Excerpt from the preliminary Preface of the Second Edition
Since
the publication of The New Science of Astrobiology (Chela-Flores,
2001), early in the year 2001, two significant events have taken place
raising the subject from the beginning of the century to its present
maturity a decade later. Firstly, at that time the Galileo Mission
still had two years to complete its task, which turned out to be an
outstanding survey of the Jovian system, especially of its intriguing
satellite Europa. Secondly, the successful outcome of the Cassini
Huygens Mission on its way to Saturn went beyond all expectations of
the European Space Agency (ESA) and the United States of America
National Aeronautics and Space Administration (NASA). Cassini had been
launched four years earlier and Huygens was to land on Titan three
years after the publication of our first edition.
Besides, we had no idea that another satellite of Saturn,
Enceladus, was going to lure the scientific community with the most
surprising jets of water exuding an air of mystery, hinting at a
submerged inhabitable ocean of salty water. Ahead of the date of
publication of our book was the awareness of the Earth-like surface
morphology and hydrosphere of Titan with its prominent lake system. It
dawned upon us that Titan was the fourth body of the Solar System that
possibly contained a water ocean, thus joining our planet and Jupiter's
three Galilean satellites: Ganymede, Callisto and Europa. Titan appears
now to be the only planetary body besides the Earth to have persistent,
almost permanent liquid bodies on its surface. These surprising aspects
of Titan were unknown to us in 2001. In our first edition, at the end
of Chapter 9, we anticipated the possibility of the emergence of an
autochthonous biology on Titan, but left our readers with a word of
caution to wait until the present post Cassini-Huygens era before
advancing further hypotheses on this most basic issue of astrobiology.
We now discuss this issue in Chapter 9. The new scientific landmarks of
the first decade of the present century warrant a new look at the same
subject matter. The urgency of this undertaking is emphasized by the
much deeper insights that we have gained into the geophysics of Mars.
Some remarkable events include the analysis of its surface by the Mars
Reconnaissance Orbiter and the Martian water ice exposed by the Phoenix
Mars Lander in 2008, not forgetting the much clearer views that are now
emerging on Martian paleolimnology. Some of this progress due largely
to the stunning images retrieved by ESA's Mars Express and subsequent
missions to the Red Planet.
We have sadly witnessed during the three decades preceding the
publication of the first edition of this book, The New Science of
Astrobiology, a most unfortunate missed opportunity regarding the
acquisition of further insights into our own satellite. In the present
Second Edition this particular topic is being reviewed, namely the
ongoing revolution of interest in the Moon. In October 2007, Japan sent
up the Kaguya spacecraft. A month later, China's Chang'e-1 entered
lunar orbit. This was followed by India's Chandrayaan-1, whose
objective was to map not only the surface of the moon, but also what
lies underneath. We are convinced that promising new instrumentation,
such as the penetrator technology, especially the work of the British
Penetrator Consortium, will be able to demonstrate in the coming decade
communication and navigation technologies that will support the
eventual return to the Moon and the exploration of other planets and
satellites of the inner and outer Solar System.
Beyond the terrestrial planets this renewed interest in our own
satellite will be useful as a platform to improve on the achievements
of the Galileo Mission. The benefits will concern all the satellites of
Jupiter, especially Europa's intriguing non-water elements on its icy
surface that will be elucidated by the forthcoming Europa-Jupiter
System Mission (EJSM). With combined efforts focused on our own
satellite by India, China, Japan, Russia, the United Kingdom, ESA and
NASA, The Science of Astrobiology has new exciting results and
discoveries to review. Consequently, at the present time it is
appropriate to attempt to reflect on current scientific progress with a
broad canvas ranging from cosmic evolution to the implications in the
humanities of the inevitable discovery of universality of biology.
There is still the challenge of taking into account the search
for exo-intelligence—intelligent behavior elsewhere in the
universe—with the help of the gigantic leaps in radio astronomy that
are expected to come early in the 2020s from the Square Kilometer Array
(SKA discussed in Chapter 11). Since the year 2001, only six years
after the seminal discovery of a planet of the star 51 Pegasi that was
reported in our first edition, a whole spectrum of further "exoplanets"
have arisen amongst our galactic neighbors: Jovian-like gaseous giants,
super Neptunes and super-Earths are constantly being added to the
astronomer's catalogs. With the Kepler Space Telescope, a NASA Mission
launched in 2009, Earth-like planets are now within reach of
observation. Not only a large number of exoplanets are now known, but
also solar systems with several planets each have been identified. The
possibility of searching for exomoons will also be raised in Chapter
10. This new broad vision of the cosmos and its possible habitability
has given additional strong support to the search for intelligent
behavior with the tools of the bioastronomers. One of the factors of
the Drake Equation—the number of possible inhabitable planets—is
slowly, but steadily coming to our attention, especially with Kepler.
The many books that are now available represent another
significant progress in astrobiology. In 2001 we found it difficult to
identify a single-author book especially written on astrobiology. They
were not generally known (not even to the present author). Now the
situation is much better and our bibliography at the end of this volume
is consequently much richer, providing our readers with a most
enjoyable, instructive and comprehensive view of our subject (cf., the
bibliographic references listed at the end of the Preface offer the
reader a small sample of a growing list of books).
The writing this second edition of the book coincided in its
first stages with the double anniversary of Charles Darwin, the 200th
anniversary of his birth and the 150th anniversary of the publication
of The Origin of Species, possibly the most influential book ever
published in any branch of science. We have profited from this
remarkable coincidence, in order to underline “the biology” of
astrobiology (cf., Introduction). Being a multidisciplinary subject,
astrobiology sometimes regretfully neglects the life sciences, as there
are so many other aspects to keep in mind, such as chemical evolution,
the earth sciences, the physical sciences and cutting-edge technology.
Finally, the emphasis we attempted to imprint on our previous
book The New Science of Astrobiology made a very modest effort in
setting the scientific subject appropriately amongst other sectors of
culture that are the natural frontiers of astrobiology. These
boundaries are philosophy and theology, branches of the humanities
asking similar questions to the basic issues of astrobiology (origin,
evolution, distribution and destiny of life in the universe). In the
meantime I have dedicated a full volume to this aspect of astrobiology
in A Second Genesis Stepping-Stones Towards the Intelligibility of
Nature (Chela-Flores, 2009). We have tried in this new edition of The
Science of Astrobiology to benefit from the experience gained during
these last decade while enjoying the multiple fascinating aspects of
astrobiology and its cultural frontiers. Julian Chela-Flores,
Trieste, Italy,
February 15, 2011
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