Magnitude of displacement vector

AI Thread Summary
The discussion focuses on calculating the magnitude of the displacement vector for Earth's position around the Sun at different intervals. The Earth’s circular motion is compared to a clock hand, with specific positions at 3, 6, 9, and 12 months. The correct approach for calculating the displacement vector's magnitude involves using the Pythagorean theorem for the 3-month interval, resulting in the square root of the sum of the squares of the radius. For the 6-month interval, the displacement is simply the sum of the radius values. The conversation clarifies misconceptions about the diagram and calculation methods.
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Homework Statement


The Earth moves around the Sun in a circle of radius 1.50 X 10^11 m at approximately constant speed. Taking today's position of the Earth as origin, draw a diagram showing the position vector 3 months, 6 months, 9 months, and 12 months later. Draw the displacement vector between the 0 month and 3 month positions and calculate the magnitude of the displacement vector for this 3-month interval.


Homework Equations


x= rcos\phi
y= rsin\phi
x^2 + y^2 = r^2



The Attempt at a Solution


my friend told me that the diagram is supposed to look like the sine function and that the amplitude= 1.5 X 10^11 m, but I still don't understand how to calculate the magnitude of the displacement vector.
 
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Your friend told you wrong. The Earth goes around the Sun much like the tip of a clock hand goes around the face of the clock. If "today" the tip is at 12 o' clock (0 month position), it will be at the 3 o' clock position 3 months later, the 6 o'clock position 6 months later and so on. Can you draw the displacement vectors and calculate their magnitudes now?
 
So do I just take the square root of ((1.50 X 10^11)^2 + (1.50 X 10^11)^2) to get the magnitude of the displacement vector?
 
For 3 months, yes. What about 6 months?
 
Between the 0 month and 6 month positions would I take (1.50 X 10^11) + (1.50 X 10^11)?
 
Yup.
 
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