Cosmology 20B Homework 2 solutions
... 14. Discuss the controversy between Darwin and Kelvin over the age of the Sun. What were the arguments behind each of their views and who was right in the end? Taking into account Darwin’s authoritative view on the timescales required for evolution, do you think that life in the Universe would be po ...
... 14. Discuss the controversy between Darwin and Kelvin over the age of the Sun. What were the arguments behind each of their views and who was right in the end? Taking into account Darwin’s authoritative view on the timescales required for evolution, do you think that life in the Universe would be po ...
Test#3
... 1. A measurement of the parallax of a star allows us directly to determine the star's a) rotation rate, b) temperature, c) distance, d) age 2. How much brighter would a star be if an observer moved from 3 to 1 parsec from the star? a) 3 times, b) 9 times, c) 27 times, d) 81 times 3. The difference b ...
... 1. A measurement of the parallax of a star allows us directly to determine the star's a) rotation rate, b) temperature, c) distance, d) age 2. How much brighter would a star be if an observer moved from 3 to 1 parsec from the star? a) 3 times, b) 9 times, c) 27 times, d) 81 times 3. The difference b ...
Astronomy 100 Homework #2 Solutions 1, Problem 3‐27 (2 pts
... 5. Problem 4‐34 (2 pts). If Earth were twice as far from the Sun, the force of gravity attracting Earth to the sun would be (c) one‐quarter as strong. Gravity follows an inverse square law in proportion to distance. 6. Problem 4‐36 (2 pts). If the Moon were closer to the Earth, high tides would b ...
... 5. Problem 4‐34 (2 pts). If Earth were twice as far from the Sun, the force of gravity attracting Earth to the sun would be (c) one‐quarter as strong. Gravity follows an inverse square law in proportion to distance. 6. Problem 4‐36 (2 pts). If the Moon were closer to the Earth, high tides would b ...
Day 2
... Once the star is close to hydrostatic equilibrium, the contraction slows down. However, the star must continue to contract until the temperature in the core is high enough that nuclear fusion can begin and support the star! During the contraction the star's temperature stays about the same, but its ...
... Once the star is close to hydrostatic equilibrium, the contraction slows down. However, the star must continue to contract until the temperature in the core is high enough that nuclear fusion can begin and support the star! During the contraction the star's temperature stays about the same, but its ...
Lecture Notes-PPT
... collect together by gravity. During the exchange of energy between the stars, some stars reach escape velocity from the protocluster and become runaway stars. The rest become gravitationally bound, meaning they will exist as collection orbiting each other forever. ...
... collect together by gravity. During the exchange of energy between the stars, some stars reach escape velocity from the protocluster and become runaway stars. The rest become gravitationally bound, meaning they will exist as collection orbiting each other forever. ...
Questions for this book (Word format)
... 4. What are the observed properties of a Cepheid variable (or Delta Cephei star)? How are these properties produced? 5. What information about stellar evolution is provided by the properties of comets? Using Kippenhahn’s figure for the mass loss caused by this mechanism, calculate how much mass the ...
... 4. What are the observed properties of a Cepheid variable (or Delta Cephei star)? How are these properties produced? 5. What information about stellar evolution is provided by the properties of comets? Using Kippenhahn’s figure for the mass loss caused by this mechanism, calculate how much mass the ...
Star Name __Direction ___ Degrees
... 21. Name three stars that are second magnitude or brighter. Give their location in direction and degrees above the horizon on the celestial sphere. Star Name __Direction Example: Polaris North ___________ ____________ ...
... 21. Name three stars that are second magnitude or brighter. Give their location in direction and degrees above the horizon on the celestial sphere. Star Name __Direction Example: Polaris North ___________ ____________ ...
Measuring the Properties of Stars
... being radiated by the surface of a particular star. Astronomers call this power Luminosity, and it has dependancy on two properties of a star; it’s surface size (4R2) and its surface temperature (T). These are direct relationships. An increase in either of the properties, results in an increase in ...
... being radiated by the surface of a particular star. Astronomers call this power Luminosity, and it has dependancy on two properties of a star; it’s surface size (4R2) and its surface temperature (T). These are direct relationships. An increase in either of the properties, results in an increase in ...
Astronomy 2
... most stars are made of hydrogen & helium (determined by temperature & composition no two are alike) ...
... most stars are made of hydrogen & helium (determined by temperature & composition no two are alike) ...