ASTR 101 Fall 2014 Stars: From Suns to Black Holes

What makes a star shine? For how long will the Sun keep shining? What are black holes and how can they form? Astronomy 101, a non-major, general introduction to the part of contemporary astronomy that includes how stars form and how they end their existence, will provide answers to these questions and more. The course gives special attention to the exciting discoveries of the past few years. Topics include modern astronomical instruments such as the Hubble Space Telescope, the Chandra X-ray Observatory, the Kepler mission to discover extrasolar planets, the new generation of 8- and 10-meter mountaintop telescopes, results from them, and their even-larger planned successors of 30-meter-diameter equivalents; how astronomers interpret the light received from distant celestial objects; the Sun as a typical star (and how its future will affect ours); and our modern understanding of how stars work and how they change with time. We will also discuss how pulsars and black holes result from the evolution of normal, massive stars and how supermassive black holes lurk at the center of galaxies and quasars. We will discuss the discovery of planets around stars other than the Sun. We regularly discuss the latest news briefs and developments in astronomy and relate them to the topics covered in the course. This course is independent of and on the same level as Astronomy 102 (solar system) and 104 (galaxies and cosmology), and students who have taken those courses are welcome. Observing sessions will include use of the 24-inch telescope and other telescopes for nighttime observations of stars, star clusters, planets and their moons, nebulae, and galaxies, as well as use of other telescopes for daytime observations of the Sun.
Class Format: lecture (three hours per week), observing sessions (scattered throughout the semester), afternoon labs (five times per semester), and a planetarium demonstration
Requirements/Evaluation: evaluation will be based on two hour tests, a final exam, an observing portfolio, and laboratory reports
Additional Info: to be eligible for the Gaudino grade, which stipulates "intellectual presence", a student must demonstrate commitment to engaging the course material in all its aspects: lectures, reading, labs, observing, homework and exams
Additional Info2:
Prerequisites: none
Enrollment Preference:
Department Notes: non-major course
Material and Lab Fees:
Distribution Notes:
Divisional Attributes: Division III
Other Attributes:
Enrollment Limit: 48
Expected Enrollment: 48
Class Number: 1024
CLASSES ATTR INSTRUCTORS TIMES CLASS NUMBER ENRL CONSENT
ASTR 101 - 01 (F) LEC Stars:From Suns to Black Holes Division 3: Science and Mathematics Jay M. Pasachoff
TR 09:55 AM-11:10 AM Physics 203 1024 Open
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