate, and closely fitted to surrounding grains. Cryptocrystalline
geometries in the transition from amorphous silica to recrystallized quartz are
complex. Thin-section studies don’t help much because the quartz is too fine.
 Chert comes in two distinct varieties, nodular chert and bedded chert, whose
sedimentological occurrence is rather different. The problems with chert come
in its origin; it’s another one of those rocks whose origin we have a hard time
observing directly. The relative importance of nodular chert and bedded chert
has changed through geologic time: bedded chert is much more common in the
Precambrian, and nodular chert is more common in the Phanerozoic.
Terminology
Here are a few terms for kinds of amorphous silica and chert:
 amorphous silica: material composed of relatively pure SiO2 but with only very
local crystallographic order. Amorphous silica includes various kinds of hydrated
and dehydrated silica gels, silica glass, siliceous sinter formed in hot springs, and
(certainly of greatest geological importance) the skeletal materials of silica-
secreting organisms (see below, under opal).
 opal (or opaline silica) is a solid form of amorphous silica with some included
water. It’s abundant in young cherts, back into the Mesozoic. Its geological
occurrence is by alteration of volcanic ash, precipitation from hot springs, and, by
far most importantly, precipitation as skeletal material by certain silica-secreting
organisms (see a later section). Opal starts out as what is called opal-A, which
shows only a very weak x-ray diffraction pattern, indicating that any
crystallographic order is very local. With burial, during the initial stage of
diagenesis, opal-A is transformed into opal-CT, which shows a weak x-ray
diffraction pattern characteristic of cristobalite another silica mineral; see below).
Upon further diagenesis, opal-CT is transformed into crystalline quartz, resulting in
chart that consists of an equant mosaic of microquartz crystals. By that stage, most
or all of the fossil evidence of origin is obliterated.
 chalcedony is a very finely crystalline form of silica consisting of radiating needles
or fibers, often spherulitic, of quartz. There’s probably amorphous silica in among
the needles, and a variable water content. This stuff is metastable with respect to
ordinarily crystalline quartz, but it hangs around a long time; it’s found even in
Paleozoic cherts.
 flint is the general-language equivalent of chert, usually applied to dark gray chert
in nodules or as beds.
 jasper: chert that’s red because it contains hematite (often more than a few
percent).
 porcelanite (also spelled porcellanite): a minutely porous form of chert with a dull
appearance on the fresh surface.
Silica Geochemistry
The solubility of quartz in pure water is very small, several parts per million.The
Figure shows a graph of quartz solubility as a function of pH. You can see that the
solubility of quartz is very low for pH values up to about 8 (slightly alkaline) but
then rises sharply with increasing pH. It’s hard to measure, but it can be calculated.
Moreover, attainment of equilibrium is very slow. The solubility of amorphous silica
is an order of magnitude higher, and attainment of equilibrium is also slow, but
much faster than for quartz; you can do it in the laboratory. The dominant species of
silica in solution in natural waters in the usual range of pH is silicic acid, H4
SiO4
, a
weak acid.
Figure: The solubility of quartz and amorphous silica at 25°C
At room temperature and pressure, amorphous silica is metastable with respect to
quartz, but precipitates formed from supersaturated solutions are always amorphous
silica. This is because the building of the quartz crystal structure at low temperatures
takes a very long time. Solutions unsaturated with respect to amorphous silica but
supersaturated with respect to quartz remain stable for many years if not longer. Clear
crystalline quartz can’t be precipitated in the laboratory at the low temperatures and
pressure of sedimentary environments. Presumably nature can do it because of the longer
times involved.
The concentrations of dissolved silica in rivers, streams, and lakes are a few tens of parts
per million. Concentrations are also in this range in groundwater; the deeper the
groundwater, the higher the silica concentration
Prepared By Md. Asif Hasan
47th Batch
What are the sources of silica in solution?
 Weathering of silicate minerals: this is the ultimate source of most of the silica in
solution in the Earth’s surface waters.
 Thermal springs: the concentration of dissolved silica concentration is very high
but the absolute volume is small.
 Dissolution of amorphous silica: this must be important in areas underlain by
silica-containing sedimentary rocks, but it is certainly not as important overall as
weathering of silicates
 Dissolution of quartz: most natural fresh waters are in the pH range for which the
solubility of quartz is very low, so dissolution of quartz is not an important source of
silica in solution.
Here’s the bottom line: it’s generally agreed that by far the greater part of dissolved
silica comes from weathering of silicate minerals in source rocks.
The concentration of dissolved silica in the oceans is surprisingly and extremely small:
only a few tenths of a part per million. In the present oceans, there’s no possibility of
precipitating silica inorganically. The reason for this very low silica concentration in the
oceans is that several kinds of organisms are very effective in extracting silica from sea
water and fixing it in the form of opaline silica in their skeletons. They do this out of
equilibrium, by metabolic concentration processes.
Silica-Secreting Organisms
Several kinds of important marine organisms secrete amorphous silica to form part
or all of their skeletons: diatoms, radiolarians, and sponges. These organisms play an
important part, directly or indirectly, in the deposition of chert.
Diatoms :
 Diatoms are unicellular photosynthesizing organisms, a kind of algae, mostly from
20 to 200 μm in size. The cell wall of the organism is silicified with opaline silica to
form what’s called a frustule, consisting of two valves that overlap one another like
the lid of a shallow dish.
 Some diatoms are benthic (living on the sea floor), others (by far the most important
sedimentologically) are planktonic, living in the photic zone of the oceans (the
uppermost layer in the oceans, in which there is abundant sunlight), in less than 200
m water depth. They solve the problem of buoyancy by being fitted with tiny fat
droplets. They like cool water best, apparently because of greater nutrient supply,
higher water density, and upwelling. At certain times of the year diatom blooms
produce concentrations of up to a billion organisms per cubic meter.
 Diatoms first evolved in the Cretaceous and have been expanding in importance
since. A fairly high percentage of the total number of known diatom species are
living today.
 Like foraminifera, diatoms rain onto the floor of the deep ocean over large areas.
The resulting sediment is called diatom ooze. Fossil diatomaceous deposits are
called diatomite, or diatomaceous earth if friable. It’s mined as a filtration
medium for water filters. Diagenesis of diatomite leads to diatomaceous chert, and
if diagenesis is sufficiently intense, most or even all the evidence of the originally
diatomaceous nature of the rock is obliterated.
Radiolarians :
 Radiolarians are planktonic protozoans with approximately spherical skeletons
generally from 100 to 2000 μm in diameter. The protoplasm of the cell is
divided into endoplasm and ectoplasm, separated by what’s called a central
capsule. The ectoplasm has frothy gelatinous material in which are embedded
swarms of symbiotic algae called zooxanthellae, in the shallow-water species.
Radiating outward from the central capsule through the ectoplasm are
threadlike pseudopods. The skeleton, situated within the cell, consists of radial
and tangential elements of highly varied geometry: spicules, spines, bars,
spheres, spindles, and cones. The composition of the skeletal material is either
celestite, SrSO4 (a strontium sulfate mineral, which is unimportant geologically
because the celestite dissolves too fast), or opaline silica. Radiolarians have
been around since at least the Cambrian.
 Radiolarian species live in a wide range of water depths. They like warmer
water. They trap and paralyze passing small plankton with their sticky
pseudopods. They maintain buoyancy by fat globules or gas-filled vacuoles.
 Like diatoms, radiolarians sink to the bottom and can accumulate to form
radiolarian ooze if they are not dissolved before burial. Radiolarian ooze tends
to be found at greater depths than calcareous ooze, and at low latitudes. Fossil
deposits of radiolarian ooze are called radiolarite, and chert containing
radiolarians is called radiolarian chert. The effects of diagenesis are similar to
those on diatomaceous cherts.
Sponges :
 Sponges are filter-feeding organisms that live attached to the bottom in shallow and
deep marine environments. They are multicellular but are not considered to be true
metazoans because they are not organized into tissues and they have no nervous
systems; in degree of organization they fall between protozoans and metazoans.
 Here’s how sponges work: they have an upright body shaped like a bag or vase with
a hole at the top. The outer surface of the sponge has tiny holes leading inward to
small chambers in the wall of the sponge that are lined with cells with flagella that
whirl continually to create a current flowing inward into the central cavity. Plankton
sticks to the surface of these cells, which then ingest the material. Sponges are thus
low-pressure water pumps, which can pump a volume equal to their body volume in
a minute.
 Sponges have skeletons composed of spongin (an insoluble and chemically inert
protein, what you buy as a “natural sponge”), calcareous spicules, or siliceous
spicules. It’s the siliceous spicules that we’re interested in here. They can be
straight, radiating, or irregular in shape, and they range in size from microscopic to
quite large. Silica-secreting sponges have been around since the Cambrian.
Nodular Chert
 Chert is widespread as nodules in limestone. Chert nodules are varied in shape, from
more or less regular discoidal or egg-shaped bodies (that’s the common shape for
relatively small chert nodules) to highly irregular knobby and warty bodies (the
common shape of relatively large chert nodules). Their size ranges from a few
centimeters to a few tens of centimeters. They tend to be concentrated along certain
bedding planes. Where abundant, they often form a two-dimensionally or three-
dimensionally interconnected network.
 Chert nodules are usually structureless, but some show faint traces of stratification
coincident with that in the enclosing limestone. If the limestone is fossiliferous, the
fossils in the chert can be either calcareous or silicified. And the fossils in the rest of
the limestone may or may not be silicified themselves. Sometimes the boundary
between the nodule and the limestone passes right through fossils—suggesting that
the nodules are a diagenetic feature, not a primary feature.
 Although in the past some geologists believed that nodules form by direct
precipitation of silica gel on the ocean bottom, today the evidence for a replacement
origin is considered to be overwhelming:
 irregular shape and interconnectedness of many nodules;
 presence of irregular patches of limestone in nodules;
 association of chert and silicified fossils in many limestones;
 presence of replaced fossils in some nodules;
 traces of bedding passing through nodules;
 contacts of nodules passing through fossils.
But the source of the silica is a problem.
Did it come from within the bed or from somewhere else?
 The general feeling seems to be that, in most cases at least, the nodules can be
explained by the presence of abundant biogenic amorphous silica in the original
sediment and then diagenetic reorganization. By diagenetic reorganization is meant
the process by which the disseminated bodies of opaline silica (sponge spicules,
diatoms, radiolarians) are dissolved, whereupon the silica in solution migrates to
certain places in the sediment where it is reprecipitated in the form of opal-CT to
form the nodules. This happens because the pore fluids are undersaturated with
respect to the original biogenic silica, which consists of opal-A, but are
supersaturated with respect to opal-CT, which has lower solubility than opal-A.
Frustratingly (for me, at least), the literature on chert nodules never seems to
provide the classic “straight answer” for what the controls are on the origin of the
nodules: Why do they form where they do? Why is are the size and spacing the
way they commonly are, rather than much smaller or much larger?
 Where the chert nodules form only a small part of the bulk volume of the rock, a
good case can be made that the silica that forms the nodules was present in the
sediment from the time of deposition. But how about when the chert forms the
greater part of the rock? Then a stronger case could be made for introduction of
silica in solution after deposition, by circulating pore solutions.
 The chert in shallow marine limestones probably comes mostly from sponge
spicules; that in deep marine cherts probably comes mostly from diatoms and
radiolarians. In either case, the limestones that contain chert nodules are commonly
fine-grained wackestones and mudstones, because the remains of the organisms
responsible for the silica were deposited in quiet-water carbonate environments
conducive to the various silica-secreting organisms.
Bedded Chert
Chert is also found as continuous beds, from centimeters up to as much as a few meters
thick, often, but not always, interbedded with shale. Bedded cherts are also often
interbedded with turbidite sandstones and submarine volcanics. Most such bedded cherts
show abundant evidence of having been deposited in the deep ocean.
Two scenarios seem most attractive for explaining these cherts:
 Open-ocean siliceous ooze is conveyor-belted to subduction margins and
incorporated into a subduction mélange.
 Siliceous sediment is deposited near a subduction margin, interbedded with
subduction-zone volcanics and turbidites shed from the island arc, and
incorporated into a subduction mélange.
Here we need to distinguish between Phanerozoic bedded cherts and Precambrian
bedded cherts.
 Phanerozoic bedded cherts usually contain radiolarians, and they can be
explained by lithification and diagenesis of radiolarian-rich bottom sediments,
although some may have been inorganically precipitated with radiolarians as a
nonessential constituent.
 Precambrian bedded cherts, on the other hand, show no convincing evidence of
having started out as biogenic sediment, inasmuch as no silica-secreting marine
organisms are known from the Precambrian. (Some of the oldest and most exotic
unicellular organisms are found preserved in Precambrian cherts, going way back
into the Archean—but that does not mean that the cherts were formed biogenically
from silica-secreting organisms). Most Precambrian cherts seem have been
inorganically precipitated, although the processes involved are not entirely clear.
The concentrations of dissolved silica in the Precambrian oceans, before the
appearance of the silica-secreting organisms characteristic of the Phanerozoic, were
probably in the range of tens of parts per million, almost an order of magnitude
greater than today. It’s common for such cherts to be interbedded with chemically
precipitated ironstones. Some of the very oldest sedimentary rocks, in greenstone
terranes, are bedded cherts. Chert is characteristically interbedded, down to
centimeter scale, with Precambrian iron formations.
FOSSIL FUELS
The modern world operates largely on fossil fuels, mainly coal and fluid petroleum
hydrocarbons. For almost a hundred years much of the practice of geology has centered
around exploration for such fossil fuels, as well as for the “hard” or metallic minerals. It
seems important in a course like this to give some attention to the geology of fossil fuels.
COAL
Have you ever had the opportunity to hold a lump of coal in your hand? The average
person”s contact with coal has lessened greatly in the last fifty years, since the great
increase in use of oil and natural gas in home heating. Only if you're associated with the
mining of coal or its use in industrial steam plants are you likely to have had hands-on
experience with coal. But coal represents the world’s greatest remaining storehouse of
energy—for better or for worse. Coal represents almost 90% of the world's recoverable
reserve of fossil fuels. The United States, with about 20% of the world’s coal supply, is well
endowed.
 Coal is a sedimentary rock! It could be defined as a combustible rock that had its
origin in the accumulation and partial decomposition of vegetation. That’s akay as
far as definitions go, but it’s not very descriptive.
 Coal is found to be interbedded with other sedimentary rocks you might consider to
be ordinary rather than extraordinary: sandstones, shales, and limestones. Coal
itself, however, should be viewed as a rare sedimentary rock, albeit widely
distributed: even in the relatively few formations around the world in which it is
found, coal constitutes only a small percentage of the stratigraphic section, rarely
more than one or two percent and often much smaller. But in absolute terms, the
quantity of coal remaining after centuries of mining is staggering: it has been
estimated that there's something like 1015 to 1016 kilograms of coal locked up in
the Earth’s continental crust.
 Coal is found in beds (or seams, in coal terminology) ranging in thickness from just
millimeters to many meters. Typical thickness of coal beds is half a meter to a few
meters.
Properties and Terminology
Coal varies greatly in its properties, depending in part upon its composition but for the
most part in the degree of diagenesis or even metamorphism it's undergone. This degree
of diagenesis is called the rank of the coal. In terms of extent of diagenesis, coal ranges
from low-rank (brown, porous, semilithified, and of low density, something like 1.0
g/cm3) to high-rank (jet black, hard, nonporous, hard, and much more dense, up to almost
2.0 g/cm3). Figure shows this spectrum, with conventional names along the way.
You can see from Figure that the principal way-
stations along this spectrum are lignite (brown
coal) → bituminous (soft coal) → anthracite
(hard coal). Lignite burns readily but with a
smoky flame; anthracite is hard to ignite but
burns with a clean, hot flame.
Material even less diagenetized than lignite is
called peat, which is a porous aggregate of
largely nondecomposed but stable plant
residues. In some areas peat is mined as a
domestic fuel, in addition to being ground up
for agricultural and horticultural use. At the
other end of the spectrum, under conditions of real metamorphism (the interbedded rocks
then being metamorphic rather than sedimentary), anthracite coal is converted to meta-
anthracite, and finally to graphite.
Composition
Almost by definition, coal consists mostly of carbon. The plant materials from which
coal is derived are largely carbohydrates of various kinds, only the most resistant of which
(mainly cellulose and lignin) remain after partial decomposition after death of the plants.
The initial plant residues that are buried to become coal therefore consist largely of
carbon even at the very beginning. But coals—even lignites—contain appreciable
percentages of other constituents as well. Here’s a list:
 Nitrogen: a couple of percent; doesn’t vary much. Probably from the organic
matter itself, not from entrapped air.
 Sulfur: small percentages, a couple of percent, but undesirable because of
production of sulfuric acid (the main constituent of acid rain) upon combustion.
 Water: varies with rank from a few percent to as much as 90% (conventionally
measured after drying at a temperature a little greater than 100 °C, to get rid of
liquid water in pore spaces).
 Gases: CO2, O2, N2, CH4, variable percentages.
 Ash: the solid residue upon combustion: sand, silt, and clay in variable
proportions, either carbonate or siliciclastic (mostly the latter). From fractions
of a percent in the cleanest coal to such large values that the rock should be
called a carbonaceous shale or a carbonaceous sandstone rather than coal. Very
impure coal is called bone coal.
Figure: The rank of coal in relation to a carbon-hydrogen-oxygen composition triangle
Figure shows one segment of a composition triangle whose end members are percent of
carbon, hydrogen, and oxygen. Only the area nearest the carbon corner is occupied by
rocks we would call coal. You can see that the increase in rank is associated with a
progressive decrease in the percentages of hydrogen and oxygen, presumably owing to
driving off of the volatile constituent water.
 The plant constituents of coal have been classified both macroscopically and
microscopically. The basic idea is that all coal is composed of a small number of
kinds of fragments of plant debris called macerals, which are analogous to the
minerals of an ordinary sedimentary rock.
 Macerals represent such things as branches, twigs, leaves, bark, interior tissue of
various kinds, and pollen or spores, among many others. Study and classification of
coal macerals is highly botanical and can be done only with the aid of a microscope.
 The macroscopic study and classification of coals, on the other hand, while not as
fundamental, is easier to deal with. Coal has long been recognized to consist of just a
few macroscopic constituents, usually interlaminated. These constituents form
strata that are typically from fractions of a millimeter to tens of millimeters thick.
 vitrain: brilliant, vitreous (glassy-looking), jetlike coal with conchoidal (shell-
like) fracture
 clarain: coal layers that appear silky from the presence of very delicate internal
lamination
 durain: dull, lusterless, matte layers of coal with a close or dense texture,
without internal lamination
 fusain: friable and highly porous coal, usually appearing as irregular chips and
wedges lying along the bedding; often called mineral charcoal.
Origin
 Coal can form wherever growth of vegetation is abundant enough, and accumulation
of the sediment is scanty enough, that plant material can accumulate in high
concentrations and large quantities before complete decomposition. For this, one
has to appeal to extensive swamps, usually termed coal swamps, either fresh water
or sea water (probably mainly fresh water) in climatic conditions conducive to lush
growth of vegetation and far from sources of siliciclastic sediments.
 Most coal seems to have formed in place, by gradual accumulation of plant material
right where it grew. You can imagine thick accumulations of earlier plant material
into which the present crop puts down its roots, only to succumb eventually and
form the substrate for yet another crop. Such coal is said to be autochthonous.
Some coal, however, seems to consist of plant fragments that were transported far
from where they grew, presumably by flowing water, and deposited in some rather
different sedimentary environment—but again one without an abundance of
“ordinary” siliciclastic sediment. Such coal is said to be allochthonous.
 The overall association of other sedimentary facies with coals—mainly shallow
marine and fluvial sediments—tells us that, broadly, coal accumulates in coastal
environments of one kind or other. Perhaps the most common kind of environment
of this kind could be termed deltaic. Imagine a broad river carrying mud and sand to
the shoreline. The river flow in deltas tends to be well channelized, with strong
flows carrying sand to the channel mouths. Mud carried by such channels is either
spilled widely over the banks of the channels along the way or disgorged into the
sea at the mouths of the channels. In certain settings, in between the channels are
low-lying areas that receive little fluvial sediment and are conducive to dense
vegetation. Such areas tend to experience slow subsidence, from compaction of
earlier-deposited sediments; this subsidence makes room for further accumulation
of plant materials. (Keep in mind that there must be great compaction of the plant
material as it's buried.)
Cyclothems
 The coastal nature of most coal is emphasized by the mode of occurrence of late
Paleozoic coal. (You will see below that the Pennsylvanian was one of the great
epochs of coal deposition around the world.) Most Pennsylvanian coal is found in
distinctive cyclic units called cyclothems. A cyclothem consists of a systematic
alternation or cycle of sedimentary deposits that represent a regular alternation of
depositional environments.
 Interpretation of a cyclothem like that shown in Figure 12-4 is clear: there’s a cyclic
alternation of marine and nonmarine deposits. The nonmarine part of the cyclothem
extends from the disconformable base of the sandstone to the coal; the rest of the
cyclothem represents shallow-marine deposition. We are forced to assume that
there was a cyclic rise and fall of sea level relative to land, to produce inward and
outward migration of the shoreline over the area where the deposits were
accumulating. The lowest stand of sea level is represented by the sandstone at the
base of the cyclothem, which by its features is best interpreted as fluvial or deltaic.
The coal represents a time when the sea level was starting to rise again, and the
flooding of the river system prevented extensive deposition of siliciclastic sediment
and allowed development of coal swamps. Eventually the site of coal deposition was
flooded by the sea, and limestone and shale was deposited. Then, as sea level fell
again, the river was rejuvenated, and cut into previous sediments to lay down more
fluvial sand.
 The origin of the fluctuations in sea level were controversial for a long time. It’s now
generally agreed that the sea-level fluctuations were not tectonic but eustatic: the
late Paleozoic was by good evidence a time of widespread continental glaciation,
which would have produced substantial and cyclic fluctuation of sea level
worldwide.
 The variability in the nature of the cyclothems from place to place provides further
evidence for coastal deposition during eustatic fluctuations in seal level. At points on
the continent that were at lower elevations and therefore closer to the ocean on
average, a greater percentage of the cyclothems are represented by marine deposits,
whereas at points that were at higher elevations, farther from the ocean, a greater
part of the cyclothems are nonmarine. Coals are most abundant in the cyclothems
that were intermediate in position; in the US, the Pennsylvanian cyclothems richest
in coal are found in Illinois.
Coal Through Geologic Time
Coal was not common before the spread of plants from the oceans onto the land, in
the Silurian. For this reason, the earliest extensive coal deposits date from the Devonian.
Since then, the times of most abundant coal deposition were in the Pennsylvanian, the
Jurassic, the Cretaceous, and the earlier part of the Tertiary—most especially in the
Pennsylvanian. Since the Devonian the time of scantiest coal, by far, was the Triassic. The
reasons for such a grossly uneven distribution of coal deposition through time are not
entirely clear: it must have had to do with the extent of climatic and tectonic settings
around the world favorable to coal deposition. But it might surprise you to learn that there
is some coal even as far back as the Early Proterozoic! Proterozoic coal, minor in extent
and volume, was formed by accumulation and appropriate coalification of algae in certain
marine environments.
Prepared By Md. Asif Hasan
47th Batch

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Evaporites and coal

  • 1. SEDIMENTARY ROCKS Evaporites & Coal Md. Asif Hasan
  • 2. EVAPORITES Enormous volumes of sediment in the ancient sedimentary record are composed mainly or entirely of what are called evaporite minerals: minerals precipitated from a saline solution that has been concentrated by evaporation. Most evaporites in the sedimentary record are marine evaporites (solutions derived from normal sea water by evaporation are said to be hypersaline), but there are also non-marine evaporites. There are a great many evaporite minerals, but only a few are common. It’s been estimated that something like one percent of Phanerozoic rocks are evaporites, and that a quarter to a third of the area of the continents is underlain by evaporite deposits in the subsurface, with thicknesses ranging from a few meters to hundreds of meters. (Think “salt mines”: there really are such things)  The Permian Period was the time of greatest evaporite deposition— presumably because much of the great supercontinent of Pangea lay in a low- latitude belt of continental aridity in what we call, in the present time, the “horse latitudes”, where the troposphere experiences widespread subsidence in the downgoing leg of the low-latitude Hadley cell of the general circulation of the atmosphere.  If you leave dolomite out of consideration (and some nearly primary dolomite must have been associated with hypersaline conditions), the three most common evaporite minerals are gypsum (a hydrated calcium sulfate mineral), anhydrite (an anhydrous calcium sulfate mineral), and halite, NaCl. But the only evaporite you as field geologists are likely to see is gypsum, because halite dissolves so readily in surface waters except in the most arid regions, and anhydrite, being the high-pressure anhydrous form of calcium sulfate, is mostly restricted to depths greater than tens to hundreds of meters.  Are you likely to see evaporites in outcrop? The answer is yes, for gypsum, but no, for halite (the two most voluminous evaporite deposits). Only in the driest of climates—in the interior of Iran, for example—is rock salt exposed at the Earth’s surface.  Evaporites are excellent indicators of paleoclimate: it takes a hot and arid climate for major evaporite deposits to form. As you will see in a later chapter on economic sedimentology, evaporites can form seals for the accumulation of petroleum hydrocarbons in reservoir rocks. On a more prosaic note, gypsum is the mineral that’s used to make plaster and “drywall” (gypsum wallboard).
  • 3.  Evaporite deposits are known from all the continents, with ages ranging from Precambrian to Late Cenozoic (although Precambrian evaporites are scarce, either because they were not deposited or because they have been dissolved away during diagenesis through geologic time). Unfortunately, however, there are no modern evaporite depositional environments representative of the extensive areas of evaporite deposition that existed at various times and places in the geologic past. As with dolostones, this has led to great difficulties and a diversity of competing theories in interpreting the depositional environments of evaporites. Evaporite Minerals anhydrite CaSO4 calcite CaCO3 carnallite KMgCl3 .6H2 O) dolomite CaMg(CO3 )2 gypsum CaSO4 .2H2 O halite NaCl kainite KMg(SO4 )2 .H2 O kieserite Mg SO4 .H2 O langbeinite K2 Mg2 (SO4 )3 magnesite MgCO3 polyhalite K2 Ca2 Mg(SO4 )4 .2H2 O sylvite KCl More than eighty naturally occurring evaporite minerals have been identified. The intricate equilibrium relationships among these minerals have been the subject of many studies over the years. But there are only about a dozen major evaporite minerals. But of the above minerals, only three are of paramount importance: gypsum, anhydrite, and halite.  Gypsum is a calcium sulfate mineral containing water of hydration. It’s monoclinic with one perfect cleavage, and usually white or colorless but sometimes gray or reddish. It’s one of the softest of common minerals: you can scratch it with your fingernail. Its specific gravity is relatively low, 2.32. Although phase equilibria in the CaSO4–H2O system are far from clear, because of the difficulty of studying equilibrium precipitation and dissolution in the laboratory, it seems clear that gypsum is the mineral that is stable at surface conditions and is virtually always the primary evaporite precipitation product.
  • 4.  Anhydrite is an anhydrous calcium sulfate mineral. It’s orthorhombic, has one perfect cleavage and two other good cleavages, and is usually white to colorless but sometimes gray. Its specific gravity is relatively high, 2.93. It is usually seen as massive granular aggregates rather as well formed crystals. It’s stable at higher pressures and temperatures than is gypsum, so gypsum is converted to anhydrite when the evaporite deposit is buried. The deepest reported occurrence of gypsum is about 1300 m.  Halite is a cubic mineral with a perfect cubic cleavage. It’s colorless when pure but can be reddish from iron and various other colors as well. It’s easy to identify by its salty taste. It forms surface outcrops only in the most arid regions. It’s also a relatively low-density mineral: the specific gravity is 2.16. Not all evaporites are marine deposits. Nonmarine evaporites are common, although the volume of nonmarine evaporites is not nearly as great as that of marine evaporites. Nonmarine evaporites are common in continental extensional basins. There is a great variety of nonmarine evaporite minerals. Chemistry of Evaporites You know, of course, that the oceans are salty. The salinity of sea water is close to 35 parts per thousand, ppt (parts dissolved materials, by mass, per thousand parts of bulk sea water, by mass). Generally the salinity varies only slightly from place to place in the oceans, because of dilution and evaporation, although these slight differences are of extreme importance in controlling the circulation and also the biology of the oceans. But in certain unusual situations, the salinity can rise to much higher values, giving rise to evaporite precipitation. Almost all of the salt in sea water is accounted for by seven ions. Here’s a table that lists these ions and their concentration in percent by weight. These seven ions account for 99.7% by weight of all the dissolved salts in sea water. Cl - 55 Na + 31 SO4 2- 7.7 Mg 2+ 3.7 Ca 2+ 1.16 K + 1.10 HCO3 - 0.41
  • 5. Of these, the last is controlled by the equilibrium between sea water and the CO2 of the atmosphere. The dominant control on the rest is the dissolved-salt content of river runoff. Back in 1849 an Italian chemist named Usiglio made a classic, widely cited, but somewhat misleading experiment on evaporite deposition. He took a volume of normal sea water and slowly evaporated it, and kept track of the composition and mass of precipitated salts as a function of extent of evaporation. He found that when the water is reduced in volume to about 50% of the original volume, a little iron oxide and some aragonite are precipitated, but precipitation of the major evaporite minerals doesn’t begin until the volume is reduced to about 20%, when gypsum is precipitated. Then when the volume is reduced to about 10%, halite begins to be precipitated. Further reduction in volume then leads to the precipitation of various magnesium sulfates and chlorides, and finally to NaBr and KCl. In terms of volumes of precipitated salts, experiments like that of Usiglio show that if a column of sea water 1000 m thick is evaporated to dryness, the precipitated salt deposit would be about 15 m thick. Of this, 0.5 m would be gypsum, 11.8 m would be halite, and the rest, 2.7 m, would be mainly salts of potassium and magnesium. But is this how most evaporite deposits are formed? No; read on. Kinds of Evaporite Deposits  Gypsum rock is usually finely granular but sometimes coarsely crystalline. The mode of occurrence of gypsum is rather variable, because, as you will see presently, diagenetic changes are usually far-reaching. Details of bedding are usually not well preserved. Gypsum is also common as nodules in a matrix of carbonate or shale.  Anhydrite rock is usually bedded, often with delicate lamination that’s continuous for long distances. It’s usually fine grained. You seldom see anhydrite in outcrop, however, for reasons that will become apparent soon.  Rock salt is a massive, coarsely crystalline, and nonjointed rock. It sometimes shows bedding, especially by alternation of beds with greater or lesser concentration of nonhalite impurities (gypsum, anhydrite, carbonates, and siliciclastics).
  • 6. Diagenesis of Evaporites Changes in evaporites during burial and unroofing are usually substantial, for three reasons: Evaporite minerals in general are very susceptible to solution and reprecipitation. • Gypsum is converted to anhydrite upon burial, and then the anhydrite is usually reconverted to gypsum as it makes it way to the surface again. When gypsum is replaced by anhydrite, there is a 38% loss in volume, because of the great difference in density between the two minerals. So there’s great extra compaction on the way down (which, incidentally, is conducive to nontectonic deformation, because if the pore water, preexisting and newly released, can’t drain away fast enough, the reduction in solids volume tends to cause a liquefied state in which the pore-water pressure can approach the lithostatic pressure). Conversely, on the way up the anhydrite is reconverted to gypsum, provided that extra water is available. This expansion tends to cause even more local deformation of the deposit. The change from anhydrite to gypsum on the way up is usually delayed until the near-surface zone of influence of surface groundwater is reached. This gypsum–anhydrite diagenetic cycle is shown in Figure : The gypsum-anhydrite diagenetic cycle
  • 7. • Halite tends to flow plastically on a large scale, because it’s relatively weak and because its deposits have a substantially lower bulk density than the “normal” rocks (carbonates and siliciclastics) with which it’s interstratified on a large scale. A horizontal layer of halite lying between layers of denser rock represents a gravitationally unstable situation, and even slight preexisting nonplanarity of the layer leads to uprise of columns or domes of salt, called diapirs, typically on scales of several kilometers. Hence the term salt tectonics. Sedimentary Structures in Evaporites  Do evaporites precipitate as bottom growths or as discrete mineral particles? The former is demonstrable in some cases, but the widespread existence of primary sedimentary structures, like lamination, cross stratification, ripple marks, and graded bedding—just as in siliciclastic sediments and rocks— gives good evidence that the latter is the more important mode of deposition. It’s clear that once evaporite crystals are precipitated they are susceptible to reworking and transportation before final deposition.  Evaporites are highly susceptible to early and significant diagenesis, owing to the extreme solubility of the evaporite minerals. Most of the sedimentary structures in evaporites are diagenetic. Various kinds of postdepositional folds and veins are common. Veins of gypsum cutting fine siliciclastic rocks (mudrocks and fine sandstones), both parallel and oblique to stratification, are c presumably the largely siliciclastic sediment contained an admixture of gypsum, which was remobilized upon shallow burial.  A striking and common diagenetic structure in calcium sulfate evaporites is nodular anhydrite Theories of Evaporite Deposition  The great thickness of some evaporite deposits, as well as the common dominance of gypsum in the deposit, argue against simple evaporation of a body of sea water to dryness. One has to appeal to a continuous evaporation process whereby a water body partially isolated from the open ocean is subjected to net evaporation (evaporation is greater than fresh-water runoff into the basin).
  • 8.  If in such a continuous-evaporation basin there is no outflow of water, only inflow, then all of the dissolved salts must be precipitated somehow, whatever the ratio of sea-water inflow and fresh-water runoff. The common dominance of one or another evaporite mineral suggests, however, that some percentage of the concentrated brine flows out of the basin, somehow, during the evaporation process. Presumably the outflow would contain a disproportionate concentration of the harder-to-precipitate salts. The outflow could be as an outgoing underflow of denser, more saline water beneath an inflowing surface current of normal sea water (Figure A). Or it could be as a gravity-driven diffuse flow through a permeable barrier (Figure B).  If a greater percentage of the water is returned to the open ocean by reflux, then gypsum would be the dominant evaporite, whereas if a lesser percentage of the water is returned by reflux, then halite would be the dominant evaporite. In the least common situation, where an even smaller percentage of the basin water is returned by reflux, the more exotic evaporites would be formed.  Shallow ocean-margin continuous-evaporation basins of the kind described above are a natural way of accounting for the thick and extensive deposits of evaporites seen in the sedimentary record, but keep in mind that no good examples are known from the modern, so it’s all a matter of deduction rather than of observation.  Many evaporite deposits are relatively thin and intimately associated with sediments of other compositions, and show excellent evidence of very shallow-
  • 9. water conditions, like desiccation cracks. An appealing way of accounting for such evaporites is to assume that they are sabkha deposits. A sabkha is a low-lying but supratidal surface along a coast with net evaporating conditions and little supply of siliciclastic sediment. (The adjective supratidal refers to elevations just above the high-tide level.) Most of the time the sabkha surface is emergent, but occasional storms cover the surface with sea water. That water tends to seep down into the sabkha surface, and during later evaporation the water rises again by capillary action, and the dissolved salt is precipitated as evaporite minerals. If the shoreline is prograding, a layer of evaporites some meters thick may be deposited in that way. Figure: Major evaporite deposits of the world Prepared By Md. Asif Hasan 47th Batch
  • 10. CHERT Introduction  Chert is the general term for very fine-grained and nonporous sedimentary rocks that consist mostly or entirely of silica, in the form of either amorphous silica or microcrystalline quartz presumably derived from recrystallization of amorphous silica. The non-scientific equivalent term is flint.  Cherts are fairly easy to identify, even though you can’t see the constituents with your unaided eye, because of the way they fracture and the way they look on fracture surfaces. Cherts are widespread (they are the last of the rocks we’ll consider in this course that you are likely to see commonly), but their total contribution to the sedimentary record is probably not much more than a percent or two.  The crystal size of quartz in recrystallized chert is usually in the range 5–20 μm. Electron microscopy of fractured surfaces shows the quartz to be polyhedral, equant to elongate, and closely fitted to surrounding grains. Cryptocrystalline geometries in the transition from amorphous silica to recrystallized quartz are complex. Thin-section studies don’t help much because the quartz is too fine.  Chert comes in two distinct varieties, nodular chert and bedded chert, whose sedimentological occurrence is rather different. The problems with chert come in its origin; it’s another one of those rocks whose origin we have a hard time observing directly. The relative importance of nodular chert and bedded chert has changed through geologic time: bedded chert is much more common in the Precambrian, and nodular chert is more common in the Phanerozoic. Terminology Here are a few terms for kinds of amorphous silica and chert:  amorphous silica: material composed of relatively pure SiO2 but with only very local crystallographic order. Amorphous silica includes various kinds of hydrated and dehydrated silica gels, silica glass, siliceous sinter formed in hot springs, and (certainly of greatest geological importance) the skeletal materials of silica- secreting organisms (see below, under opal).
  • 11.  opal (or opaline silica) is a solid form of amorphous silica with some included water. It’s abundant in young cherts, back into the Mesozoic. Its geological occurrence is by alteration of volcanic ash, precipitation from hot springs, and, by far most importantly, precipitation as skeletal material by certain silica-secreting organisms (see a later section). Opal starts out as what is called opal-A, which shows only a very weak x-ray diffraction pattern, indicating that any crystallographic order is very local. With burial, during the initial stage of diagenesis, opal-A is transformed into opal-CT, which shows a weak x-ray diffraction pattern characteristic of cristobalite another silica mineral; see below). Upon further diagenesis, opal-CT is transformed into crystalline quartz, resulting in chart that consists of an equant mosaic of microquartz crystals. By that stage, most or all of the fossil evidence of origin is obliterated.  chalcedony is a very finely crystalline form of silica consisting of radiating needles or fibers, often spherulitic, of quartz. There’s probably amorphous silica in among the needles, and a variable water content. This stuff is metastable with respect to ordinarily crystalline quartz, but it hangs around a long time; it’s found even in Paleozoic cherts.  flint is the general-language equivalent of chert, usually applied to dark gray chert in nodules or as beds.  jasper: chert that’s red because it contains hematite (often more than a few percent).  porcelanite (also spelled porcellanite): a minutely porous form of chert with a dull appearance on the fresh surface. Silica Geochemistry The solubility of quartz in pure water is very small, several parts per million.The Figure shows a graph of quartz solubility as a function of pH. You can see that the solubility of quartz is very low for pH values up to about 8 (slightly alkaline) but then rises sharply with increasing pH. It’s hard to measure, but it can be calculated. Moreover, attainment of equilibrium is very slow. The solubility of amorphous silica is an order of magnitude higher, and attainment of equilibrium is also slow, but much faster than for quartz; you can do it in the laboratory. The dominant species of
  • 12. silica in solution in natural waters in the usual range of pH is silicic acid, H4 SiO4 , a weak acid. Figure: The solubility of quartz and amorphous silica at 25°C At room temperature and pressure, amorphous silica is metastable with respect to quartz, but precipitates formed from supersaturated solutions are always amorphous silica. This is because the building of the quartz crystal structure at low temperatures takes a very long time. Solutions unsaturated with respect to amorphous silica but supersaturated with respect to quartz remain stable for many years if not longer. Clear crystalline quartz can’t be precipitated in the laboratory at the low temperatures and pressure of sedimentary environments. Presumably nature can do it because of the longer times involved. The concentrations of dissolved silica in rivers, streams, and lakes are a few tens of parts per million. Concentrations are also in this range in groundwater; the deeper the groundwater, the higher the silica concentration Prepared By Md. Asif Hasan 47th Batch
  • 13. What are the sources of silica in solution?  Weathering of silicate minerals: this is the ultimate source of most of the silica in solution in the Earth’s surface waters.  Thermal springs: the concentration of dissolved silica concentration is very high but the absolute volume is small.  Dissolution of amorphous silica: this must be important in areas underlain by silica-containing sedimentary rocks, but it is certainly not as important overall as weathering of silicates  Dissolution of quartz: most natural fresh waters are in the pH range for which the solubility of quartz is very low, so dissolution of quartz is not an important source of silica in solution. Here’s the bottom line: it’s generally agreed that by far the greater part of dissolved silica comes from weathering of silicate minerals in source rocks. The concentration of dissolved silica in the oceans is surprisingly and extremely small: only a few tenths of a part per million. In the present oceans, there’s no possibility of precipitating silica inorganically. The reason for this very low silica concentration in the oceans is that several kinds of organisms are very effective in extracting silica from sea water and fixing it in the form of opaline silica in their skeletons. They do this out of equilibrium, by metabolic concentration processes. Silica-Secreting Organisms Several kinds of important marine organisms secrete amorphous silica to form part or all of their skeletons: diatoms, radiolarians, and sponges. These organisms play an important part, directly or indirectly, in the deposition of chert. Diatoms :  Diatoms are unicellular photosynthesizing organisms, a kind of algae, mostly from 20 to 200 μm in size. The cell wall of the organism is silicified with opaline silica to form what’s called a frustule, consisting of two valves that overlap one another like the lid of a shallow dish.  Some diatoms are benthic (living on the sea floor), others (by far the most important sedimentologically) are planktonic, living in the photic zone of the oceans (the
  • 14. uppermost layer in the oceans, in which there is abundant sunlight), in less than 200 m water depth. They solve the problem of buoyancy by being fitted with tiny fat droplets. They like cool water best, apparently because of greater nutrient supply, higher water density, and upwelling. At certain times of the year diatom blooms produce concentrations of up to a billion organisms per cubic meter.  Diatoms first evolved in the Cretaceous and have been expanding in importance since. A fairly high percentage of the total number of known diatom species are living today.  Like foraminifera, diatoms rain onto the floor of the deep ocean over large areas. The resulting sediment is called diatom ooze. Fossil diatomaceous deposits are called diatomite, or diatomaceous earth if friable. It’s mined as a filtration medium for water filters. Diagenesis of diatomite leads to diatomaceous chert, and if diagenesis is sufficiently intense, most or even all the evidence of the originally diatomaceous nature of the rock is obliterated. Radiolarians :  Radiolarians are planktonic protozoans with approximately spherical skeletons generally from 100 to 2000 μm in diameter. The protoplasm of the cell is divided into endoplasm and ectoplasm, separated by what’s called a central capsule. The ectoplasm has frothy gelatinous material in which are embedded swarms of symbiotic algae called zooxanthellae, in the shallow-water species. Radiating outward from the central capsule through the ectoplasm are threadlike pseudopods. The skeleton, situated within the cell, consists of radial and tangential elements of highly varied geometry: spicules, spines, bars, spheres, spindles, and cones. The composition of the skeletal material is either celestite, SrSO4 (a strontium sulfate mineral, which is unimportant geologically because the celestite dissolves too fast), or opaline silica. Radiolarians have been around since at least the Cambrian.  Radiolarian species live in a wide range of water depths. They like warmer water. They trap and paralyze passing small plankton with their sticky pseudopods. They maintain buoyancy by fat globules or gas-filled vacuoles.  Like diatoms, radiolarians sink to the bottom and can accumulate to form radiolarian ooze if they are not dissolved before burial. Radiolarian ooze tends to be found at greater depths than calcareous ooze, and at low latitudes. Fossil
  • 15. deposits of radiolarian ooze are called radiolarite, and chert containing radiolarians is called radiolarian chert. The effects of diagenesis are similar to those on diatomaceous cherts. Sponges :  Sponges are filter-feeding organisms that live attached to the bottom in shallow and deep marine environments. They are multicellular but are not considered to be true metazoans because they are not organized into tissues and they have no nervous systems; in degree of organization they fall between protozoans and metazoans.  Here’s how sponges work: they have an upright body shaped like a bag or vase with a hole at the top. The outer surface of the sponge has tiny holes leading inward to small chambers in the wall of the sponge that are lined with cells with flagella that whirl continually to create a current flowing inward into the central cavity. Plankton sticks to the surface of these cells, which then ingest the material. Sponges are thus low-pressure water pumps, which can pump a volume equal to their body volume in a minute.  Sponges have skeletons composed of spongin (an insoluble and chemically inert protein, what you buy as a “natural sponge”), calcareous spicules, or siliceous spicules. It’s the siliceous spicules that we’re interested in here. They can be straight, radiating, or irregular in shape, and they range in size from microscopic to quite large. Silica-secreting sponges have been around since the Cambrian. Nodular Chert  Chert is widespread as nodules in limestone. Chert nodules are varied in shape, from more or less regular discoidal or egg-shaped bodies (that’s the common shape for relatively small chert nodules) to highly irregular knobby and warty bodies (the common shape of relatively large chert nodules). Their size ranges from a few centimeters to a few tens of centimeters. They tend to be concentrated along certain bedding planes. Where abundant, they often form a two-dimensionally or three- dimensionally interconnected network.  Chert nodules are usually structureless, but some show faint traces of stratification coincident with that in the enclosing limestone. If the limestone is fossiliferous, the fossils in the chert can be either calcareous or silicified. And the fossils in the rest of the limestone may or may not be silicified themselves. Sometimes the boundary
  • 16. between the nodule and the limestone passes right through fossils—suggesting that the nodules are a diagenetic feature, not a primary feature.  Although in the past some geologists believed that nodules form by direct precipitation of silica gel on the ocean bottom, today the evidence for a replacement origin is considered to be overwhelming:  irregular shape and interconnectedness of many nodules;  presence of irregular patches of limestone in nodules;  association of chert and silicified fossils in many limestones;  presence of replaced fossils in some nodules;  traces of bedding passing through nodules;  contacts of nodules passing through fossils. But the source of the silica is a problem. Did it come from within the bed or from somewhere else?  The general feeling seems to be that, in most cases at least, the nodules can be explained by the presence of abundant biogenic amorphous silica in the original sediment and then diagenetic reorganization. By diagenetic reorganization is meant the process by which the disseminated bodies of opaline silica (sponge spicules, diatoms, radiolarians) are dissolved, whereupon the silica in solution migrates to certain places in the sediment where it is reprecipitated in the form of opal-CT to form the nodules. This happens because the pore fluids are undersaturated with respect to the original biogenic silica, which consists of opal-A, but are supersaturated with respect to opal-CT, which has lower solubility than opal-A. Frustratingly (for me, at least), the literature on chert nodules never seems to provide the classic “straight answer” for what the controls are on the origin of the nodules: Why do they form where they do? Why is are the size and spacing the way they commonly are, rather than much smaller or much larger?  Where the chert nodules form only a small part of the bulk volume of the rock, a good case can be made that the silica that forms the nodules was present in the sediment from the time of deposition. But how about when the chert forms the greater part of the rock? Then a stronger case could be made for introduction of silica in solution after deposition, by circulating pore solutions.  The chert in shallow marine limestones probably comes mostly from sponge spicules; that in deep marine cherts probably comes mostly from diatoms and radiolarians. In either case, the limestones that contain chert nodules are commonly
  • 17. fine-grained wackestones and mudstones, because the remains of the organisms responsible for the silica were deposited in quiet-water carbonate environments conducive to the various silica-secreting organisms. Bedded Chert Chert is also found as continuous beds, from centimeters up to as much as a few meters thick, often, but not always, interbedded with shale. Bedded cherts are also often interbedded with turbidite sandstones and submarine volcanics. Most such bedded cherts show abundant evidence of having been deposited in the deep ocean. Two scenarios seem most attractive for explaining these cherts:  Open-ocean siliceous ooze is conveyor-belted to subduction margins and incorporated into a subduction mélange.  Siliceous sediment is deposited near a subduction margin, interbedded with subduction-zone volcanics and turbidites shed from the island arc, and incorporated into a subduction mélange. Here we need to distinguish between Phanerozoic bedded cherts and Precambrian bedded cherts.  Phanerozoic bedded cherts usually contain radiolarians, and they can be explained by lithification and diagenesis of radiolarian-rich bottom sediments, although some may have been inorganically precipitated with radiolarians as a nonessential constituent.  Precambrian bedded cherts, on the other hand, show no convincing evidence of having started out as biogenic sediment, inasmuch as no silica-secreting marine organisms are known from the Precambrian. (Some of the oldest and most exotic unicellular organisms are found preserved in Precambrian cherts, going way back into the Archean—but that does not mean that the cherts were formed biogenically from silica-secreting organisms). Most Precambrian cherts seem have been inorganically precipitated, although the processes involved are not entirely clear. The concentrations of dissolved silica in the Precambrian oceans, before the appearance of the silica-secreting organisms characteristic of the Phanerozoic, were probably in the range of tens of parts per million, almost an order of magnitude greater than today. It’s common for such cherts to be interbedded with chemically precipitated ironstones. Some of the very oldest sedimentary rocks, in greenstone
  • 18. terranes, are bedded cherts. Chert is characteristically interbedded, down to centimeter scale, with Precambrian iron formations. FOSSIL FUELS The modern world operates largely on fossil fuels, mainly coal and fluid petroleum hydrocarbons. For almost a hundred years much of the practice of geology has centered around exploration for such fossil fuels, as well as for the “hard” or metallic minerals. It seems important in a course like this to give some attention to the geology of fossil fuels. COAL Have you ever had the opportunity to hold a lump of coal in your hand? The average person”s contact with coal has lessened greatly in the last fifty years, since the great increase in use of oil and natural gas in home heating. Only if you're associated with the mining of coal or its use in industrial steam plants are you likely to have had hands-on experience with coal. But coal represents the world’s greatest remaining storehouse of energy—for better or for worse. Coal represents almost 90% of the world's recoverable reserve of fossil fuels. The United States, with about 20% of the world’s coal supply, is well endowed.  Coal is a sedimentary rock! It could be defined as a combustible rock that had its origin in the accumulation and partial decomposition of vegetation. That’s akay as far as definitions go, but it’s not very descriptive.  Coal is found to be interbedded with other sedimentary rocks you might consider to be ordinary rather than extraordinary: sandstones, shales, and limestones. Coal itself, however, should be viewed as a rare sedimentary rock, albeit widely distributed: even in the relatively few formations around the world in which it is found, coal constitutes only a small percentage of the stratigraphic section, rarely more than one or two percent and often much smaller. But in absolute terms, the quantity of coal remaining after centuries of mining is staggering: it has been estimated that there's something like 1015 to 1016 kilograms of coal locked up in the Earth’s continental crust.  Coal is found in beds (or seams, in coal terminology) ranging in thickness from just millimeters to many meters. Typical thickness of coal beds is half a meter to a few meters.
  • 19. Properties and Terminology Coal varies greatly in its properties, depending in part upon its composition but for the most part in the degree of diagenesis or even metamorphism it's undergone. This degree of diagenesis is called the rank of the coal. In terms of extent of diagenesis, coal ranges from low-rank (brown, porous, semilithified, and of low density, something like 1.0 g/cm3) to high-rank (jet black, hard, nonporous, hard, and much more dense, up to almost 2.0 g/cm3). Figure shows this spectrum, with conventional names along the way. You can see from Figure that the principal way- stations along this spectrum are lignite (brown coal) → bituminous (soft coal) → anthracite (hard coal). Lignite burns readily but with a smoky flame; anthracite is hard to ignite but burns with a clean, hot flame. Material even less diagenetized than lignite is called peat, which is a porous aggregate of largely nondecomposed but stable plant residues. In some areas peat is mined as a domestic fuel, in addition to being ground up for agricultural and horticultural use. At the other end of the spectrum, under conditions of real metamorphism (the interbedded rocks then being metamorphic rather than sedimentary), anthracite coal is converted to meta- anthracite, and finally to graphite. Composition Almost by definition, coal consists mostly of carbon. The plant materials from which coal is derived are largely carbohydrates of various kinds, only the most resistant of which (mainly cellulose and lignin) remain after partial decomposition after death of the plants. The initial plant residues that are buried to become coal therefore consist largely of carbon even at the very beginning. But coals—even lignites—contain appreciable percentages of other constituents as well. Here’s a list:  Nitrogen: a couple of percent; doesn’t vary much. Probably from the organic matter itself, not from entrapped air.  Sulfur: small percentages, a couple of percent, but undesirable because of production of sulfuric acid (the main constituent of acid rain) upon combustion.
  • 20.  Water: varies with rank from a few percent to as much as 90% (conventionally measured after drying at a temperature a little greater than 100 °C, to get rid of liquid water in pore spaces).  Gases: CO2, O2, N2, CH4, variable percentages.  Ash: the solid residue upon combustion: sand, silt, and clay in variable proportions, either carbonate or siliciclastic (mostly the latter). From fractions of a percent in the cleanest coal to such large values that the rock should be called a carbonaceous shale or a carbonaceous sandstone rather than coal. Very impure coal is called bone coal. Figure: The rank of coal in relation to a carbon-hydrogen-oxygen composition triangle Figure shows one segment of a composition triangle whose end members are percent of carbon, hydrogen, and oxygen. Only the area nearest the carbon corner is occupied by rocks we would call coal. You can see that the increase in rank is associated with a progressive decrease in the percentages of hydrogen and oxygen, presumably owing to driving off of the volatile constituent water.
  • 21.  The plant constituents of coal have been classified both macroscopically and microscopically. The basic idea is that all coal is composed of a small number of kinds of fragments of plant debris called macerals, which are analogous to the minerals of an ordinary sedimentary rock.  Macerals represent such things as branches, twigs, leaves, bark, interior tissue of various kinds, and pollen or spores, among many others. Study and classification of coal macerals is highly botanical and can be done only with the aid of a microscope.  The macroscopic study and classification of coals, on the other hand, while not as fundamental, is easier to deal with. Coal has long been recognized to consist of just a few macroscopic constituents, usually interlaminated. These constituents form strata that are typically from fractions of a millimeter to tens of millimeters thick.  vitrain: brilliant, vitreous (glassy-looking), jetlike coal with conchoidal (shell- like) fracture  clarain: coal layers that appear silky from the presence of very delicate internal lamination  durain: dull, lusterless, matte layers of coal with a close or dense texture, without internal lamination  fusain: friable and highly porous coal, usually appearing as irregular chips and wedges lying along the bedding; often called mineral charcoal. Origin  Coal can form wherever growth of vegetation is abundant enough, and accumulation of the sediment is scanty enough, that plant material can accumulate in high concentrations and large quantities before complete decomposition. For this, one has to appeal to extensive swamps, usually termed coal swamps, either fresh water or sea water (probably mainly fresh water) in climatic conditions conducive to lush growth of vegetation and far from sources of siliciclastic sediments.  Most coal seems to have formed in place, by gradual accumulation of plant material right where it grew. You can imagine thick accumulations of earlier plant material into which the present crop puts down its roots, only to succumb eventually and form the substrate for yet another crop. Such coal is said to be autochthonous. Some coal, however, seems to consist of plant fragments that were transported far from where they grew, presumably by flowing water, and deposited in some rather
  • 22. different sedimentary environment—but again one without an abundance of “ordinary” siliciclastic sediment. Such coal is said to be allochthonous.  The overall association of other sedimentary facies with coals—mainly shallow marine and fluvial sediments—tells us that, broadly, coal accumulates in coastal environments of one kind or other. Perhaps the most common kind of environment of this kind could be termed deltaic. Imagine a broad river carrying mud and sand to the shoreline. The river flow in deltas tends to be well channelized, with strong flows carrying sand to the channel mouths. Mud carried by such channels is either spilled widely over the banks of the channels along the way or disgorged into the sea at the mouths of the channels. In certain settings, in between the channels are low-lying areas that receive little fluvial sediment and are conducive to dense vegetation. Such areas tend to experience slow subsidence, from compaction of earlier-deposited sediments; this subsidence makes room for further accumulation of plant materials. (Keep in mind that there must be great compaction of the plant material as it's buried.) Cyclothems  The coastal nature of most coal is emphasized by the mode of occurrence of late Paleozoic coal. (You will see below that the Pennsylvanian was one of the great epochs of coal deposition around the world.) Most Pennsylvanian coal is found in distinctive cyclic units called cyclothems. A cyclothem consists of a systematic alternation or cycle of sedimentary deposits that represent a regular alternation of depositional environments.  Interpretation of a cyclothem like that shown in Figure 12-4 is clear: there’s a cyclic alternation of marine and nonmarine deposits. The nonmarine part of the cyclothem extends from the disconformable base of the sandstone to the coal; the rest of the cyclothem represents shallow-marine deposition. We are forced to assume that there was a cyclic rise and fall of sea level relative to land, to produce inward and outward migration of the shoreline over the area where the deposits were accumulating. The lowest stand of sea level is represented by the sandstone at the base of the cyclothem, which by its features is best interpreted as fluvial or deltaic. The coal represents a time when the sea level was starting to rise again, and the flooding of the river system prevented extensive deposition of siliciclastic sediment and allowed development of coal swamps. Eventually the site of coal deposition was flooded by the sea, and limestone and shale was deposited. Then, as sea level fell again, the river was rejuvenated, and cut into previous sediments to lay down more fluvial sand.
  • 23.  The origin of the fluctuations in sea level were controversial for a long time. It’s now generally agreed that the sea-level fluctuations were not tectonic but eustatic: the late Paleozoic was by good evidence a time of widespread continental glaciation, which would have produced substantial and cyclic fluctuation of sea level worldwide.  The variability in the nature of the cyclothems from place to place provides further evidence for coastal deposition during eustatic fluctuations in seal level. At points on the continent that were at lower elevations and therefore closer to the ocean on average, a greater percentage of the cyclothems are represented by marine deposits, whereas at points that were at higher elevations, farther from the ocean, a greater part of the cyclothems are nonmarine. Coals are most abundant in the cyclothems that were intermediate in position; in the US, the Pennsylvanian cyclothems richest in coal are found in Illinois. Coal Through Geologic Time Coal was not common before the spread of plants from the oceans onto the land, in the Silurian. For this reason, the earliest extensive coal deposits date from the Devonian. Since then, the times of most abundant coal deposition were in the Pennsylvanian, the Jurassic, the Cretaceous, and the earlier part of the Tertiary—most especially in the Pennsylvanian. Since the Devonian the time of scantiest coal, by far, was the Triassic. The reasons for such a grossly uneven distribution of coal deposition through time are not entirely clear: it must have had to do with the extent of climatic and tectonic settings around the world favorable to coal deposition. But it might surprise you to learn that there is some coal even as far back as the Early Proterozoic! Proterozoic coal, minor in extent and volume, was formed by accumulation and appropriate coalification of algae in certain marine environments. Prepared By Md. Asif Hasan 47th Batch