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Books > Science & Mathematics > Physics > Applied physics & special topics > Astrophysics
The development of man's understanding of planetary motions is the
crown jewel of Newtonian mechanics. This book offers a concise but
self-contained handbook-length treatment of this historically
important topic for students at about the third-year-level of an
undergraduate physics curriculum. After opening with a review of
Kepler's three laws of planetary motion, it proceeds to analyze the
general dynamics of "central force" orbits in spherical
coordinates, how elliptical orbits satisfy Newton's gravitational
law and how the geometry of ellipses relates to physical quantities
such as energy and momentum. Exercises are provided and derivations
are set up in such a way that readers can gain analytic practice by
filling in missing steps. A brief bibliography lists sources for
readers who wish to pursue further study on their own.
This Festschrift is a tribute to Susan Stepney's ideas and
achievements in the areas of computer science, formal
specifications and proofs, complex systems, unconventional
computing, artificial chemistry, and artificial life. All chapters
were written by internationally recognised leaders in computer
science, physics, mathematics, and engineering. The book shares
fascinating ideas, algorithms and implementations related to the
formal specification of programming languages and applications,
behavioural inheritance, modelling and analysis of complex systems,
parallel computing and non-universality, growing cities, artificial
life, evolving artificial neural networks, and unconventional
computing. Accordingly, it offers an insightful and enjoyable work
for readers from all walks of life, from undergraduate students to
university professors, from mathematicians, computers scientists
and engineers to physicists, chemists and biologists.
Have you ever wondered what comets are and why astronomers spend so
much time studying them? Now, a comet expert and an astronomical
historian have come together to produce this unique book. Using
their several decades of teaching experience, the authors have
concisely presented the information you need to comprehend these
majestic apparitions that grace our night skies. No mathematical
proficiency is needed. In fact, this book doesn't contain a single
equation. Comets are cosmic Rosetta stones, bridging our current
knowledge by digging back to the earliest days of our solar
systems. How did life arise on Earth? Did comets play a significant
role in bringing water and the necessary organic matter to our
early Earth? How about the dinosaurs? Were they driven to
extinction by a cometary impact 66 million years ago? Comets may be
both the enablers and destroyers of life on Earth as we know it.
These are some of the tantalizing questions discussed here. If you
so desire, steps are given to join the ranks of amateur comet
hunters. Astronomy is one of the last sciences where amateurs play
a significant role. Your reward for discovery? A comet officially
bearing your name in the history books. The next great comet is on
its way, we just do not know when it will arrive. Armed with this
book, you will be ready to enjoy this unforgettable event.
This book addresses the mechanism of enrichment of heavy elements
in galaxies, a long standing problem in astronomy. It mainly
focuses on explaining the origin of heavy elements by performing
state-of-the-art, high-resolution hydrodynamic simulations of dwarf
galaxies. In this book, the author successfully develops a model of
galactic chemodynamical evolution by means of which the neutron
star mergers can be used to explain the observed abundance pattern
of the heavy elements synthesized by the rapid neutron capture
process, such as europium, gold, and uranium in the Local Group
dwarf galaxies. The book argues that heavy elements are significant
indicators of the evolutionary history of the early galaxies, and
presents theoretical findings that open new avenues to
understanding the formation and evolution of galaxies based on the
abundance of heavy elements in metal-poor stars.
This book provides a concise introduction to the special theory of
relativity and the general theory of relativity. The format has
been chosen to provide the basis for a single semester course that
can take the students all the way from the foundations of special
relativity to the core results of general relativity: the Einstein
equation, and the equations of motion for particles and light in
curved spacetime. To facilitate access to the topics of special and
general relativity for science and engineering students, without
prior training in relativity or geometry, the relevant geometric
notions are also introduced.
Prior to the 1920s it was generally thought, with a few exceptions,
that our galaxy, the Milky Way, was the entire universe. Based on
the work of Henrietta Leavitt with Cepheid variables, astronomer
Edwin Hubble was able to determine that others had to lie outside
our own. This books looks at 60 of those that possess some unusual
qualities that make them of particular interest, from supermassive
black holes and colliding galaxies to powerful radio sources.
In the field of particle and astrophysics one of the major
unresolved problems is to understand the nature and properties of
dark matter, which constitutes almost 80% of the matter content of
the universe. This book gives a pedagogical introduction to the
field of dark matter in general, and in particular to the model
building perspective. This book focuses on teaching the basic tools
for model building of dark matter, and it aims to motivate the
reader to propose a new dark matter model.
The 1959 Stamford Electronics Laboratory research report on radar
echos in the ionized medium between the Earth and the Moon was
sponsored by the Air Force Cambridge Research Center, Air Research
and Development Command.
The invention of the semiconductor laser along with silica glass
fiber has enabled an incredible revolution in global communication
infrastructure of direct benefit to all. Development of devices and
system concepts that exploit the same fundamental light-matter
interaction continues. Researchers and technologists are pursuing a
broad range of emerging applications, everything from automobile
collision avoidance to secure quantum key distribution. This book
sets out to summarize key aspects of semiconductor laser device
physics and principles of laser operation.
This book provides a unified treatment of the characteristics of
telescopes of all types, both those whose performance is set by
geometrical aberrations and the effect of the atmosphere, and those
diffraction-limited telescopes designed for observations from above
the atmosphere. The emphasis throughout is on basic principles,
such as Fermat's principle, and their application to optical
systems specifically designed to image distant celestial
sources.
The book also contains thorough discussions of the principles
underlying all spectroscopic instrumentation, with special emphasis
on grating instruments used with telescopes. An introduction to
adaptive optics provides the needed background for further inquiry
into this rapidly developing area.
* Geometrical aberration theory based on Fermat's
principle
* Diffraction theory and transfer function approach to near-perfect
telescopes
* Thorough discussion of 2-mirror telescopes, including
misalignments
* Basic principles of spectrometry; grating and echelle
instruments
* Schmidt and other catadioptric telescopes
* Principles of adaptive optics
* Over 220 figures and nearly 90 summary tables
This 1957 Stamford Electronics Laboratory research report on
"theoretical and experimental radio studies of meteor ionization
trails, with application to radio propagation by meteor
reflections" was sponsored by the Air Force Cambridge Research
Center, Air Research and Development Command.
Our Universe is amazing. This is its story, told in simple
language. The story tells how the Universe came to be what it is
today. It starts with the Big Bang and describes how stars, black
holes, and our solar system developed. It explores the evolution of
life on Earth and investigates the possibility of extra-terrestrial
life. It peers into the future and wonders about the Universe's
likely old age and death, or whatever else may be its end. The
challenge the book takes up is to explain all of this, including
some of the astonishing concepts we have in science, such as
Einstein's theories of Relativity and Quantum Mechanics, using
virtually no mathematics and without dumbing-down. All are
described narratively and explained using examples and anecdotes.
The book is written for young people with a thirst for learning
about the science of space, as well as for 'grown-ups' who want a
better understanding of this fascinating subject.
Black holes entered the world of science fiction and films in the
1960s, and their popularity in our culture remains today. The buzz
surrounding black holes was and is due, in large part, to their
speculative nature. It is still difficult for the general public to
determine fact versus fiction as it pertains to this terrifying
idea: something big enough to swallow anything and everything in
close proximity, with a gravitational force so strong that nothing,
including light, can escape. In the fall of 2015, scientists at the
Laser Interferometry Gravitational-Wave Observatory (LIGO) detected
the first sounds from black holes, brought to earth by the
gravitational waves that emitted from the merging of two black
holes 1.4 billion light years away in space. This confirmed the
existence of gravitational waves, which Albert Einstein predicted
in 1916. In the spring of 2017, physicists and astronomers who were
working on the Event Horizon Telescope (EHT) project captured the
first image of a black hole. This was the supermassive black hole
hosted by the galaxy M87 in the constellation Virgo, 53 million
light years away, and the image shows the shadow the black hole
casts upon the bright light surrounding it. In this book, John
Moffat shares the history of black holes and presents the latest
research into these mysterious celestial objects, including the
astounding results from gravitational wave detection and the shadow
of the black hole.
This thesis provides new insights into the seemingly anomalous
ubiquity of lithium-rich red giant stars. The theory of stellar
evolution, one of the most successful models of modern
astrophysics, predicts that red giant stars should display
negligible levels of lithium (Li) on their surfaces. However,
Li-rich giants, defined as those showing more than three times the
Li content of the Sun, are found everywhere astronomers look in
apparent defiance of established theory. The author addresses this
problem, analyzing the different possible explanations for such an
anomaly, which include interaction with a binary companion, the
production of Li in the interior of the star with its subsequent
transport to stellar exteriors, and the stellar interaction with
planets. The author focuses on this last possibility, where the Li
enrichment may be due to the ingestion of planets or brown dwarfs
as the stars in question grew in size while becoming giants. She
shows that this process is indeed able to explain an important
fraction of giants with Li levels above the three times solar
threshold, but that some other mechanism is needed to explain the
remaining fraction. While this is an important discovery in its own
right, the result that makes this thesis groundbreaking is its
demonstration that the threshold between Li-normal and Li-rich is
mass dependent rather than a fixed proportion of the Sun's content.
This corrects a fundamental misapprehension of the phenomenon and
opens up a new framework in which to understand and solve the
problem. Finally, the author presents interesting observational
applications and samples with which to test this new approach to
the problem of Li enrichment in giants.
This book highlights a major advance in low-energy scattering
theory: the Multi-Channel Algebraic Scattering (MCAS) theory, which
represents an attempt to unify structure and reaction theory. It
solves the Lippmann-Schwinger equations for low-energy
nucleon-nucleus and alpha-nucleus scattering in momentum space,
allowing both the bound and scattering states in the compound
nucleus formed to be described. Results of various cases are
presented and discussed.
It's happening now-plans are being formulated under the
coordination of NASA to launch a permanent, manned space station by
the year 1990. Studies surveying user requirements, system
attributes, and architectural options have been conducted, and
you're on the top of these far-reaching considerations on the next
big step taken within space! Now that the Shuttle and Spacelab are
realities, NASA has set sights on a new horizon-a permanent, manned
space station in the high frontier. The precedents have been
set-Skylab hosted human visits for up to 84 days, and the Soviet's
Salyut was and is a temporary base for cosmonaut crew. The
differences are the term and scope of space station living and the
accomplishments that can be realized with a permanent site and
continuous experimentation within its facilities. Brian O'Leary,
writer, astrophysicist, and former astronaut, describes the
"tinkermodules" that will be carried to the earth's orbit to be
assembled as a space station. His inside track information also lay
Mass human migrations into outer space may begin this century! Are
Earth's inhabitants prepared for this next giant leap? Millions of
tax dollars are being employed in NASA and Defense Department
research facilities to answer this urgent question. Can humankind
migrate to space intelligently, in a civilized manner without real
Star Wars? Are these justifiable economic, political, and
philosophical reasons for undertaking such a vast project? What
legal and institutional implications will surface in distinguishing
Earthkind from Spacekind? The immediate and long-range effects of
space migration-on earth and its inhabitants, on the solar system
and its pioneers-are brought into sharp focus here, within the
perspective of the heated debates now taking place in the highest
government, scientific, business, and academic circles. From the
development of the space shuttle Enterprise and the uses and
objectives of the Space Transportation System to the U.S. and
Soviet space arsenals of hunter-killer satellites and
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