91755 |
SCI 125 A Photographic Processes |
Simeen Sattar |
M . . . . . . W . . |
8:30- 10:30 am 8:30- 11:30 am |
HEG 106 / ROSE 205 |
SCI |
Topics
covered in this course range from the chemistry of silver and non-silver
photographic processes to the physics of CCD cameras. Laboratory work
emphasizes the chemical transformations involved in making gum dichromate
prints, cyanotypes, blueprints, salted paper prints and black-and-white silver
emulsion prints. Registered students undertake to review elementary
topics from high school chemistry and take an online quiz before the start of
the semester to assess their understanding of these topics. Class
size: 18
91756 |
SCI 125 B Photographic Processes |
Simeen Sattar |
. T . . . . . . Th . |
3:00-5:00 pm 3:00-6:00 pm |
HEG 106 / ROSE 205 |
SCI |
See
above. Class size: 18
91754 |
SCI 130 Nuclear & ChemICAL Weapons |
Simeen Sattar |
. . W . . |
6:00 pm -7:30 pm |
HEG 102 |
N/A |
(1 credit) Cross-listed: Human Rights Nuclear and chemical weapons
are much in the news and likely to remain so. Consequently, students aiming for
careers such as journalism and foreign service will
benefit from a working knowledge of the terminology associated with these
weapons. For nuclear weapons, we will
begin by developing familiarity with the atomic nucleus and types of nuclear
reactions. We will then focus on
uranium, from mining to enrichment to its uses in nuclear reactors and in
fission bombs. We will conclude by
discussing reprocessing spent reactor fuel to concentrate plutonium, which is
also used in fission bombs. For chemical
weapons, we will start with the structures of the small molecules that make up
these weapons and go on to their classification, design and destruction. (This
course will meet for the first 8 weeks of the semester.) Class size: 18
91757 |
SCI 161 Astronomy |
Peter Skiff |
. T . Th . |
1:30 pm -2:50 pm |
HEG 102 |
N/A |
An introductory course in
astronomy and astrophysics, developing the current status of knowledge and
theories of the solar system, individual stars, galaxies, and the interstellar
medium. Theories of particular unique objects (quasars,
pulsars, supernovae, X-ray stars, and black holes) will be discussed in terms
of models of stellar, galactic, and cosmic evolution. Class
size: 36
91758 |
SHP 222 THE History OF Science before Newton |
Peter Skiff |
. T . Th . |
3:10 pm -4:30 pm |
HEG 102 |
HIST |
Cross-listed: Science,
Technology & Society;
related interest:
Classical Studies An introduction to the
history and philosophy of science. T. S. Kuhn's model of historical progress
will be used to examine selected parts of discourses involving pre‑Socratic
philosophy, mythology, Copernican astronomy, Galileo's trial, and Newton's
philosophy. A critique of method will introduce modern historiographic
and philosophic controversy. Designed as a core course for studies in history,
philosophy, and sociology of science; no prior mathematical or technical
expertise will be presumed at this level. Readings include excerpts from the Enuma Elish, the Milesians,
Pythagoras, Heraclitus, Plato, Aristotle, Ptolemy, Copernicus, Kepler, Galileo, and Newton. Secondary
commentary by Nahm, Butterfield, Kuhn, Munitz, and others.
Class size: 18
91759 |
SHP 225 Einstein |
Peter Skiff |
. . W . F |
1:30 pm -2:50 pm |
HEG 102 |
N/A |
Cross-listed: Science,
Technology & Society An examination of
Einstein’s life and work, the impact of his work on current world views, and
some of the many controversies involved therein, using biography and popular
descriptions of the relativity theories, atomic theories, and optical theories.
We will compare the advantages of methods of positivism and realism in
philosophy and of "internalism" and
"externalism" in the history of science. Readings include some
primary sources; secondary authors include Overbye, F`lsing and Holton. Accessible to students with no prior college‑level scientific
or mathematical experience. Class
size: 36