See the answer on the
NASA Goddard Space Flight Center
`Imagine the Universe!' web page.
The easiest way to solve these problems is to draw pictures
of the Sun, Moon, and Earth, and a person on the Earth.
The trick is
to remember that people are really tiny compared
to the Earth, so can't see over their horizon
(a line tangent to the Earth where they are located),
and that the Sun and Moon are *really* far away from the
Earth, compared to the size of the Earth--essentially
at infinity (so parallel
lines intersect at the Sun or Moon). Also, remember
that sunset (i.e., about 6 PM) occurs when the location of
the viewer is turning away from the Sun, and the Sun is
on the observer's horizon.
This is easiest to explain with a picture:
s o- m
Imagine the "o" is the Earth, the "s" is the Sun, the "m"
is the Moon, and the "-" is a person
on the Earth. The person is on the opposite side of
the Earth from the Sun, so it is midnight
for the person.
The Moon is also opposite the Sun, so it is a full moon.
The Moon is directly above the person, so the Moon is
on the meridian for that person at midnight.
Here's another drawing:
|
This is still the full moon.
Looking down on the north pole, the Earth is spinning counterclockwise.
For this person, the Sun is on the eastern horizon (i.e., the person
is turning towards the Sun, that is, the Sun is rising). (remember,
the person can't see past his/her horizon, which is tangent to
its location on the Earth, and parallel lines intersect at infinity).
Here's the same drawing with the horizon marked, as well as parallel
lines going to the Sun and Moon:
The Sun is on the horizon for the observer, and the person is
turning towards the Sun, so it is 6 AM for this person.
The person is turning away from the moon, and the moon
is on the horizon. This means the moon is setting. So a full moon
sets at 6 AM.
Here's another drawing:
m
In this case, we see half the face of the Moon (i.e., its a quarter
Moon).
Looking down on the North Pole, not only is the Earth spinning
counterclockwise, but the Moon is orbiting the Earth counterclockwise.
So the Moon is getting closer to the Sun. So its a waning Moon,
or 3rd quarter.
Like in the last picture, it is 6 AM for the person, so at 6 AM
a 3rd quarter Moon is directly above the person.
Here's another picture:
m
Again, it is 3rd quarter, but now the person is on the side
of the Earth facing the Sun, that is, it is noon. The Earth is
spinning counterclockwise, so the person is moving away
from the Moon. The moon is on the horizon for that person,
i.e., it is setting. So a third quarter moon sets at noon.
lambdamax(A) prop to 1/T(A)
lambdamax(B) prop to 1/T(B)
Then divide the two equations. When you divide two proportionalities,
you can change the proportional signs to an equal sign:
lambdamax(A)/lambdamax(B)
= 1/T(A)/1/T(B)
You are dividing two fractions. To simplify, flip over the
bottom fraction and multiply:
lambdamax(A)/lambdamax(B)
= 1/T(A) * T(B)/1 = T(B)/T(A)
Then plug in the numbers. For question 12,
the numbers are: T(A) = 3000K and T(B) = 12,000K:
lambdamax(A)/lambdamax(B) = 12,000K/3,000K = 4.
Then write in the final form:
lambdamax(A) = 4 lambdamax(B)
This is option c).
Last updated 11/30/07
Students are NOT permitted to attend
a different lab section. If you miss a lab, you can make it up
by either: 1) doing one of the take-home labs,
2) attending the 11th meeting of your regularly-scheduled lab period.
Since only 10 labs are required for full credit, the 11th lab can be
used as a make-up or as extra credit,
NOTE THAT THE MAXIMUM NUMBER OF LABS A STUDENT
CAN DO DURING THE SEMESTER IS 12; if a student has attended
all 11 regular evening labs, they cannot do both take-home
labs for extra credit.
Before the final exam, I will email everyone the grade they
will get in the course
IF THEY DO NOT TAKE THE FINAL.
Note that if you have missed a quiz, a zero will be averaged into
your pre-final grade, thus your pre-final grade does not
necessarily represent the grade you will get in the class
if you take the exam.
Remember that the final exam is worth two quizzes. The grade on
the final can be used to replace your two lowest quiz grades,
or can be used as a make-up if you have missed 1 or 2 quizzes.
If you have taken all 6 quizzes, you do not have to take the
final unless you want to improve your grade. If you do not
have an A in the course before the final, I strongly advise you
to take the final. Taking the final cannot hurt your grade;
it can just help. If you have a pre-final grade of a C and do worse on
the final than your two lowest quizzes, your course grade will be a C.
s o m
horizon--------|-------------
s -----------o------------- m
|
s o
s -o
See the description
of Celestial Coordinates
here.
This is a comparison problem, involving two objects.
The equation you use is Wien's Law, lambdamax is proportional to 1/T.
To solve these kinds of problems, write down the equation twice, once
for each object:
See the
pictures of Venus from
the Magellanic satellite.