Energy and Environment II
HW #1
Due Friday, January 11, 2002
Suggested Answers in Red
In class we learned the following:
1367 w/m2.
Multiple this value by the disk area of the earth, and one has the solar power striking the earth on average at any instant: pde2/4 x 1367 = 174,700 x 1012 watts, which is close to the text value of 173,000 TW.
Because of the eccentricity of the earth’s orbit, the solar power striking the earth changes by ± 3.5% over the year. It is greatest in late December, 3.5% greater than the average, and it is least in late June, 3.5% less than average.
Annual energy used by humankind = 13 x 1012 J/s x (3600 x 24 x 365) s/yr = 4.1 x 1020 J = 410 x 1018 J = 410 exajoules.
Solving 173,000 x 1012 J/s x 3600 s/hr x NUMBER OF HRS = 4.1 x 1020 J gives 0.66 hr.
According to Figure 1.1 in the text, the main primary energies used by humankind are: oil, coal, natural gas, biomass, hydro (hydroelectric), and nuclear (nuclear electric). Two of these are renewable: biomass and hydro.
According to Figure 1.14 in the text, 173,000 TW of solar power strikes the earth and 52,000 TW is reflected back into space, leaving a net of 121,000 TW of solar power absorbed by the earth and its atmosphere. For the earth to be in steady-state with its surroundings, an equal power must leave the earth and its atmosphere. That is, 121,000 TW of long wavelength (or thermal or infrared) radiation must leave the earth at each instant.
Derived from the sun – solar direct or indirect:
Not derived from the sun:
Individual choice and discussion.