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Martha Vasquez
Beatriz Sarabia
Alma Vaca
Heidi Miedecke
Geography 300
February 28, 2013
Lesson Plan 5

                             Lesson Title/Focus: Measuring the Earth

      6th Grade


      Math GLEs:
      1.3.1 Make and test conjectures about two-dimensional and three-dimensional shapes and
      their individual attributes and relationships using physical, symbolic and technological
      models.

          5.2.2. Recognize the mathematical contribution of a person or culture.

    NETS-S:
      3.b. Students will use the Internet to find map sites. They need to look up Alexandria,
      Egypt, and Scene (currently called Aswan) to see where these cities are located. The
      students will also locate the cooperating school by the Internet map and evaluate its
      distance from their location.

    3.d. After collect all values, students use calculators to process data and evaluate problems.

    Science GLEs:
        1.2.5. Understand that the Solar System is in a galaxy in a universe composed of an
        immense number of stars and other celestial bodies.

             3.2.1. Analyze how scientific knowledge and technological advances discovered
             and developed by individuals and communities in all cultures of the world
             contribute to changes in societies.


      2. Input: Benjamin Peirce said mathematics is the science that draws necessary
      conclusions. To study science, people have to learn math first. This lesson is guiding
      students to experience the method that the ancient Greek mathematicians used to estimate
      circumference of the Earth by limited tools and math knowledge.

      3. Instructional Materials Needed: Calculators, papers, pencils, computers with
      Internet, and a meter stick.

      4. Lesson Objective (Learning Targets)
Teacher: I will ensure that the students can calculate volume, circumference, and surface
    area of a sphere.

    I will ensure that the students can read maps and discuss planets.

Students: Students will be able to calculate various measurement of the Earth.

  Students will be able determine distances on a map.

 5. Grouping Students for Instruction: Students will work in small groups of at least
 three.

 6. LEARNING EXPERIENCES:

 Engage

     Eratosthenes, a Greek mathematician, was the first to measure the circumference of
     the earth. He based his measurement of the earth on the assumptions that the earth
     was round and the sun’s rays are parallel. This is interesting since the Italians refuted
     his claim that the earth was round about 1000 years later. He knew that at noon on the
     day of the summer solstice in Alexandrian, Egypt, a vertical post casts a shadow. At
     the same time in Scene, a town directly to the south, a vertical post casts no shadow.
     Eratosthenes used Euclidean geometry to determine that the angle formed by the
     shadow and an imaginary line from the end of the shadow to the top of the post
     equals and angle at the earth’s center formed by imaginary lines from the two towns.
     He calculated the earth’s circumference by measuring the distance between
     Alexandria and Scene, and multiplying it by the number of times the angle at the
     earth’s center is contained in 360 degrees.

    Explore

    The students will use the Internet to find map sites. They will look up Alexandria,
    Egypt, and Scene (currently called Aswan) to see where these cities are located.

    The students should also locate a cooperating school on a map and evaluate its
    distance from their location. Students may need to measure the tangent, as this
    concept will be used in the calculation. If the students have not yet learned this
    concept the instructor will do this portion of the calculation or bring in some pare
    calculus students to work with the groups. This experience will show the students of
    how math will be applied in upper level classes. Students will need to practice the
    activity prior to the actual experiment. The measurements will need to be done at both
    schools at noon at the same date. They should measure the height of a stick and the
    length of its shadow. Students should be asked prior to the experiment to conjecture
    about the circumference, volume, surface area and radius of the earth.

  Explain
The measure of the angle is found by dividing the length of the shadow by the height
   of the object, which would be the tangent of the angle you will be using for this
   experiment. The angle measure can then be determined. This is not the central angle.
   The angle from the other school must be subtracted from this angle measure and the
   absolute value of this difference is the central angle. The circumference of the earth
   can then be calculated by setting up a ratio and solving for the circumference.




Elaborate

   Once the students have solved the circumference, they can then use the equation 2eπr
   to find the radius. The students could then use the radius to find the volume and
   surface area of the earth. Students should research these measurements to determine
   the accuracy of their calculations.
Evaluate

            Students would write a short paper about their experiment and the accuracy of their
            calculations. This paper would then be graded on the use of proper vocabulary and
            the correct use of the equations. Students should be encouraged to include any
            conjectures they made during the experiment and whether they were validated or not.

       Checking for Understanding/Questions:


            What do you think the circumference, volume, surface area, and radius of the earth
            are?

                   How do we calculate each of these measurements?

                   Why do you suppose this math was lost to later civilizations after
            Eratosthenes discovered it?

                   What other applications are there for these measures?

       Closure:

Aristarchus used similar triangles to create a relationship between the radius of the Sun and Earth
and the diameter of the Moon to the distances between these objects. Once Eratosthenes
discovered this method for calculating the circumference of the earth the radius was then
calculated and could be plugged into the equations to determine our distance from the Sun and
Moon. Math and science have evolved this way with conjectures that are later proved and used in
ways the person who discovered the technique had not imagined. Being able to read a map and
determine distances is useful in many situations. You have discovered with this experiment how
this information can be used to calculate volume, surface area, and circumference.

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Lesson5

  • 1. Martha Vasquez Beatriz Sarabia Alma Vaca Heidi Miedecke Geography 300 February 28, 2013 Lesson Plan 5 Lesson Title/Focus: Measuring the Earth 6th Grade Math GLEs: 1.3.1 Make and test conjectures about two-dimensional and three-dimensional shapes and their individual attributes and relationships using physical, symbolic and technological models. 5.2.2. Recognize the mathematical contribution of a person or culture. NETS-S: 3.b. Students will use the Internet to find map sites. They need to look up Alexandria, Egypt, and Scene (currently called Aswan) to see where these cities are located. The students will also locate the cooperating school by the Internet map and evaluate its distance from their location. 3.d. After collect all values, students use calculators to process data and evaluate problems. Science GLEs: 1.2.5. Understand that the Solar System is in a galaxy in a universe composed of an immense number of stars and other celestial bodies. 3.2.1. Analyze how scientific knowledge and technological advances discovered and developed by individuals and communities in all cultures of the world contribute to changes in societies. 2. Input: Benjamin Peirce said mathematics is the science that draws necessary conclusions. To study science, people have to learn math first. This lesson is guiding students to experience the method that the ancient Greek mathematicians used to estimate circumference of the Earth by limited tools and math knowledge. 3. Instructional Materials Needed: Calculators, papers, pencils, computers with Internet, and a meter stick. 4. Lesson Objective (Learning Targets)
  • 2. Teacher: I will ensure that the students can calculate volume, circumference, and surface area of a sphere. I will ensure that the students can read maps and discuss planets. Students: Students will be able to calculate various measurement of the Earth. Students will be able determine distances on a map. 5. Grouping Students for Instruction: Students will work in small groups of at least three. 6. LEARNING EXPERIENCES: Engage Eratosthenes, a Greek mathematician, was the first to measure the circumference of the earth. He based his measurement of the earth on the assumptions that the earth was round and the sun’s rays are parallel. This is interesting since the Italians refuted his claim that the earth was round about 1000 years later. He knew that at noon on the day of the summer solstice in Alexandrian, Egypt, a vertical post casts a shadow. At the same time in Scene, a town directly to the south, a vertical post casts no shadow. Eratosthenes used Euclidean geometry to determine that the angle formed by the shadow and an imaginary line from the end of the shadow to the top of the post equals and angle at the earth’s center formed by imaginary lines from the two towns. He calculated the earth’s circumference by measuring the distance between Alexandria and Scene, and multiplying it by the number of times the angle at the earth’s center is contained in 360 degrees. Explore The students will use the Internet to find map sites. They will look up Alexandria, Egypt, and Scene (currently called Aswan) to see where these cities are located. The students should also locate a cooperating school on a map and evaluate its distance from their location. Students may need to measure the tangent, as this concept will be used in the calculation. If the students have not yet learned this concept the instructor will do this portion of the calculation or bring in some pare calculus students to work with the groups. This experience will show the students of how math will be applied in upper level classes. Students will need to practice the activity prior to the actual experiment. The measurements will need to be done at both schools at noon at the same date. They should measure the height of a stick and the length of its shadow. Students should be asked prior to the experiment to conjecture about the circumference, volume, surface area and radius of the earth. Explain
  • 3. The measure of the angle is found by dividing the length of the shadow by the height of the object, which would be the tangent of the angle you will be using for this experiment. The angle measure can then be determined. This is not the central angle. The angle from the other school must be subtracted from this angle measure and the absolute value of this difference is the central angle. The circumference of the earth can then be calculated by setting up a ratio and solving for the circumference. Elaborate Once the students have solved the circumference, they can then use the equation 2eπr to find the radius. The students could then use the radius to find the volume and surface area of the earth. Students should research these measurements to determine the accuracy of their calculations.
  • 4. Evaluate Students would write a short paper about their experiment and the accuracy of their calculations. This paper would then be graded on the use of proper vocabulary and the correct use of the equations. Students should be encouraged to include any conjectures they made during the experiment and whether they were validated or not. Checking for Understanding/Questions: What do you think the circumference, volume, surface area, and radius of the earth are? How do we calculate each of these measurements? Why do you suppose this math was lost to later civilizations after Eratosthenes discovered it? What other applications are there for these measures? Closure: Aristarchus used similar triangles to create a relationship between the radius of the Sun and Earth and the diameter of the Moon to the distances between these objects. Once Eratosthenes discovered this method for calculating the circumference of the earth the radius was then calculated and could be plugged into the equations to determine our distance from the Sun and Moon. Math and science have evolved this way with conjectures that are later proved and used in ways the person who discovered the technique had not imagined. Being able to read a map and determine distances is useful in many situations. You have discovered with this experiment how this information can be used to calculate volume, surface area, and circumference.