How to Live on a Planet

27 September 2017

Wednesday


Humanity is learning, slowly, how to live on a planet. What does it mean to live on a planet? Why is this significant? How has our way of living on a planet changed over time? How exactly does an intelligent species capable of niche-construction on a planetary scale go about revising its approach to niche construction to make this process consistent with the natural history and biospheric evolution of its homeworld?

Once upon a time the Earth was unlimited and inexhaustible for human beings for all practical purposes. Obviously, Earth was was not actually unlimited and inexhaustible, but for a few tens of thousands or hundreds of thousands of hunter-gatherers distributed across the planet in small bands, this was an ecosystem that they could not have exhausted even if they had sought to do so. Human influence over the planet at this time was imperceptible; our ancestors were simply one species among many species in the terrestrial biosphere. Even before civilization this began to change, as our ancestors have been implicated in the extinction of ice age megafauna. The evidence for this is still debated, but human populations had become sufficiently large and sufficiently organized by the upper Paleolithic that their hunting could plausibly have driven anthropogenic extinctions.

In this earliest (and longest) period of human history, we did not know that we lived on a planet. We did not know what a planet was, the relation of a planet to a star, and the place of stars in the galaxy. The Earth for us at this time was not a planet, but a world, and the world was effectively endless. Only with the advent of civilization and written language were we able to accumulate knowledge trans-generationally, slowly working out that we lived on a planet orbiting a star. This process required several thousand years, and for most of these thousands of years the size of our homeworld was so great that human efforts seemed to not even make a dent in the biosphere. It seemed the the forests could not be exhausted of trees or the oceans exhausted of fish. But all that has changed.

In the past few hundred years, the scope and scale of human activity, together with the size of the human population, has grown until we have found ourselves at the limits of Earth’s resources. We actively manage and limit the use of resources, because if we did not, the seven billion and growing human population would strip the planet clean and leave nothing. This process had already started in the Middle Ages, when many economies were forced to manage strategic resources like timber for shipbuilding, but the process has come to maturity in our time, as we are able to describe and explain scientifically the impact of the human population on our homeworld. We have, today, the conceptual framework necessary to understand that we live on a planet, so that we understand the limitations on our use of resources theoretically as well as practically. When earlier human activities resulted in localized extinctions and shortages, we could not put this in the context of the big picture; now we can.

Today we know what a planet is; we know what we are; we know the limitations dictated by a planet for the organisms constituting its ecosystems. This knowledge changes our relationship to our homeworld. Many definitions have been given for the Anthropocene. One way in which we could define the anthropocene in this context is that it is that period in terrestrial history when human beings learn to live on Earth as a planet. Generalized beyond this anthropocentric formulation, this becomes the period in the history of a life-bearing planet in which the dominant intelligent species (if there is one) learns to live on its planet as a planet.

In several posts I have written about the transition of the terrestrial energy grid from fossil fuels to renewable resources (cf. The Human Future in Space, The Conversion of the Terrestrial Power Grid, and Planetary Constraints 9). This process has already started, and it can be expected to play out over a period of time at least equal to the period of time we have been exploiting fossil fuels.

I recently happened upon the article How to Run the Economy on the Weather by Kris De Decker, which discusses in detail how economies and technologies prior to the industrial revolution were adapted to the intermittency of wind and water, and the adaptability of such habits to contemporary technologies. And I recall some years ago when I was in Greece, specially the island of Rhodes, every house had solar water heaters on the roof (and, of course, sunshine is plentiful in Greece), and everyone seemed to accept as a matter of course that you must shower while the sun is out. A combination of very basic behavioral changes supplemented by contemporary technology could facilitate the transition of the terrestrial power grid with little or no decline in standards of living. This is part of what it means to learn to live on a planet.

As we come to better understand biology, astrobiology, ecology, geology, and cosmology, and we thus come to better understand our homeworld and ourselves, we will learn more about how to live on a planet. But the expansion of our knowledge of exoplanets and astrobiology will be predicated upon our ability to travel to other worlds in order to study them, and if we are fortunate enough to endure for such a time and to achieve such things, then we will have to learn how to live in a universe.

The visible universe is finite. Though the visible universe may be part of an infinitistic cosmology (or even an infinitistic multiverse), the expansion of the universe has created a cosmological horizon beyond which we cannot see. I have previously quoted a passage from Leonard Susskind to this effect:

“In every direction that we look, galaxies are passing the point at which they are moving away from us faster than light can travel. Each of us is surrounded by a cosmic horizon — a sphere where things are receding with the speed of light — and no signal can reach us from beyond that horizon. When a star passes the point of no return, it is gone forever. Far out, at about fifteen billion light years, our cosmic horizon is swallowing galaxies, stars, and probably even life. It is as if we all live in our own private inside-out black hole.”

Leonard Susskind, The Black Hole War: My Battle with Stephen Hawking to make the World Safe for Quantum Mechanics, New York, Boston, and London: Little, Brown and Company, 2008, pp. 437-438

We know, then, scientifically, that the universe is effectively finite as our homeworld is finite, but the universe is so large in comparison to the scale of human activity, indeed, so large even in comparison to the aspirational scale of human activity, that the universe is endless for all practical purposes. Though we are already learning how to live on a planet, in relation to the universe at large we are like our hunter-gather ancestors dwarfed by a world that was, for them, effectively endless.

Only at the greatest reach of the scale of supercivilizations will we — if we last that long and achieve that scale of development — run into the limits of our home galaxy, and then into the limits of the universe, at which time we will have to learn how to live in a universe. I implied as much in an illustration that I created for my Centauri Dreams post, Stagnant Supercivilizations and Interstellar Travel (reproduced below), in which I showed a schematic representation of the carrying capacity of the universe. At this scale of activity we would be engaging in cosmological niche construction in order to make a home for ourselves in the universe, as we are now engaging in planetary-scale niche construction as we learn how to live on a planet.

. . . . .

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Advertisements

Sunday


Looking down on Earth from above may not only make us reevaluate out relationship to the planet, but may also help us to understand the planet better.

Science is a way to better understand the world, but science itself is not always easy to understand, and we often find that, after clarifying some problem through science, we must then clarify the science so that the science makes sense to us. Some call this science communication; I call it the pursuit of intuitive tractability.

While it is not part of science proper to seek intuitively tractable formulations, it is part of human nature to seek intuitively tractable formulations, as we are more satisfied with science formulated in intuitively tractable forms than with science that is not intuitively tractable. For example, there is, as yet, no intuitively tractable formulation of quantum theory, and this may be why Einstein famously wrote in a letter to Max Born that, “Quantum Mechanics is very impressive. But an inner voice tells me that it is not yet the real thing.”

When the concept of zero was introduced into mathematics, it was thought to be an advanced and difficult idea, but we now teach a number system starting with zero to children in primary school. In a similar way, the Hindu-Arabic system of numbers has displaced almost every other system of numbers because it is what I would paradoxically call an intuitive formalism, i.e., it is a formalization of the number concept that is both adequate to mathematics and closely follows our intuitive conception of number. Mathematics is easier with Hindu-Arabic numerals than other numbering systems because this numbering system is intuitively tractable. There are other formalisms for number that are equally valid and equally correct, but not as intuitively tractable.

The pursuit of intuitive tractability has also been evident in geometry, and especially the axiomatic exposition of geometry that begins with postulates accepted ab initio as self-evident, and which has been the model of rigorous mathematics ever since Euclid. Euclid’s fifth postulate, the famous parallel postulate, is difficult to understand and was a theoretical problem for geometry until its independence was proved, but whether or not the fifth postulate was demonstrably independent of the other postulates, Euclid’s opaque exposition did not help. Here is Euclid’s parallel axiom from the Elements:

“If a line segment intersects two straight lines forming two interior angles on the same side that sum to less than two right angles, then the two lines, if extended indefinitely, meet on that side on which the angles sum to less than two right angles.”

Almost two thousand years later, in 1846, John Playfair formulated what we now call “Playfair’s axiom,” which tells us everything that Euclid’s postulate sought to communicate, but in a far more intuitively tractable form: “In a plane, given a line and a point not on it, at most one line parallel to the given line can be drawn through the point.” Once this more intuitively tractable formulation of the parallel postulate was available, Euclid’s formulation was largely abandoned. There is, then, a process of cognitive selection, whereby the most intuitively tractable formulations are preserved and the less intuitively tractable formulations are abandoned.

Those concepts that are the most intuitively tractable are those concepts that are familiar to us all and which are seamlessly integrated into ordinary thought and language. I have called such concepts “folk concepts.” Folk concepts that have persisted from their origins in our earliest evolutionary psychology up into the present have been subjected to the cognitive equivalent of natural selection, so that we can reasonably speak of folk concepts as having been refined and elaborated by the experience of many generations.

In a series of posts — Folk Astrobiology, Folk Concepts of Scientific Civilization, and Folk Concepts and Scientific Progress — I have considered the nature of “folk” concepts as they have been frequently invoked, and it is natural to ask, in the light of such an inquiry, whether there is a “folk Weltanschauung” that is constituted by a cluster of folk concepts that naturally hang together, and which inform the pre-scientific (or non-scientific) way of thinking about the world.

Arguably, the idea of a folk Weltanschauung is already familiar by a number of different terms that philosophers have employed to identify the concept (or something like the concept) — naïve realism or common sense realism, for example. What Husserl called “natürliche Einstellung” and which Boyce Gibson translated as “natural standpoint” and Fred Kersten translated as “natural attitude” could be said to approximate a folk Weltanschauung. Here is how Husserl describes the natürliche Einstellung:

“I am conscious of a world endlessly spread out in space, endlessly becoming and having endlessly become in time. I am conscious of it: that signifies, above all, that intuitively I find it immediately, that I experience it. By my seeing, touching, hearing, and so forth, and in the different modes of sensuous perception, corporeal physical things with some spatial distribution or other are simply there for me, ‘on hand’ in the literal or the figurative sense, whether or not I am particularly heedful of them and busied with them in my considering, thinking, feeling, or willing.”

Edmund Husserl, Ideas Pertaining to a Pure Phenomenology and to a Phenomenological Philosophy: First Book: General Introduction to a Pure Phenomenology, translated by Fred Kersten, section 27

Husserl characterizes the natural attitude as a “thesis” — a thesis consisting of a series of posits of the unproblematic existence of ordinary objects — that can be suspended, set aside, as it were, by the phenomenological procedure of “bracketing.” These posits could be identified with folk concepts, making the thesis of the natural standpoint into a folk Weltanschauung, but I think this interpretation is a bit forced and not exactly what Husserl had in mind.

Perhaps closer to what I am getting at than the Husserlian natural attitude is what Wilfrid Sellars has called the manifest image of man-in-the-world, or simply the manifest image. Sellars’ thought is no easier to get a handle on than Husserl’s thought, so that one never quite knows if one has gotten it right, and one can easily imagine being lectured by a specialist in the inadequacies of one’s interpretation. Nevertheless, I think that Sellers’ manifest image is closer to what I am trying to get at than Husserl’s natürliche Einstellung. Closer, but still not the same.

Sellars develops the idea of the manifest image in contrast to the scientific image, and this distinction is especially given exposition in his essay Philosophy and the Scientific Image of Man. After initially characterizing the philosophical quest such that, “[i]t is… the ‘eye on the whole’ which distinguishes the philosophical enterprise,” and distinguishing several different senses in which philosophy could be said to be a synoptic effort at understanding the world as a whole, Sellars introduces terms for contrasting two distinct ways of seeing the world whole:

“…the philosopher is confronted not by one complex many dimensional picture, the unity of which, such as it is, he must come to appreciate; but by two pictures of essentially the same order of complexity, each of which purports to be a complete picture of man-in-the-world, and which, after separate scrutiny, he must fuse into one vision. Let me refer to these two perspectives, respectively, as the manifest and the scientific images of man-in-the-world.”

Wilfrid Sellars, Philosophy and the Scientific Image of Man, section 1

Sellars’ distinction between the manifest image and the scientific image has been quite influential. A special issue of the journal Humana Mente, Between Two Images: The Manifest and Scientific Conceptions of the Human Being, 50 Years On, focused on the two images. Bas C. van Fraassen in particular has written a lot about Sellars, devoting an entire book to one of the two images, The Scientific Image, and has also written several relevant papers, such as “On the Radical Incompleteness of the Manifest Image” (Proceedings of the Biennial Meeting of the Philosophy of Science Association,Vol. 1976, Volume Two: Symposia and Invited Papers 1976, pp. 335-343). All of this material is well worth reading.

Sellars is at pains to point out that his distinction between manifest image and scientific image is not intended to be a distinction between pre-scientific and scientific worldviews (“…what I mean by the manifest image is a refinement or sophistication of what might be called the ‘original’ image…”), though it is clear from this exposition that the manifest image, however refined and up-to-date, has its origins in a pre-scientific conception of the world. (“It is, first, the framework in terms of which man came to be aware of himself as man-in-the-world.”) The essence of this distinction between the manifest image and the scientific image is that the manifest image is correlational while the scientific image is postulational. What this means is that the manifest image “explains” the world (in so far as it could be said to explain the world at all) by correlations among observables, while the scientific image explains the world by positing unobservables that connect observables “under the surface” of things, as it were (involving, “…the postulation of imperceptible entities”). Sellars also maintains that the manifest image cannot postulate in this way, and therefore cannot be improved or refined by science, although it can improve on itself by its own correlational methods.

I do not yet understand Sellars well enough to say why he insists that the manifest image cannot incorporate insights from the scientific image, and this is a key point of divergence between Sellars’ manifest image and what I above called a folk Weltanschauung. If a folk Weltanschauung consists of a cluster of tightly-coupled folk concepts (and perhaps a wide penumbra of associated but loosely-coupled folk concepts), then the generation of refined scientific concepts can slowly, one-by-one, replace folk concepts, so that the folk Weltanschauung gradually evolves into a more scientific Weltanschauung, even if it is not entirely transformed under the influence of scientific concepts. Science, too, consists of a cluster of tightly-coupled concepts, and these two distinct clusters of concepts — the folk and the scientific — might well resist mixing for a time, but the human mind cannot keep such matters rigorously separate, and it is inevitable that each will bleed over into the other. Sometimes this “bleeding over” is intentional, as when science reaches for metaphors or non-scientific language as a way to make its findings understood to a wider audience. This is part of the pursuit of intuitively tractable formulations, but it can also go very wrong, as when scientists adopt theological language in an attempt at a popular exposition that will not be rejected out-of-hand by the Great Unwashed.

Despite my differences with Sellars, I am going to here adopt his terminology of the manifest image and the scientific image, and I will hope that I don’t make too much of a mess of it. I will have more to say on this use of Sellars’ concepts below (especially in relation to the postulational character of the scientific image). In the meantime, I want to use Sellars’ concepts in a exposition of intuitive tractability. Sellars’ uses the metaphor of “stereoscopic vision” as the proper way to understand how we must bring together the manifest image and the scientific image as a single way of understanding the world (“…the most appropriate analogy is stereoscopic vision, where two differing perspectives on a landscape are fused into one coherent experience”). I think, on the contrary, that intuitively tractable formulations of scientific concepts can make the manifest image and the scientific image coincide, so that they are one and the same, and not two distinct images fused together. A slightly weaker formulation of this is to assert that intuitively tractable formulations allow us to integrate the manifest image and the scientific image.

Now I want to illustrate this by reference to the overview effect, that is to say, the cognitive effect of seeing our planet whole — preferably from orbit, but, if not from orbit, in photographs and film that make the point as unmistakably as though one were there, in orbit, seeing it with one’s own eyes.

Before the overview effect, we saw our planet with the same eyes, but even after it is proved to us that the planet is (roughly) a sphere, hanging suspended in space, it is difficult to believe this. All manner of scientific proofs of the world as a spherical planet can be adduced, but the science lacks intuitive tractability and we have a difficult time bringing together our scientific concepts and our folk concepts of the world — or, if you will, we have difficulty reconciling the manifest image and the scientific image. The two are distinct. Until we achieve the overview effect, there is an apparent contradiction between what we experience of the world and our scientific knowledge of the world. Our senses tell us that the world is flat and solid and unmoving; scientific knowledge tells us that the world is round and moving and hanging in space.

Once we attain the overview effect, this changes, and the apparent contradiction is revealed as apparent. The overview effect shows how the manifest image and the scientific image coincide. The things we know about ordinary objects, which shapes the manifest image, now applies to Earth, which is seen as an object rather than as surrounding us as an environment with an horizon that we can never reach, and which therefore feels endless to us. Seen from orbit, this explains itself intuitively, and an explicit explanation now appears superfluous (as is ideally the case with an axiom — it is seen to be true as soon as it is understood). The overview effect makes the scientific knowledge of our planet as a planet intuitively tractable, transforming scientific truths into visceral truths. One might say that the overview effect is the lived experience of the scientific truth of our homeworld. In this particular case, we have replaced a folk concept with a scientific concept, and the scientific concept is correct even as intuition is satisfied.

The use of the overview effect to illustrate the manifest and scientific images, and their possible coincidence in a single experience, is especially interesting in light of Sellars’ insistence that the scientific image is distinctive because it is postulational, and more particularly that it postulates unobservables as a way to explain observables. When, in a scientific context, someone speaks of unobservables or “imperceptible entities” the assumption is that we are talking about entities that are too small to see with the naked eye. The germ theory of disease and the atomic theory of matter both exemplify this idea of unobservables being observable because they are smaller than the resolution of unaided human vision. We can only observe these unobservables with instruments, and then this experience is mediated by complex instruments and an even more complex conceptual framework so that no one ever speaks of the “lived experience” of particle physics or microbiology.

In contrast to this, the Earth is unobservable to the human eye not because it is too small, but because it is too large. When shown scientific demonstrations that the world is round, we must posit an unobservable planet, and then identify this unobservable entity with the actual ground under our feet. This is difficult to do, intuitively speaking. We see the world at all times, but we do not see it as a planet. We do not see enough of the world at any one moment to see it as a planet. Enter the overview effect. Seeing the Earth whole from space reveals the entity that is planet Earth, and if one has the good fortune to lift off from Earth and experience the process of departing from its surface to then see the same from space, this makes a previously unobservable postulate into a concretely experienced entity.

We are in the same position now vis-à-vis our place within the Milky Way galaxy, and our place within the larger universe, as we were once in relation to the spherical Earth. Our accumulated scientific knowledge tells us where we are at in the universe, and where we are at in the Milky Way. We can even see a portion of the Milky Way when we look up into the night sky, but we cannot stand back and see the whole from a distance, taking in the Milky Way and pointing of the position of our solar system within one of the spiral arms of our galaxy. We know it, but we haven’t yet experienced it viscerally. We have to posit the Milky Way galaxy as a whole, the Virgo supercluster, and the filaments of galaxies that stretch through the cosmos, because they are too large for us to observe at present. They are partially observed, in the way we might say that an atom is partially observed when we look at a piece of ordinary material composed of atoms.

Our postulational scientific image of the universe in which we live is redeemed for intuition by experiences that put us in a position to view these entities with our own eyes, and so to see them in an intuitively tractable manner. Perhaps one of the reasons that quantum theory remains intuitively intractable is that the unobservables that it posits are so small that we have no hope of ever seeing them, even with an electron microscope.

Ultimately, intuitively tractable formulations of formerly difficult if not opaque scientific ideas is a function of the conceptual framework that we employ, and this is ultimately a philosophical concern. Sellars suggests that the manifest and scientific conceptual framework might be harmonized in stereoscopic vision, but he doesn’t hold out any hope that the manifest image can be integrated with the scientific image. I think that the example of the overview effect demonstrates that there are at least some cases when manifest image and scientific image can be shown to coincide, and therefore these two ways of grasping the world are not entirely alien from each other. Cosmology may be the point of contact at which the two images coincide and through which the two images can communicate.

The pursuit of intuitive tractability is, I submit, a central concern of scientific civilization. If there ever is to be a fully scientific civilization, in which scientific ways of knowing and scientific approaches to problems and their solutions are the pervasively held view, this scientific civilization will come about because we have been successful in our pursuit of intuitive tractability, and we are able to make advanced scientific concepts as familiar as the idea of zero is now familiar to us. Since the question of a conceptual framework in which rigorous science and intuitively tractable concepts can be brought together is not a scientific question, but a philosophical question, the contemporary contempt for philosophy in the special sciences is invidious to the effective pursuit of intuitive tractability. The fate of scientific civilization lies with philosophy.

. . . . .

astronaut-above-earth

. . . . .

Overview Effects

The Epistemic Overview Effect

The Overview Effect as Perspective Taking

Hegel and the Overview Effect

The Overview Effect in Formal Thought

Brief Addendum on the Overview Effect in Formal Thought

A Further Addendum on the Overview Effect in Formal Thought, in the Way of Providing a Measure of Disambiguation in Regard to the Role of Temporality

Our Knowledge of the Internal World

Personal Experience and Empirical Knowledge

The Overview Effect over the longue durée

Cognitive Astrobiology and the Overview Effect

The Scientific Imperative of Human Spaceflight

Planetary Endemism and the Overview Effect

The Overview Effect and Intuitive Tractability

Homeworld Effects

The Homeworld Effect and the Hunter-Gatherer Weltanschauung

The Martian Standpoint

Addendum on the Martian Standpoint

Hunter-Gatherers in Outer Space

What will it be like to be a Martian?

. . . . .

night-sky-0

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Our Terrestrial Heritage

27 February 2017

Monday


Étienne-Louis Boullée, Cénotaphe à Newton (1784)

Étienne-Louis Boullée, Cénotaphe à Newton (1784)

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.

. . . . .

Antonio Sant'Elia's La Città Nuova, or Frank Lloyd Wright's Broadacre City, or even Le Corbusier's Voisin plan for Paris might yet be built on other worlds.

Antonio Sant’Elia’s La Città Nuova, or Frank Lloyd Wright’s Broadacre City, or even Le Corbusier’s Voisin plan for Paris might yet be built on other worlds.

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Friday


figure-against-stars

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.

stars-0

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 surfaces

Planetary Endemism

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.

21refPicsSORT

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.

surface-earth-space

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.

starship-john-harris

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.

. . . . .

astronaut-above-earth

. . . . .

Overview Effects

The Epistemic Overview Effect

The Overview Effect as Perspective Taking

Hegel and the Overview Effect

The Overview Effect in Formal Thought

Brief Addendum on the Overview Effect in Formal Thought

A Further Addendum on the Overview Effect in Formal Thought, in the Way of Providing a Measure of Disambiguation in Regard to the Role of Temporality

Our Knowledge of the Internal World

Personal Experience and Empirical Knowledge

The Overview Effect over the longue durée

Cognitive Astrobiology and the Overview Effect

The Scientific Imperative of Human Spaceflight

Homeworld Effects

The Homeworld Effect and the Hunter-Gatherer Weltanschauung

The Martian Standpoint

Addendum on the Martian Standpoint

Hunter-Gatherers in Outer Space

What will it be like to be a Martian?

. . . . .

night-sky-0

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Folk Astrobiology

6 August 2016

Saturday


If some alien species had encountered Earth during one of its snowball periods, the planet would have resembled a biosphere with a single biome.

If some alien species had encountered Earth during one of its snowball periods, the planet would have resembled a biosphere with a single biome.

Can there be folk concepts in (and of) recent and sophisticated scientific thought, such as astrobiology? Astrobiology is a recent discipline, and as such is a beneficiary of a long history of the development of scientific disciplines; in other words, astrobiology stands on the shoulders of giants. In From an Astrobiological Point of View I characterized astrobiology as the fourth and latest of four revolutions in the life sciences, preceded by Darwinism, genetics, and evolutionary developmental biology (i.e., evo-devo). Can there be folk concepts that influence such a recent scientific discipline?

In Folk Concepts and Scientific Progress and Folk Concepts of Scientific Civilization I considered the possibility of folk concepts unique to a scientific civilization, and the folk concepts of recent sciences like astrobiology constitute paradigmatic examples of folk concepts unique to scientific civilization. The concepts of folk astrobiology, far being being rare, have proliferated as science fiction has proliferated and made a place for itself in contemporary culture, especially in film and television.

One idea of folk astrobiology that is familiar from countless science fiction films is that of planets the biosphere of which is dominated by a single biome. Both Frank Herbert’s planet Arrakis from the novel Dune and the planets Tatooine and Jakku from Star Wars are primarily desert planets, whereas the Star Wars planet Dagobah is primarily swamp, the planet Kamino is a global ocean, and the planet Hoth is primarily arctic. Two worlds that appear in the Alien films, Zeta Reticuli exomoon LV-426 in Alien and Aliens and LV-223 in Prometheus, are both desolate, rocky, and barren, like the landscapes we have come to expect from the robotic exploration of the other worlds in our own solar system.

The knowledge we have assembled of the long-term history of the biosphere of Earth, that our planet has passed through “hothouse” and “icehouse” stages, suggest it is reasonable to suppose that we will find similar conditions elsewhere in the universe, though Earth today has a wide variety of biomes that make up its biosphere. We should expect to find worlds both with diverse biospheres and with biospheres primarily constituted by a single biome. Perhaps this idea of folk astrobiology will someday be formalized, when we know more about the evolution of biospheres of multiple worlds, and we have the data to plot a bell curve of small, rocky, wet planets in the habitable zone of their star. This bell curve almost certainly exists, we just don’t know as yet where Earth falls on the curve and what kinds of worlds populate the remainder of the curve.

Biosphere diversity is thus a familiar concept of folk astrobiology. But let me backtrack a bit and try to formulate more clearly an explication of folk astrobiology.

In an earlier post I quoted the following definition of folk biology:

Folk biology is the cognitive study of how people classify and reason about the organic world. Humans everywhere classify animals and plants into species-like groups as obvious to a modern scientist as to a Maya Indian. Such groups are primary loci for thinking about biological causes and relations (Mayr 1969). Historically, they provided a transtheoretical base for scientific biology in that different theories — including evolutionary theory — have sought to account for the apparent constancy of “common species” and the organic processes centering on them. In addition, these preferred groups have “from the most remote period… been classed in groups under groups” (Darwin 1859: 431). This taxonomic array provides a natural framework for inference, and an inductive compendium of information, about organic categories and properties. It is not as conventional or arbitrary in structure and content, nor as variable across cultures, as the assembly of entities into cosmologies, materials, or social groups. From the vantage of EVOLUTIONARY PSYCHOLOGY, such natural systems are arguably routine “habits of mind,” in part a natural selection for grasping relevant and recurrent “habits of the world.”

Robert Andrew Wilson and Frank C. Keil, The MIT Encyclopedia of the Cognitive Sciences

And here is a NASA definition of astrobiology that I have previously quoted:

“Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe. This multidisciplinary field encompasses the search for habitable environments in our Solar System and habitable planets outside our Solar System, the search for evidence of prebiotic chemistry and life on Mars and other bodies in our Solar System, laboratory and field research into the origins and early evolution of life on Earth, and studies of the potential for life to adapt to challenges on Earth and in space.”

Drawing on both of these definitions — “Folk biology is the cognitive study of how people classify and reason about the organic world” and “Astrobiology is the study of the origin, evolution, distribution, and future of life in the universe” — we can formulate a fairly succinct definition of folk astrobiology:

Folk astrobiology is the cognitive study of how people classify and reason about the origin, evolution, distribution, and future of life in the universe.

I hope that the reader immediately sees how common this exercise is, both in scientific and non-scientific thought. On the scientific side, folk astrobiology is pervasively present in the background assumptions of SETI, while on the non-scientific side, as we have seen above in examples drawn from scientific fiction films, folk astrobiology informs our depiction of other worlds and their inhabitants. These concepts of folk astrobiology are underdetermined by astrobiology, but well grounded in common sense and scientific knowledge as far as it extends today. We will only be able to fully redeem these ideas for science when we have empirical data from many worlds. We will begin to accumulate this data when, in the near future, we are able to get spectroscopic readings from exoplanet atmospheres, but that is only the thin edge of the wedge. Robust data sets for the evolution of multiple independent biospheres will have to await interstellar travel. (This is one reason that I suggested that a starship would be the ultimate scientific instrument; cf. The Interstellar Imperative.)

Folk astrobiology remains “folk” until its concepts are fully formalized as part of a rigorous scientific discipline. As few disciplines ever attain complete rigor (logic and mathematics have come closest to converging on that goal), there is always a trace of folk thought that survives in, and is even propagated along with, scientific thought. Folk concepts and scientific concepts, then, are not mutually exclusive, but rather they overlap and intersect in a Wittgensteinian fashion. However, the legacy of positivism has often encouraged us to see folk concepts and scientific concepts as mutually exclusive, and if one adopts the principle that scientific concepts must be reductionist, therefore no non-reductionist concepts are not scientific, then it follows that most folk concepts are eliminated when a body of knowledge is made scientifically rigorous (I will not further develop this idea at present, but I hope to return to it when I can formulate it with greater precision).

We have a sophisticated contemporary biological science, and thus scientific biological concepts are ready to hand to employ in astrobiology, so that astrobiology has an early advantage in converging upon scientific rigor. But if a science aspires to transcend its origins and to establish itself as a new science co-equal with its progenitors, it must be prepared to go beyond familiar concepts, and in this case this means going beyond the sophisticated concepts of contemporary biology in order to establish truly astrobiological scientific concepts, i.e., uniquely astrobiological concepts, and these distinctive and novel concepts must then, in their turn, converge on scientific rigor. In the case of astrobiology, this may mean formulating a “natural history” where “nature” is construed as to include the whole of the universe, and this idea transcends the familiar idea of natural history, forcing the astrobiologist to account for cosmology as well as biology.

As an example of an uniquely astrobiology concept I above suggested the idea of biosphere diversity. Biosphere diversity, in turn, is related to ideas of biosphere evolution, developmental stages on planets with later emergent complexities, and so on. The several posts I have written to date on planetary endemism (Part I, Part II, Part III, Part IV, Part V, and more to come) may be considered expositions of the folk astrobiological idea of planetary endemism. Similarly, the homeworld concept is both a folk concept of astrobiology and scientific civilization (cf. The Homeworld Effect and the Hunter-Gatherer Weltanschauung, Hunter-Gatherers in Outer Space, and The Martian Standpoint).

. . . . .

The idea of a homeworld is a folk concept of astrobiology and scientific civilization.

The idea of a homeworld is a folk concept of astrobiology and scientific civilization.

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Saturday


planetary surfaces

During the Stelliferous Era planetary surfaces are uniquely suited for emergent complexity such as life and civilization. Planetary surfaces are by their nature complex, being the interface between planet and planetary atmosphere. Planetary surfaces are moreover a “Goldilocks” zone for energy flows during the Stelliferous Era; energy flows on stars themselves are too great for life, while energy flows in space (in the clouds of gas and dust that surround a star) are too little for life. Planetary surfaces, then, provide “just right” energy flows at the interface of atmospheric gases and the minerals constituting the planet. If emergent complexity is going to arise during the Stelliferous, it is going arise here, hence civilizations begin on planets.

That civilizations begin on planets during the Stelliferous Era has certain consequences. Civilizations originate at the bottom of a gravity well, and if they are to expand beyond a planetary surface, they must reach a level of technological sophistication adequate to lift off from its homeworld a demographically significant proportion of its population of the intelligent organism upon which the civilization supervenes. This is the first and the most significant of the horizons of spacefaring civilization, and the spacefaring horizon that provides the initial overview effect of the civilization’s homeworld.

What this means is that there is thus a natural tendency to planetary endemism among civilizations of the Stelliferous Era. In my posts on planetary constraints I outlined the limitations imposed upon a civilization the development of which is limited to the surface of a planet. These constraints include: 1. the spatial constraint, 2. the temporal constraint, 3. the gravitational constraint, 4. the agrarian constraint, 5. the population constraint, 6. the energy constraint, 7. the material constraint, 8. the ontic constraint, and 9. the endemic constraint. These constraints define the scope of the civilizations of planetary endemism.

A planetary civilization is the limit (and, some might argue, the telos) of planetary endemism. Let us define a planetary civilization as a single civilization uniquely determined by the biosphere of a single planet, which means that, for planetary civilizations, there is a one-to-one correspondence between civilizations and their homeworlds. (Here “planet” is to be understood in the broadest possible sense, including dwarf planets, moons, and so on.) In my post Origins of Globalization I argued that terrestrial civilization today is a planetary civilization (and I further commented on this in Civilization and Uniformity).

In the particular case of terrestrial civilization, a single planetary civilization has emerged from the concrescence of multiple civilizations formerly geographically isolated. Once we think of civilization in this schematic and formal way, at least some alternatives to the particular pattern of terrestrial development become obvious. For example, civilization might begin at a single geographical locus on a planet, and spread outward from there, rather than originating independently on multiple occasions. Even given these alternative pathways to planetary civilization, from the most formal perspective these are variations on a theme of planetary civilization, and the big picture distinctions we can make, and which we can expect to be exemplified in the case of other civilizations (if there are other civilizations), can be narrowed to a few classes. If we think of planetary civilization as a classification in a developmental account of civilization, other classifications naturally grow out of this idea. For example:

● Nascent Civilization What I have also called proto-civilization, are cultures on the verge of producing civilization, i.e., intelligent species at a level of social organization immediately anterior to the threshold of civilization. The Human World of the Upper Paleolithic frequently approximated nascent civilization.

● Developing Sub-planetary Civilization Before a civilization or civilizations reach their planetary limit, they may be called sub-planetary. A sub-planetary civilization still undergoing development, and retaining the capability to expanding to its planetary limit, is a developing sub-planetary civilization. As noted above, developing sub-planetary civilizations may be one or many prior to converging upon a planetary civilization.

● Arrested Sub-planetary Civilization A less-than-planetary civilization that has ceased in its development and so no longer retains the capability of expanding to its planetary limit may be called an arrested sub-planetary civilization. Arrested sub-planetary civilizations, which constitute instances of suboptimal civilization, and will eventually become extinct when planetary conditions eventually change beyond the ability of the civilization to adapt. A sub-planetary civilization is, by definition, a geographically regional civilization, so it is a civilization predicated upon the ecological conditions of a particular region of a planet, and is probably limited to inhabiting one or two biomes of its homeworld. This makes an arrested sub-planetary civilization especially vulnerable to extinction, and, in fact, many local civilizations in terrestrial history have gone extinct leaving no successor civilization (e.g., Minoan civilization, Nazca civilization, etc.).

● Developing Planetary Civilization A civilization that has reached the limits of its homeworld, and yet continues in its development, is a planetary civilization on the cusp of making the transition to becoming a spacefaring civilization. While such development might be cut short by the realization of some existential risk, there is nevertheless a distinction to be made between a planetary civilization in possession of the resources (potentially) to make the transition to spacefaring civilization, and a civilization that happens to reach the limits of its homeworld, but which has no hope of making the transition to spacefaring civilization.

● Arrested Planetary Civilization Arrested planetary civilizations, like arrested sub-planetary civilizations, are also a species of suboptimal civilization, and are also subject to inevitable extinction. However, arrested planetary civilizations are somewhat less vulnerable and more robust than arrested sub-planetary civilizations, since the ability to establish a planetary civilization means that transportation and communication networks unify the homeworld and the civilization in possession of such an infrastructure can compensate for regional ecological changes that could mean the end for a geographically regional civilization. Thus, in general, it is to be expected that arrested planetary civilizations can endure for a longer period of time than arrested sub-planetary civilizations, though a planetary civilization is, in turn, likely to endure for a shorter period of time than a spacefaring civilization, which latter possesses access to far greater resources and can achieve redundancy on a scale than no planetary civilization can achieve.

It is interesting to observe that a sub-planetary civilization might seek existential risk mitigation through redundancy by “seeding” copies of itself in different regions of its homeworld. How would we distinguish between such a project and more familiar categories of civilizational expansion or colonization? I will not attempt to answer this question at present. However, I will make the further observation that this approach to redundancy is closed off to any planetary civilization, whether arrested or still in the process of development.

Several of the terms I have employed here are admittedly rather awkward; my point is to try to capture the most general, “big picture” features of a civilization as we might observe its development from outside. For if SETI, in any of its forms, is eventually successful, we will be scientists of civilization looking from the outside in, and if there are many civilizations to be discovered, they will be roughly sortable into a handful of varieties. The varieties of civilization outlined above are based on the root idea of a planetary civilization, which is in turn based on the idea of the planetary endemism of civilizations, which is likely to be a feature of the Stellierous Era.

The argument implied in the above classification is that this classification possesses a certain conceptual naturalness as a consequence of its being rooted in structural features of the universe in which we happen to find ourselves. A different universe, or a different kind of universe, or a universe with a different natural history, might demand a scheme for the classification of any civilizations it hosted which differed from the above, which is an artifact of particular conditions. Thus if we depart sufficiently from the Stellierous Era, a different taxonomy for the classification of civilization may be necessary. For example, in the case of Degenerate Era civilizations, which would probably consist of civilizations descended with modification from civilizations of the Stellierous Era, the above scheme of classification would not likely be very helpful.

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .

Wednesday


Saturn with astronaut

Our first view of Earth was from its surface; every other planet human beings eventually visit will be first perceived by a human being at a great distance, then from orbit, and last of all from its surface. We will descend from orbit to visit a new world, rather than, as on Earth, emerging from the surface of that world and, only later, much later, seeing it from orbit, and then as a pale blue dot, from a great distance.

With our homeworld, the effect of looking up from the surface of our planet precedes the overview effect; with every other world, the overview effect precedes the surface standpoint. We might call this the homeworld effect, which is a consequence of what I now call planetary endemism (and which, when I was first exploring the concept, I called planetary constraint). We have already initiated this process when human beings visited the moon, and for the first time in human history descended to a new world, never before visited by human beings. With this first tentative experience of spacefaring, humanity knows one world from its surface (Earth) and one world from above (the moon). Every subsequent planetary visit will increase the relative proportion of the overview effect in contradistinction to the homeworld effect.

In the fullness of time, our normative assumptions about originating on a plant and leaving it by ascending in to orbit will be displaced by a “new normal” of approaching worlds from a great distance, worlds perhaps first perceived as a pale blue dot, and then only later descending to familiarize ourselves with surface features. If we endure for a period of time sufficient for further human evolution under the selection pressure of spacefaring civilization, this new normal will eventually replace the instincts formed in the environment of evolutionary adaptedness (EEA) when humanity as a species branched off from other primates. The EEA of our successor species will be spacefaring civilization and the many worlds to which we travel, and this experience will shape our minds as well, producing an evolutionary psychology adapted not to survival on the surface of a planet, but to survival on any planet whatever, or no planet at all.

The Copernican principle is the first hint we have of the mind of a species adapted to spacefaring. It is a characteristic of Copernicanism to call the perspective borne of planetary endemism, the homeworld effect, into question. We have learned that the Copernican principle continually unfolds, always offering more comprehensive perspectives that place humanity and our world in a context that subsumes our previous perspective. Similarly, the overview effect will unfold over the development of spacefaring civilization that takes human beings progressively farther into space, providing ever more distant overviews of our world, until that world becomes lost among countless other worlds.

In my Centauri Dreams post The Scientific Imperative of Human Spaceflight, I discussed the possibility of further overview effects resulting from attaining ever more distant perspectives on our cosmic home — thus attaining an ever more rigorous Copernican perspective. For example, although it is far beyond contemporary technology, it is possible to imagine we might someday have the ability to go so far outside the Milky Way that we could see our own galaxy in overview, and point out the location of the sun in the Orion Spur of the Milky Way.

There is, however, another sense in which additional overview effects may manifest themselves in human experience, and this would be due less to greater technical abilities that would allow for further first person human perspectives on our homeworld and on our universe, and rather due more to cumulative human experience in space as a spacefaring civilization. With accumulated experience comes “know how,” expertise, practical skill, and intuitive mastery — perhaps what might be thought of as the physical equivalent of acculturation.

We achieve this physical acculturation to the world through our bodies, and we express it through a steadily improving facility in accomplishing practical tasks. One such practical task is the ability to estimate sizes, distances, and movements of other bodies in relation to our own body. An astronaut floating in space in orbit around a planet or a moon (i.e., on a spacewalk) would naturally (i.e., intuitively) compare himself as a body floating in space with the planet or moon, also a body floating in space. Frank White has pointed out to me that, in interviews with astronauts, the astronauts themselves have noted the difference between being inside a spacecraft and being outside on a spacewalk, when one is essentially a satellite of Earth, on a par with other satellites.

The human body is an imperfectly uniform, imperfectly “standard” standard ruler that we use to judge the comparative sizes of the objects around us. Despite its imperfection as a measuring instrument, the human body has the advantage of being more intimately familiar to us than any other measuring device, which makes it possible to achieve a visceral understanding of quantities measured in comparison to our own body. At first perceptions of comparative sizes of bodies in space would be highly inaccurate and subject to optical illusions and cognitive biases, but with time and accumulated experience an astronaut would develop a more-or-less accurate “feel” for the size of the planetary body about which he is orbiting. With accumulated experience one would gain an ability to judge distance in space by eye, estimate how rapidly one was orbiting the celestial body in question, and perhaps even familiarize oneself with minute differences in microgravity environments, perceptible only on an intuitive level below the threshold of explicit consciousness — like the reflexes one acquires in learning how to ride a bicycle.

This idea came to me recently as I was reading a NASA article about Saturn, Saturn the Mighty, and I was struck by the opening sentences:

“It is easy to forget just how large Saturn is, at around 10 times the diameter of Earth. And with a diameter of about 72,400 miles (116,500 kilometers), the planet simply dwarfs its retinue of moons.”

How large is Saturn? We can approach the question scientifically and familiarize ourselves with the facts of matter, expressed quantitatively, and we learn that Saturn has an equatorial radius of 60,268 ± 4 km (or 9.4492 Earths), a polar radius of 54,364 ± 10 km (or 8.5521 Earths), a flattening of 0.09796 ± 0.00018, a surface area of 4.27 × 1010 km2 (or 83.703 Earths), a volume of 8.2713 × 1014 km3 (or 763.59 Earths), and a mass of 5.6836 × 1026 kg (or 95.159 Earths) — all figures that I have taken from the Wikipedia entry on Saturn. We could follow up on this scientific knowledge by refining our measurements and by going more deeply in to planetary science, and this gives us a certain kind of knowledge of how large Saturn is.

Notice that the figures I have taken from Wikipedia for the size of Saturn notes Earth equivalents where relevant: this points to another way of “knowing” how large Saturn is: by way of comparative concepts, in contradistinction to quantitative concepts. When I read the sentence quoted above about Saturn I instantly imagined an astronaut floating above Saturn who had also floated above the Earth, feeling on a visceral level the enormous size of the planet below. In the same way, an astronaut floating above the moon or Mars would feel the smallness of both in comparison to Earth. This is significant because the comparative judgement is exactly what a photograph does not communicate. A picture of the Earth as “blue marble” may be presented to us in the same size format as a picture of Mars or Saturn, but the immediate experience of seeing these planets from orbit would be perceived very differently by an orbiting astronaut because the human body always has itself to compare to its ambient environment.

This is kind of experience could only come about once a spacefaring civilization had developed to the point that individuals could acquire diverse experiences of sufficient duration to build up a background knowledge that is distinct from the initial “Aha!” moment of first experiencing a new perspective, so one might think of the example I have given above as a “long term” overview effect, in contradistinction to the immediate impact of the overview effect for those who see Earth from orbit for the first time.

The overview effect over the longue durée, then, will continually transform our perceptions both by progressively greater overviews resulting from greater distances, and by cumulative experience as a spacefaring species that becomes accustomed to viewing worlds from an overview, and immediately grasps the salient features of worlds seen first from without and from above. In transforming our perceptions, our minds will also be transformed, and new forms of consciousness will become possible. This alone ought to be reason enough to justify human spaceflight.

The possibility of new forms of consciousness unprecedented in the history of terrestrial life poses an interesting question: suppose a species — for the sake of simplicity, let us say that this species is us, i.e., humanity — achieves forms of consciousness through the overview effect cultivated in the way I have described here, and that these forms of consciousness are unattainable prior to the broad and deep experience of the overview effect that would characterize a spacefaring civilization. Suppose also, for the sake of the argument, that the species that attains these forms of consciousness is sufficiently biologically continuous that there has been no speciation in the biological sense. There would be a gulf between earlier and later iterations of the same species, but could we call this gulf speciation? Another way to pose this question is to ask whether there can be cognitive speciation. Can a species at least partly defined in terms of its cognitive functions be said to speciate on a cognitive level, even when no strictly biological speciation has taken place?

I will not attempt to answer this question at present — I consider the question entirely open — but I would like to suggest that the idea of cognitive speciation, i.e., a form of speciation unique to conscious beings, is deserving of further inquiry, and should be of special interest to the field of cognitive astrobiology.

. . . . .

The Overview Effect

The Epistemic Overview Effect

Hegel and the Overview Effect

The Overview Effect and Perspective Taking

The Overview Effect in Formal Thought

Our Knowledge of the Internal World

The Human Overview

Personal Experience and Empirical Knowledge

Cognitive Astrobiology and the Overview Effect

The Scientific Imperative of Human Spaceflight

Brief Addendum on the Overview Effect in Formal Thought

A Further Addendum on the Overview Effect in Formal Thought, in the Way of Providing a Measure of Disambiguation in Regard to the Role of Temporality

The Overview Effect over the longue durée

Civilizations of Planetary Endemism

. . . . .

deep field astronaut 3

. . . . .

signature

. . . . .

Grand Strategy Annex

. . . . .

project astrolabe logo smaller

. . . . .