Astronomy
The Department of Astronomy offers courses on cosmology, the universe, astrophysics, and astronomy.
Departmental Chair: David Helfand, 1020 Pupin
212-854-2150
djh@astro.columbia.edu
Undergraduate Adviser: Frederik Paerels, 1020 Pupin
212-854-0181
frits@astro.columbia.edu
Office Hours: Tuesday, 3:30 PM-5:30 PM
Departmental Office: 1328 Pupin
212-854-3278
Office Hours: Monday-Friday, 9:00 AM-5:00 PM
NOTE
Course scheduling is subject to change. Days, times, instructors, class locations, and call numbers are available on the Directory of Classes.
Fall course information begins posting to the Directory of Classes in February; Summer course information begins posting in March; Spring course information begins posting in June. For course information missing from the Directory of Classes after these general dates, please contact the department or program.
Click on course title to see course description and schedule.
Fall 2009
Astronomy
Credit Courses
Recommended preparation: a working knowledge of high school algebra. The
overall architecture of the solar system. Motions of the celestial sphere.
Time and the calendar. Major planets, the earth-moon system, minor planets,
comets. Life in the solar system and beyond. This course is similar to
ASTR BC 1753. You cannot enroll in both courses and receive credit for
both.
Milestones in the science of cosmology over the past 6000 years. Skylore
and observation in ancient cultures. The twin revolutions of the Greeks:
Pythagoras and Ptolemy. Aristotle, Aquinas, and the Great Chain of Being.
The "scientific revolution": the impersonal and deterministic world-order
of Newton, Laplace, and Kelvin. The erosion of that world-order by
mathematics and experiment in the 20th century (relativity, quantum
physics, dark matter, and the expanding universe). Today's searches for a
new grand order in the Universe, which can cope-or maybe not-with these
blows to yesterday's comfortable wisdom.
Recommended preparation: a working knowledge of high school algebra.
Introduction to astronomy intended primarily for nonscience majors.
Includes the history of astronomy; the apparent motions of the moon, sun,
stars, and planets; gravitation and planetary orbits; the physics of the
earth and its atmosphere; and the exploration of the solar system.
Recommended preparation: a working knowledge of high school algebra. A
study of the life cycles of stars, from their birth in cold gas clouds to
their final throes in supernova explosions. The turn-of-the-century
revolution in physics: X-rays, radioactivity, the nuclear atom, and the
quantum theory. Energy production by nuclear fission and fusion, and its
consequences.
Laboratory for ASTR C1403. Projects include observations with the
department's telescopes, computer simulation, laboratory experiments in
spectroscopy, and the analysis of astronomical data.
Prerequisite: a working knowledge of calculus. Corequisite: a course in
calculus-based general physics. First term of a two-term calculus-based
introduction to astronomy and astrophysics. Topics include the physics of
stellar interiors, stellar atmospheres and spectral classifications,
stellar energy generation and nucleosynthesis, supernovae, neutron stars,
white dwarfs, and interacting binary stars.
Prerequisites: one year of calculus-based general physics.
Einstein's General Theory of Relativity replaced Newtonian gravity with an
elegant theory of curved spacetime. Einstein's theory led to unforseen and
unnerving predictions of singularities and cosmological instabilities.
Nearly a century later, these mathematical oddities have been confirmed
astrophysically in the existence of black holes, an expanding universe, and
a big bang. The course will cover Einstein's General Theory, beginning with
special relativity, with an emphasis on black holes and the big bang.
Spring 2010
Astronomy
Credit Courses
Prerequisites: Recommended preparation: a working knowledge of high-school algebra.
Distances to, and fundamental properties of, nearby stars; nucleosynthesis
and stellar evolution; novae and supernovae; galaxies; the structure of the
universe and theories concerning its origin, evolution, and ultimate fate.
This course is similar to ASTR BC 1754 and ASTR C1420. You cannot enroll in more than one of these
courses and receive credit.
Galaxies contain stars, gas dust and (usually) super-massive black holes.
They are found throughout the Universe, traveling through space and
occasionally crashing into each other. This course will look at how these
magnificent systems form and evolved, and what can they tells us about the
formation and evolution of the Universe itself. This course is similar to
ASTR BC 1754 and ASTR C1404. You cannot enroll in more than one of these
courses and receive credit.
Recommended preparation: a working knowledge of high school algebra. The
properties of stars, star formation, stellar evolution and nucleosynthesis,
the Milky Way and other galaxies, and the origin and evolution of the
universe.
Laboratory for ASTR C1404. Projects include use of telescopes,
laboratory experiments in the nature of light, spectroscopy, and the
analysis of astronomical data.
Prerequisite: a working knowledge of calculus. Corequisite: the second term
of a course in calculus-based general physics. Continuation of
ASTR C2001; these two courses constitute a full year
of calculus-based introduction to astrophysics. Topics include the
structure of our galaxy, the interstellar medium, star clusters, properties
of external galaxies, clusters of galaxies, active galactic nuclei, and
cosmology.
Prerequisites: one year of calculus based physics.
The emerging field of extrasolar planets and astrobiology will be covered
at a quantitative level, with a major emphasis on astrophysical phenomenae
and techniques. The subject will be introduced through an investigation of
current planetary formation theories and approaches to planet detection,
including what we currently know about extrasolar planets and detailed
reference to state-of-the-art studies. An astronomer's view of the origin
of life and extreme biology will be developed and applied to questions of
cosmo-chemistry, observable life-signatures, habitable zones and other
astrophysical constraints on the development of organisms.
Prerequisite: one year of calculus-based general physics. Physics majors
could take this course with no previous astronomy background. The
properties of compact astronomical objects such as white dwarfs, neutron
stars, and black holes; and their manifestations in pulsars, novae,
supernova remnants, quasars, and active galactic nuclei. High-energy
radiation mechanism and the instrumentation of high-energy astrophysics are
also covered.
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