Physics 5 The Universe with Prof. D. Tytler
ANSWERS to Homework 2
The key here is the last sentence. This Q is about phases in general. Io is nearly identical to our Moon. This Q is amongst the best ways of checking whether you understand the concept of phases. The answer should be immediately obvious once you understand phases.
These diagrams should look just like diagrams for our moon & it’s phases
(see text fig. 3-3), except for the labels and the times.
Io’s period is only 1.77 days. So, the time between each of the quarter phases (1st, full, 3rd, new) is about 0.45 Earth days.
This question is about the definition of the DAY and MONTH. Two types of both day and month: sidereal & synodic.
The former is measured an Earth rotation with respect to the stars, the latter a rotation with respect to the Sun. For the month a lunar revolution is the key motion. See text box 2-4 and fig. 3-5. Know which is longer, and why. You’re really doing well if you can calculate the time difference between them, but this is beyond what is required in this class.
Name them.
These are the solar and lunar eclipse, illustrated in your text in figs. 3-8 and 3-12.
They are not seen monthly due to the inclination of our moon’s orbit; see text p57.
Solar eclipses occur more often, but since the area of Earth able to witness the eclipse is small, fewer see it. Lunar eclipses occur less often, but half the globe can see them (weather permitting). See text pg. 60-62. Sketches must explain this situation, and no single one in text does alone – there is a need to synthesize.
There is, of course, no single way to do this. If you followed the above criteria and demonstrated understanding of what you wrote you should do well.
Page 4 of your text has the definitions in hard-to-miss boldface. Copying them verbatim is acceptable, provided you say that you copied, but you must explain the difference in your own words.
Also easily found on pg 4.