19
For each chapter, a brief summary of its subject matter is provided. Also shown are the key scientific disciplines covered by the chapters, where A is astronomy/astrophysics, B is biological sciences, C is chemistry, G is geosciences, and H denotes chapters that contain material that intersects with humanities/social sciences.
A great deal of this book is unapologetically focused on a basic understanding of biology. Indeed, even if alien life is your focus, you still need to know about the one type of life we currently know – life on Earth – before you can embark on any discussion about the conditions and possibilities for life elsewhere.
The textbook therefore begins with a study of life on Earth (Figure 1.4). There is another reason for starting with biology. If we want to investigate how the elements required for life were produced during and after the Big Bang or why a habitable environment needs certain characteristics, or why certain molecules and environments might have been needed for life to emerge, we need to know about biology first. We need to understand its structure, its requirements, and what conditions it can subsist under in order to question how those characteristics were made possible. In that sense, the first part of this book looks very much like standard biology textbook material and, at its core, it is. However, I have written it specifically to provide you with the necessary understanding of biology to enable you to think about the major questions of astrobiology. Throughout these chapters, I address some of the topics in biology that relate to questions about the conditions and possibilities for life elsewhere. These chapters are biology with an astrobiology flavor.
Figure 1.4 The one example we have of a planet that harbors life: Earth. Astrobiology seeks to understand how the phenomenon of life came about and whether it is unique in the Universe. Here, Earth rises over the lunar landscape in this iconic image taken by Apollo 8 in 1968. The image is sometimes called “Earthrise”.
Source: Reproduced with permission of NASA.
We start this tour of life by looking at the fundamental properties of matter and how those properties underpin the structure of the molecules of life. We then consider how these molecules are assembled into the major components of living cells. With a knowledge of the structure of life, we can then move on to think about how these cells can get the energy they need to grow and reproduce, all the time being mindful of those factors that might be specific to terrestrial life or from which we could learn something about life anywhere.
Once life did become established on Earth, what were its limits? We will investigate the physical and chemical boundaries of life that might define how diverse or extensive this life can become in extreme environments at the limits of planetary habitability. If we can find out what the physical and chemical extremes of life are, i.e. the most extreme conditions it can tolerate, we can begin to assess the habitability of other planetary bodies as locations for life. This knowledge even helps us to assess what the impact of human activity and industry might be on the biosphere. Questions that fascinate astrobiologists in this area of research include: What are the limits of life? How does life survive at physical and chemical extremes? Are these limits universal? What do these limits tell us about habitable conditions or the possible presence of life elsewhere? These probing lines of thought drive us to study life in unusual environments, from the deep oceans to the freezing wastes of Antarctica.
Supported by our knowledge of living things, we then explore how all life on Earth is related or linked into a “tree of life.” Buried within this tree of life are profound questions. The diversity of life on Earth is extraordinary. But what unites organisms and what is the relationship between them? How has this diversity changed over time? (Figure 1.5). Astrobiologists want to gain a better understanding of the evolutionary links between diverse organisms. We take an introductory look at the tree of life and see how biologists can construct phylogenetic trees to make sense of all the diversity of life on the planet, and to address certain scientific hypotheses.
Figure 1.5 A schematic of the history of Earth. Understanding this history and the co-evolution of life and the planet constitutes a key objective in astrobiology.
Source: Reproduced with permission of William Crochot.
At this point, we will be equipped with a solid understanding of the structure, interrelationships, and capabilities of the life that we know on Earth. It is time to put this into a more cosmic context.
In the next part of the textbook, we rewind and return to the beginning of the Universe and investigate how stars and planets formed. This distinctly astronomical turn of events in the book is a good way to address the question: How did the elements required for life (which we identified in the first part of the textbook) form, and where did they form? In particular, we examine the conditions for the formation of carbon compounds in the Universe, since carbon-containing compounds are the most important class of compounds for life.
I should stress that one could tackle astrobiology in the opposite direction. We could start at the beginning of the Universe and work our way through to the emergence of life. Chronologically, this does make sense. However, to know which elements that were formed in the early Universe are relevant for life, it's important to know something about biology in the first place, which is why I have started the textbook with biology. However, I have attempted to write each chapter as a stand-alone text. If you want to select chapters and work through them in a different order, such as from the beginning of the Universe in a more astronomically focused class, you can do that.
Once we have investigated the history of the Universe, the formation of the elements of life and the important role of carbon, the textbook then returns to Earth to examine the emergence of life on this habitable planet. We investigate the environmental characteristics of our planet during its first billion years to understand what sort of environments and habitats could have existed on Earth at that time.
The question of how life might have originated in this early environment is our next task. We consider the chemical reactions and environments in which life could have originated and discuss some of the ideas for the reactions that allowed simple precursor molecules to come together to make the macromolecules of biology – how chemical reactions led to the formation of the first self-replicating cell. This leads to questions such as: How did life originate? Where did life originate? Was it inevitable? When did it happen? All of these questions encompass the question of the origin of life on Earth and might tell us something about whether an origin of life could happen somewhere else.
We follow this up by considering the evidence of early life on Earth. We consider some of the complexities and controversies associated with the evidence
