18 March 2017
Many years ago, reading a source I cannot now recall (and for which I searched unsuccessfully when I started writing this post), I came upon a passage that has stayed with me. The author was making the argument that no sciences were consistent except those that had been reduced to mere catalogs of facts, like geography and anatomy. I can’t recall the larger context in which this argument appeared, but the observation that sciences might only become fully consistent when they have matured to the point of being exhaustive but static and uninteresting catalogs of facts, implying that the field of research itself had been utterly exhausted, was something I remembered. This idea presents in miniature a developmental conception of the sciences, but I think that it is a developmental conception that is incomplete.
Thinking of this idea of an exhausted field of research, I am reminded of a discussion in Conversations on Mind, Matter, and Mathematics by Jean-Pierre Changeux and Alain Connes, in which mathematician Alain Connes distinguished between fully explored and as yet unexplored parts of mathematics:
“…the list of finite fields is relatively easy to grasp, and it’s a simple matter to prove that the list is complete. It is part of an almost completely explored mathematical reality, where few problems remain. Cultural and social circumstances clearly serve to indicate which directions need to be pursued on the fringe of current research — the conquest of the North Pole, to return again to my comparison, surely obeyed the same type of cultural and social motivations, at least for a certain time. But once exploration is finished, these cultural and social phenomena fade away, and all that’s left is a perfectly stable corpus, perfectly fitted to mathematical reality…”
Jean-Pierre Changeux and Alain Connes, Conversations on Mind, Matter, and Mathematics, Princeton: Princeton University Press, 1995, pp. 33-34
To illustrate a developmental conception of mathematics and the formal sciences would introduce additional complexities that follow from the not-yet-fully-understood relationship between the formal sciences and the empirical sciences, so I am going to focus on developmental conceptions of the empirical sciences, but I hope to return to the formal sciences in this connection.
The idea of the development of science as a two-stage process, with discovery followed by a consistent and exhaustive catalog, implies both that most sciences (and, if we decompose the individual special sciences into subdivisions, parts of most or all sciences) remain in the discovery phase, and that once the discovery phase has passed and we are in possession of an exhaustive and complete catalog of the facts discovered by a science, there is nothing more to be done in a given science. However, I can think of several historical examples in which a science seemed to be converging on a complete catalog, but this development was disrupted (one might say) by conceptual change within the field that forced the reorganization of the materials in a new way. My examples will not be perfect, and some additional scientific discovery always seems to have been involved, but I think that these examples will be at least suggestive.
Prior to the great discoveries of cosmology in the early twentieth century, after which astronomy became indissolubly connected to astrophysics, astronomy seemed to be converging slowly upon an exhaustive catalog of all stars, with the limitation on the research being simply the resolving power of the telescopes employed to view the stars. One could imagine a counterfactual world in which technological innovations in instrumentation supplied nothing more than new telescopes able to resolve more stars, and that the task of astronomy was merely to supply an exhaustive catalog of stars, listing their position in the sky, intrinsic brightness, and a few other facts about the points of light in the sky. But the cataloging of stars itself contributed to the revolution that would follow, particularly when the period-luminosity relationship in Cepheid variable stars was discovered by Henrietta Swan Leavitt (discovered in 1908 and published in 1912). The period-luminosity relationship provided a “standard candle” for astronomy, and this standard candle began the process of constructing the cosmological distance ladder, which in turn made it possible to identify Cepheid variables in the Andromeda galaxy and thus to prove that the Andromeda galaxy was two million light years away and not contained within the Milky Way.
Once astronomy became scientifically coupled to astrophysics, and the resources of physics (both relativistic and quantum) could be brought to bear upon understanding stars, a whole new cosmos opened up. Stars, galaxies, and the universe entire were transformed from something static that might be exhaustively cataloged, to a dynamic and changing reality with a natural history as well as a future. Astronomy went from being something that we might call a Platonic science, or even a Linnaean science, to being an historical science, like geology (after Hutton and Lyell), biology (after Darwin and Wallace), and Paleontology. This coupling of the study of the stars with the study of the matter that makes up the stars has since moved in both directions, with physics driving cosmology and cosmology driving physics. One result of this interaction between astronomy and physics is the illustration above (by Jennifer Johnson) of the periodic table of elements, which prominently exhibits the origins of the elements in cosmological processes. The periodic table once seemed, like a catalog of stars, to be something static to be memorized, and divorced from natural history. This conceptualization of matter in terms of its origins puts the periodic table in a dramatically different light.
As the cosmos was once conceived in Platonic terms as fixed and eternal, to be delineated in a Linnaean science of taxonomical classification, so too the Earth was conceived in Platonic terms as fixed and eternal, to be similarly delineated in a Linnaean science of classification. The first major disruption of this conception came with geology since Hutton and Lyell, followed by plate tectonics and geomorphology in the twentieth century. Now this process has been pushed further by the idea of mineral evolution. I have been listening through for the second time to Robert Hazen’s lectures The Origin and Evolution of Earth: From the Big Bang to the Future of Human Existence, which exposition closely follow the content of his book, The Story of Earth: The First 4.5 Billion Years, from Stardust to Living Planet, in which Hazen wrote:
“The ancient discipline of mineralogy, though absolutely central to everything we know about Earth and its storied past, has been curiously static and detached from the conceptual vagaries of time. For more than two hundred years, measurements of chemical composition, density, hardness, optical properties, and crystal structure have been the meat and potatoes of the mineralogist’s livelihood. Visit any natural history museum, and you’ll see what I mean: gorgeous crustal specimens arrayed in case after glass-fronted case, with labels showing name, chemical formula, crystal system, and locality. These most treasured fragments of Earth are rich in historical context, but you will likely search in vain for any clue as to their birth ages or subsequent geological transformations. The old way all but divorces minerals from their compelling life stories.”
Robert M. Hazen, The Story of Earth: The First 4.5 Billion Years, from Stardust to Living Planet, Viking Penguin, 2012, Introduction
This illustrates, from the perspective of mineralogy, much of what I said above in relation to star charts and catalogs: mineralogy was once about cataloging minerals, and this may have been a finite undertaking once all minerals had been isolated, identified, and cataloged. Now, however, we can understand mineralogy in the context of cosmological history, and this is as revolutionary for our understanding of Earth as the periodic table understood in terms of cosmological history. It could be argued, in addition, that compiling the “particle zoo” of contemporary particle physics is also a task of cataloging the entities studied by physics, but the cataloging of particles has been attended throughout with a theory of how these particles are generated and how they fit into the larger cosmological story — what Aristotle would have called their coming to be and passing away.
The best contemporary example of a science still in its initial phases of discovery and cataloging is the relatively recent confirmation of exoplanets. On my Tumblr blog I recently posted On the Likely Existence of “Random” Planetary Systems, which tried to place our current Golden Age of Exoplanet Discovery in the context of a developing science. We find the planetary systems that we do in fact find partly as a consequence of observation selection effects, and it belongs to the later stages of the development of a science to attempt to correct for observation selection effects built into the original methods of discovery employed. The planetary science that is emerging from exoplanet discoveries, however, and like contemporary particle physics, is attended by theories of planet formation that take into account cosmological history. However, the discovery phase, in terms of exoplanets, is still underway and still very new, and we have a lot to learn. Moreover, once we learn more about the possibilities of planets in our universe, hopefully also we will learn about the varied possibilities of planetary biospheres, and given the continual interaction between biosphere, lithosphere, atmosphere, and hydrosphere, which is a central motif of Hazen’s mineral evolution, we will be able to place planets and their biospheres into a large cosmological context (perhaps even reconstructing biosphere evolution). But first we must discover them, and then we must catalog them.
These observations, I think, have consequences not only for our understanding of the universe in which we find ourselves, but also for our understanding of science. Perhaps, instead of a two-stage process of discovery and taxonomy, science involves a three-stage process of discovery, taxonomy, and natural history, in which latter the objects and facts cataloged by one of the special sciences (earlier in their development) can take their place within cosmological history. If this is the case, then big history is the master category not only of history, but also of science, as big history is the ultimate framework for all knowledge that bears the lowly stamp of its origins. This conception of the task of science, once beyond the initial stages of discovery and classification, to integrate that which was discovered and classified into the framework of big history, suggests a concrete method by which to “cash out” in a meaningful way Wilfrid Sellars’ contention that, “…the specialist must have a sense of how not only his subject matter, but also the methods and principles of his thinking about it, fit into the intellectual landscape.” (cf. Philosophy and the Scientific Image of Man) Big history is the intellectual landscape in which the sciences are located.
A developmental conception of science that recognized stages in the development of science beyond classification, taxonomy, and an exhaustive catalog (which is, in effect, the tombstone of what was a living and growing science), has consequences for the practice of science. Discovery may well be the paradigmatic form of scientific activity, but it is not the only form of scientific activity. The painstakingly detailed and disciplined work of cataloging stars or minerals is the kind of challenge that attracts a certain kind of mind with a particular interest, and the kind of individual who is attracted to this task of systematically cataloging entities and facts is distinct from the kind of individual who might be most attracted by scientific discovery, and also distinct from the kind of individual who might be attracted to fitting the discoveries of a special science into the overall story of the universe and its natural history. There may need to be a division of labor within the sciences, and this may entail an educational difference. Dividing sciences by discipline (and, now, by university departments), which involves inter-generational conflicts among sciences and the paradigm shifts that sometimes emerge as a result of these conflicts, may ultimately make less sense than dividing sciences according their stage of development. Perhaps universities, instead of having departments of chemistry, geology, and botany, should have departments of discovery, taxonomy, and epistemic integration.
Speaking from personal experience, I know that (long ago) when I was in school, I absolutely hated the cataloging approach to the sciences, and I was bored to tears by memorizing facts about minerals or stars. But the developmental science of evolution so intrigued me that I read extensively about evolution and anthropology outside and well beyond the school curriculum. If mineral evolution and the Earth sciences in their contemporary form had been known then, I might have had more of an interest in them.
What are the sciences developing into, or what are the sciences becoming? What is the end and aim of science? I previously touched on this question, a bit obliquely, in What is, or what ought to be, the relationship between science and society? though this line of inquiry is more like a thought experiment. It may be too early in the history of the sciences to say what they are becoming or what they will become. Perhaps an emergent complexity will arise out of knowledge itself, something that I first suggested in Scientific Historiography: Past, Present, and Future, in which I wrote in the final paragraph:
We cannot simply assume an unproblematic diachronic extrapolation of scientific knowledge — or, for that matter, historical knowledge — especially as big history places such great emphasis upon emergent complexity. The linear extrapolation of science eventually may trigger a qualitative change in knowledge. In other words, what will be the emergent form of scientific knowledge (the ninth threshold, perhaps?) and how will it shape our conception of scientific historiography as embodied in big history, not to mention the consequences for civilization itself? We may yet see a scientific historiography as different from big history as big history is different from Augustine’s City of God.
It is only a lack of imagination that would limit science to the three stages of development I have outlined above. There may be developments in science beyond those we can currently understand. Perhaps the qualitative emergent from the quantitative expansion of scientific knowledge will be a change in science itself — possibly a fourth stage in the development of science — that will open up to scientific knowledge aspects of experience and regions of nature currently inaccessible to science.
. . . . .
. . . . .
. . . . .
. . . . .
9 March 2017
Some time ago in Extrapolating Plato’s Definition of Being I discussed a famous passage in Plato that gives an explicit definition of being. The passage is as follows:
STRANGER: Let us push the question; for if they will admit that any, even the smallest particle of being, is incorporeal, it is enough; they must then say what that nature is which is common to both the corporeal and incorporeal, and which they have in their mind’s eye when they say of both of them that they ‘are.’ Perhaps they may be in a difficulty; and if this is the case, there is a possibility that they may accept a notion of ours respecting the nature of being, having nothing of their own to offer.
THEAETETUS: What is the notion? Tell me, and we shall soon see.
STRANGER: My notion would be, that anything which possesses any sort of power to affect another, or to be affected by another, if only for a single moment, however trifling the cause and however slight the effect, has real existence; and I hold that the definition of being is simply power.
The Greek text of the Eleatic Stranger’s crucial formulation is as follows:
Ξένος: λέγω δὴ τὸ καὶ ὁποιανου̂ν [τινα] κεκτημένον δύναμιν [247e] εἴτ’ εἰς τὸ ποιει̂ν ἕτερον ὁτιου̂ν πεφυκὸς εἴτ’ εἰς τὸ παθει̂ν καὶ σμικρότατον ὑπὸ του̂ φαυλοτάτου, κἂν εἰ μόνον εἰς ἅπαξ, πα̂ν του̂το ὄντως εἰ̂ναι: τίθεμαι γὰρ ὅρον [ὁρίζειν] τὰ ὄντα ὡς ἔστιν οὐκ ἄλλο τι πλὴν δύναμις.
My extrapolation of Plato’s definition of being was to derive four permutations from this definition of beings, in this way:
1. Beings that act only and do not suffer
2. Beings that suffer only and do not act
3. Beings that both act and suffer
4. Beings that neither act nor suffer, which may be non-beings
Another way to extrapolate Plato’s definition of being would be the ability of some entity to act or to suffer in kind, that is, to engage in reciprocal relations with a peer, to interact with another entity of the same (or similar) kind in the same (or similar) way. With this extrapolation, the fourth permutation above — beings that neither act nor suffer — becomes meaningful, because a given entity might possess a minimal ontological status in regard to interactions of acting and suffering without the opportunity to engage in such relationships with a peer entity. Thus a contradictory, or at least problematic, permutation of Plato’s definition of being can be given meaning.
An entity might be analyzed in terms of the classes of relationships across which it interacts, and where a class of interactions is absent, the entity is a non-being in this respect even if it is clearly a being in other respects. For example, Robinson Crusoe, living alone as a castaway on a desert island, interacts with the island, its flora and fauna, but initially interacts with no other human beings. Crusoe has not been cast out of existence by being marooned on a desert island, but he has been deprived of human society; no human society exists on his island (at first). Crusoe has lost his status as a member of human society by being deprived of the kind of interactions that constitute human society, i.e., interactions with other human beings, even as he continues to interact with the world across broad categories of existence that have nothing to do with human society.
This example of Robinson Crusoe and his interaction with peers (or lack thereof) can be scaled up and applied to larger human societies. Human society at the level of organization of the hunter-gatherer band, such as characterized the human world of the upper Paleolithic, brought into being relationships between such bands, which relationships were almost certainly implicated in the human expansion across the entire surface of Earth. When, near the beginning of the Holocene, some bands settled down into agricultural villages, these villages would have interacted with each other, and when some of the villages expanded in size and complexity and became cities, these early cities would have interacted with each other. What I would like to suggest there is that interaction among cities as cities is what characterizes civilization.
Recently in Another Counterfactual: the Single City Civilization I discussed a couple of different definitions of civilization that I have been employing, particularly in my Centauri Dreams post Martian Civilization, one of these definitions abstract and the other concrete:
● Concrete — A network of cities engaged in relationships of cooperation and conflict.
● Abstract — A society with a central project that unifies its economic infrastructure and its intellectual superstructure.
My “concrete” definition of civilization interpreted in the light of Plato’s definition of being suggests that civilization comes into being when cities interact on the ontological level distinctive to cities, i.e., cities interacting on a civic level. Before this, isolated cities would not have had an opportunity to interact with ontological peers; a city would interact with the surrounding countryside, and perhaps also with hunter-gatherer bands that might pass by for raiding or trading, but these sub-urban interactions would not yet rise to the level of civilization.
The class of relationships that are distinctive of civilization come into being when multiple cities interact with each other as cities. Before this, individual cities may emerge and interact with their surroundings, but these relationships belong to another order of being.
This is, I think, a conception of civilization that is consistent with V. Gordon Childe and the “urban revolution” that I discussed in my Centauri Dreams post Martian Civilization, but also a definition that goes beyond Childe and fills in the gap between Childe’s formulations specifically concerned with the nature of cities but not yet with the nature of cities in mutual interaction.
This Platonic interpretation of my “concrete” definition of civilization transforms it into a theoretical definition that may yet point to implications that I have not yet fully realized.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
27 February 2017
In my previous post, Do the clever animals have to die?, I considered the “ultimate concern” (to borrow a phrase from Paul Tillich) of existential risk mitigation: the survival of life and other emergent complexities beyond the habitability of its homeworld or home planetary system. While a planetary system could be inhabited for hundreds of millions of years in most cases, and possibly for billion or tens of billions of years (the latter in the case of red dwarf stars, as in the recently discovered planetary system at TRAPPIST-1, which appears to be a young star with a long history ahead of it), there are yet many events that could occur that could render a homeworld or an entire planetary system uninhabitable, or which could be sufficiently catastrophic that a civilization clustered in the vicinity of a single star would almost certainly be extirpated by them (e.g., a sufficiently large gamma ray burst, GRB, from outside our solar system, or a sufficiently large coronal mass ejection, CME, from within our solar system).
Because any civilization that endures for cosmologically significant periods of time must have established multiple independent centers of civilization, and will probably have survived its homeworld having become uninhabitable, mature advanced civilizations may view this condition as definitive of a mature civilization. Having ensured their risk of extinction against existential threats through establishing multiple independent centers of civilization, these advanced civilizations may not regard as a “peer” (i.e., not regard as a fellow advanced civilization) any civilization that still remains tightly-coupled to its homeworld.
It nevertheless may be the case (if there are, or will be, multiple examples of advanced civilizations) that some civilizations choose to remain tightly-coupled to their homeworlds. We can posit this as the condition of a certain kind of civilization. In the question and answer segment following my 2015 talk, What kind of civilizations build starships? a member of the audience, Alex Sherwood, suggested, in contradistinction to the expansion hypothesis, a constancy hypothesis, according to which a civilization does not expand and does not contract, but rather remains constant; I would prefer to call this the equilibrium hypothesis. One way in which a civilization might exemplify the constancy hypothesis would be for it to remain tightly-coupled to its homeworld.
Some subset of homeworld-coupled civilizations will probably experience extinction due to this choice. Such a homeworld-coupled civilization might choose, instead of establishing multiple independent centers of civilization as existential risk mitigation, to instead establish de-extinction and backup measures that would allow civilization to be restored on its homeworld despite any realized existential risks. However, while this approach to civilizational longevity may ensure the existence of a civilization over the billions of years of the life of its parent star, if a civilization does not want the historical accident of the age of its parent star to determine its ongoing viability, then such a civilization must abandon its homeworld and eventually also its home planetary system.
A civilization might continue to exemplify the equilibrium hypothesis by maintaining the unity and distinctiveness of its civilization despite needing to pursue megastructure-scale projects in order to ensure its ongoing existential viability. The idea of constructing a Shkadov thruster to move a star was partly inspired by this particular conception of the equilibrium hypothesis, as a star might, by this method, be moved to another, younger star, and the homeworld transferred into the orbit of that younger star. In this way, the relationship to the parent star is de-coupled, but the relationship to homeworld remains exclusive. At yet another remove, an entire civilization might simply choose to pick up from its homeworld and transfer itself to another chosen world. (As an historical analogy, consider the ancient city of Knidos, which was founded on the Datça Peninsula, but as the city grew in size and wealth, the city fathers decided that they needed to start again, so they built themselves a new and grander city nearby, and moved the entire city to this new location.) This conception of the equilibrium hypothesis would de-couple a civilization from both parent star and homeworld, but could still maintain the civilization as a unique and distinctive whole, thus continuing that civilization in its equilibrium condition.
A civilization that establishes multiple independent centers of civilization (and thus, to some degree, exemplifies the expansion hypothesis) might still retain strong connections to its homeworld — only not the connection of dependency. Such civilizations fully independent of a homeworld might be said to be loosely-coupled to their homeworld, in contradistinction to civilizations tightly-coupled to their homeworld and exemplifying the equilibrium hypothesis. Expansionary civilizations might remain in close contact with a homeworld for as long as the homeworld was habitable, only to fully abandon it when the homeworld could no longer support life.
Eventually, as the climate changes and the continents move and the surface of Earth is entirely rearranged, as would be experienced by a billion-year-old civilization, almost all terrestrial cities and monuments will disappear, and even the familiar look of Earth will change until it eventually becomes unrecognizable. The heritage of terrestrial civilization might be preserved in part by moving entire monuments to other worlds, or to no world at all, but perhaps to a permanent artificial habitat that is not a planet. Terrestrial places might be recreated on other worlds (or, again, on no world at all) in a grand gesture of historical reconstruction.
There might be other surprising ways of preserving our terrestrial heritage, such as building projects that were never realized on Earth. For example, some future civilization might choose to build Étienne-Louis Boullée’s design for an enormous cenotaph commemorating Isaac Newton, or Antoni Gaudí’s unbuilt skyscraper, or indeed any number of countless projects conceived but never built. An entire city of unbuilt buildings could be constructed on other worlds, which would be new cities, cities never before built, but cities in the tradition of our terrestrial heritage, maintaining the connection to our homeworld even while looking to a future de-coupled from that homeworld.
A civilization that outlasts its homeworld could be said to be de-coupled from its homeworld, though the homeworld will always be the origin of the intelligent agent that is the progenitor of a civilization, and hence a touchstone and a point of reference — like a hometown that one has left in order to pursue a career in the wider world. One would expect historical reconstruction and reenactment in order to maintain our intimacy with the past, which is, at the same time, our intimacy with our homeworld, should we become de-coupled from Earth. If humanity goes on to expand into the universe, establishing multiple independent centers of civilization, including gestures of respect to our terrestrial past in the form of reconstruction, the eventual loss of the Earth to habitability may not come as such a devastating blow if some trace of Earth was preserved.
When the uninhabitability of the Earth does become a definite prospect, and should civilization endure up to that time, that future civilization’s opportunities for historical preservation and conservation will be predicated upon the technological resources available at that time, and what conception of authenticity prevails in that future age. A civilization of sufficiently advanced technology might simply preserve its homeworld entire, as a kind of museum, moving it to wherever would be convenient in order to maintain it in some form that it would be visited by antiquaries and eccentrics. Or such a future civilization might deem such preservation to be undesirable, and only certain artifacts would be removed before the planet entire was consumed by the sun as it expands into a red giant star. In an emergency abandonment of Earth, what could be evacuated would be limited, and principles of selection therefore more rigorous — but also constrained by opportunity. In the event of emergency abandonment, there might also be the possibility of returning for salvage after the emergency had passed.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
14 February 2017
Nietzsche’s Big History
One of the most succinct formulations of Big History of which I am aware is a brief paragraph from Nietzsche:
“In some remote corner of the universe, poured out and glittering in innumerable solar systems, there once was a star on which clever animals invented knowledge. That was the highest and most mendacious minute of ‘world history’ — yet only a minute. After nature had drawn a few breaths the star grew cold, and the clever animals had to die.
“On Truth and Lie in an Extra-Moral Sense,” Friedrich Nietzsche, Fragment, 1873: from the Nachlass. Translated by Walter Kaufmann
…and in the original German:
In irgend einem abgelegenen Winkel des in zahllosen Sonnensystemen flimmernd ausgegossenen Weltalls gab es einmal ein Gestirn, auf dem kluge Tiere das Erkennen erfanden. Es war die hochmütigste und verlogenste Minute der “Weltgeschichte”: aber doch nur eine Minute. Nach wenigen Atemzügen der Natur erstarrte das Gestirn, und die klugen Tiere mußten sterben.
Über Wahrheit und Lüge im außermoralischen Sinne, Friedrich Nietzsche, 1873, aus dem Nachlaß
This passage has been translated several times, so, for purposes of comparison, here is another translation:
“In some remote corner of the universe that is poured out in countless flickering solar systems, there once was a star on which clever animals invented knowledge. That was the most arrogant and the most untruthful moment in ‘world history’ — yet indeed only a moment. After nature had taken a few breaths, the star froze over and the clever animals had to die.”
ON TRUTH AND LYING IN AN EXTRA-MORAL SENSE (1873), Edited and Translated with a Critical Introduction by Sander L. Gilman, Carole Blair, and David J. Parent, New York and Oxford: OXFORD UNIVERSITY PRESS, 1989
Bertrand Russell, who rarely passed over an opportunity to criticize Nietzsche in the harshest terms, expressed a tragic interpretation of human endeavor that is quite similar to Nietzsche’s capsule big history:
“That Man is the product of causes which had no prevision of the end they were achieving; that his origin, his growth, his hopes and fears, his loves and his beliefs, are but the outcome of accidental collocations of atoms; that no fire, no heroism, no intensity of thought and feeling, can preserve an individual life beyond the grave; that all the labours of the ages, all the devotion, all the inspiration, all the noonday brightness of human genius, are destined to extinction in the vast death of the solar system, and that the whole temple of Man’s achievement must inevitably be buried beneath the debris of a universe in ruins–all these things, if not quite beyond dispute, are yet so nearly certain, that no philosophy which rejects them can hope to stand. Only within the scaffolding of these truths, only on the firm foundation of unyielding despair, can the soul’s habitation henceforth be safely built.”
Bertrand Russell, “A Free Man’s Worship”
Even closer to Nietzsche, in both style and spirit, is the passage that immediately precedes this in the same essay by Russell, told, as with Nietzsche, in the form of a parable:
“For countless ages the hot nebula whirled aimlessly through space. At length it began to take shape, the central mass threw off planets, the planets cooled, boiling seas and burning mountains heaved and tossed, from black masses of cloud hot sheets of rain deluged the barely solid crust. And now the first germ of life grew in the depths of the ocean, and developed rapidly in the fructifying warmth into vast forest trees, huge ferns springing from the damp mould, sea monsters breeding, fighting, devouring, and passing away. And from the monsters, as the play unfolded itself, Man was born, with the power of thought, the knowledge of good and evil, and the cruel thirst for worship. And Man saw that all is passing in this mad, monstrous world, that all is struggling to snatch, at any cost, a few brief moments of life before Death’s inexorable decree. And Man said: `There is a hidden purpose, could we but fathom it, and the purpose is good; for we must reverence something, and in the visible world there is nothing worthy of reverence.’ And Man stood aside from the struggle, resolving that God intended harmony to come out of chaos by human efforts. And when he followed the instincts which God had transmitted to him from his ancestry of beasts of prey, he called it Sin, and asked God to forgive him. But he doubted whether he could be justly forgiven, until he invented a divine Plan by which God’s wrath was to have been appeased. And seeing the present was bad, he made it yet worse, that thereby the future might be better. And he gave God thanks for the strength that enabled him to forgo even the joys that were possible. And God smiled; and when he saw that Man had become perfect in renunciation and worship, he sent another sun through the sky, which crashed into Man’s sun; and all returned again to nebula.
“`Yes,’ he murmured, `it was a good play; I will have it performed again.'”
Here Russell, unlike Nietzsche, gives theological meaning to the spectacle, however heterodox that meaning may be; I can easily imagine someone preferring Russell’s theological version to Nietzsche’s secular version, though both highlight the meaninglessness of human endeavor in a thermodynamic universe.
Our sun — a star among stars — will be a relatively early casualty in the heat death of the universe. While the life of the sun is orders of magnitude beyond the life of the individual human being, as soon as we understood that the sun’s life will pass through predictable stages of stellar evolution, we understood that the sun, like any human being, was born, will shine for a time, and then will die, and, when the sun dies, everything that is dependent upon the light of the sun for life will die also. It is only if we can make ourselves independent of the sun that we will not inevitably share the fate of the sun.
The idea that the sun is a star among stars, and that any star will do in terms of supporting human life, is embodied in a quote attributed to Wernher von Braun by Tom Wolfe and reported in Bob Ward’s book about von Braun:
“The importance of the space program is not surpassing the Soviets in space. The importance is to build a bridge to the stars, so that when the Sun dies, humanity will not die. The Sun is a star that’s burning up, and when it finally burns up, there will be no Earth… no Mars… no Jupiter.”
quoted in Dr. Space: The Life of Wernher von Braun, Bob Ward, Chapter 22, p. 218, with a footnote giving as the source, “Transcript, NBC’s Today program, New York, November 11, 1998”
Wernher von Braun had seized upon the essential insight of existential risk mitigation, as had many involved in the space program from its inception. As soon as one adopts a naturalistic understand of the place of humanity in the universe, and when technology develops to a point at which its extrapolation offers human beings options and alternatives within the universe, anyone will draw the same conclusion. Another quote from von Braun makes the same point in another way:
“…man’s newly acquired capability to travel through outer space provides us with a way out of our evolutionary dead alley.”
Bob Ward, Dr. Space: The Life of Wernher von Braun, Annapolis, US: Naval Institute Press, 2013.
I have previously written about the idea that humanity is a solar species, but the fact that humanity and the biosphere from which we derive has been utterly dependent upon solar insolation has been an accident of history. Any sun will do. We can, accordingly, re-conceive humanity as a stellar species, the kind of species that requires a star and its planetary system to make a home for ourselves. In this sense, all species of planetary endemism are stellar species.
Even this idea of immigration to another star, and of any other star being as good as the sun, is ultimately too narrow. Our sun, or any star, can be the source of energy that powers our civilization, but it can easily be seen that substitute forms of energy could equally well power the future of our civilization, and that it has merely been an historical contingency — a matter of our planetary endemism — that we have been dependent upon a single star, or upon any star, for our energy needs.
This more radical and farther-reaching vision is embodied in a quote attributed to Ray Bradbury by Oriana Fallaci:
“Don’t let us forget this: that the Earth can die, explode, the Sun can go out, will go out. And if the Sun dies, if the Earth dies, if our race dies, then so will everything die that we have done up to that moment. Homer will die. Michelangelo will die, Galileo, Leonardo, Shakespeare, Einstein will die, all those will die who now are not dead because we are alive, we are thinking of them, we are carrying them within us. And then every single thing, every memory, will hurtle down into the void with us. So let us save them, let us save ourselves. Let us prepare ourselves to escape, to continue life and rebuild our cities on other planets: we shall not be long of this Earth! And if we really fear the darkness, if we really fight against it, then, for the good of all, let us take our rockets, let us get well used to the great cold and heat, the no water, the no oxygen, let us become Martians on Mars, Venusians on Venus, and when Mars and Venus die, let us go to the other solar systems, to Alpha Centauri, to wherever we manage to go, and let us forget the Earth. Let us forget our solar system and our body, the form it used to have, let us become no matter what, lichens, insects, balls of fire, no matter what, all that matters is that somehow life should continue, and the knowledge of what we were and what we did and learned: the knowledge of Homer and Michelangelo, of Galileo, Leonardo, Shakespeare, of Einstein! And the gift of life will continue.”
Oriana Fallaci, If the Sun Dies, New York: Atheneum, 1966, pp. 14-15
Fallaci refers to this as a “prayer,” and indeed we might see this as a prayer or a catechism of the Space Age — not a belief, not merely belief, but an imperative ever-present in the hearts and minds of those who have fully imbibed the spirit of the age and who seek to carry that spirit forward with evangelical fervor, proselytizing to the masses and bringing them to the True Faith through purity of will and vision — another way of saying naïveté.
Do the clever animals have to die? No, not yet. Not if they are clever enough to move on to another planet, another star, another galaxy. Not if they are clever enough to change themselves so that, when the changed conditions of the universe in which they exist no longer allow the lives of clever animals to continue, what the clever animals have achieved can be preserved in some other way, and they themselves can be preserved in another form.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
3 February 2017
A Conceptual Overview
What is the relationship between planetary endemism and the overview effect? This is the sort of question that might be given a definitive formulation, once once we have gotten sufficiently clear in our understanding of these ideas and their ramifications. I’m not yet at the point of formulating a definitive expression of this relationship, but I’m getting closer to it, so this post will be about formulating relationships among these and related concepts in a way that is hopefully clear and illuminating, while avoiding the ambiguities inherent in novel concepts.
This post is itself a kind of overview, attempting to show in brief compass how a number of interrelated concepts neatly dovetail and provide us with a rough outline of a conceptual overview for understanding the origins, development, distribution, and destiny of civilization (or some other form of emergent complexity) in the universe.
The Stelliferous Era
The Stelliferous Era is that period of cosmological history after the formation of the first stars and before the last stars burn out and leave a cold and dark universe. In the cosmological periodization formulated by Fred Adams and Greg Laughlin, the Stelliferous Era is preceded by the Primordial Era and followed by the Degenerate Era. During the Primordial Era stars have not yet formed, but matter condenses out of the primordial soup; during the Degenerate Era, the degenerate remains of stars, black holes, and some exotic cosmological objects are to the found, but the era of brightly burning stars is over.
What typifies the Stelliferous Era is its many stars, radiating light and heat, and whose nucleosynthesis and supernova explosions forge heavier forms of matter, and therefore the chemical and minerological complexity from which later generations of (high metallicity) stars and planets will form. (A Brief History of the Stelliferous Era is an older post about the Stelliferous Era that needs to be revised and updated.)
In comparison to the later Degenerate Era, Black Hole Era, and Dark Era of cosmological history, the Stelliferous Era is rather brief, extending from 106 to 1014 years from the origins of the universe, and almost everything that concerns us can be further reduced to the eleventh cosmological decade (from 10 billion to 100 billion years since the origin of the universe). Since this cosmological periodization is logarithmic, the later periods are even longer in duration than they initially appear to be.
Our interest in the Stelliferous Era, and, more narrowly, our interest in the eleventh decade of the Stelliferous Era, does not rule out interesting cosmological events in other eras of cosmological history, and it is possible that civilizations and other forms of emergent complexity that appear during the Stelliferous Era may be able to make the transition to survive into the Degenerate Era (cf. Addendum on Degenerate Era Civilization), but this brief period of starlight in cosmological history is the Stelliferous Era window in which it is possible for peer planetary systems, peer species, and peer civilization to exist.
Planetary Endemism is the condition of life during the Stelliferous Era as being unique to planetary surfaces and their biospheres. Given the parameters of the Stelliferous Era — a universe with planets, stars, and galaxies, in which both water (cf. The Solar System and Beyond is Awash in Water) and carbon-based organic molecules (cf. Mixed aromatic–aliphatic organic nanoparticles as carriers of unidentified infrared emission features by Sun Kwok and Yong Zhang) are common — planetary surfaces are a “sweet spot” for emergent complexities, as it is on planetary surfaces that energy from stellar insolation can drive chemical processes on mineral- and chemical-rich surfaces. The chemical and geological complexity of the interface between atmosphere, ocean, and land surfaces provide an opportunity for further emergent complexities to arise, and so it is on planetary surfaces that life has its best opportunity during the Stelliferous Era.
Planetary endemism does not rule out exotic forms of life not derived from water and organic macro-molecules, nor does it rule out life arising in locations other than planetary surfaces, but the nature of the Stelliferous Era and the conditions of the universe we observe points to planetary surfaces being the most common locations for life during the Stelliferous Era. Also, the “planetary” in “planetary endemism” should not be construed too narrowly: moons, planetesimals, asteroids, comets and other bodies within a planetary system are also chemically complex loci where stellar insolation can drive further chemical processes, with the possibility of emergent complexities arising in these contexts as well.
The Homeworld Effect
The homeworld effect is the perspective of intelligent agents still subject to planetary endemism. When the emergent complexities fostered by planetary endemism rise to the level of biological complexity necessary to the emergence of consciousness, there are then biological beings with a point of view, i.e., there is something that it is like to be such a biological being (to draw on Nagel’s formulation from “What is it like to be a bat?”). The first being on Earth to open its eyes and look out onto the world possessed the physical and optical perspective dictated by planetary endemism. As biological beings develop in complexity, adding cognitive faculties, and eventually giving rise to further emergent complexities, such as art, technology, and civilization, embedded in these activities and institutions is a perspective rooted in the homeworld effect.
The emergent complexities arising from the action of intelligent agents are, like the biological beings who create them, derived from the biosphere in which the intelligent agent acts. Thus civilization begins as a biocentric institution, embodying the biophilia that is the cognitive expression of biocentrism, which is, in turn, an expression of planetary endemism and the nature of the intelligent agents of planetary endemism being biological beings among other biological beings.
The homeworld effect does not rule out the possibility of exotic forms of life or unusual physical dispositions for life that would not evolve with the homeworld effect as a selection pressure, but given that planetary endemism is the most likely existential condition of biological beings during the Stelliferous Era, it is to be expected that the greater part of biological beings during the Stelliferous Era are products of planetary endemism and so will be subject to the homeworld effect.
The Overview Effect
The overview effect is a consequence of transcending planetary endemism. As biocentric civilizations increase in complexity and sophistication, deriving ever more energy from their homeworld biosphere, biocentric institutions and practices begin to be incrementally replaced by technocentric institutions and practices and civilization starts to approximate a technocentric institution. The turning point in this development is the industrial revolution.
Within two hundred years of the industrial revolution, human beings had set foot on a neighboring body of our planetary system. If a civilization experiences an industrial revolution, it will do so on the basis of already advancing scientific knowledge, and within an historically short period of time that civilization will experience the overview effect. But the unfolding of the overview effect is likely to be a long-term historical process, like the scientific revolution. Transcending planetary endemism means transcending the homeworld effect, but as the homeworld effect has shaped the biology and evolutionary psychology of biological beings subject to planetary endemism, the homeworld effect cannot be transcended as easily as the homeworld itself can be transcended.
For biological beings of planetary endemism, the overview effect occurs only once, though its impact may be gradual and spread out over an extended period of time. An intelligent agent that has evolved on the surface of its homeworld leaves that homeworld only once; every subsequent world studied, explored, or appropriated (or expropriated) by such beings will be first encountered from afar, over astronomical distances, and known to be a planet among planets. A homeworld is transcended only once, and is not initially experienced as a planet among planets, but rather as the ground of all being.
The uniqueness of the overview effect to the homeworld of biological beings of planetary endemism does not rule out further overview effects that could be experienced by a spacefaring civilization, as it eventually is able to see its planetary system, its home galaxy, and its supercluster as isolated wholes. However, following the same line of argument above — stars and their planetary systems being common during the Stelliferous Era, emergent complexities appearing on planetary surfaces characterizing planetary endemism, organisms and minds evolving under the selection pressure of the homeworld effect embodying geocentrism in their sinews and their ideas — it is to be expected that the overview effect of an intelligent agent first understanding, and then actually seeing, its homeworld as a planet among other planets, is the decisive intellectual turning point.
Bifurcation of Planetary and Spacefaring Civilizations
What I have tried to explain here is the tightly-coupled nature of these concepts, each of which implicates the others. Indeed, the four concepts outlined above — the Stelliferous Era, planetary endemism, the homeworld effect, and the overview effect — could be used as the basis of a periodization that should, within certain limits, characterize the emergence of intelligence and civilization in any universe such as ours. Peer civlizations would emerge during the Stelliferous Era subject to planetary endemism, and passing from the homeworld effect to the overview effect.
If such a civilization continues to develop, fully conscious of the overview effect, it would develop as a spacefaring civilization evolving under the (intellectual) selection pressure of the overview effect, and such a civilization would birfurcate significantly from civilizations of planetary endemism still exclusively planetary and still subject to the homeworld effect. These two circumstances represent radically different selection pressures, so that we would expect spacefaring civilizations to rapidly speciate and adaptively radiate once exposed to these novel selection pressures. I have previously called this speciation and adaptive radiation the great voluntaristic divergence.
. . . . .
. . . . .
● The Scientific Imperative of Human Spaceflight
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
15 January 2017
Early in the history of this blog I wrote about a snowstorm in Portland during December 2008, Snow in Portland, More Snow, and Lessons from a Snowstorm, and now Portland has had another uncharacteristically heavy snowfall eight years on. I am always fascinated to watch the rapidly changing behaviors of the population of a city as it responds to rapidly changing conditions, and I can’t help but extrapolate from these observations to other disruptions to the ordinary business of life.
The initial impact of a big snowstorm (in a temperate climate where snowstorms are infrequent) is chaos and frantic activity. After the initial chaos, the city goes quiet, and driving around a city after it has gone quiet gives an apocalyptic feeling, as though the end of the world has come. A snowstorm is, in miniature, the collapse of a complex society, such as Joseph Tainter wrote about:
“Collapse, as viewed in the present work, is a political process. It may, and often does, have consequences in such areas as economics, art, and literature, but it is fundamentally a matter of the sociopolitical sphere. A society has collapsed when it displays a rapid, significant loss of an established level of sociopolitical complexity. The term ‘established level’ is important. To qualify as an instance of collapse a society must have been at, or developing toward, a level of complexity for more than one or two generations. The demise of the Carolingian Empire, thus, is not a case of collapse — merely an unsuccessful attempt at empire building. The collapse, in turn, must be rapid — taking no more than a few decades — and must entail a substantial loss of sociopolitical structure. Losses that are less severe, or take longer to occur, are to be considered cases of weakness and decline.”
Joseph A. Tainter, The Collapse of Complex Societies, Cambridge: Cambridge University Press, 1988, p. 4
Of course, the collapse precipitated by a snowstorm is not a political collapse, but it is a rapid and significant loss of an established level of complexity, and a temporary return to a simpler way of life.
When someone abandons their car and walks away, eventually walking around their neighborhood rather than driving, this is a significant simplification of life, and the simplest level to which life can be reduced is that of mere survival, or perhaps I should say subsistence. Because the conditions of a snowstorm or a flood or some similar disruption (say, a power outage) are temporary it does not force a return to subsistence agriculture, but there are occasions when one finds oneself no longer concerned by the technical details of one’s work, and one is only fighting to stay alive, as all other considerations are thrust aside in order to deal with the immediacy of the circumstances. However, it is easy to imagine (especially with the looming specter of climate change) that a storm could be the first disruption in a series of escalating disruptions that could force society to abandon its complex institutions and way of life, returning to subsistence agriculture, or even nomadic hunting and gathering. If a large flood failed to recede after a few days because water levels had crept higher, the disruption of the the storm that caused the flood would be a mere foretaste of things to come.
There is a great deal of social momentum behind the ordinary business of life, and one can observe that people continue to go about their routines in the routine way for as along as possible — right up the moment when it becomes actually physically impossible to continue to going about things as usual. Thus one sees people setting out for work as usual even as the snow is beginning to fall, and as the snow piles up they try to continue to go about their business. It is only when, on the drive home, their car will not move forward another inch, when they abandon it and walk away. As long as a choice remains, most will choose to continue with the ordinary business of life; the routine is only abandoned when no choice remains and one is forced by circumstances to alter one’s behavior.
There is also a strong desire to return to normalcy after the disruption of a storm, so that at the first sign of conditions improving, people head out again in large numbers. In the case of the snowstorms I have seen in my years, this creates a problem because the main roads will be cleared of snow, but the secondary roads and parking lots are still icy, and many people over-confidently driving at full speed on the highways cause problems for themselves and others. The desire for the return to normalcy is a desire for the familiar normalcy, the old normal, while the conditions of the storm, strange and unfamiliar at first, dictate a new normal, and there is a tension between the old normal and the new normal as society attempt to adjust and compensate for changed conditions. As long as the conditions of the new normal are temporary, the old normal will return, but the longer the conditions persist, the longer the new normal persists, and, as the phrase implies, the new normal eventually becomes familiar if it endures for a sufficient period of time.
I imagine that in the case of the true collapse of societies, and not merely an ephemeral collapse precipitated by a weather event, that this desire to return to normalcy results in a lot of false starts, like commuters returning to the roads too soon after a snowstorm. There are probably many hopeful moments in the collapse of a society when people come out of their hiding places and venture out into the world again, hoping that they can return to their routines. When Sarajevo was under siege during the Balkan wars of the 90s, it was several years before life could return to normal. Similarly, when the First and Second World Wars began, it would be several years before normalcy would return.
When a society well and truly collapses, never to rise again, one can imagine for years or for decades people looked for a return to normalcy that would never come. Or if life seemed to return to normal for a time — for weeks or months or years — it was only a deceptive return to old ways that would soon disappear forever. When Roman cities in the west began to fail, there was probably a movement like the ebb and flow of the tide, when people would abandon their city, then go back, then abandon it again. Each time those who returned would be fewer in number, there would be fewer shops open, and fewer goods for sale, and there might be increasing lengths of time between abandonment and return, until eventually the period of abandonment stretched into years, and the city fell into disrepair, fit only for looting from the ruins.
. . . . .
. . . . .
. . . . .
. . . . .
In my recent paper “A Manifesto for the Scientific Study of Civilization” I argued that the study of civilization should be scientific, and that a scientific theory of civilization would be a formal theory. Prior to this, I argued in Rational Reconstructions of Time that a formal historiography is possible. What is the connection between these two claims? In A Metaphysical Disconnect I suggested that it is a philosophical problem that philosophies of time have not been tightly-coupled with philosophies of history. This implies that a formal theory of time could be tightly-coupled with a formal theory of history, and a formal theory of history would presumably encompass (or, at least, overlap) a theory of civilization. A formal theory of civilization, then, might ultimately follow from formal historiography.
I fully understand that these are strange claims for me to be making. What in the world do I mean by a formal theory of time, of history, or of civilization? How could a science of civilization be a formal science? What is a formal science, anyway? Despite the burgeoning growth of computer science in our time, which is the latest addition to the formal sciences, the very idea of the formal as a distinct category of thought (distinct, especially, from the material) seems odd and alien to us, and the distinction between the formal sciences and the natural sciences seems archaic. What are the formal sciences? Here is one view:
“To put it in Kantian terms, the formal sciences dealt with the Reine Anschauung as opposed to empirical data. By that they have been connected to the methodology of mathematics and logic, thereby being part of both the philosophical tradition and the newly won applications of mathematical sciences to the natural sciences and engineering. Both the object and the methods of the Formal sciences were recognized as different from the Natural and the Social sciences.”
“The Formal Sciences: Their Scope, Their Foundations, and Their Unity” by Benedikt Löwe, Synthese, Vol. 133, No. 1/2, Foundations of the Formal Sciences I (Oct.-Nov., 2002),pp. 5-11
In the same paper there is an explicit attempt to answer the question, “What are the Formal Sciences?” Two answers are given:
● Answer 1: “There is a profound duality in the classification of sciences according to their scientific approaches: some sciences are empirical, some are formal. The former deal with predictions and their falsification, the latter with the understanding of systems without empirical component, be it man-made systems (literary systems, the arts or social systems) or formal systems”.
● Answer 2: “Formal sciences are those that deal with the deductive analysis of formal systems (i.e., systems independent of direct human influence)”.
At present I am not going to analyze these differing definitions of the formal sciences, but I will leave them to percolate in the back of the mind of the reader in order to return to the question at hand: the study of civilization as a formal science, i.e., one formal science among many other formal sciences, however we choose to define them.
We can get a hint of what a formal science of civilization would look like from structuralist historians and historians of the Annales school, the chief representatives of the latter being Marc Bloch, Lucien Febvre, and Fernand Braudel. Marc Bloch’s two volume history of feudalism, in particular, stands out as a great achievement in the genre, with chapters devoted to features of feudal society rather than to great events and historical turning points. Whereas John Florio had Montaigne say that I describe not the essence but the passage, Bloch sought to describe not the passage, but the essence. (I previously quoted from Bloch in Hegel and the Overview Effect.)
There is (or, there will be) no one, single way to approach formal historiography, in the same way that there is no one, single axiomatization of set theory. Even if one agrees with Gödel that set theory describes a “well-determined reality” (a realist conception that most people today would agree describes the past, even if they would hesitate to say the same of set theory), there are, as yet, many distinct approaches to that reality. So too with formal historiography; there will be many distinct formalisms for the organization, exhibition, and exposition of the well-determined reality of history.
I reveal myself as being more of a traditionalist than Bloch by my preference for approaching a theory of civilization by way of a theory of history, and a theory of history by way of a theory of time. This is “traditional” in the sense that, as I have remarked many times in other places, it has been traditional to study civilization by studying history, rather than studying civilization as an object of knowledge in its own right. I retain the historical perspective, and indeed even many of the prejudices of historians (these come naturally to me), but I can also see beyond history sensu stricto and to a science of time, a science of history, and a science of civilization that lies beyond history even as it draws from the tradition all that that tradition has to offer.
Both the essentialist approach of Bloch and the Annales school, and my own quasi-historical approach to a formal science of civilization, may each have something to contribute to a theory of civilization. Obviously, these are not the only ways to study civilization. Civilization also can be studied as an empirical science — this is probably how most would conceive a science of civilization — and even as an adventure science. What is adventure science?
Together with Dr. Jacob Shively, I wrote an article about adventure science, Adventure Science Enters the Space Age, noting that “big science” has become the paradigm of scientific activity at the present time, but when individual human beings are able to go exploring they will be able to pluck the low-hanging fruit of exploration and discovery. Adventure science characterizes the earliest stage of a science when discoveries can be made simply by traveling to an exotic locale and being the first to describe some phenomenon never before documented by science. Such discoveries are difficult for us now, because the low-hanging fruit of terrestrial discovery has all been plucked, but once off Earth, new worlds will beckon with new discoveries waiting to be made. This will be a new Golden Age of adventure science.
Paradoxically, the science of civilization will become an adventure science (if it ever becomes one) quite late in its history, so that adventure science will characterize a science of civilization not in its earliest stages, but in its latest stages. But civilization has had a kind of early adventure science phase as well. Archaeology was once the paradigm of adventure science — as attested to by the cinematic adventures of Indiana Jones and the television adventures of Relic Hunter — when real life explorers entered jungles and deserts and swamps to search for long lost cities. Archaeology is perhaps the closest existing discipline that we have to a true science of civilization — archaeologists have many theories of civilization — so that the adventure science that archaeology once was, was at the same time (at least in part) an adventure science of civilization. And it may be so again, when xenoarchaeologists lead the way, looking for the ruins of alien civilizations.
All of the resources of contemporary big science, with its thousands of researchers and multi-generational socially-organized research programs, will be necessary in order to develop the science that will make possible the production of interstellar vessels. In my Centauri Dreams post, The Interstellar Imperative, I wrote, “A starship would be the ultimate scientific instrument produced by technological civilization, constituting both a demanding engineering challenge to build and offering the possibility of greatly expanding the scope of scientific knowledge by studying up close the stars and worlds of our universe, as well as any life and civilization these worlds may comprise.” Once starships become a reality, they will make possible the empirical study of civilizations, which will begin as an adventure science, the primary qualification for which will be a willingness to tolerate discomfort and to travel to distant places with a determination to document every new sight that one sees.
Geology will become an adventure science like this once again as soon as human beings have the freedom to travel around our solar system; biology and ecology will become adventure sciences once again as soon as we can visit other living worlds. The study of civilization will not become an adventure science until human beings are free to travel about the cosmos, so that this is a very distant prospect, but still a hopeful one. If we do not find a number of interesting civilizations to study, we will build a number of interesting civilizations, and eventually these will be studied in their turn. In this latter instance, the science of civilization will only become an adventure science after civilization has expanded throughout the cosmos, has forgotten the saga of its expansion, and then rediscovers itself across a plurality of worlds. And once again we will be forced to reckon with Hegel’s prescience for having said that the owl of Minerva takes flight only with the setting of the sun.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
26 December 2016
In my recent Manifesto for the Study of Civilization I employed the phrase history in an extended sense. Here is a bit more context:
“One form that the transcendence of an exclusively historical study of civilization can take is that of extrapolating historical modes of thought so that these modes of thought apply to the future as well as to the past (and this could be called history in an extended sense).”
In several posts I have developed what I call concepts in an extended sense, as in Geocentrism in an Extended Sense and “biocentrism in an extended sense” in Addendum on the Technocentric Thesis and “ecology in an extended sense” in Intelligent Invasive Species.
In Developmental Temporality I wrote:
“With the advent of civilization in the most extended sense of that term, comprising organized settled agricultural societies and their urban centers, planning for the future becomes systematic.”
And in Reduction, Emergence, Supervenience I wrote:
“Philosophy today, then, is centered on the extended conceptions of ‘experience’ and ‘observation’ that science has opened up to us, and these extended senses of experience and observation go considerably beyond ordinary experience, and the prima facie intellectual intuitions available to beings like ourselves, whose minds evolved in a context in which perceptions mattered enormously while the constituents and overall structure of the cosmos mattered not at all.”
In these attempts to extrapolate, expand, and extend concepts beyond their ordinary usage — the result of which might also be called overview concepts — each traditional concept must be treated individually, as there is a limit that is demarcated by the intrinsic meaning of the concept, and these limits are different in each case. With history, the extrapolation of the concept is obvious: history has taken the past as its remit, but history in an extended sense would apply to the totality of time. This is already being done in Big History.
When I attended the second IBHA conference in 2014 I was witness to a memorable exchange that I described in 2014 IBHA Conference Day 2:
“During the question and answer session, a fellow who had spoken up in previous sessions with questions stood up and said that there were (at least) two conceptual confusions pervasive throughout discussions at this conference: 1) that something could come from nothing (presumably a reference to how the big bang is framed, though this could have been intended more generally as a critique of emergentism) and, 2) that history can say anything about the future. The same individual (whose name I did not get) said that no one had given an adequate definition of history, and then noted that the original Greek term for history meant ‘inquiry.’ Given this Grecian (or even, if you like, Herodotean) origin for the idea of history as an inquiry, I immediately asked myself, ‘If one can conduct an inquiry into the past, why cannot one also conduct an inquiry into the future?’ No doubt these inquires will be distinct because one concerns the past and the other the future, but cannot they be taken up in the same spirit?”
There was a note of frustration in the voice of the speaker who objected to any account of the future as a part of history, and while I could appreciate the source of that frustration, it reminded me of every traditionalist protest against the growth of scientific knowledge made possible by novel methods not sanctioned by tradition. In this connection I think of Isaiah Berlin’s critique of scientific historiography, which I previously discussed in Big History and Scientific Historiography.
Berlin argued that the historical method is intrinsically distinct from the scientific method, so that there can be no such thing as scientific historiography, i.e., that the intrinsic limitations of the concept of history restricts history from being scientific in the way that the natural sciences are scientific. While Berlin’s objection to scientific historiography is not stated in terms of restricting the expansion of historical modes of thought, his appeal to a nature of history intrinsically irreconcilable with science and the scientific method is parallel to an appeal to the nature of history as being intrinsically about the past (thus intrinsically not about the future), hence there can be no such thing as a history that includes within it the study of the future in addition to the study of the past.
Here is a passage in which Berlin characterizes distinctively historical modes of thought, contrasting them to scientific modes of thought:
“Historians cannot ply their trade without a considerable capacity for thinking in general terms; but they need, in addition, peculiar attributes of their own: a capacity for integration, for perceiving qualitative similarities and differences, a sense of the unique fashion in which various factors combine in the particular concrete situation, which must at once be neither so unlike any other situation as to constitute a total break with the continuous flow of human experience, nor yet so stylised and uniform as to be the obvious creature of theory and not of flesh and blood. The capacities needed are rather those of association than of dissociation, of perceiving the relation of parts to wholes, of particular sounds or colours to the many possible tunes or pictures into which they might enter, of the links that connect individuals viewed and savoured as individuals, and not primarily as instances of types or laws.”
Isaiah Berlin, “The Concept of Scientific History,” in Concepts and Categories, p. 140
Every cognitive capacity that Berlin here credits to the historian can be equally well exercised in relation to the future as to the past (I should point out that, as far as I know, Berlin did not take up the problem of the relation of the historian to the future). Indeed, one of the weaknesses of futurism has been that futurists have not immersed themselves in these distinctively historical modes of thought; our conception of the future could greatly benefit from a capacity for integration and perceiving the relation of parts to wholes. I don’t think Berlin would ever have imagined his critique of scientific historiography as advice for futurists, but it could be profitably employed in developing history in an extended sense.
It is common for historians to invoke distinctively historical modes of thought, and I believe that this is a valid concern. Indeed, I would go farther yet. Human modes of thought are primarily temporal, and non-temporal modes of thought come very late in our history as a species in comparison to the effortless way we learn to think of time in subtle and sophisticated ways. For example, when one learns a language, one finds that one spends an inordinate amount of time attempting to master past, present, and future tenses — the tenses of our mother tongue are so fixed in our minds that any other schema strikes us as counterintuitive (and, interestingly, even those who attain fluency in another language or languages usually revert to their mother tongue for counting). But in order to communicate effectively we must master the logic of time as expressed in linguistic tenses. Human beings are inveterate planners, preparers, and schemers; our present is pervasively animated by a concern for the future. We are so taken up with our plans for the future that it is considered something of a “gift” to be able to “live in the moment.”
Many of Berlin’s examples of distinctively historical thought position the historian as attempting to explain historical change. The emphasis on describing change in history results in an indirect deemphasis of continuity, though continuity is arguably the overwhelming experience of time and history. It would be almost impossible for us to delineate all of the things that we know will happen tomorrow, and which we do not even bother to think of as predictions because they fall so far near certainty on the epistemic continuum of historical knowledge. All of the laws of science that have been discovered up to the present day will continue to be in effect tomorrow, and all of the events and processes that make up the world will continue to be governed by these laws of nature tomorrow. We could exhaust ourselves describing the nomological certainties of the morrow, and still not have exhausted the predictions we might have made. Thus it is we know that the sun will rise tomorrow, and we can explain how and why the sun will rise tomorrow. If you are an anchorite living in a cave, the sun will not rise for you, but you can nevertheless be confident that Earth will continue to orbit the sun while rotating, and that this process will result in the appearance of the sun rising for everyone else not so confined.
But our sciences that describe the laws of nature that govern the world are incomplete, and they are in particular incomplete when it comes to history. I have noted elsewhere that there is (as yet) no science of time, and it is interesting to speculate that the absence of a science of time may be related to a parallel absence of a truly scientific historiography or a science of civilization. Because we have no science of time, we have no formal concepts of time — or, rather, we have no concepts of time recognized to be formal concepts. I have argued elsewhere that the idea of the punctiform present is a formal concept of time, i.e., interpreted as a formal concept it can be employed in a formal theory of time which can illuminate actual time as an ideal, simplified model. But as soon as you try to interpret the idea of the punctiform present as an empirical concept you run into difficulties. Would it be possible to measure a dimensionless instant? The punctiform present is like a pendulum with a weightless string, frictionless fulcrum, and no air drag. No such pendulum exists in actual fact, but the ideal pendulum remains a useful fiction for us. Similarly, the punctiform present is a useful fiction for a formal science of time.
A truly (perhaps exhaustively) scientific historiography would not only employ the methods of the special sciences in the exposition of history, but would also incorporate a science of time that would allow us to be as definite about history to come as we can now be definite about our predictions for the natural world as governed by laws of nature. It is not difficult to imagine what Berlin would have thought of such an idea. Here is another quote from Berlin’s essay on scientific historiography:
“…the attempt to construct a discipline which would stand to concrete history as pure to applied, no matter how successful the human sciences may grow to be — even if, as all but obscurantists must hope, they discover genuine, empirically confirmed, laws of individual and collective behaviour — seems an attempt to square the circle.”
Isaiah Berlin, “The Concept of Scientific History,” in Concepts and Categories, p. 142
What Berlin here condemns as an attempt to square the circle is precisely my ideal in history, and it is what I called formal historiography in Rational Reconstructions of Time. A formulation of history in an extended sense would be a step toward a formal historiography.
While on one level I am interested in history as an intellectual discipline in its own right — history for history’s sake — and therefore I am interested in formal historiography as a sui generis discipline, I also have an ulterior motive in the pursuit of a formal historiography that can develop history in an extended sense. Such a formal historiography will be one tool in the interdisciplinary toolkit of future scientists of civilization, who must study civilization both in terms of its past and its future.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .
7 December 2016
The full awareness of our sun being a star, and the stars being suns in their own right, was a development nearly coextensive with the entire history of science, from its earliest stirrings in ancient Greece to its modern form at the present time. During the Enlightenment there was already a growing realization of this, as can be seen in a number of scientific works of the period, but scientific proof had to wait for a few generations more until new technologies made available by the industrial revolution produced scientific instruments equal to the task.
The scientific confirmation of this understanding of cosmology, which is, in a sense, the affirmation of Copernicanism (as distinct from heliocentrism) came with two scientific discoveries of the nineteenth century: the parallax of 61 Cygni, measured by Friedrich Wilhelm Bessel and published in 1838, which was the first accurate distance measured to a star other than the sun, and the spectroscopy work of several scientists — Fraunhofer, Bunsen, Kirchhoff, Huggins, and Secchi, inter alia (cf. Spectroscopy and the Birth of Astrophysics) — which demonstrated the precise chemical composition of the stars, and therefore showed them to be made of the same chemical elements found on Earth. The stars were no longer immeasurable or unknowable; they were now open to scientific study.
The Ptolemaic conception of the universe that preceded this Copernican conception painted a very different picture of the universe, and of the place of human beings within that universe. According to the Ptolemaic cosmology, the heavens were made of a different material than the Earth and its denizens (viz. quintessence — the fifth element, i.e., the element other than earth, air, fire, and water). Everything below the sphere of the moon — sublunary — was ephemeral and subject to decay. Everything beyond the sphere of the moon — superlunary — was imperishable and perfect. Astronomical bodies were perfectly spherical, and moved in perfectly circular lines (except for the epicycles). Comets were a problem (i.e., an anomaly), because their elliptical orbits ought to send them crashing through the perfect celestial spheres.
This Ptolemaic cosmology largely satisfied the scientific, philosophical, moral, and spiritual needs of western thought from classical antiquity to the end of the Middle Ages, and this satisfaction presumably follows from a deep consonance between this conception of the cosmos and a metaphysical vision of what the world ought to be. Ptolemaic cosmology is the intellectual fulfillment of a certain kind of heart’s desire. But this was not the only metaphysical vision of the world having its origins (or, at least, its initial expression) in classical antiquity. Another intellectual tradition that pointed in a different direction was mathematics.
Mathematics was the first science to attain anything like the rigor that we demand of science today. It remains an open question to this day — an open philosophical question — whether mathematics is a science, one of the sciences (a science among sciences), or whether it is something else entirely, which happens to be useful in the sciences, as, for example, the formal propaedeutic to the empirical sciences, in need of formal structure in order to organize their empirical content. The sciences, in fact, get their rigor from mathematics, so that if there were no mathematical rigor, there would be no possibility of scientific rigor.
Mathematics has been known since antiquity as the paradigm of exact thought, of precision, the model for all sciences to follow (remembering what science meant to the ancients, which is not what it means today: a demonstrative science based on first principles), and this precision has been seen as a function of its formalism, which is to say its definiteness, it boundedness, its participation in the peras. Despite this there was yet a recognition of the infinite (apeiron) in mathematics. I would go further, and assert that, while mathematics as a rigorous science has its origins in the peras, it has its telos in the apeiron. This is a dialectical development, as we will see below in Proclus.
Proclus expresses the negative character of the infinite in his commentary on Euclid’s Elements:
“…the infinite is altogether incomprehensible to knowledge; rather it takes it hypothetically and uses only the finite for demonstration; that is, it assumes the infinite not for the sake of the infinite, but for the sake the infinite.”
Proclus, A Commentary on the First Book of Euclid’s Elements, translated, with an introduction and notes, by Glenn R. Morrow, Princeton: Princeton University Press, 1992, Propositions: Part One, XII, p. 223. This whole section is relevant, but I have quoted only a brief portion.
There is no question that the apeiron appeared on the inferior side of the Pythagorean table of opposites, but it is also interesting to note what Proclus says earlier on:
“The objects of Nous, by virtue of their inherent simplicity, are the first partakers of the Limit (περας) and the Unlimited (ἄπειρον). Their unity, their identity, and their stable and abiding existence they derive from the Limit; but for their variety, their generative fertility, and their divine otherness and progression they draw upon the Unlimited. Mathematicals are the offspring of the Limit and the Unlimited…”
Proclus, Commentary on the First Book of Euclid, Prologue: Part One, Chap. II
Here the apeiron appears on an equal footing with the peras, both being necessary to mathematical being. “Mathematicals” are born of the dialectic of the finite and the infinite. Both of these elements are also found (hundreds of years earlier) in the foundations of geometry. As the philosophers produced proofs that there could be no infinite number or infinite space, Euclid spoke of lines and planes extended “indefinitely” (as “apeiron” is usually translated in Euclid). Even later when the Stoics held that the material world was surrounded by an infinite void, this void had special properties which distinguished it from the material world, and indeed which kept the material world from having any relation with the void. The use of infinities in geometry, however, even though in an abstract context, force one to maintain that space locally, directly before one, is essentially of the same kind as space anywhere else along the infinite extent of a line, and indeed the same as space infinitely distant. All spaces are of the same kind, and all are related to each other. This constitutes a purely formal conception of the uniformity and continuity of nature. One might interpret the subsequent history of science as redeeming, through empirical evidence, this formal insight.
The infinite is the “internal horizon” (to use a Husserlian phrase) and the telos of mathematical objects. Given this conception of mathematics, the question that I find myself asking is this: what was the mathematical horizon of the Greeks? Did the idea of a line or a plane immediately suggest to them an infinite extension, and did the idea of number immediately suggest the infinite progression of the series, or were the Greeks able to contain these conceptions within the peras, using them not unlike we use them, but allowing them to remain limited? Did ancient mathematical imagination encompass the infinite, or must such a conception of mathematical objects (as embedded in the infinite) wait for the infinite to be disassociated from the apeiron?
The wait was not long. While the explicit formulation of the mathematical infinite had to wait until Cantor in the nineteenth century, Greek thought was dialectical, so regardless of the nature of mathematical concepts as initially conceived, these concepts inevitably passed into their opposite numbers and grew in depth and comprehensiveness as a result of the development of this dialectic. Greek thought may have begun with an intellectual commitment to the peras, and a desire to contain mathematics within the peras, consequently an almost ideological effort to avoid the mathematical infinite, but a commitment to dialectic confounds the demand for limitation. It is, then, this dialectical character of Greek thought that gives us the transition from purely local concepts to a formal concept of the uniformity of nature, and then the transition from a formal conception of uniformity to an empirical conception of uniformity, and this latter is the cosmological principle that is central to contemporary cosmology.
The cosmological principle brings us back to where we started: To say that the sun is a star, and every star a sun, is to say that the sun is a star among stars. Earth is a planet among planets. The Milky Way is a galaxy among galaxies. This is not only a Copernican idea, it is also a formal idea, like the formal conception of the uniformity of nature. (In A Being Among Beings I made a similar about biological beings.) To be one among others of the same kind is to be a member of a class, and to be a member of a class is to be the value of a variable. Quine, we recall, said that to be is to be the value of a variable. This is a highly abstract and formal conception of ontology, and that is precisely the importance of the formulation. This is the point beyond which we can begin to reason rigorously about our place in the universe.
We require a class of instances before we can draw inductive inferences, generalize from all members of this class, or formalize the concept represented by any individual member of that class. This is one of the formal presuppositions of scientific thought never made explicit in the methodology of science. We could not formulate the cosmological principle if we did not have a concept of “essentially the same,” because the “same” view that we see looking in any direction in the universe is not identically the same, but rather essentially the same. Of any two views of the universe, every detail is different, but the overview is the same. The cosmological principle is not a generalization, not an inductive inference from empirical evidence; it is a formal idea, a regulative idea that makes a certain kind of cosmological thought possible.
Formal principles like this are present throughout the sciences, though not often recognized for what they are. Bessel’s observations of 61 Cygni not only required industrialized technology to produce the appropriate scientific instruments, these observations also presupposed the mathematics originating in classical antiquity, so that the nineteenth century scientific work that proved the stars to be like our sun (and vice versa) was predicated upon parallel formal conceptions of universality structured into mathematical thought since its inception as a theoretical discipline (in contradistinction to the practical use of mathematics as a tool of engineering). Formal Copernicanism preceded empirical Copernicanism. Without that formal component of scientific knowledge, that scientific knowledge would never have come into being.
. . . . .
. . . . .
. . . . .
. . . . .
. . . . .