91417 |
SCI 123 Paint &
Exam of Paintings |
Simeen Sattar |
M . . . . . . W . . |
8:30 - 10:30
am 8:30 - 11:30 am |
HEG 106 HEG 106/ ROSE 205 |
SCI |
This course is about the
composition of pigments, dyes and paints, the chemistry underlying selected
techniques (e.g. Attic vase and fresco painting), and scientific methods for
examining paintings, with an emphasis on case studies. As light and atoms and molecules are central
to paints and techniques for examining paintings, the course begins with these
foundational topics. Laboratory work
includes synthesis and analysis of pigments and dyes, preparation of binders
and paints, and fresco painting.
Students pre-registered for the course undertake to review selected
topics from high school chemistry and take an online quiz before the start of
the semester to assess their understanding.
Class size: 18
91418 |
SCI 133 Milk and
Its Contents |
Simeen Sattar |
. T . . . . . . Th . |
3:00 -5:00 pm 3:00 -6:00 pm |
HEG 204 HEG 204/ ROSE 205 |
SCI |
What
is milk made of, and why, and how is it transformed into foods such as yogurt
and cheese? The answers to these
questions, which lie in the chemical composition of milk, are the subject of
this course. The effect of milk on
humans, the effect of milk production on animals and the environment, and the
politics and marketing of milk and dairy foods are among the topics that will
arise naturally. However, the focal
points of this course are the chemical analysis of milk and the chemistry
underlying its transformations into other foods. Three visits to dairy farms and a
milk-processing plant will be scheduled on Fridays (probably). Students registering for this class commit to
reviewing elementary topics from high school chemistry and taking an online
quiz before the start of the semester. Class
size: 18
91419 |
SCI 161 Astronomy |
Peter Skiff |
. T . Th . |
1:30 -2:50 pm |
HEG 102 |
|
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
91420 |
SHP 222 The History of Science before Newton |
Peter Skiff |
. T . Th . |
3:10 -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: 24