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Books > Science & Mathematics > Astronomy, space & time > General
"Why is it dark at night?" might seem a fatuous question at first
sight. In reality it is an extremely productive question that has
been asked from the very beginning of the modern age, not only by
astronomers, for whom it is most appropriate, but also by
physicists, philosophers, and even poets. The book you have just
opened uses this question as a pretext to relate in the most
interesting way the history of human thought from the earliest
times to the here and now. The point is that if we want to
appreciate the magic power of this ostensibly naive question we
need to discover how it fits into the wider context of the natural
sciences and learn something of the faltering steps towards an
answer. In doing so the author guides us through periods that we
regard as the dim and distant past. However, as we start reading
these passages we are amazed to discover just how searching were
the questions the ancient philosophers asked themselves in spite of
their fragmentary knowledge of the universe, and how clairvoyantly
they were able to gaze into its mysterious structure. The author
goes on to explain very graphically how this increasingly prickly
question was tackled by many great men of science. It is bound to
come as a surprise that it was not a philosopher, a physicist or an
astronomer, but instead the poet Edgar Alan Poe, who hinted at the
right answer. I know of no other similar publication that has dealt
so graphically or so succinctly with a question which, after four
centuries of fumbling and chasing up blind alleys, was only solved
in our lifetime. Ji i Grygar, president of Czech Learned Society,
honorary Chairman of the Czech Astronomical Society
This well-documented and fascinating book tells how, over the
centuries, a series of visionaries, scientists, technologists, and
politicians fostered the involvement of Italy in space exploration.
The lives of these pioneers was often far from easy, yet they
persevered. The fruits of their efforts can today be witnessed in
Italy's success within the cutting-edge space sector. Italy's
history in space started at the end of the fourteenth century and
continued with the development of fireworks. Later, the nineteenth
century marked the beginning of research into rockets in a more
scientific way. After World War II, rocket technology was advanced
with the aid of German scientists, and in the 1960s Luigi Broglio,
the father of Italian space exploration, designed the San Marco
satellite. In 1979 the first Italian Space Plan was launched, but
it was the foundation of the Italian Space Agency in 1988 that
kick-started a program of exploration in various fields of cosmic
research. The outcome was construction of the Vega launcher and
collaboration in the International Space Station. Now the Italian
space industry stands ready to play an important role in the
Gateway orbital station. All of this history, and more, is explored
in this riveting book.
Offers an accessible text and reference (a cosmic-ray manual) for
graduate students entering the field and high-energy
astrophysicists will find this an accessible cosmic-ray manual Easy
to read for the general astronomer, the first part describes the
standard model of cosmic rays based on our understanding of modern
particle physics. Presents the acceleration scenario in some detail
in supernovae explosions as well as in the passage of cosmic rays
through the Galaxy. Compares experimental data in the atmosphere as
well as underground are compared with theoretical models
This book describes the development and design of a unique combined
data and power management infrastructure for small satellites. This
new edition became necessary because in the frame of the system's
impressive evolution from an academic prototype to one of today's
most advanced core avionics, many elements were upgraded to their
next technology generation and diverse new components complement
the upgraded design. All elements are presented in updated
respectively new chapters. This modular infrastructure was selected
by the Swiss start-up ClearSpace SA for ESA's first mission
ClearSpace-1 to remove space debris. Furthermore it is the baseline
for the Thai national satellite development program and is used by
an increasing number of universities worldwide for research
studies.
Written by a leading expert on comets, this textbook is divided
into seven main elements with a view to allowing advanced students
to appreciate the interconnections between the different elements.
The author opens with a brief introductory segment on the
motivation for studying comets and the overall scope of the book.
The first chapter describes fundamental aspects most usually
addressed by ground-based observation. The author then looks at the
basic physical phenomena in four separate chapters addressing the
nucleus, the emitted gas, the emitted dust, and the solar wind
interaction. Each chapter introduces the basic physics and
chemistry but then new specific measurements by Rosetta instruments
at comet Churyumov-Gerasimenko are brought in. A concerted effort
has been made to distinguish between established fact and
conjecture. Deviations and inconsistencies are brought out and
their significance explained. Links to previous observations of
comets Tempel 1, Wild 2, Hartley 2, Halley and others are made. The
author then closes with three smaller chapters on related objects,
the loss of comets, and prospects for future exploration. This
textbook includes over 275 graphics and figures - most of which are
original. Thorough explanations and derivations are included
throughout the chapters. The text is therefore designed to support
MSc. students and new PhD students in the field wanting to gain a
solid overview of the state-of-the-art.
The development of nuclear weapons during the Manhattan Project is
one of the most significant scientific events of the twentieth
century. This revised and updated 4th edition explores the
challenges that faced the scientists and engineers of the Manhattan
Project. It gives a clear introduction to fission weapons at the
level of an upper-year undergraduate physics student by examining
the details of nuclear reactions, their energy release, analytic
and numerical models of the fission process, how critical masses
can be estimated, how fissile materials are produced, and what
factors complicate bomb design. An extensive list of references and
a number of exercises for self-study are included. Revisions to
this fourth edition include many upgrades and new sections.
Improvements are made to, among other things, the analysis of the
physics of the fission barrier, the time-dependent simulation of
the explosion of a nuclear weapon, and the discussion of tamped
bomb cores. New sections cover, for example, composite bomb cores,
approximate methods for various of the calculations presented, and
the physics of the polonium-beryllium "neutron initiators" used to
trigger the bombs. The author delivers in this book an
unparalleled, clear and comprehensive treatment of the physics
behind the Manhattan project.
High-resolution X-ray spectroscopy has become a powerful tool for
astrophysics since the launch of Chandra and XMM-Newton, ten years
ago. The grating spectrometers on both instruments still continue
to provide excellent data, while imaging calorimeters are being
prepared for future missions like Astro-H and IXO. The synergy with
other wavelength bands like the UV has been boosted by the addition
of COS to HST. X-ray spectroscopy offers unique diagnostics to
study almost any object in the Universe. This book contains review
papers on highlights and the state-of-the-art of X-ray spectroscopy
for a broad range of objects and on the prospects for future
studies.
With illustrations and photographsp in full color.
This book reports on the extraordinary observation of TeV gamma
rays from the Crab Pulsar, the most energetic light ever detected
from this type of object. It presents detailed information on the
painstaking analysis of the unprecedentedly large dataset from the
MAGIC telescopes, and comprehensively discusses the implications of
pulsed TeV gamma rays for state-of-the-art pulsar emission models.
Using these results, the book subsequently explores new testing
methodologies for Lorentz Invariance Violation, in terms of a
wavelength-dependent speed of light. The book also covers an
updated search for Very-High-Energy (VHE), >100 GeV, emissions
from millisecond pulsars using the Large Area Telescope on board
the Fermi satellite, as well as a study on the promising Pulsar
Wind Nebula candidate PSR J0631. The observation of VHE gamma rays
is essential to studying the non-thermal sources of radiation in
our Universe. Rotating neutron stars, also known as pulsars, are an
extreme source class known to emit VHE gamma rays. However, to date
only two pulsars have been detected with emissions above 100 GeV,
and our understanding of their emission mechanism is still lacking.
In an expanding world with limited resources, optimization and
uncertainty quantification have become a necessity when handling
complex systems and processes. This book provides the foundational
material necessary for those who wish to embark on advanced
research at the limits of computability, collecting together
lecture material from leading experts across the topics of
optimization, uncertainty quantification and aerospace engineering.
The aerospace sector in particular has stringent performance
requirements on highly complex systems, for which solutions are
expected to be optimal and reliable at the same time. The text
covers a wide range of techniques and methods, from polynomial
chaos expansions for uncertainty quantification to Bayesian and
Imprecise Probability theories, and from Markov chains to surrogate
models based on Gaussian processes. The book will serve as a
valuable tool for practitioners, researchers and PhD students.
Until now, important research on the historical records of comets
and meteor showers from China, Japan, and Korea has remained the
exclusive preserve of those with expertise in the relevant
languages. With a compilation like the present volume the authors
hope to ameliorate that situation. Applying the same rigorous
selection criteria and style of presentation as in the previous
catalogue, assembled and translated here are some 1,500 additional
observations of comets and meteor showers from China, Japan, and
Korea spanning nearly three millennia. With the publication of this
volume, most of the important historical records of East Asian
astronomical observations are now accessible in English. The
introductions and appendices provide all the required information
on specialized terminology, recording conventions, and nomenclature
the reader will need to make use of the records. In addition to
being an invaluable resource for professional astronomers, East
Asian astronomical records have materially aided the research of
scholars in fields as diverse as mythology, medieval iconography,
ancient chronology, and the oral history of pre-literate societies.
The book should be of great interest to cultural astronomers, as
well as to those engaged in historical and comparative research.
This book highlights the technological and managerial fundamentals
and frontier questions of space science. Space science is a new
interdisciplinary and comprehensive subject that takes spacecraft
as the main tools to study the planet Earth, the solar-terrestrial
space, the solar system, and even the whole universe, to answer
significant questions covering the formation and evolution of the
solar system and the universe, the origin and evolution of life and
the structure of the material. The book introduces major scientific
questions in various branches of space science and provides related
technological and managerial knowledge. It also discusses the
necessity of international cooperation and elaborates on the
strategic planning of space science in China. The book can be used
as a reference book or textbook for scientists, engineers, college
students, and the public participating in space science programs.
This book provides in-depth explanations of design theories and
methods for remote sensing satellites, as well as their practical
applications. There have been significant advances in spacecraft
remote sensing technologies over the past decade. As the latest
edition of the book "Space Science and Technology Research," it
draws on the authors' vast engineering experience in system design
for remote sensing satellites and offers a valuable guide for all
researchers, engineers and students who are interested in this
area. Chiefly focusing on mission requirements analyses and system
design, it also highlights a range of system design methods.
This book tells the story of how, over the past century, dedicated
observers and pioneering scientists achieved our current
understanding of the universe. It was in antiquity that humankind
first attempted to explain the universe often with the help of
myths and legends. This book, however, focuses on the time when
cosmology finally became a true science. As the reader will learn,
this was a slow process, extending over a large part of the 20th
century and involving many astronomers, cosmologists and
theoretical physicists. The book explains how empirical
astronomical data (e.g., Leavitt, Slipher and Hubble) were
reconciled with Einstein's general relativity; a challenge which
finally led Friedmann, De Sitter and Lemaitre, and eventually
Einstein himself, to a consistent understanding of the
observational results. The reader will realize the extraordinary
implications of these achievements and how deeply they changed our
vision of the cosmos: From being small, static, immutable and
eternal, it became vast and dynamical - originating from (almost)
nothing, and yet now, nearly 14 billion years later, undergoing
accelerated expansion. But, as always happens, as well as precious
knowledge, new mysteries have also been created where previously
absolute certainty had reigned.
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