In this project, students use the Internet to gather
information on tides and then use this information to determine
the period of revolution of the moon around the earth (part 1) and
the relative pull of the sun and the moon on the tides (part
2).
Prior Knowledge
Part 1
Computing the difference between two times of day
Finding Averages
Solving proportions
Part 2 (additional)
Solving proportions involving cubes
Tasks
Part 1
Each student or partners will use the Internet to find the
local time of daily high tides over a 4 day span in 4 different
locations. They will then use the average of the daily time
differences to determine the number of degrees the moon revolves
in one day. This number will then be divided into 360° to
determine the number of days required for a complete orbit. An
alternate worksheet is provided for students who are more self
directed and can work with less structure.
Part 2
Each student or partners will use the Internet to find the
masses and distances of the sun and moon from the earth. They will
then compare the ratio of the sun to the moon in each instance and
find the ratios of the results using the formula for gravity. An
alternate worksheet is provided for students who are more self
directed and can work with less structure.
Resources
Note: If not logging on to the following sites from within
the math SCORE site, append the following before each of the URL
page names:
6. Compute the ratio of the pulls during spring and neap
tides
7. Access Tug of
War to see the cumulative effect of the sun and moon on the
tides.
Learning Advice
The Science S.C.O.R.E. site has a lesson on tides which might
serve as an introduction. This will be particularly useful for
students with no experience or knowledge of tides. A review of
finding the difference in minutes between two times and solving
proportions will also be helpful.
Depending on your class, you may want to provide fewer steps,
allowing students to explore and solve the problem on their own
without the help of the chart and step-by-step directions.
Extensions
The Alternate Worksheets contain additional questions for
explorations. Some students using the standard worksheets may be
interested in these as well:
Part 1
a). The time period we found on this worksheet is called the
synodic month. Discover what a sidereal month is.
b.)See what explanation you can find on the web to explain why
the daily differences between the time of high tide varies so
much. Since the movement of the moon around the earth is constant,
shouldn't the time difference be the same each day? Why isn't
it?
Part 2
a. Do you think the planet Mars has any effect on our
tides? Do some research and use the proportion formula in step 5
above to compute the greatest force Mars could have on the tides
compared to the force of the moon.
b. The planet Jupiter is a sea of gasses and has many
moons. The four largest are Io, Europe, Ganymede, and Callisto.
Compare the pull of the sun on Jupiter to the pull of its 4
largest moons if they were all aligned.
Evaluation
Part 1
Check that the computation of the daily differences is
correct. The theoretical daily difference should be around 54.8
minutes, however these will be different in each location and on
each day. 54.8 minutes results in a daily movement of the moon
around the earth of 13.17°, or an orbit of 27.3 days. Here
are some results for various results:
Minutes of Delay
40
45
50
55
60
Daily Degrees
10
11.25
12.5
13.75
15
Days for Orbit
36
32
28.8
26.18
24
Part 2
The ratio of the masses should be around 2.7x10^7 and the
ratio of distances around 387.1
The ratio of forces is about .465. The ratio of spring tide to
neap tide forces is about 2.74. Accuracy will differ dependent on
calculator used and the number of decimal places used for
rounding
Grade 8-12: Probability and
Statistics 3.0 Students demonstrate an
understanding of the notion of discrete random variables by
using them to solve for the probabilities of outcomes, such as the
probability of the occurrence of five heads in 14 coin tosses. 5.0 Students determine the
mean and standard deviation of a normally distributed random
variable. 6.0 Students know the
definitions of the mean, median, and mode of
distribution of data and can compute each in particular
situations. 8.0 Students organize and
describe distributions of data by using a number of different
methods, including frequency tables, histograms, standard line and
bar graphs, stem-and-leaf displays, scatterplots, and
box-and-whisker plots.
NCTM 9-12: Mathematics as Problem Solving; Mathematics
as Communication; Mathematics as Reasoning; Mathematical
Connections; Algebra; Statistics.