Introductory Courses and Courses for Non-Concentrators.
Astronomy 101/111 discusses our explorations of the solar system. Astronomy 102/112 deal with stars and the rest of the Universe beyond the solar system. Students in Astronomy 101 and 102 attend a weekly discussion section. Students in Astronomy 111 and 112 actively participate in a laboratory which meets in the evening every other week and in the daytime in alternate weeks. Astronomy 130 covers selected topics from the whole field of astronomy. None of these courses is a prerequisite for any of the others. High school mathematics through plane geometry is useful. All students in each course will have opportunities for a planetarium visit and for evening observations with the telescopes mounted on Angell Hall.
101. Introductory Astronomy: The Solar System. No
credit is granted to those who have completed 111 or 130. (4).
Section 001. Astronomy 101 students attend the same lectures as Astronomy 111 students. For course description, see Astronomy 111, section 001. (Teske)
Section 006. Astronomy 101 students attend the same lectures as Astronomy 111 students. For course description, see Astronomy 111, Section 007. (Cowley)
102. Introductory Astronomy: Stars, Galaxies, and the
Universe. No credit is granted to those who have
completed 112 or 130. (4). (NS).
Section 001. Astronomy 102 students attend the same lectures as Astronomy 112 students. For course description, see Astronomy 112, section 001. (Sears)
Section 006. Astronomy 102 students attend the same lectures as Astronomy 112 students. For course description, see Astronomy 112, Section 007. (Kirshner)
111. Introductory Astronomy: The Solar System. No credit is granted to those who have completed 101 or 130. (4). (NS).
Section 001. Lectures are the same for both Astronomy 101 and 111. They deal with the beginnings of astronomy, motions of bodies in the solar system, properties of light and atoms, the Sun, the Earth, the Moon, individual planets and satellites, comets and meteors, and the origin of the solar system and life. The exploration of the solar system by spacecraft will be emphasized. Astronomy 111 has laboratory and discussion sections alternating every week. Astronomy 101 has only discussion sections. Course requirements include two midterms and a final examination. Laboratory sections include observations with telescopes. A planetarium visit will be arranged. Textbook: Exploration of the Solar System, by W. J. Kaufman, III (Macmillan, 1978). (Teske)
Section 007. Lectures (the same for both Astronomy 101 and 111) deal with the beginnings of astronomy, motions of bodies in the solar system, properties of light and atoms, the Sun, the Earth, the Moon, individual planets and satellites, comets and meteors, and the origin of the solar system and life. Elementary concepts of physics, chemistry, and geology are introduced in order to elucidate the new understanding of the solar system made possible by the space program. Emphasis is placed on an understanding of the composition, nature, and history of matter in the solar system. Special attention is devoted to terrestrial, lunar and meteoritic rock samples, as well as surface land features on terrestrial planets. Astronomy 101 has discussion sections. Astronomy 111 has laboratory sections. Course requirements include homework observations and exercises, two one-hour quizzes, and a final examination. Observations with telescopes and a planetarium visit will be arranged. Textbook: Exploration of the Solar System, by W. J. Kaufman, III (Macmillan, 1978). (Cowley)
112. Introductory Astronomy:
Stars, Galaxies, and the Universe. No credit is granted
to those who have completed 102 or 130. (4). (NS).
Section 001. Lectures are the same for Astronomy 102 and 112. This course is intended for non-science majors who want to learn about the structure and evolution of stars, galaxies, and the Universe. (Astronomy 101/111, which is not a prerequisite for this course, describes our Solar System.) Lectures deal with distances and properties of stars, their origins from interstellar dust and gas, and their final fates as white dwarfs, supernovae, black holes, etc. Further lectures treat our stellar system (the Milky Way Galaxy) and then explore other galaxies and quasars to the farthest reaches of the Universe. Attention will be given to observational evidence relating to the origin of the Universe, its present structure, and clues to its future. Course work includes assigned reading, short quizzes, midterm and final examinations, and section meetings. Astronomy 112 students have evening laboratory and observation periods every other week, and daytime discussions in alternate weeks. Astronomy 102 has only discussion sections. The textbook will probably be Exploration of the Universe (4th ed., 1982), by Abell. (Sears)
Section 007. Lectures are the same for Astronomy 102 and 112. This course treats modern ideas concerning the origin and evolution of stars, galaxies, and of the Universe as a whole. The lectures emphasize current knowledge of the formation and evolution of stars toward their ultimate destiny as white dwarfs, neutron stars, or black holes. The course will outline the evidence that the Universe is currently expanding from a hot dense phase in the distant past toward a fate that is accessible to observation. Specific objects such as supernovae, quasars, and galaxies are also examined. Course work includes assigned reading, short quizzes, midterm and final examinations, and section meetings. Astronomy 112 students have evening laboratory and observation periods every other week, and daytime discussions in alternate weeks. Astronomy 102 has only discussion sections. (Kirshner)
130. Explorations in Astronomy. No credit is granted to those who have completed 101, 102, 111, or 112. I. (4). (NS).
This course covers selected topics concerning the solar system, stars, the galaxy, and the universe. Some of the subjects discussed are: the planets and the results of the space program, the sun and its effect on the Earth, the life history of stars, interstellar nebulae, pulsars, black holes, normal and peculiar galaxies, quasars, and the evolution of the universe. There are four lectures per week and observations with telescopes and a planetarium visit will be arranged. The course grade will be based upon periodic homework assignments, two one-hour tests, and a final examination. A term paper will be optional. (Aller)
162. Cosmology I. (4). (NS).
During Fall Term, 1982, this course is jointly offered with Residential College (N Sci 261).
An introduction to astronomy for non-science majors. The following topics will be treated: basic astronomy, matter, light, energy, and stars. Big bang origin of the universe. Life cycle of the universe: a model. Cosmic time scale. Hubble constant and its evolution. Relics of big bang, helium production, cosmic fireball radiation. Future of the universe. Evaluations on the basis of tests, a term project, and class participation. (Haddock)
221. General Astronomy: The Solar System. Prior or concurrent election of Math. 115. No credit is granted to those who have completed 101, 111, or 130. (4). (NS).
Astronomy 221-222 is a two-term introductory sequence intended primarily for students in the sciences and engineering. In the Fall Term, Astronomy 221 deals with the astronomy and physics of the solar system. Topics covered include: (1) principles of orbit theory; (2) interior structure, surface features and atmospheres of the planets; (3) the minor constituents of the solar system; (4) the sun. Laboratory work will include observations with the telescopes atop Angell Hall, experiments and discussions. Homework problems are assigned almost weekly. There will be a final, two one-hour examinations, and periodic quizzes. (Aller)
261/NOEP 301. Navigation. (2). (Excl).
The purpose of this course is to educate students in all aspects of marine navigation, from getting a vessel underway from port through open ocean navigation using both celestial and electronic means. The content of the course is divided into three major areas. The first section focuses on piloting, emphasizing the safe navigation of vessels in coastal waters. This section provides an introduction to navigational instruments and aids to navigation. The second section concerns celestial navigation, the ability to determine position through observation of celestial bodies. Students learn how to determine position based on the use of the sextant and various almanacs and mathematical tables. The third section of the course considers electronic navigation and the maritime law covering the movement of sail and power-driven vessels. The course consists of two ninety-minute lectures a week. Grading is done on the basis of homework, quizzes, and examinations. The primary textbooks for the course are Marine Navigation I and Marine Navigation II by Richard R. Hobbs and are available on loan from the NOEP. (Nelson)
321. Solar-Terrestrial Relations. Four credits of astronomy. (2). (NS).
For students who wish to learn more about our sun, its activity cycle, and the influence on our earth. Objectives: To work toward a better understanding of the many phenomena observed from ground as well as from satellites. The physical processes involved will be sketched using a minimum of mathematics. Mathematics background is advantageous but not required. Topics as follows: The Quiet Sun: nuclear energy sources in the interior; the surface layers; interplanetary space. The Earth and its Immediate Surroundings: atmosphere, ionosphere, radiation belts. Solar Activity: sunspots, magnetic fields, plages, prominences, corona, flares; the 11/22 year cycle; high-energy radiation and particle events; changes in the earth's atmosphere caused by solar events; possible long term effects. Instruction by lectures with slides and occasional movies. Exercises on interpretation of observations. Evaluation of participation in discussions, two or three tests, final exam, or term paper. (Elste)
421. Advanced General Astronomy. Phys. 140 and 240 and Math. 116, or the equivalent; or permission of instructor. (3). (NS).
50% of the course will be based on independent reading of William K. Hartmann's Moons and Planets (second edition). The remaining 50% of the course will be based on material presented in the lectures. This is divided into 3 parts. Part I deals with the mechanics of the solar system, and covers topics such as the two-body problem, N-body relations, the virial theorem, potential about an oblate spheroid, equations of rigid-body motion, etc. Part II treats geochemistry and cosmochemistry with special reference to the solar system. Included topics are fundamental principles of thermodynamics and chemical reactions, meteorites, geochemical classification of the elements, models of the solar nebula, condensation sequences from the solar nebula and the composition of planets. Part III deals with planetary structure, and emphasizes comparative planetology of the moon and terrestrial planets. The level of difficulty will be similar to that of junior and senior courses in physics and chemistry. (Cowley)
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