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Instructions for an exercise aimed at demonstrating the Coriolis effect, an apparent deflection of moving objects on rotating planets. The exercise involves using a turntable to draw straight lines while spinning it in different directions. Students are expected to understand the concept of the Coriolis effect and its implications for weather patterns and large-scale movements on Earth and other planets.
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EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences
Exercise Seven: Coriolis Effect
The objective of this exercise is to demonstrate that an object which moves in latitude over the sur- face of a rotating planet experiences the Coriolis effect, an apparent deflection of its path from a straight line. Upon completion of this exercise the student should understand the concept of the Coriolis effect and be able to understand viewing an event from different frames of reference.
Suggested: lazy susan type turntable (must be able to be rotated clockwise and counterclockwise), paper, tape, markers (3 colors)
The Coriolis effect is caused by an “imaginary” force but has very real effects on the weather of Earth and other planets. On Earth, which spins counterclockwise as viewed from above its north pole, objects are deflected to the right in the north- ern hemisphere and to the left in the southern hemi- sphere. This deflection is only apparent, however, as an observer watching from space would see the object’s path as a straight line. It is because we are viewing in the frame of reference of the rotating Earth that we see the apparent deflection.
This exercise demonstrates the Coriolis effect by using a rotating turntable. Students will draw straight lines while spinning the turntable in differ- ent directions. To their surprise the resultant lines
will be curves on the paper covering the turntable. This apparent deflection, the Coriolis effect, only occurs in the frame of reference of the turntable. The students, in a different frame of reference, know that the path of the marker used to draw the line was straight. On the sphere of the Earth, we occupy the same reference frame as the motion, so we “see” the Coriolis effect in action. To an outside observer, who is occupying another reference frame, there is no deflection and the motion is a straight line.
This concept has important implications for the motion of ocean currents, storms on Earth, and even missiles, but is unimportant at smaller scales. In combination with pressure effects, the Coriolis deflection gives rise to a counterclockwise rotation of large storms, such as hurricanes, in the northern hemisphere, and clockwise rotation in the southern hemisphere. This could be illustrated to students through pictures of hurricanes or other large storms found in newspapers, magazines, or elsewhere in this lab manual. Students should work in pairs, one spinning the turntable at a constant speed and the other marking the line. Instructors should note that the spinning of the Earth once a day on its axis is called rotation. Students can experiment with rotating their turntable faster or slower to see the effect on the drawn lines. A faster spin will result in greater deflection. If time or materials are a problem, this exercise can be done as a demonstration by the instructor. Vector motion of the surface of a sphere is com- plex. The magnitude of the Coriolis effect is con- trolled by rotation about the vertical axis. On Earth the vertical axis of rotation is a line connecting the geographic north and south poles. On a rotating sphere, the maximum rotation is at the poles; there is no rotation about the vertical axis at the equator. To visualize this, imagine two flat disks glued onto the surface of a sphere, one at the north pole and one at the equator. As the sphere rotates, the disk at
Suggested Correlation of Topics Air and its movements, atmospheres, circula- tion of air or sea, meteorology, ocean currents, physics: forces and mechanics, planetary rotation
1.0 hours
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Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
the north pole rotates around the vertical rotation axis of the sphere. The vertical axis of the sphere is also the axis of rotation of the disk. If viewed from above, the disk spins in one spot, just as the sphere does. The surface of the disk at the equator is paral- lel to the vertical rotation axis of the sphere. When the sphere rotates, this disk revolves around the axis. There is no spin or rotation of the disk at the equator. The magnitude of the Coriolis effect increases from the equator where it has no effect to the poles. The turntable is equivalent to the disk at the pole of the sphere, and illustrates the maximum Coriolis effect.
The Coriolis effect operates on Mars in a similar way as on Earth. Because Mars rotates at about the same rate and in the same sense as Earth, Mars has
large-scale weather systems just like on the Earth. Students might try to predict the direction that the Coriolis effect would deflect objects on Venus or Uranus, which spin clockwise as viewed from “above” (north of) the solar system. Advanced stu- dents and upper grades can answer the optional starred (*) question, which applies their observa- tions to more complex situations.
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Answer Key
Exercise Seven: Coriolis Effect
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Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
Exercise Seven: Coriolis Effect
Now spin the turntable clockwise. This is the direction that the Earth turns (or rotates), when viewed from the south pole. The turntable is modeling the southern hemisphere of the Earth. Draw a straight line across the turntable using a different colored marker, while spinning it at a constant speed. Be sure to watch that your marker follows a straight path! Label the beginning of the line you drew with an arrow pointing in the direc- tion the marker moved. Note that the line you drew is again a curve.
Examine Figure 7.1, which shows part of Mars. The bright streaks associated with some craters can be used as wind direction indicators. They are deposits of dust that can form downwind from craters.
Optional Question
*16. Why is the Coriolis “force,” which causes objects to deflect from a straight path on a rotating planet, some- times called an imaginary force?
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EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences
Exercise Seven: Coriolis Effect
Figure 7.1. Centered at 20˚, 250˚W, this mosaic is of a region on Mars called Hesperia Planum, site of much aeolian (wind) activity. Note the bright streaks associated with some of the craters; they can be used as wind direction indicators. North is to the top. Viking Orbiter mosaic 211-5478.
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