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Day 5
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| Quaternary: | Obviously young deposits, retained from Steno. | |||
| Tertiary: | Young deposits with familiar looking fossils, retained from Steno. | |||
| Cretaceous: | Meaning chalk, after the white cliffs of Dover and similar deposits in France and Britain. | |||
| Jurassic: | After exposures in the Jura, part of the Alps between France and Switzerland. | |||
| Triassic: | Three parts. Three beds in England were grouped into this period. | |||
| Permian: | After exposures in Perm in the interior of Russia. | |||
| Carboniferous: | The Coal Measures. | |||
| Devonian: | After Devonshire in England. This is the oldest occurrence of land plants. | |||
| Silurian: | After localities in Wales. | |||
| Ordovician: | This period occurs in the modern time scale, but was not in use in 1850. The British geologists, Adam Sedgwick (1785-1873) and Roderick Murchison (1792-1871), could not agree on how to divide this part of the time scale. The pointless feud continued until after their deaths. Charles Lapworth (1842-1920) recognized that time is continuous and that the divisions of the time scale are for our convenience not our enslavement. He added this period as a compromise in 1879. It is based on localities in Wales. It did not become the global standard until 1960. | |||
| Cambrian: | After localities in Wales. This is the first occurrence of macroscopic hard-shelled marine animals. | |||
| Precambrian: | Anything older than Cambrian where there are no obvious large fossils. | |||
The geologists recognized that Tertiary and Quaternary fossils resembled modern life. They grouped these periods into the Cenozoic or Cainozoic Era (Ceno = recent; zoic = animals.) The Cretaceous, Jurassic, and Triassic rocks have an intermediate resemblance to modern life. They grouped these periods into Mesozoic Era (Meso = middle). They grouped the Permian through Cambrian Periods into the Paleozoic Era (Paleo = ancient). They further grouped the time with decent fossils (Cambrian and later) into the Phanerozoic Era (Phanero = obvious). This avoids having to say post-Precambrian. Modern geologists tweak the time scale as more is learned. They have greatly subdivided it. Fossils are still the best way to date most sedimentary rocks.
Three features of fossils preserved in the geological record were evident in 1850. Starting from the bottom up.
(1) The appearance of large fossils in the Cambrian was sudden. A high diversity of fossils occurred just above of beds devoid in large fossils.
(2) Mass extinctions of fossil organisms occurred. The most profound were at the ends of the Paleozoic and Mesozoic eras. The diversity of life increased toward its former levels after the extinctions.
(3) Bones of many large mammals exist in recent beds. These organisms are now extinct. The saber-toothed tiger in North America is a familiar example.
In 1850, geologists could still interpret these events in terms of gradual change or catastrophes. In fact, several architects of the time scale were catastrophists. These included the Frenchman Georges Cuvier (1769-1832), Sedgwick, and Murchinson. However, the later catastrophists were gradualists on many issues. William Buckland, for example, in his 1837 text recognized the great antiquity of the Earth. He argued quoting Galileo that the Bible should not be taken literally and that scientific knowledge is provisional. He provided strong arguments, basically those of da Vinci, against the Flood. (da Vinci’s work was rediscovered in the late 1800s after Buckland published.) Later he showed that “drift” is a glacial deposit from the Ice Age, undermining the last rational pillar for the Flood. He relegated (but at great length) divine “design” to preparing the Earth for mankind and organisms for their ways of life.
The issue of the importance of natural catastrophes (as opposed to magical ones) has not been fully resolved. I get back to this later with asteroid impacts. To make progress after 1850, geologists needed to assign numbers in years to their relative age scale.
The dust on antique time would lie unswept. (William Shakespeare (1564–1616), The Oxford Shakespeare, 1914. Coriolanus, Act II. Scene III.) Everyone knows that dust accumulates on surfaces. The Brown family returns to San Francisco from LA.
| Stella: | Billy there is dust all over your desk. Clean it up. | |||
| Billy: | Of course there is dust. We have been in LA for a week. I will get to it later. | |||
| Sally: | Billy, there is much more dust on your desk than mine. Look! Your dust is four times thicker. You must not have cleaned anything in your room for a month. Do you expect the rest of your family to live in a pigpen? I have friends coming in the morning. | |||
Sally’s method is that of nineteenth century geologists. She notes that a layer of dust from a week is on her desk. Billy has a layer four times as thick so he has not cleaned for a month. Her assumption is that the rate of dust accumulation is constant.
Geological application of this method dates from antiquity. Circa 460 B.C. A young Greek is determined to see the world. The prosperity of Athens and a period of relative peace has made this possible. He arrives at the Nile coast. There are already ancient statues partly buried by river sediments. With local help, he reads the inscriptions. The monuments are over a thousand years old. Seeing that this ship is pushed by the river current in the channel, but not pushed when it is out to sea, Herodotus realizes that sediments carried by the river drop to the bottom when the water enters the ocean. They then accumulate. The delta (his term from its shape like the Greek letter) built seaward as successive batches of sediment dropped at the end of the channel. (Figure 16) He correctly surmises that the surface of the delta that he can see has taken thousands of years to form.

Figure 16: Topography and bathymetry map shows the Nile Delta. The Nile flows north and splits into several channels near “D”. The river carries sediments into the sea. Over time 10-kilometer-thick deposits have accumulated where the river enters the sea. The coastline was more or less straight before deposition began, but now bows out toward “H.” Herodotus did not know how deep the sea was but correctly deduced that river sediments cover the DELTA-shaped region between the channels.
In retrospect, Herodotus did quite well in dating the time since sealevel stabilized at the end of the ice age, 3,500 years before his time. He had no way of estimating the total thickness of sediments in the delta. He did not even know the depth of the deep Mediterranean filled by the delta. There are over 10 kilometers of sediment at the place where Herodotus stood. Their accumulation rate measured reasonably by Herodotus is around a meter per thousand years. So it took somewhere around 10 million years for the sediments to build up.

Figure 17: Sediments cover most of the seafloor. Here white sediment dusts dark basaltic outcrops on the seafloor. Sediment covers the low-lying areas, but currents keep dust from accumulating on the exposed basalt. The sedimentary particles are sand-sized fossils from one-celled planktonic (drifting) organisms called foraminifera. They make nice microfossils for dating rocks. Photo by the author.
It was easy for nineteenth century geologists to measure the thicknesses of exposed sedimentary beds and add them up. This method gave similar results to the one discussed above. It left a lot to be desired. It is obvious that erosion rather than deposition occurs in many localities. Vast intervals of time could be missing in a geological section. The sedimentation rate obviously differed from place to place. It was also evident to many that several intervals of deposition, mountain building, erosion followed by more deposition occurred.
Old as the hills: a good do it yourself project involves using the sediments behind a dam to estimate the rate of erosion. In turn, this lets you estimate the age that the landscape from the total amount of erosion. [see Do it Yourself Box with a Dam]
1835. A young naturalist arrives on the coast of South America. His father reluctantly pays his way. He does not want his son to become an idle country gentleman. The British expedition is supposed to survey the coast and study the region on the shore. There is an immediate problem. A large earthquake has heavily damaged the port of Conception.
Charles Darwin (1809-1882) had felt the shaking far away a few days before. He gets right to work. The earthquake has uplifted the seacoast exposing lots of shells for collection if one can stand the stench. Later, he travels over the Andes Mountains. He correctly surmises that the many earthquakes over a period of millions of years gradually uplifted the range. One of Darwin’s other interests would bring the number of years in geological time to the limelight.
1859. Darwin publishes Origin of Species. He explains the evolution of fossil and modern life forms by descent with modification. This is not new. (The idea of the transformation of species was notorious by 1837. Buckland devoted much text to its refutation.) But Darwin demonstrates a viable mechanism, natural selection. Organisms with more fit inheritable characteristics tend (by definition) to be more successful in breeding. The beneficial modifications build up in the population over time and harmful ones die out. The process is similar to artificial breeding of domestic animals and plants. Over the vast length of geological time, all life descends from one (the modern answer) or at most a few common ancestors.
I get back to evolution later. Right now time is of the essence. Darwin has excellent observations of how fast animals can be modified by artificial selection. He has some idea on how little wild animals and plants have changed since antiquity. He offers a guess on how long evolution in the Phanerozic era (when there are descent fossils) has taken, several hundred million years.
Although Darwin is careful not to directly mention the evolution of humans from animals until a later book, the implication is obvious to all. At one end, animal breeders do not need to be convinced that traits are heritable. The British gentry are sure of their superior bloodlines. Social Darwinists muddy the water by considering the plight of the poor to be a beneficial form of natural selection. At the other, national selection is not for the squeamish. The gentry do not like having their ape ancestors pointed out anymore than they would ancestors hanged for horse theft. Churchmen do not like humans evolving by a natural process. Unlike the case of Galileo, the Hebrew Bible is explicit on the issue. The creation stories involve God and man, not monkeys and apes. However, Darwin and his supporters are never in physical danger. Neither do they have their activities restricted in any way. The debate proceeds, often civilly. Much of it stays on scientific issues, not religion.
Part of the debate focuses whether there has been enough time for evolution. Natural selection is slow, all agree. Perhaps inheritance of acquired characteristics worked a lot faster. This “Lamarckian” form of evolution now seems silly to us, especially when presented as a caricature. . Like one could breed tailless cats by cutting off the tail in each generation. Little is known about heredity in 1859. Darwin does not reject Lamarckian evolution altogether. It would have been premature for him to do it. Lamarckian inheritance is a testable scientific hypothesis that does not pan out; it is not an appeal to magic.
Of course, the often-explicit fallback is that if natural selection does not work, neither does evolution. This lets in various forms of somewhat old-Earth divine intervention.
Roast turkey.
| Brown family house Thanksgiving. | ||||
| Billy: | Why can’t we eat now? The turkey has been in the oven for over an hour. It must be done by now. | |||
| Jordan: | Read the turkey wrapper. It says a 24-pound bird takes 3 and a-half hours. | |||
| Sally: | Why is this? It takes only ten minutes to make fish sticks. | |||
| Stella: | It takes time for heat to flow from hot to cold. The skin of the turkey gets hot right after we put it in the oven. Heat flows slowly into the turkey. The outer part of the turkey is cooked but the center is still raw. If we took the turkey out now the raw meat would taste dreadful and might make us sick. | |||
| Sally: | Do fish sticks cook faster than turkey because they are thinner? | |||
| Stella: | Yes. The fish sticks also cool off much quicker than the inside of the turkey when we take it out of the oven. | |||
Late nineteenth century geologists viewed the Earth much like the cooling of the turkey after it left the oven. The principle of conservation of energy was a recent major accomplishment. Beginning with Jacques Fourier (1768-1830), it became possible to mathematically compute the variation of temperature within a body cooling by conduction. (For those who know French, Fourier’s name relates to his family’s involvement in the fur trade not the oven business.) Basically, the time for a body to cool depends on the square of its thickness. As in the case of the cooling turkey, the thickness of the outer cool region of the Earth increases with the square root of time.

Figure 18: Lord Kelvin modeled cooling of the Earth after it formed. The Earth cooled quickly until it froze at the melting curve. It cooled after that by conduction. The geotherm at a past time is hotter than the modern one. Kelvin could only measure the geotherm at a shallow depth (ellipse). Kelvin’s cooling depth is shallow enough, about 100 kilometers, that a flat model and drawing work OK. Kelvin used spherical geometry, which gives a more precise result, but the basic assumption of conduction is incorrect.
William Thomson (1824-1907), later Lord Kelvin, computed sophisticated models of the Earth cooling from its initially hot state ending around 1900. Unlike the turkey, spherical symmetry provided some simplification. His other assumptions were simple and logical. The Earth formed by the collapse or accretion of rocky material. He easily showed that the gravitational energy of this material was more than enough to melt it. The molten Earth convected like soup on a stove until it froze to a solid. Afterwards, it cooled slowly by conduction.
Kelvin could guess the initial conditions after the Earth first froze (Figure 18). Scientists knew the melting temperature of rocks to some extent. They also knew from tides that the inside of the Earth is mostly solid. (Modern seismology confirms that the outer 2900 km of the Earth is solid rock.) Volcanoes are local features that tap small amounts of partial melt.

Figure 19: A dried up apple provides a model for mountain building. Soon after its formation, the outside of the Earth is a cool rigid spherical shell (red). The inside is still hot. Over time the inside cools and contracts. This wrinkles the surface producing folds. The net contraction of the Earth’s circumference is several tens of kilometers. It was not evident in the 1800s that this amount is insufficient to produce the observed mountains. The process does deform the surfaces of Mars and the Moon so it is just the wrong hypothesis for our planet.
He had reasonable constraints on the present thermal state of the Earth. The invention of reliable explosives allowed miners to dig deeply. Deep mines are hot and become hotter as one goes down. The need to keep the miners cool is one limit on the practical depth of mines. (Note that shallow caves and mines equilibrate to about the mean annual temperature. They feel cool if you go in on a hot day.) Kelvin extrapolated the thermal gradient in mines downward to great depths. The thermal gradient could not continue down forever. Otherwise, the temperature would exceed the melting point of rocks. Kelvin used the intersection of the extrapolated temperature with the melting points of rocks to get the thickness of the cool rind that had formed since the Earth became solid. He got less than 100 kilometers. (This is a modest underestimate for England.) It takes tens of million years for the Earth to cool to this depth. To boot, Kelvin calculated the time for the Sun to cool. He got a similar number. This was far less than Darwin wanted. It seemed that natural selection was in deep trouble from basic physics.
Kelvin’s hypothesis provided a testable prediction (Figure 19). The outermost rind of the Earth cooled quickly to the surface temperature, like the skin of a roast turkey on the platter. Later the shell inside of the surface cooled. Rocks contract when they cool. (Bridges and roads have expansion joints so that daily heating and cooling does not produce cracks.) Contraction of the inside of the Earth caused the weak outside layer to crumple, much like the wrinkles in a dried apple. This provided an attractive mechanism for mountain building. Too little was known at the time to apply this test. This mechanism is not applicable to the Earth where there are plate tectonics. It is applicable to the Moon and much of the history of Mars.

Figure 20: Osmond Fischer modeled the cooling of the Earth by convection. The Earth consists of a thin rigid shell and an underlying convecting region. The entire deep interior of the Earth cools as a well-mixed fluid. It contains a lot more heat than does the shallow shell. The past geotherm is not much different from the present one. One cannot get the age of the Earth from the geotherm because the thickness of the lid may change with time in addition to the interior temperature. The entire Earth is cooler than the melting curve. Most geophysics did not think that solid rock could flow as a fluid until the late 1960s.
Kelvin’s reasoning came under scientific attack from Osmond Fischer (1817-1914) (Figure 20). He concentrated on Kelvin’s assumption that the Earth behaves as a conducting solid. If the inside of the Earth convected (like in Kelvin’s models of the inside of the Sun), the thickness of the outer cool rind had no simple relationship to the Earth age. In Kelvin’s model, heat could come only from the thin rind as the deep interior of the Earth stayed at its original temperature. In Fischer’s, it came from the entire interior of the Earth. There was plenty of heat to keep the inside hot for a few billion years.
Fischer’s idea of a solid that could convect slowly like a fluid was too strange in the late eighteen hundreds. It seemed absurd to most geophysicists until geologists amassed overwhelming evidence of plate tectonics in the 1960s. In the meantime, science discovered radioactivity. Convection in the Earth’s interior seemed unnecessary. Fischer died a forgotten man.
A gentlemen’s wager. Late 1800s. Physics seems to be close to a solved field. James Clerk Maxwell (1831-1879) unifies the previously mysterious effects of magnetism and electricity with 4 simple equations. He shows that light is a form of electromagnetic radiation. His equations will become the basis of radio communication through another form of electromagnetic radiation. Gravity and mechanics seem well in hand. Thermodynamics provides the platform for understanding chemistry and heat flow.
Problems remain but seem obscure, like astronomers not being able to predict the orbit of Mercury. All this changes when Henri Becquerel decides to investigate phosphorescence. You have probably seen glow-in-the-dark plastic. To glow, it needs to be exposed to light. The material absorbs energy from the light and later readmits it as light. Eventually, the glow material runs down. This process involves transformation of light energy into chemical energy in the material and then back to light energy. It is interesting and in full accord with conservation of energy.
Becquerel studies a uranium salt using film to detect feeble amounts of phosphorescence. One day it is dark and cloudy. He cannot expose his samples to sunlight so he tries to detect light from samples that had been in the dark as a control. Scientists frequently run controls, like sugar pills in medical trials. The uranium samples expose the film. This should not have happened as it violates conservation of energy.
Becquerel and Marie and Pierre Curie go right to work to repeat the experiment to see what is happening. Natural uranium minerals emit three classes of rays. The first called alpha is easily stopped by paper. It is deflected by magnetic fields and hence electrically charged. Further work, shows that alpha particles have two positively charged particles, called protons, and two neutrally charged particles called neutrons. They are the same as the nucleus of a helium atom. Beta particles turn out to be electrons and gamma rays are high-energy electromagnetic radiation. A uranium atom decays to a lead atom over a series of steps and produces several helium atoms in the process. The decay produces lots of energy. The element radium discovered by the Curies glows in the dark. It will be used to make luminous watch dials, which are now banned as dangerous. You may be able to find one if you or a relative is over 50 and a packrat.
It is painstaking but straightforward to determine the rate at which uranium atoms decay to lead and produce helium. The most common form of uranium has an atomic mass of 238 (that is, it is about a factor of 238 heavier than a proton). It contains 92 protons and 146 neutrons. It decays in a series of steps into lead-206 (82 protons and 124 neutrons) and 8 helium atoms (each with 2 neutrons and 2 protons). The uranium-238 decays with a half-life of 4.51 billion years. That is, if we had a sample of uranium-238, half the uranium would turn to lead in that time. In another 4.51 billion years 3/4 of the uranium would have turned to lead.
Uranium decay provides an immediate method of dating rocks. Uranium minerals that initially had very little lead or helium are most easily studied. One gets an age merely by measuring the amount of helium or lead and the amount of uranium in a crystal and making a simple calculation on the number (actually less than 1 for Earth samples) of half-lives that had occurred. This method works in practice on Precambrian rocks.
1904. A young scientist presents his results on the dating of some rocks with helium produced by uranium decay at the Royal Institution in England. He has samples over a billion years old. Ernest Rutherford (1871-1937) realizes that Lord Kelvin is in the audience and is wide-awake at the key point of his talk. His ages are far older than the acceptable range given by Kelvin’s calculations on the cooling of the Earth. He is prepared for this and states that Kelvin’s calculations assume that there is no unknown heat source in the Earth. Radioactivity is that that heat source and Kelvin’s calculations, though correct, are inapplicable to the Earth.

Figure 21: Geochronologists date rocks using trace amounts of uranium and lead in zircon crystals. The crystals grew like tree rings (called zoning). This makes it possible to date several events in the history of the rock. Image by Chris Mattinson.
Later the scientists retire for dinner at an estate. Kelvin is intrigued with radioactivity but does not yet know much about it. It is not clear to him that there is enough radioactivity in the Earth to matter. He is still skeptical that radioactivity really exists. He makes a bet of several pounds with Robert John Strutt (later the 4th Lord Rayleigh) on whether radioactivity exists and heats the interior of the Earth. He pays off within a year.
Today, scientists no longer need uranium minerals to study uranium decay. They have precise equipment that can measure minute amounts of uranium and lead. The mineral zircon (zirconium silicate) is particularly useful (Figure 21). So is natural cubic zirconia. Uranium atoms substitute for zirconium atoms in minor amounts. Very little lead enters the crystal when it forms. Once formed zircon crystals retain their uranium and the lead produced by its decay. They even sometimes survive partial melting of a rock in the Earth’s crust. The oldest dated samples on the Earth are 4.4 billion-year-old zircon grains within beds that were originally (over 3 billion years ago) sedimentary sandstones.
Geochronologists routinely use several radioactive parent-stable daughter pairs to date rocks. Radioactive dating works well to determine when igneous rocks froze. It can be used to tell when rocks cooled beneath a given temperature. It works poorly with sand in that each grain retains the properties of its source rock, like with the 4.4-billion-year-old zircons. Geologists use contact relationships, like interbedded volcanic rocks, to link the fossil time scale with the radioactive one. This is still being done, but the gross ages are known.
As Darwin suspected, geological time is vast. Humans, depending on how one defines that term, have been around for a few million years. Modern man evolved about 100,000 years ago. The end of the Cretaceous period occurred 65 million years ago. The Cambrian period began 540 million years ago. The oldest preserved sediments on the Earth are around 3.9 billion years old. The Earth itself is about 4.5 billion years old. The oldest meteorites and the solar system are about 4.55 billion years old.
Vestiges of Steno’s and Werner’s thinking persisted even after the advent of radioactive dating. You can guess the age of a car by how beat up it looks. On average, a banged up car is older than a shiny one. However, a new car can get lots of dents if one drives it off road. With respect to geology, it is obvious that fresh looking sediments on the beach are young. However, the Earth is quite geologically active. Sedimentary rocks get buried to great depths, heated to high temperatures, and then sometimes get exhumed to the surface. The deformation and heating of sedimentary rocks, called metamorphism, tends to destroy sedimentary structures and fossils originally in the rock.
Geologists believed that highly metamorphosed rocks were quite old. Even in the 1960s, the official policy of the United States Geological Survey was that all highly metamorphosed rocks were Precambrian unless conclusively demonstrated otherwise. This resulted in absurdities. For example, a bed with Devonian fossils in Maine was mapped Devonian at the fossil locality but Precambrian elsewhere. The official philosophy was that radioactive dating was to help mapping in areas of poor exposure. This assured that field relations could not be used to extrapolate the results. Eventually, dating became routine, the idea that the intensity of metamorphism was an indictor of age died out.
It’s dark at night. Bruno angered the Church both by pointing out the insignificance of the Earth and even the solar system as well as stating that time is infinite. He had little evidence on how old the universe is and no one did until the 1920s. Yet some problems with an infinite universe were evident at that time.

Figure 22: The sky should be bright at night if there are an infinite number of stationary stars (here shown close together to get a workable drawing). Then a line of sight from the Earth will eventually intersect the surface of a star. Alternatively, the light coming from the shell-shaped region between the green circles is independent of its distance (radius) from the Earth because the number of stars in the region increases with the radius squared while the light from each star decreases with the radius squared.
The dark night sky was a serious problem. If there were infinite numbers of (statistically) equally spaced stars, the sky would appear as bright as the surface of the Sun. This can be seen into two ways. First, a line of sight drawn in any direction eventually hits the surface of a star. The second more mathematical one involves imaginary spherical shells (of say 1 light year thickness) at distances R from the Earth. Each shell contains a number of stars proportional to R squared. The brightness of each star is proportional the inverse of R squared (Figure 22). Thus the total light from each shell is proportional to R squared stars divided by the inverse square law for light or a constant. We can add up a very large number of shells to get a bright sky.
Halley faced this problem. He realized that a finite universe would collapse towards its center. He preferred an infinite universe where no center exists. Halley contended that light from the more distant stars gets absorbed by passing through space. Light does get absorbed when passing through ordinary materials. This looked good at the time, but the absorbed light would heat up space and reradiate the energy. Astromers observe only feeble light sources from reradiated light. The existence of galaxies provides no solution. Stars are irregularly spaced but the problem remains if galaxies themselves are infinite in number.
The answer came from mundane studies to resolve the motions of stars and galaxies. Stars preferentially emit light radiation at given wavelengths where the energy matches that to change an atom (or molecule) from one energy state to another. Conversely gases surrounding a star absorb specific wavelengths. A prism produces a spectrum where these bright emission bands and dark absorption bands are evident. The wavelength (position of a band in the spectrum) is known. It depends on the physics of the energy states.
The wavelength of light from a star moving away from us is longer (redder) than it would be if the star were stationary with respect to us. Conversely, the light has shorter wavelength if the star is approaching us. This Doppler effect is the basis for radar in speed traps. A simple calculation gives the velocity of the car or the star. A similar effect occurs with sound. An approaching train is more high pitched than a receding one.
In the 1920s, telescopes were good enough to resolve stars in nearby galaxies, showing that they were vastly farther away than the stars in our own Milky Way. Astronomers inferred the distance of other galaxies using a variety of standard candles and took spectra. Nearby galaxies do not show any systematic motion, but all distant galaxies flee away from the Earth, the farther the faster. It was tempting to place the Earth stationary at the center of this motion. However, astronomers saw nothing special about our Sun or even our galaxy. Their solution would have pleased Bruno. All space is expanding on the scale of moderately distant galaxies. An observer on a distant galaxy would see everything fleeing her. A two-dimensional analogy is the surface of a rubber sheet. Spots on the sheet move away from each other as the sheet expands (Fig 23).


Figure 23: The expanding universe is shown at 4 times in 2-D. Red open square indicates region around the Milky Way “M” and another galaxy “K” in upper left of box. An observer on any galaxy “G” sees other galaxies moving away, the farther the faster. The galaxies themselves and the solar system are gravitationally bound and do not expand. One obtains the age of the Big Bang by working back to where everything was at a point.
It was a simple matter to take the velocities and the distances and to see when the universe began to inflate from a point. The early results were only a few billion years; that is less than the age of the Earth. This did not please anyone, particularly geologists who held older rocks in their hands. The velocities were good because only the Doppler effect is involved. It turned out that the distances were systematically underestimated. The current result is 13.7 billion years. Expansion quenched the worry from Halley’s time about the universe immediately collapsing under its own gravitation.
This Big Bang hypothesis yielded a testable prediction that resolved the dark sky problem. Matter was closely packed early in the Big Bang with temperatures and energies (after a slight amount of time) crudely like those in an atomic accelerator or a nuclear explosion. Physicists are familiar with these conditions. Early on, space was optically thick. It was filled with high-energy light, which was absorbed as soon as it was emitted. About 300.000 years after the big bang, space became transparent. Almost all of the light that existed at that time has continued on unimpeded.
A minute fraction of this light is now arriving at the Earth. Its sources are the age of the universe minus 300,000 light years away. They are fleeing us at almost the speed of light. The light is red-shifted by the Doppler effect into feeble radio waves. The sky is bright at night but its temperature is only 3 degrees above absolute zero. Astronomers study subtle variations in this background to infer the existence of heterogeneities that led to the formation of galaxies and clusters of galaxies.
The universe became transparent to neutrinos (small uncharged nearly massless particles) earlier. These particles would give information on its state about 200,000 years after its formation if we could reliably detect them.
Old Earth and Young Universe. The Big Bang and astrophysics in general are still poorly enough understood that philosophy enters discussions. For example, undetectable dark matter seems to keep galaxies gravitationally bound. Unseen forces accelerate distant galaxies when it seems that gravity should slow the rate of expansion down. This would have pleased René Descartes who filled the universe with vortices of unseen matter. The age of the universe in some sense gives an absolute time, yet from general relativity this time plays no part in the physics.
The Big Bang has an aura of creation. This delights the traditionally religious and disquiets some others. The comparable lengths of geological and cosmic time are part of the queasiness. Our insignificant planet has been around for a third of eternity. The lack of time for life to form and evolve intelligence becomes more striking when we consider astrophysics in the next chapter. Our Sun has already used up half of its useful life.
The Big Bang, like any hypothesis in science, undergoes continual scutiny, often by those who find it philosophically troubling. Astrophysicists including Fred Hoyle (1915-2001) of England made serious attempts to formulate a steady state, infinitely old universe where the observed expansion does not involve inflation from a small volume. To date, none have proved viable.
Neither are there off-limits signs around topics that might trouble the religious. Physicists attempt to look back beyond the start of the Big Bang. Have other universes formed so that things are really infinitely old? Why does our universe have its physics? These efforts have yet to yield anything that is observable and testable. They certainly have not yielded anything with respect to planetary habitability beyond that the universe needs to be habitable to be observable.
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