The Cosmic Perspective (9th Edition)
The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 17, Problem 43EAP
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To Explain:Reason for the rarity of rare elements likeLithium, beryllium, and boron despite their being three of the five simplest elements.

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Why don’t we see hydrogen Balmer lines in the spectra of stars with temperatures of 3,200 K?   a. There is no hydrogen in stars this cool.   b. The stars are hot enough that most of the hydrogen is ionized and the atoms cannot absorb energy.   c. These stars are so cool that nearly all of the hydrogen atoms are in the ground state.   d. Stars of this temperature are too cool to produce an absorption spectrum.   e. Stars of this temperature are too hot to produce an absorption spectrum.
A planet has been discovered orbiting a K type main sequence star.  A spectrum taken of this planet shows a blackbody shape to the spectrum that peaks at a wavelength of 8.67x10-5 cm.    a) Find the temperature of this planet. Hint: Always make sure your units match!!!!   b) Describe the prospects for life as we know it on this planet.  Note that water remains in a liquid state between temperatures of 273 K and 373 K.
An isotope of a radioactive element has half-life equal to 5 thousand years. Imagine a sample that is so old that most of its radioactive atoms have decayed, leaving just 20 percent of the initial quantity of the isotope remaining. How old is the sample? Give your answer in thousands of years, correct to one decimal place. Age :  ___ thousand years.
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