Home

Author's blog

On this page, observations of various kinds will appear that are related to big history teaching, as well as to big history in general.
 
Earlier blogs
- Big history and web site design
- Did Galileo overstate the magnification of his telescope? 
- Did Columbus falsify his latitude measurements?
- Reflections on observations in big history
- What about questions in learning goals?
- What to think about machines that think?
- Was the Juan de la Cosa map (1500 CE) an instrument to stake claims?
 
 
 
HOW CAN WE EXAMINE CHANCE AND NECESSITY IN BIG HISTORY?
 
Introduction
 
How can we examine chance and necessity in big history? The thoughts expressed in this short essay  were provoked by Walter Alvarez’s book A Most Improbable Journey: A Big History of Our Planet and Ourselves (2016).  In the last chapter Alvarez argues that, because everything in big history very much depends on chance and contingency, the current situation on our planet is most improbable.
 
I could not more agree with such a view. Yet we do observe our own planet, and a great many galaxies, stars, and now also a considerable number of other planets. They are all different, of course, but they also exhibit certain similarities. That is exactly why we can use the words ‘galaxies,’ ‘stars,’ and ‘planets’ to characterize these objects and, by doing so, put them into these specific categories.
 
This leads to the following question: because, as Walter Alvarez argues, virtually all processes are improbable seen from the point of view of probability theory, how is it possible that processes leading to similar forms of greater complexity actually do occur?
 
At the beginning of chapter 2 my book, my general position on these questions was stated as follows:
 
'explaining the past always implies striking a balance between chance and necessity. This point of view had already been expressed by the natural philosopher Democritus of ancient Greece (460–370 BCE), while more recently French biochemist Jacques Monod (1910–76 CE) said essentially the same (with proper reference to Democritus). My explanatory scheme is about necessity. It consists of general trends that not only make possible certain situations but also constrain them. Yet within these boundaries there is ample room for chance.'
 
So far the quotation. In sum: even though chance effects are everywhere, they do not only produce pure chaos. How is that possible? What causes these combined chance effects to produce all the levels of complexity that we witness today, including ourselves?
 
While writing my book, first published in 2010, I did not examine chance effects any further, although I did, for instance, point out the need for constrained processes while discussing the emergence of life at the end of chapter 4.
 
In his 2012 keynote speech during the first IBHA conference in Allendale, Michigan, Walter Alvarez explained the importance of chance in big history. In fact, the last chapter of his book can be seen as a further elaboration of the thoughts he then shared with all of us.
 

How improbable are processes and outcomes?
 
Before examining possible causes of structure and regularities, let us first examine the starting point of his argument: namely that virtually all processes in big history are improbable in their specific outcomes. In order to do so, let us throw a die a few times.
 
What would be the chance of throwing a die once and throwing a six? Obviously, if throwing such a die does not exhibit any irregularities that will introduce a bias in the outcomes, there will be a chance of one out of six of doing so. After throwing any number of times we will obtain the same chance result for any predetermined single outcome. Nothing new here.
 
But what happens when we consider the specific trajectory of throwing the die, for example ten times? Perhaps surprisingly, the probability of exactly replicating that specific entire trajectory is (1/6)(to the power of 10) = 0.000000017. That is a far smaller number, in fact one million times smaller, than the probability of throwing a certain specific outcome in any single throw, which is 1/6 = 0.17. In other words, repeating the specific trajectory of throwing a die is far less likely than obtaining a specific outcome of one single throw.
 
How much time would be needed to throw and have a reasonable probability of replicating a certain predetermined outcome, or of replicating a certain specific trajectory? In doing so, let us assume that a person is able to throw a die and write down the result once every 2 seconds.
 
Let us first look at the probability of replicating a certain outcome. If we want to have a reasonable probability of throwing a five, for instance, we would need to throw six times on average. Throwing six times does not guarantee the outcome of a five, of course. But it offers a reasonable probability. This means that on average we will need 6 x 2 = 12 seconds to achieve our goal, even though this goal will not be guaranteed within such a time span.
 
For repeating a specific trajectory of ten throws with a similar probability, however, we would need much more time on average, namely: 12 (to the power of 10) seconds = 1963.38 years. That is far longer than the time needed on average to reach a specific outcome, which is only 12 seconds, as we just saw.
 
This difference becomes even more impressive as soon as the number of throws is increased. What would happen if one throws a die more than ten times? How long ago would that person have had to start throwing to have a reasonable probability of replicating that specific trajectory and end up in our present at the end of that exercise? This is the result:
 
Number of
Throws:
     Time required:
10 :              1,963 years (Roman empire)
11 :             23,561 years (coldest period of last ice age)  
12 :           282,728 years (before Homo sapiens)
13 :         3,392,732 years (period of Homo australopithecus)
14 :       41,278,243 years (long before humans emerged)
15 :     488,553,449 years (life moves on land)
16 :  5,862,641,391 years (before our solar system emerged)
17 : 70,351,696,690 years (long before the universe emerged)
 
Apparently, standing a reasonable chance of replicating a specific sequence of only 17 throws requires almost five times as much time as the entire history of the universe (supposedly 13.8 billion years). That is how improbable even that very simple specific trajectory is.
 
If such a very simple trajectory is already so improbable, virtually all processes in big history must be extraordinarily improbable in their specific trajectories. Such a conclusion is much in line with Walter Alvarez’s argument, but perhaps even more extreme. As mentioned earlier, this raises the profound question of why structured processes would occur at all.
 
More about that below. But let us first raise an objection: one could argue that all of this does not matter, because the probability of the outcome of any throw is still 1/6 with any and every throw. This is surely correct. But what would happen if  at every throw the specific trajectory is connected to the outcome of that particular throw?
 
To model that, let us assume that with each throw the die is slightly changed randomly, for instance by the random replacement of a few atoms on the outside of the die by different ones, while this change does not affect the probability of  throwing a specific number, which remains one out of six.
 
While this probability remains the same, the die itself will randomly change with each throw. And because that change of the die is random, the probability of replicating that change is even lower than the change in trajectory per throw, which remains 1/6. In this case, not only is the specific trajectory extremely unlikely to be replicated, but the specific outcome, the specific arrangement of atoms in the die, is even more improbable.
 
In my opinion, this model of coupling trajectory with outcome is much closer to what we observe in the real world than the first trajectory model outlined above. If such a simple thought experiment already very soon results in a most improbable specific trajectory and outcome, what is the probability that all of cosmic evolution, which consists of zillions of often far more complex process, happened exactly the way it did? Obviously very, very close to zero.
 
In other words, no other conclusion seems possible other than that virtually all specific trajectories and outcomes, large and small, are unique and highly improbable. They are very unlikely to be replicated exactly the same way within the presumed age of the universe.
 
This conclusion raises a few important questions.
1. Given these observations, to what extent has the current probability theory based on chance and statistics focused on outcomes while perhaps neglecting the probability of a certain specific trajectory (because it does not seem to matter at first sight)?
 
I do not yet know a good answer to this question. A short exploration on the Internet has not yet yielded any clear answers. But it may well be that the theory of stochastic processes deals with this problem. Especially modeling complex processes such as weather forecasts would include such approaches. Yet I am not aware of a generalized formalized approach. This is a question that specialists in probability theory may be able to answer.
 
2. What could be gained by developing a probability theory that combines specific trajectories with outcomes? I do not know, but perhaps this may be a promising research field. But perhaps it is already included in the theory of stochastic processes.
 

What about constraints in these processes?
 
One may wonder whether all these arguments are, perhaps, to some extent an artefact of our own possibly prejudiced starting point, namely that we are looking for a specific trajectory and outcome of big history that we observe and then start wondering about the chance that it would have happened in such a specific way. What would happen, one may wonder, if we looked at these processes from some greater distance?
 
Surely, throwing a die 10 times or more will yield a very random specific trajectory. Yet this trajectory will always be within certain boundaries. It will never fluctuate below one and above six, simply because that is the range of numbers on the die. Seen from that point of view, all these random trajectories are actually very similar. The same can be argued for the changes of the die. Surely, the die may change a little as a result of the random replacement of a few atoms. But it will very recognizably remain a die.
 
In other words, the similarities of these processes and outcomes are the result of certain specific constraints that are operating, in this case the range of numbers on the die as well as our assumption that the random replacement of a few atoms does not change the die very much. This is a very fundamental conclusion, because it means that these constraints make specific processes possible and, in fact, likely, even though these specific processes themselves may still be very random within those constraints.
 
A simple example from daily life would be observing a barometer every day. The barometer on the wall of our house fluctuates between ‘storm’ (relatively low pressure) and ‘very dry’ (relatively high pressure). The needle rarely reaches those extreme values, though, and never goes beyond them. It spends most of its time fluctuating on ‘variable’ and a bit above or below that (between ‘nice weather’ and ‘rain’).
 
The specific trajectory of these fluctuations throughout the year will, in all likelihood, never be repeated. Yet the boundaries are unambiguous and predictable, because they result from the properties of Earth’s atmosphere and the location of the barometer. A very similar argument can be made for a thermometer measuring outside temperatures or, in fact, for any instrument measuring long-term trends within a relatively stable environment.
 
Let us now apply a few more constraints to the die to see what will happen. We could, for instance, mount a little magnet on one of the sides, for instance on the side with number three. If we were to throw the die many times on an iron table, quite likely the opposite side, number four, would end up on top most, if not all, of the time. As a result, both the outcome and the trajectory of this experiment would become extremely predictable. We could also make both the trajectory and the outcome very predictable simply by putting the same number on all six sides.
 
An example of such a similarly constrained process would be the emergence of salt crystals out of a watery salt solution that is evaporating its water. This process leads to an increase of the salt concentration to the point where crystals begin to form, because the solution has become saturated, which means that it cannot contain a higher concentration of salt.
 
The formation of these crystals may be triggered by impurities in the solution. Yet the general structure of such crystals is very regular, cubic, because in the prevailing circumstances this structure is mostly dictated by the properties of the sodium and chloride ions that it consists of. That is what constrains the crystal formation process. Yet all crystals will be slightly different as well, especially their sizes.
 
Let us now imagine that we try to remove all constraints. If, for instance,  we could make a die with endless numbers of sides, all with different numbers on them, both the trajectory and the outcome would become entirely unpredictable. In other words, without constraints throwing such a die would result in a totally random sequence of numbers (the process of throwing the die would still be still fairly regular, of course).
 
Let us now introduce selection into the process of throwing a standard die. Let us assume that we are allowed to repeat the first throw until we get it right, and then proceed with the next throw, etc. How long would it take in this case to achieve a reasonable probability of replicating a specific trajectory of 17 throws? The answer is simple: 6 x 2 x 17 seconds = 3.4 minutes.
 
That is a lot quicker than almost five times the history of the universe. In other words: introducing a specific form of selection can change very improbable trajectories into reasonably likely ones. This thought experiment may offer a rough first-order model of how biological evolution works.
 
Let us now imagine that we are able to influence the throws intentionally, simply by putting the right number on top by hand (in this case we would not really throw the die anymore). Obviously, in such a case we would need only 17 x 2 seconds = 34 seconds to replicate any specific trajectory of 17 throws. That is even a lot quicker than 3.4 minutes.
 
Would such a thought experiment represent a rough first-order approach to cultural evolution? If so, this may illustrate and explain why cultural evolution proceeds so much quicker than biological evolution.
 
In conclusion: to understand the probability of the emergence and development of relatively-structured processes we must examine both chance effects and the constraints involved (necessity). That is why I argued along the lines quoted earlier at the beginning of chapter two of my book. It seems to me that a systematic theoretical exploration of this theme in big history has barely begun, while doing so it may yield most delicious fruits.
 
In most of the themes discussed in Walter Alvarez’s book, the force of gravity provides such a constraint, which makes possible many of the examples described in such exquisite detail. It is, of course, not the only constraint that is operating on our planet. All the natural forces can be seen as providing constraints, and all of them play a role in Alvarez’s book.
 

Do relatively-structured processes involve more than only constraints?
 
Posing this question is almost answering it. Clearly there is more to the emergence of structured processes than only constraints. What is needed for such processes to occur are certain favorable circumstances, which in my book are called Goldilocks circumstances.
 
These good circumstances very much depend on the type of complexity involved. Within the context of this little essay, a relevant question may be: what would be the Goldilocks circumstances for throwing a die? The obvious answer is: those circumstances that favor the die to exist as well as  those that make it possible to throw it.
 
While these conditions may seem obvious, in most of the universe dice do not exist, while the conditions for throwing them do not exist either. Throwing a die in space, even as close to Earth as inside the International Space Station (ISS), would not work for lack of any effects of gravity. That is the case, because the IIS including everything inside it is falling around the Earth with the same velocity. As a result, little or no gravity is experienced inside those amazing living quarters in space. Inside the ISS, the die would simply float around and would hardly ever end up on one side, if at all.
 
More in general, Goldilocks circumstances are those opportune circumstances that facilitate processes to occur, while the constraints limit them, and, by doing so, also make them possible. Perhaps one can interpret constraints as Goldilocks boundaries, beyond which these processes cannot occur anymore. But already in the case of the die that seems a little too artificial to me. One could easily make a die with more, or fewer, than six numbers, all of which could be thrown without any problems within the same further Goldilocks circumstances. Yet these processes and their outcomes would be different.
 
If this is already the case with this very simple experiment, it may be wise to make a distinction between Goldilocks circumstances and their boundaries on the one hand and other types of constraints on the other hand. But I immediately admit that this distinction may sometimes be vague.
 
This subject may, therefore, represent unexplored territory from a theoretical point of view. To my knowledge, a careful exploration of big history in terms of  constraints and Goldilocks circumstances has barely begun. Further systematic investigations could yield wonderful results. Such an investigation should first of all include making inventories of the available knowledge about these aspects in all academic fields, and then seeking to systematize them within the field of big history.
 
While studying human history in the 1980s and early 1990s, the Dutch sociologist Joop Goudsblom and I agreed on the formulation that we were not trying to explain how history had to happen, but that we instead sought to explain how it could have happened. We had reached that conclusion, because of the role of chance and contingency that we observed. It seems to me that the same reasoning very much applies to all of big history.
 
 
In conclusion
 
Chance and necessity depend on the amount of detail examined, and on the factors that constrain chance and make it possible. Clearly, chance and necessity are both important aspects of all processes. If we observe structures, they will be unique, yet they will also be constrained and facilitated by certain circumstances. In order to understand those situations better, we need to examine all these aspects. Without constraints and Goldilocks circumstances big history would only consist of utterly irreproducible chaos without any structure whatsoever.
 

How could we further proceed along these lines?
 
I see the following possibilities. We could try to assess to what extent processes in reality conform to this general model, ranging from our personal histories all the way to the history of the universe. As a result, a whole field may be open to further for investigation.
 
In many cases, these processes may influence one another, thus leading to more complicated circumstances. How would we analyze that both qualitatively and perhaps also mathematically? Again, a whole new field may be open to exploration. Perhaps weather models do already incorporate such schemes to some extent. These are only my first thoughts. There may well be many more possibilities.
 

Returning to Walter Alvarez’s book
 
In chapter ten of his book A Most Improbable Journey Walter Alvarez convincingly argued how improbable our current situation is. Yet in the preceding chapters he hardly mentioned this theme at all. Instead he nicely demonstrated some of the geological constraints and opportunities that have contributed to shaping human history which, jointly, have made this most improbable journey possible.
bhi_005029001.jpg
International Big History Association
Un. of Amsterdam big history
Cosmic Evolution
Big History Project
Chronozoom
Book: Teaching Big History
Bill Bryson: Short History of Nearly Everything
Other useful stuff on the web
Other big history
resources
Feedback
How to use the book
Course models
Learning goals and objectives
Teaching tools
Assignments (little big histories)
Answers to FAQs by students
Questions by students and teachers that go beyond the book
Examination models
Teaching big history