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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
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Solar Wind
(Hardcover)
Catherine Waltz
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R2,297
R2,100
Discovery Miles 21 000
Save R197 (9%)
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Ships in 18 - 22 working days
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The Witness of the Stars stands as one of the best explanations of
the constellations in the context of Biblical wisdom. This edition
includes all of E. W. Bullinger's original charts and illustrations
of the heavens above. To compose this book, E. W. Bullinger used
his Biblical scholarship alongside research of the origins of the
astronomical constellations. He demonstrates, through a close
reading of the Old and New Testaments, how each of the star signs
relates to the Bible's stories. Gradually, it is revealed how God
makes himself known to us through the Bible's astronomy. The
symbolism of the star signs are shown as important in the Bible.
Their presence in verse relates not simply to their appearances,
such as Libra's scales or Aries as a ram, but also the way in which
Biblical figures behave after looking at the heavens for guidance.
The Book of Job is highlighted by Bullinger for being significantly
influenced by the stars.
With illustrations and photographsp in full color.
Astronomical and astrological knowledge circulated in many ways in
the ancient world: in the form of written texts and through oral
communication; by the conscious assimilation of sought-after
knowledge and the unconscious absorption of ideas to which scholars
were exposed. The Circulation of Astronomical Knowledge in the
Ancient World explores the ways in which astronomical knowledge
circulated between different communities of scholars over time and
space, and what was done with that knowledge when it was received.
Examples are discussed from Mesopotamia, Egypt, the Greco-Roman
world, India, and China.
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.
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