Planet Formation and Panspermia. Группа авторов

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Название Planet Formation and Panspermia
Автор произведения Группа авторов
Жанр Физика
Серия
Издательство Физика
Год выпуска 0
isbn 9781119640936



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and living systems, and that under suitable physical conditions the emergence of life is highly probable [given enough time]. It is the adoption of the “continuity thesis”, concerning the philosophical dimension of life-matter relationship, which has turned the origin of life into a legitimate scientific question, and which constitutes a necessary condition for any scientific research in this domain.

      In [3.13], I have elaborated the case for extending the continuity thesis to the origin of intelligence (or noogenesis) and other major evolutionary transitions, or “crucial steps” in overall cosmic evolution. In particular, I suggest an extended continuity thesis, which brings the reasoning of Fry to its logical conclusion, namely, that there are no unbridgeable gaps between simple life and a complex one and between complex life and an intelligent one (possibly also between biological intelligent life and a postbiological intelligent one). Whenever and wherever physical, chemical, geophysical, ecological, etc., conditions are suitable, the emergence of complex life is highly probable—and ditto for intelligent life. This is not particularly new either. John B. S. Haldane, among others, suggested that cultural evolution is an extension of biological evolution (e.g., [3.34]). Of course, he was aware of the seeming disparity of the relevant timescales; the solution is to “zoom-out” sufficiently and seek macro-trends. Hence, the Haldanian insistence on observing evolutionary phenomena “in the fullness of time”, which is followed here (cf. [3.1]). An alternative approach is to encompass all timescales into what has been called “Big History” (e.g., [3.38]).

      That said, the rest of this chapter is organized as follows. Section 3.2 discusses versions of the continuity thesis and briefly speculates on the sources of resistance it encounters in various contexts which need not be necessarily be connected with astrobiology. The concept of chronocentrism is highlighted, representing a key underlying source of confusion, bias, and short-sightedness in considering the entire astrobiological landscape. A particular interesting consequence of an extended continuity thesis, related to the concept of directed panspermia, is considered in Section 3.3. Some ramifications for both astrobiology and SETI studies, as well as the futures studies, are outlined in the concluding section.

      The suggested extension of the continuity thesis just extends the very same reasoning to noogenesis and subsequent cultural evolution (or gene-culture coevolution; see, e.g., [3.59]). There is nothing spectacularly different here—again, one might reason that noogenesis was a “lucky accident” or a rather regular occurrence whenever all physical, chemical, and biological preconditions exist. It does not matter for the continuity thesis itself and its role as a heuristic that we do not know and do not understand all these preconditions at present. As we gain better insight into those, we will update our understanding and our credence in hypotheses derived from the continuity thesis. It is quite similar to Copernicanism—it was in the beginning a purely philosophical assumption, which gradually obtained support as we gained knowledge about the stellar, galactic, and, in recent years, planetary populations of our universe. Our improved astronomical insights have corroborated the Copernican thesis (with full understanding that it can never be strictly proved). Needless to say, the extended continuity thesis has been implicitly accepted in most SETI studies to date, since any expectation of detecting a radio signal or any other technosignature is based upon the assumption that noogenesis both occurs in naturalistic manner and with a reasonable, non-infinitesimal probability. (In fact, the traditional SETI uses even stronger assumptions, dealing with convergence in cultural evolution; cf. [3.45, 3.65].)