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SOLUTIONS TO EXERCISE 23
(a) The Sun's luminosity is 3.9 * 10^26 J/s. (1 J = 1 kg m^2/s^2)
If this luminosity is generated by converting matter into energy, then each
second, 3.9 * 10^26 J worth of mass must be converted. Using E = mc^2,
m = E/c^2 = (3.9 * 10^26 J) / (3 * 10^8 m/s)^2 = 4.3 * 10^9 kg
There are about 8 million people in New York City, with average weight
about 40 kg (from babies to big-and-tall people included). That's
m(people) = 8 * 10^6 * 40 = 3.2 * 10^8 kg
So each second, the Sun consumes matter equivalent to about 13 times the
entire population of New York City. Good thing the Sun is so massive.
(b) The proton-proton chain describes four protons coming together
to form a helium nucleus. A proton's mass is about 1.673 * 10^(-27) kg.
The difference, then, between the mass of four protons and one helium
nucleus is ((4 * 1.00794) - 4.00260) * 1.673 * 10^(-27) kg, and that
converts to
E = mc^2 = (4.03176 - 4.00260) * 1.673 * 10^(-27) * (3 * 10^8)^2
= 4.39 * 10^(-12) J
(c) For every four protons - that is, hydrogen nuclei - used in fusion,
we get 4.4 * 10(-12) J. so produce 3.9 * 10^26 Watts, the Sun must use
3.9 * 10^26 J/s
----------------------------- = 3.55 * 10^38 hydrogen nuclei per second.
4.39 * 10^(-12) J/(4 H-nuclei)
There two hydrogen atoms in each water molecule, and the molecular weight
of water is 18 (H-two-O). So one mole of water weighs 18 grams, and
contains two moles of hydrogen atoms (1 mole = 6 * 10^23). A gallon of
water contains 4 quarts; 1 quart is slightly less than 1 liter, which
is 1000 cm^3; and water's density is 1000 kg/m^3 = 1 gram/cm^3. So,
approximately, one gallon of water contains about 4000 grams of water, or
(2 * 6 * 10^23 H-nuclei/mole) * (4000 g) / (18 g/mole) = 2.67 * 10^26
hydrogen nuclei. So one would need (3.55 * 10^38)/(2.67 * 10^26)
= 1.3 * 10^12 gallons. Over a trillion gallons of water each second!
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