Charles S. Cockell

Astrobiology


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information shown in boxes. Some of the boxes present points of debate in astrobiology that are worth discussing with others or contemplating yourself. These “Discussion Points” are an opportunity to get you to think about ideas in different fields that link to astrobiological questions. I have also written them in places where the material might seem very conventional. I hope they will stimulate you to think about the material being described in new ways. For example, is the biochemical structure of life on Earth something universal or a very particular outcome of Earth's experiment in biological evolution? Such a question should encourage you to think about what the basics of biology might, or might not, tell us about life elsewhere, if it exists. I have attempted to provide some similar thoughts and questions in all the chapters. The content and questions in these boxes are by no means exhaustive, and you should use them to encourage other discussions or come up with new questions. In particular, try to think about questions that bridge different chapters and the different fields in the book.

      Here and there I have included some textboxes about some of the major facilities that astrobiologists use. There are a vast number of techniques that astrobiologists employ in the laboratory, but some large facilities, coordinated internationally, such as space telescopes, expand the reach of the science significantly. They also give you a flavor of the modern nature of international science.

      I have included some further reading. This was, perhaps, the most difficult task. It is impossible to do justice to all the literature that exists in every field that comprises astrobiology, let alone list all the main contributions. Instead, I've suggested two or three popular and/or technical books that relate to each chapter that might provide some enjoyable additional reading. I have also listed a set of papers. They are papers I think will give a representative sprinkling of just some of the possible avenues an interested reader might pursue and that relate to the main themes and subjects covered in each chapter. Again, no significance should be placed on the omission of many important papers or the inclusion of the ones listed.

      There is yet another dimension of astrobiology that I have touched on in this book. I often get asked by students, “What degree do I need for astrobiology? What field should I take an interest in to become an astrobiologist?” Any degree allows a person to explore aspects of astrobiology from different angles. Science should never be closed to inquisitive minds on account of narrow human discipline definitions. Throughout the book, I've included sections that contain some personal information about a selection of astrobiologists, particularly colleagues early in their careers. I've shown their original degree areas, what motivates them, and how they got into astrobiology. Their career interests are not necessarily directly aligned to the subject of the chapter in which they appear, but their stories are distributed throughout the book. There are many fine people in astrobiology, and I'd like to emphasize that there is no significance to my selection or omission of these astrobiologists. I chose a selection of outstanding colleagues whom I thought would exemplify the variety of disciplines from which astrobiologists are currently launching their careers.

      Having explored the main questions in astrobiology and summarized them, we might ask ourselves when all this scientific interest began. Sometimes a historical perspective on any science can be useful to understand how we got here and why certain questions have become prominent lines of enquiry. A thorough review of the history of space sciences and where astrobiology fits within it could (and indeed does) consume entire books. This textbook is more about the science than the history of astrobiology, but at this point it is worth making some observations about its historical origins to provide some introductory context.

Portrait of Metrodorus of Chios.

       Figure 1.8 Metrodorus of Chios, ancient Greek philosopher. He wondered about the existence of other worlds like our own.

      Source: Reproduced with permission of Keith Schengili-Roberts, https://commons.wikimedia.org/wiki/File:Metrodorus-PergamonMuseum.png.

      Metrodorus's view of the world was very different from Aristotle's (384–322 BCE), who asserted the uniqueness of Earth in the cosmos. The idea that Earth was the center of the Universe was based on the observation that the stars never moved with respect to one another, which the ancients interpreted to be a result of the fixed position of Earth rather than the great distances to the stars. Aristotle's view would dominate for many centuries. Until the Enlightenment (during the seventeenth and eighteen centuries), the idea that Earth was the sole inhabited world in the cosmos held its grip on the public view, bolstered by religious doctrine.

      In the sixteenth century, the geocentric view of the Universe, which firmly placed Earth as the center of the action, was overturned by Nicolaus Copernicus (1473–1543) (Figure 1.9). He was not the first person to consider that the Sun was at the center of the Solar System and Earth orbited around it. Greek philosopher Aristarchus proposed a heliocentric model, but Copernicus's treatise, De revolutionibus orbium coelestium (On the Revolutions of the Heavenly Spheres), caused a landmark shift away from the geocentric view. The Copernican outlook paved the way for a view of the cosmos that would allow for the idea that stars may be other suns.

Portrait of Nicolaus Copernicus.

       Figure 1.9 Nicolaus Copernicus, renaissance mathematician and astronomer. He advanced a heliocentric model of the Solar System.

      Source: Reproduced from the “Torun portrait,” anonymous, c. 1580.

      In the sixteenth century, more enquiring and inquisitive minds appeared and, with them, new speculations about Earth's place in the larger order of things. One of the most astonishing speculations about worlds beyond Earth was made by the Italian Dominican friar, mathematician, and philosopher Giordano Bruno (1548–1600; Figure 1.10), who stated in his book On the Infinite Universe and Worlds: “In space there are countless constellations, suns and planets; we see only the suns because they give light; the planets remain invisible, for they are small and dark. There are also numberless earths circling around their suns, no worse and no less than this globe of ours. For no reasonable mind can assume that heavenly bodies that may be far more