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Exam Study Tips Exam 1 Will Cover the Day of the Exam Astronomy Picture of the day ASTR 1020: Stars & Galaxies February 18, 2008 • MasteringAstronomy Homework on The HR Diagram is due Feb. 25th. • Reading: Chapter 15, section 15.2. • Exam 1: February 20thth. (Next Class) Young Stars in the Rho Ophiuchi Cloud Cosmic dust clouds and embedded newborn stars glow at infrared wavelengths in this tantalizing false-color view from the Spitzer Space Telescope. 400 ly distance, view is 5 ly across. 1 2 Exam Study Tips Exam 1 will cover • Study with a friend! • Check PowerPoints (on class website) against • All material discussed in class, readings, your notes, homeworks- are you comfortable and tutorial up through today’s class. with the relevant concepts? • Textbook: Chapters 1 (Sections 1.1-1.2), • Do more quiz and review questions in your text and in MasteringAstronomy. Chapter 4, Chapter 5, Chapter 14, Chapter • Check out textbook “Learning Goals” at the 15. beginning of each textbook Chapter and Key • MasteringAstronomy Homeworks on Concepts at end of Chapter. “Scales of the Universe”, “Light and • Review Clicker Questions. Spectroscopy”, “The Sun”, and “The • Exam is closed book but you may bring one sheet of paper (both sides) with notes. Properties of Stars”. 3 4 • Can you use the formula? Examples in The Day of the Exam class, homeworks, sample questions. Bring a #2 pencil and eraser • You may need to “invert” the equation– for example, solve for T using the equation: Bring a calculator if you think you’ll need one wavelength = 2,900,000 nm / T Please be prepared to get started right away For numerical work- remember units!! Does at 10:00 am your answer make sense? (1 nm = 10-9 m; know cm, mm, km) 5 6 1 Today’s Lecture: What is a An H-R Hertzsprung-Russell (H-R) diagram? diagram plots the luminosity and temperature of stars Luminosity 7 Temperature 8 Most stars fall Clicker Question: A star near the top somewhere on of the main sequence has a luminosity the main about: sequence of the H-R diagram a) Twice the Sun’s luminosity b) Five times the Sun’s luminosity c) 20 to 30 times the Sun’s luminosity d) 10,000 times the Sun’s luminosity 9 10 Clicker Question:A star near the top of Large radius Stars with lower the main sequence has a luminosity T and higher L about: than main- sequence stars a) Twice the Sun’s luminosity must have larger radii: b) Five times the Sun’s luminosity c) 20 to 30 times the Sun’s luminosity giants and d) 10,000 times the Sun’s luminosity supergiants 11 12 2 A star’s full classification includes spectral type Stars with higher (line identities) and luminosity class (line shapes, T and lower L related to the size of the star): than main- sequence stars I - supergiant must have II - bright giant smaller radii: III - giant IV - subgiant white dwarfs V - main sequence Examples: Sun - G2 V Small radius Sirius - A1 V Proxima Centauri - M5.5 V Betelgeuse - M2 I 13 14 H-R diagram What is the significance of the depicts: main sequence? Temperature y Color Spectral Type Luminosity Luminosit Radius Temperature 15 16 Main-sequence Mass stars are fusing High-mass stars measurements of hydrogen into main-sequence helium in their stars show that the cores like the Sun hot, blue stars are much more massive than the Luminous main- cool, red ones sequence stars are hot (blue) Less luminous Low-mass stars ones are cooler (yellow or red) 17 18 3 The mass of a High-mass stars normal, hydrogen- burning star determines its luminosity and spectral type! Low-mass stars 19 4.
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