CHM101, Section 5, Fall
2000
Third hourly exam, Tuesday 14 November 2000
Chapters 7–9
Instructions:
Read over the entire exam first. Begin
with the questions you feel most confident about. Pace yourself so that you will
have time enough to try everything. If you don’t know how to get all the way
to an answer, go as far as you can and state how you would approach the rest.
And keep your handwriting neat! Use the back of the sheets if necessary.
Definitions (2 points each; 20
points total)
1. Photon
2. Line spectrum
3. Atomic orbital
4. Orbital angular momentum quantum number
5. Ionization energy
6. Aufbau principle
7. Transition element
8. Octet rule
9. Skeletal structure
10. Electronegativity
Short answers (4 points each; 40 points total)
c = 3.00x108 m s-1
1. Show the difference in shapes of an s orbital, a p
orbital, and a typical d orbital. Use separate XYZ plots.
2. When Neptune is 4.4 x 109 km
from the earth, how many hours does it take light from Neptune to reach us?
3. Write the abbreviated electron
configuration (1s22s22p4, etc.) for each of these elements and ions. Use the
positional rather than the sequential option.
(a) B
______________________________________
(b) K
______________________________________
(c) As
______________________________________
(d) Sc3+
____________________________________
4. Explain why atomic radii increase down
a column of the periodic table.
5. (a) Why are the properties of elements
in a transition series relatively similar to one another compared to elements in
the main groups of the periodic table?
(b) Why are the properties of the
lanthanides even more similar to one another?
6. Describe the Rutherford scattering
experiment and what conclusions it led to.
7. Why is the second ionization energy for
an element considerably larger than the first?
8. How do we know that neutrons exist?
9. Where in the periodic table do you
expect to find elements whose atoms can use expanded valence shells to bond with
more than four other atoms?
10. Explain why metals, nonmetals, and
semimetals are found in the lower left, the upper right, and intermediate
positions of the periodic table, respectively.
Problems (5 points each; 40 points total)
Planck’s constant h = 6.626x10-34 J s
1. Niels Bohr discovered that the energy of an electron around a hydrogen
atom existed only in discrete states En
= -B/n2, where n
is an integer (n = 1, 2, 3.…) and B
is a constant. Start from this equation and derive the equation for the
difference in energy between final and initial states of an electron, using nf
and ni, respectively.
2. Draw a diagram that illustrates the
aufbau principle, and show how to use it.
3. Fill in the blanks with acceptable
quantum numbers.
(a) n
= ______, l = 2, ml = 0, ms
= __________
(b) n
= 2, l = _________, ml
= -1, ms = -½
(c) n
= 4, l = _______, ml
= 2, ms = _____________
(d) n
= _______, l = 0, ml =
__________, ms = ½
4. Draw the orbital diagram (with the
boxes and the arrows) for the V atom.
5. The laser in a CD player uses light
with a wavelength of 780 nm. Calculate the energy of this radiation in joules
per photon and in kilojoules per mole of photons.
6. Use a diagram to show how the potential
energy of a system of two hydrogen atoms varies with the distance between their
nuclei. Make the distances extend from ∞ to less than the distance of the
H–H bond. Show the zones of attraction and repulsion between the atoms, and
show how to locate the length of the H–H bond on the diagram.
7. Draw the Lewis structures for (a) NH3
and (b) SeF4.
8. Draw the Lewis resonance structures for
the nitrate ion, NO3-.