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Books > Science & Mathematics > Astronomy, space & time > Space travel & exploration
Structure and Evolution of Single Stars: An introduction is
intended for upper-level undergraduates and beginning graduates
with a background in physics. Following a brief overview of the
background observational material, the basic equations describing
the structure and evolution of single stars are derived. The
relevant physical processes, which include the equation of state,
opacity, nuclear reactions and neutrino losses are then reviewed.
Subsequent chapters describe the evolution of low-mass stars from
formation to the final white dwarf phase. The final chapter deals
with the evolution of massive stars.
"And it was then that all these kinds of things thus established
received their shapes from the Ordering One, through the action of
Ideas of Numbers" (Plato: in Timaeus). Indeed, the Hamilton's
'Principle of Least Action' is a mathematical discrimination
between inorganic and organic systems. The geometrical progression
of organic life has the property of producing by simple addition, a
succession of numbers or similar shapes making the homothetic
(gnomonic) growth-work by 'imbibition' (from inside outwards).
Whereas, inorganic matters (crystals, snowflakes, rocks) grow by
'agglutination' (from outside inwards) and final distribution of
energy to cause no further motion. While in inorganic growth
(hexagonal), the Principle of Least Actions tends to save energy,
in organic or gnomonic growth (pentagonal) there is a tendency to
save the substance. Involving the avid travelers "father jaguar and
the cub," this tourbook of the "snow gallery" mathematically and
geometrically analyzes the deposition, aggregation, capacitance,
and velocity of the snowflake formation, vis a vis the hexagonal
(honeycomb) tendency. When the tour is over, the cub classifies his
most favorite snowflakes, giving them names.
Space and Space Travel is a comprehensive introductory overview of
subject matter related to exploration of the solar system. After an
initial discussion of energy, power, and the atom, the book
explores the Sun and its impact on planets and the space
environment, the conditions in space, the fundamentals of space
travel, and planetary destinations. Specific topics include the
solar interior and atmosphere, space plasma environments and
weather, advanced propulsion, the inner solar system, and asteroids
and beyond. Photographs, charts, and graphs support the text and
enhance learning. Space and Space Travel is broadly based, and can
be used in classes that discuss planetary science, space science,
space technology, and human space flight. It is suitable for junior
and senior level high school courses, as well as survey courses at
the university level. The book is also an excellent jumping off
point for technical classes that explore a specific topic in
detail, but require general background knowledge.
In 2005, Palla & Baraffe proposed that brown dwarfs and very
low mass stars (
What's in the dark? Countless generations have gazed up at the
night sky and asked this question--the same question that
cosmologists ask themselves as they study the universe.
The answer turns out to be surprising and rich. The space between
stars is filled with an exotic substance called "dark matter" that
exerts gravity but does not emit, absorb, or reflect light. The
space between galaxies is rife with "dark energy" that creates a
sort of cosmic antigravity causing the expansion of the universe to
accelerate. Together, dark matter and dark energy account for 95
percent of the content of the universe. News reporters and science
journalists routinely talk about these findings using terms that
they assume we have a working knowledge of, but do you really
understand how astronomers arrive at their findings or what it all
means?
Cosmologists face a conundrum: how can we study substances we
cannot see, let alone manipulate? A powerful approach is to observe
objects whose motion is influenced by gravity. Einstein predicted
that gravity can act like a lens to bend light. Today we see
hundreds of cases of this--instances where the gravity of a distant
galaxy distorts our view of a more distant object, creating
multiple images or spectacular arcs on the sky. Gravitational
lensing is now a key part of the international quest to understand
the invisible substance that surrounds us, penetrates us, and binds
the universe together.
"A Ray of Light in a Sea of Dark Matter" offers readers a concise,
accessible explanation of how astronomers probe dark matter.
Readers quickly gain an understanding of what might be out there,
how scientists arrive at their findings, and why this research is
important to us. Engaging and insightful, Charles Keeton gives
everyone an opportunity to be an active learner and listener in our
ever-expanding universe.
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