NATS-101
Introduction to Global Change- Pretend Quiz 1
__SAMPLE____________
_SOLUTIONS_____________
First
Name
Family Name
FOR
MULTIPLE CHOICE,
SELECT THE SINGLE BEST ANSWER
AMONG CHOICES, AND PLACE LETTER OF BEST ANSWER IN BLANK
TO
LEFT OF
QUESTION NUMBER. (Quiz
1 will be
based on lectures and readings from 8/21 through 8/28)
B 1.
Evidence
for the Big Bang event comes from .
A. the very very small size of atoms
C. the extensive oceans on
planet Earth
B. distance and speed of galaxies
D. the moons found around many planets
_5_2. You can
earn up to _____ extra credit points toward your final course grade.
A. 3
B.
5
C. 10
D. 15
_A_3. The universe is made
up of galaxies, and .
A. galaxies are made up of stars
C. our solar system is made up of galaxies
B. galaxies are made up of planets
D. our planet is at the center of the universe
A 4.
42He
represents .
A. helium with 2 neutrons & 2 protons
C. hydrogen with 4
neutrons and 2 protons
B. helium with 4 neutrons & 2 protons
D. helium with 4 protons
and 2 neutrons
B 5.
Terrestrial
radiation has its
peak in (1)____, whereas solar radiation has its peak in (2)________.
A. 1-x-ray radiation; 2-infrared radiation
C. 1-visible; 2-infrared
B. 1-infrared; 2-visible
D.
1-infrared; 2-ultraviolet
E 6.
The
most abundant gas in the
Earth's atmosphere is .
A. krypton
B. argon
C.
oxygen D.
carbon dioxide
E. nitrogen F.
hydrogen
A 7.
Chemical reactions
involve (1) and
are relatively low energy compared to nuclear reactions that involve (2) .
A. 1-electrons
2-neutrons
& protons
C.
1-electrons & protons
2-neutrons
B. 1-neutrons & protons
2-electrons
D. 1-neutrons
2-electrons & protons
_A_8. Most of the mass
(matter) in our solar system is .
A. in the sun
C. in the Earth's core
B. in the planets
D.
in Jupiter
_C_9. Amazing as it may
sound, you can pass
this course with a final grade of ________%.
A.
45.5
B.
50.5
C. 55.5
C 10.
is an example of an important greenhouse gas.
A. nitrogen
B.
oxygen
C. water vapor
D. argon
B 11. The
layer of the atmosphere in which we live is the .
A. asthenosphere
B.
troposphere
C. mesosphere
D. stratosphere
_D_12. Infrared
electromagnetic radiation with a
wavelength of 1.23 x 10-4 meters would be _______ in
expanded
general notation.
A. 1,234m
B.
0.01234m
C. 12,300m
D. 0.000123m
E. –12,300m
_D_13. The
temperature at "absolute zero", would have the value of
zero on the scale.
A. Celsius
C.
Richter E.
A & D
B. Fahrenheit
D. Kelvin
F. all of the above
_B_14. The Doppler effect
results in which of the
following observations when distant galaxies are viewed?
A. atoms
B.
red shift C.
Big Bang D. fusion E.
molecules
15. If our sun is only producing He by fusion reactions,
why does Earth contain all the elements of the Periodic Table?
Our sun is a "young" star, only about 4.6
billion years old, and the fusion reactions taking place in its
interior are not currently forming elements beyond helium (He,
p=2). The nebula from which our solar system formed therefore must have
already been composed of all the elements of the Periodic Table. All
those elements would have been formed earlier in stellar (star)
processes (up to iron (Fe, p=26) by fusion and the rest of the elements
by neutron flux in supernova) during the period between the Big Bang
13-15 billion years ago and the formation of our solar system.
16.
What is a nebula?
A nebula is
a rotating ball of dust thought to be the precursor to the formation of
stars and planets in solar systems.
17.
Earth's
temperature is about 300K and the temperature of the surface of
the sun is 6000K. How much more energy
would a body with the temperature of the sun radiate compared to a
similar-size
body at Earth's temperature? (show work)
Using
the
Stefan-Boltzmann Law, we can form the ratio of the radiative flux from
the Sun to that of Earth:
Fsun
=
s*Tsun4
Fearth
s*Tearth4
with s=Stefan Boltzmann constant. For the ratio, the variable "s" cancels out. Then the flux ratio is the ratio of the solar to earth temperatures, taken to the fourth power. Using the suggested values for these temperatures, Fsun/Fearth = (6000/300)4 = 204 = 160,000. The radiative flux from the Sun is about 160,000 times greater than the radiative flux from the Earth!
18.
State Wien's Displacement Law in your own words.
The characteristic wavelength at
which the maximum radiation is emitted from a black body is
inversely proportional to the temperature of the black body.
19.
State the Stefan-Boltzmann Law in your own words.
The radiation flux from a black body is
proprtional to its temperature taken to the fourth power.
20.
How does the "greenhouse effect" work in the
Earth-Atmosphere system? About how much
warmer is the Earth's surface than it would be with no
atmosphere?
The atmosphere is
largely transparent to solar radiation mostly arriving in the
visible wavelengths; but greenhouse gases absorb the mainly
infrared energy re-radiated by Earth. This keeps the
Earth's surface warmer than it would be without an atmosphere by about
50 degrees Celsius.