Magnitude of displacement vector

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Homework Help Overview

The problem involves calculating the magnitude of the displacement vector for the Earth's position as it orbits the Sun over a year, specifically at intervals of 3, 6, 9, and 12 months. The context is circular motion with a defined radius.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the geometric representation of the Earth's orbit and the calculation of displacement vectors at specified time intervals. There is a question about the correct method to calculate the magnitude of the displacement vector, particularly for the 3-month and 6-month intervals.

Discussion Status

Some participants have provided guidance on visualizing the problem and calculating the displacement vectors. There is an ongoing exploration of how to compute the magnitudes for different time intervals, with participants confirming each other's approaches.

Contextual Notes

The original poster expresses confusion regarding the calculation of the displacement vector's magnitude, indicating a potential gap in understanding the geometric interpretation of the problem. There is also a reference to a friend's incorrect explanation of the diagram's shape.

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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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