Astronomy Lesson
Plan
Name:
Leah Coutorie
Title of lesson: Using a Dobsonian
Telescope to find Proportions
Date of lesson: March 23, 2005
Length of lesson: 1 ½ hours
Description of the class:
Name
of course: Algebra I
Grade
level: 9th grade
Honors
or regular: regular
Source of the lesson:
Optics
seminars with Eric Hooper.
TEKS addressed:
¤111.32. Algebra I (One Credit).
(a) Basic understandings.
(1) Foundation concepts for
high school mathematics. As presented in Grades K-8, the basic understandings
of number, operation, and quantitative reasoning; patterns, relationships, and
algebraic thinking; geometry; measurement; and probability and statistics are
essential foundations for all work in high school mathematics. Students will continue
to build on this foundation as they expand their understanding through other
mathematical experiences.
(2) Algebraic thinking and
symbolic reasoning. Symbolic reasoning plays a critical role in algebra;
symbols provide powerful ways to represent mathematical situations and to
express generalizations. Students use symbols in a variety of ways to study
relationships among quantities.
(3) Function concepts.
Functions represent the systematic dependence of one quantity on another.
Students use functions to represent and model problem situations and to analyze
and interpret relationships.
(4) Relationship between
equations and functions. Equations arise as a way of asking and answering
questions involving functional relationships. Students work in many situations
to set up equations and use a variety of methods to solve these equations.
(5) Tools for algebraic
thinking. Techniques for working with functions and equations are essential in
understanding underlying relationships. Students use a variety of representations
(concrete, numerical, algorithmic, graphical), tools, and technology,
including, but not limited to, powerful and accessible hand-held calculators
and computers with graphing capabilities and model mathematical situations to
solve meaningful problems.
(6) Underlying mathematical
processes. Many processes underlie all content areas in mathematics. As they do
mathematics, students continually use problem-solving, computation in
problem-solving contexts, language and communication, connections within and
outside mathematics, and reasoning, as well as multiple representations,
applications and modeling, and justification and proof.
(b) Foundations for
functions: knowledge and skills and performance descriptions.
(1) The student understands
that a function represents a dependence of one quantity on another and can be
described in a variety of ways. Following are performance descriptions.
(B) The student gathers
and records data, or uses data sets, to determine functional (systematic)
relationships between quantities.
(C) The student describes
functional relationships for given problem situations and writes equations or
inequalities to answer questions arising from the situations.
(D) The student
represents relationships among quantities using concrete models, tables,
graphs, diagrams, verbal descriptions, equations, and inequalities.
(E) The student
interprets and makes inferences from functional relationships.
(3) The student understands
how algebra can be used to express generalizations and recognizes and uses the
power of symbols to represent situations. Following are performance
descriptions.
(A) The student uses
symbols to represent unknowns and variables.
I. Overview
This lesson will teach
students to use a Dobsonian telescope indoors in order to find angle of view. They will work with measuring lengths
and solving for angles to find the field of view. By using the telescopes, the students will be able to make
real world connections and use math in real world contexts.
II. Performance or learner outcomes
Students
will be able to:
Measure
various distances
Solve
for angle of view
Measure
field of view
III. Resources, materials and supplies needed
1
Dobsonian telescope per group
1
meter stick per group
IV. Supplementary materials, handouts.
Wrap-up Handout
Five-E Organization
Teacher
Does Probing
Questions
Student Does
Engage: IÕll explain that
everything we see is in our field of view, which depends on the angle of
view. I will ask them various
questions about these ambiguous terms and call on them as they raise their
hands and listen to them as they call out answers. |
1. What do you think our field of view
is? 2. Then what is the angle of view? 3. When you look at something up close,
do you think the angle of view is smaller or larger than if you look at it
far away? Why? |
1. Everything we can see, everything
that fits in the horizontal distance in which we can see 2. The angle at which sight eaves our
eye, this angle (making motions with their arms and hands going from their
eyes) 3. The angle gets smaller as the thing
moves further away. This is
because if something is really close to you it looks wider and so the angle
of view gets wider. |
Explore: I will have the students explore this idea by
finding the angle of view when looking at their own thumb at armÕs
length. They will be put into
groups (as many as we have telescopes) to try to answer the question of how
to find this angle. |
1. How will you go about solving for the
angle? 2. What did you get for these
measurements? What did you get
for the angle? |
1. Do something with equilateral
triangles. Make measurements of
the distance from eye to thumb and width of thumb. 2. Answers will vary. |
Explain: At this point, I will
either choose a group that figured out what to do to present their finding,
or explain to them myself how to find this angle. |
1. How do you find this angle? 2. How do you put that measurement in
degrees? 3. Does this seem about accurate? Why? |
1. (theta) = (width of field of view) /
focal length) in radians. 2. Multiply it by 360. 3. ES, because it is a pretty small
angle and it seems like the angle of view would be pretty small. |
Extend / Elaborate: After the formula has been
established, I will have them stay in their groups to work with the
telescopes. They will go in the
hallway and use the telescopes to find the field of view and measure the focal
length to find the angle of view. |
1. How will you find the field of view? 2. Where will you measure the focal
length from and to? 3. How will you find the angle of view? |
1. Have someone stand in a designated
spot holding a meter stick and have each other person in the group look
through the eyepiece and see how many centimeters across of the meter stick
they can see. Have multiple
people look and take the average just in case there are discrepancies over
how much they can see. 2. From about where the primary mirror
is in the telescope to the designated spot. 3. Divide the field of view by the focal
length to get the angle in radians and then convert it into degrees so that
it will make more sense to them. |
Evaluate: After they have completed
this exercise, if there is time I will have them answer a few questions as a
group and then we will discuss the answers as a class. If thereÕs not enough time for that,
I will quickly call on people to answer the questions. |
1. What did you do when using the
telescope? 2. How did you find the field of view? 3. What was your answer for the angle of
view? Show your work. 4. How did the thumb measurements relate
to what we found using the telescopes? |
1. Make the telescope about parallel to
the ground, move the eyepiece up and down to focus. 2. [A variation of the answer above.] 3. Show use of formula to find theta and
then convert to degrees. Answers
will vary depending on their different focal lengths. 4. The thumb example was what we did
with the telescopes on a smaller scale. |