Courses in Astronomy (Division 326)

Introductory Courses and Courses for Non-Concentrators.

Astronomy 101/111 discusses our explorations of the solar system. Astronomy 102/112 deals 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 each week. 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 telescopes.

101. Introductory Astronomy: The Solar System. No credit granted to those who have completed or are enrolled in 111, 130, or 160. (4). (NS). (BS). (QR/2).
Astronomy 101 students attend the same lectures as Astronomy 111 students (see course description below). (Cowley)
Check Times, Location, and Availability

102. Introductory Astronomy: Stars, Galaxies, and the Universe. No credit granted to those who have completed or are enrolled in 112, 130, or 160. (4). (NS). (BS). (QR/2).
Astronomy 102 students attend the same lectures as Astronomy 112 students (see course description below). Instead of laboratory sections, Astronomy 102 incorporates weekly one-hour discussions and associated exercises, which is considered along with examinations and quizzes for course grades. Cost:2 WL:4 (Section 001:Bregman; Section 007:MacAlpine)
Check Times, Location, and Availability

111. Introductory Astronomy: The Solar System. No credit granted to those who have completed or are enrolled in 101, 130, or 160. (4). (NS). (BS). (QR/2).
This course presents an introduction to the field of astronomy and astrophysics with an emphasis on the discoveries from space exploration. The first third of the course deals with understanding the history of astronomy, orbits, gravitation, optics, and the properties of light and matter. The rest of the course explores the properties, origin and evolution of the major planets, asteroids, comets, the Sun and other components of the Solar System with particular emphasis on comparative aspects with respect to the Earth. The origin and formation of the Solar System and the origin of life will also be discussed. This course is intended for non-science concentrators with a basic high school math and science background. Astronomy 111 has a two-hour laboratory section every week. Astronomy 101 has a one-hour discussion section. Course requirements include assigned reading, section meetings, homework, observations, quizzes, midterm, and a final examination. Laboratory sections include observations with telescopes. Cost:2 WL:4 (Cowley)
Check Times, Location, and Availability

112. Introductory Astronomy: Stars, Galaxies, and the Universe. No credit granted to those who have completed or are enrolled in 102, 130, or 160. (4). (NS). (BS). (QR/2).
Section 001.
Three lectures and a two-hour evening laboratory section each week. Lectures deal with such topics as the properties and evolution of stars; interstellar luminous nebulae; recent discoveries involving galaxies, quasars, and black holes in space; and the present state of our knowledge regarding the origin and ultimate fate of the universe and possibilities of finding and communicating with life outside the solar system. The laboratories and discussions feature planetarium demonstrations, observation with telescopes, and student-inspired dialogue. Familiarity with logarithms and basic geometry is recommended. Cost:2 WL:4 (Bregman)

Section 007. This course is intended primarily for non-science concentrators, who wish to understand the phenomena and properties of the universe beyond our solar system. There are no astronomy prerequisites, and a basic high school math background (e.g., not calculus) will suffice. Students examine the widest possible range of interrelated natural phenomena, from sub-atomic particles to the Universe as a whole. Lectures inventory the different types of stars and examine how red giants, white dwarfs, black holes, supernovae, and people all fit together in one grand, remarkable scheme. The larger picture includes our Milky Way galaxy, less hospitable exploding galaxies, and enigmatic quasars. The present state of knowledge or speculation regarding the origin and ultimate fate of our universe will also receive special attention. It all came from somewhere, but where...and why? Course grades will be derived from scheduled quizzes or exams, and laboratory exercises. Laboratory sections, which meet for two evening hours each week, will include planetarium demonstrations and observations with telescopes (weather permitting). Cost:2 WL:4 (MacAlpine)
Check Times, Location, and Availability

125. Observational Astronomy. No credit granted to those who have completed or are enrolled in Astro. 120. (4). (NS).
This course will teach how astronomical discoveries are made, from what naked eye observations tell us about the solar system and the universe (example: why is the night sky dark?) through what modern telescopes on the ground and in space tell us. We will use all available optical telescopes on campus to explore the different types of telescopes and how they are used to explore the universe. Through this, students will learn how modern astronomical research is conducted. The course will involve lectures, assigned readings, written assignments, and one evening laboratory session per week. Cost:2 WL:4 (Bernstein)
Check Times, Location, and Availability

127. Naked Eye Astronomy. (1). (NS).
The purpose of this course is to examine and understand the observational phenomena that everyone has observed and become familiar with. Students will learn about the nature of the most common astronomical objects that can be observed by eye, such as the Sun, Moon, planets, and the stars. Students will come to understand astronomical phenomena such as the motion of these objects on the sky and their implications: seasons, phases of the moon, solar and lunar eclipses, and the perplexing motions of the planets. Another important topic is the changing stellar sky, including the identification of the brighter stars and constellations during the different seasons. Transient objects such as comets and meteors will be discussed, and a meteorite shower will be observed. The course will conclude with a discussion of ancient observatories and the historical efforts by humanity to measure important astronomical phenomena. A planetarium will be one of the primary teaching facilities, but students will make their own observations and also work with computer programs, such as "The Sky." There will be homework assignments and a final. (Bregman)
Check Times, Location, and Availability

135/AOSS 135. Exploration of the Solar System. Astro. 101 or 111. (3). (NS). (QR/2).

Over the last 30 years we have learned most of what we know about the planets, and the space environment on the Earth. This will present the development of space exploration with a concentration on the major scientific breakthroughs resulting from the exploration of the solar system by U.S. and Soviet spacecraft, from the earliest rockets to the latest GALILEO and HST measurements. Topics will include the constraints that the environment of space places on the designs of space probes, the history of space science in studying the Earth's environment, and the deep-space missions of the other planets. The course is intended for science and non-science concentrators, and all exams will consist of conceptual, not mathematical questions. The course will be an extension of the Intro. Astronomy courses with a focus on the methods of space exploration and the solar system. Assigned reading from a textbook, tentatively The Planetary System by Morrison and Owen, weekly homework sets with mainly conceptual questions, two hourly exams, and one final exam with conceptual questions. (Clarke)
Check Times, Location, and Availability

160. Introduction to Astrophysics. Math. 115, and prior or concurrent enrollment in Phys. 140. No credit granted to those who have completed or are enrolled in 102, 112, or 130. (4). (NS). (BS). (QR/2).
Some of the most exciting phenomena and concepts in astronomy and astrophysics are explored in this survey course. One major theme is the structure and evolution of stars from their birth in giant molecular clouds through their death as white dwarfs, neutron stars, and black holes. Another important theme is galaxies, with discussions about the missing or dark matter in galaxies, galaxy-galaxy interactions, and the large-scale distribution of galaxies in the Universe. We conclude with an examination of the Big Bang, the Inflationary Universe, and the Cosmic Background radiation. This course is directed toward students with an interest in science and mathematics. There are problem sets and a weekly two-hour laboratory using telescopes. Cost:2 WL:3 (Mateo)
Check Times, Location, and Availability

361. Astronomical Techniques. Astro. 160. (4). (Excl). (BS).
This course is intended primarily for students concentrating in astronomy, but other science and engineering students may elect it. It is an introduction to various techniques for obtaining and analyzing observational data. The areas covered are stellar trigonometric distance (parallax), imaging and photometry with electronic detectors, radiometric techniques, and interferometry. In addition, there will be a series of lectures on error theory and least squares, to provide expertise needed in the analysis of observational data. Students will use optical telescopes and instrumentation and the Radio Observatory near Dexter to make observations. Three lectures and one two-hour laboratory period each week. Course work will also include homework exercises and reading in original sources but there are no examinations. (Aller, Sears, and Seitzer)
Check Times, Location, and Availability

389. Individual Studies in Astronomy. Permission of instructor. (1-3). (Excl). (INDEPENDENT). May be repeated for credit.
Individual reading and study in astronomy under the guidance of the instructor.
Check Times, Location, and Availability

399. Introduction to Research. Permission of instructor. (1-3). (Excl). (INDEPENDENT). May be repeated for credit.
For students in astronomy who are prepared to undertake a limited research project under the guidance of a member of the staff of the Department of Astronomy. Open to qualified students in other departments subject to approval by concentration advisors and members of the staff of the Department of Astronomy.
Check Times, Location, and Availability

404. Galaxies and the Universe. Math. 216, and prior or concurrent enrollment in Phys. 340. (3). (Excl). (BS).
This class focuses on the content of the universe on size scales larger than individual stars. We will study the mechanics of stellar orbits and the structure of galaxies, the evidence for dark matter in our galaxy and others, the interstellar gas in galaxies, the morphology of galaxies, and evolution of stellar populations. On scales larger than individual galaxies, we will study the structure and dynamics of clusters of galaxies and larger scale structure. On even larger scales, we will look at the evolution of the universe as a whole, the cosmic microwave background radiation and inferences from its smoothness, and the formation of galaxies and structure on larger scales. This class is designed for science concentrators interested in a fairly serious introduction to the subject, and for upper-level astronomy concentrators. Cost:2 WL:3 (Mateo)
Check Times, Location, and Availability

406. Computational Astrophysics. Math. 216, prior or concurrent enrollment in Phys. 240, and some knowledge of programming. (3). (Excl). (BS).
This course provides an introduction to numerical techniques used in astrophysics, both for analyses of observational data and for constructing theoretical models of astrophysical systems and processes. Topics: programming and coding; error theory; interpolation and curve fitting; analysis and display of data sets; solutions of differential equations; Fourier methods; matrix methods; statistical techniques. Some prior acquaintance with astronomy will be helpful, although astrophysical concepts will be explained in as much detail as necessary. Some prior knowledge of computer programming will be helpful, although the course will begin with elementary coding exercises and illustrations of computer limitations and pitfalls. The computer language used is FORTRAN; users of BASIC or PASCAL will have little difficulty in translation. The course work will consist primarily of coding, running, and displaying various astrophysical algorithms, from simple to complex. One or more term projects will be undertaken. Students will also use, and perhaps adapt and improve, various nationally used standard programs. The recommended text is Numerical Recipes in FORTRAN, Second Edition, by Press et al. (Cambridge, 1992). Not all of this classic will be covered, but it will be useful for anyone involved in scientific computing. Cost:2 WL:3 (Sears)
Check Times, Location, and Availability

520. Cosmochemistry. Astro. 401, 402, and 404. (3). (Excl). (BS).
This is a general survey of the chemical evolution of the universe and its contents from terrestrial materials to the contents of the most distant galaxies. The introductory sections cover traditional differentiation, Goldschmidt's laws of ionic substitution and the Bowen Principle. There is a resume of thermodynamics and statistical mechanics, since these disciplines provide the basis for an understanding of many of the regularities of cosmic chemistry. Radioactive dating is discussed within the context of the chemical history of moon rocks and meteorites. Special emphasis is placed on the derivation of a standard (cosmic) abundance distribution for the solar nebula, and the evidence for deviations from it. Sufficient nuclear structure is introduced to allow an understanding of the synthesis of the chemical elements through stellar and cosmological processes. Students run programs that solve the CNO reaction networks illustrating equilibrium abundance ratios and the rate of approach to them. Atomic and molecular structure are reviewed and applied to the chemical analysis of stars and diffuse matter (dust and gas) in our own and external galaxies. Analytical models of the overall chemical evolution of galaxies are compared to observations and more elaborate numerical predictions. Text: Cowley, An Introduction to Cosmochemistry, 1995, Cambridge University Press. Cost:1 WL:3 (Cowley)
Check Times, Location, and Availability

lsa logo

University of Michigan | College of LS&A | Student Academic Affairs | LS&A Bulletin Index

This page maintained by LS&A Academic Information and Publications, 1228 Angell Hall

The Regents of the University of Michigan,
Ann Arbor, MI 48109 USA +1 734 764-1817

Trademarks of the University of Michigan may not be electronically or otherwise altered or separated from this document or used for any non-University purpose.