Chapter 11 - USD Home Pages
... 35. a. What is the approximate mass of a main sequence star that is 10,000 times as luminous as the Sun? b. What is the approximate lumniosuty of a main-sequence star whose mass is one-tenth that of the Sun? Answer: a. Reading Fig 11-14: Find 104 L on the vertical scale; trace horizontally until yo ...
... 35. a. What is the approximate mass of a main sequence star that is 10,000 times as luminous as the Sun? b. What is the approximate lumniosuty of a main-sequence star whose mass is one-tenth that of the Sun? Answer: a. Reading Fig 11-14: Find 104 L on the vertical scale; trace horizontally until yo ...
For each statement or question, select the word or expression that
... B. titanium and hydrogen C. hydrogen and helium D. helium and iron ____ 15. Red giants that lose their atmospheres leave faint, Earth-sized stars called A. Cepheid variables B. blue superiants C. white dwarfs D. proton stars ____ 16. Cepheid variable stars have been used to determine the A. ages of ...
... B. titanium and hydrogen C. hydrogen and helium D. helium and iron ____ 15. Red giants that lose their atmospheres leave faint, Earth-sized stars called A. Cepheid variables B. blue superiants C. white dwarfs D. proton stars ____ 16. Cepheid variable stars have been used to determine the A. ages of ...
Extension worksheet – Topic 6 - Cambridge Resources for the IB
... A large, cool cloud of gas may collapse under gravity to form a star. State where the energy comes from to heat up the star so that nuclear fusion may take place. In this question assume a mass–luminosity relation of L M 3.5 . a ...
... A large, cool cloud of gas may collapse under gravity to form a star. State where the energy comes from to heat up the star so that nuclear fusion may take place. In this question assume a mass–luminosity relation of L M 3.5 . a ...
An Introduction to the Night Sky Stars and Constellations
... An Introduction to the Night Sky Stars and Constellations 1. What is the Latin root word of star? 2. Why do stars “twinkle”? 3. Why do planets “shine”? ...
... An Introduction to the Night Sky Stars and Constellations 1. What is the Latin root word of star? 2. Why do stars “twinkle”? 3. Why do planets “shine”? ...
Understanding Stars
... Stefan-Boltzman Law A dense hot object emits light of all colors – More of one color than others • “peak” color – The peak color is determined by the temperature • Hotter = bluer! – demo Stellar Spectroscopy Astronomers can tell what elements are in a star by the lines in its spectrum Peak color det ...
... Stefan-Boltzman Law A dense hot object emits light of all colors – More of one color than others • “peak” color – The peak color is determined by the temperature • Hotter = bluer! – demo Stellar Spectroscopy Astronomers can tell what elements are in a star by the lines in its spectrum Peak color det ...
Chapter 25 Study guide Answer Key
... 3) Which property of a star can be determined by its color? Temperature 4) About how many stars are estimated to occur in pairs or multiples? 50% ...
... 3) Which property of a star can be determined by its color? Temperature 4) About how many stars are estimated to occur in pairs or multiples? 50% ...
Earth
... standard distance from Earth) from 20 pc. • Since the star will be “closer”, it will be brighter. • A brighter star has a smaller magnitude • Thus, we expect an absolute magnitude less than ...
... standard distance from Earth) from 20 pc. • Since the star will be “closer”, it will be brighter. • A brighter star has a smaller magnitude • Thus, we expect an absolute magnitude less than ...
Answers Universe Cornell Notes Chapter 8, Sec 2
... and size. Supergiant star, giant star, medium-sized star, white dwarf star, neutron star A star’s color reveals its temperature. Red, yellow - white, blue - white Brightness depends on the star’s size and temperature. It’s brightness as seen from Earth. Apparent brightness is how bright it appears t ...
... and size. Supergiant star, giant star, medium-sized star, white dwarf star, neutron star A star’s color reveals its temperature. Red, yellow - white, blue - white Brightness depends on the star’s size and temperature. It’s brightness as seen from Earth. Apparent brightness is how bright it appears t ...
A Brief History of Planetary Science
... Each spectral type is divided into 10 sub classes 0 - 9 (from high to low T) ...
... Each spectral type is divided into 10 sub classes 0 - 9 (from high to low T) ...
Chapter 8 lesson 4 Notes
... Stars form when matter comes together and starts to give off energy. ...
... Stars form when matter comes together and starts to give off energy. ...
Weekly Homework Questions #3, Sep. 14, 2010
... 1. How can one measure the mass of a star other than the Sun? (a) measuring the color of the star and using a color-mass relationship (b) the apparent magnitude of a star tells its mass (c) the gravitational force on a companion star in a double star (d) the mass of a star is determined by its locat ...
... 1. How can one measure the mass of a star other than the Sun? (a) measuring the color of the star and using a color-mass relationship (b) the apparent magnitude of a star tells its mass (c) the gravitational force on a companion star in a double star (d) the mass of a star is determined by its locat ...