Universe
Universe
11th Edition
ISBN: 9781319039448
Author: Robert Geller, Roger Freedman, William J. Kaufmann
Publisher: W. H. Freeman
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Chapter 19, Problem 5Q
To determine

The reason behind the fact that no main-sequence star with mass less than 0.4 MΘ has yet converted all of its hydrogen to helium, even if there is evidence that proves the universe is about 13.7 billion years old.

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Suppose that stars were born at random times over the last 1010 years. The rate of star formation is simply the number of stars divided by 1010 years. The fraction of stars with detected extrasolar planets is at least 10 %. The rate of star formation can be multiplied by this fraction to find the rate planet formation. How often (in years) does a planetary system form in our galaxy? Assume the Milky Way contains 9 × 1011 stars.
Let us assume that our galaxy consists of 2.5 × 1011 stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution ? Take the diameter of the Milky Way to be 105 light year.
Stars formed after the Big Bang had cooled down. From globular cluster dating and from stellar uranium spectrum, what is the approximate age of the oldest known stars?   6,000 years         4.6 billion years         7 billion years         12 billion years         13.8 billion years
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