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184_notes:examples:week9_earth_field [2017/10/20 15:24] – [Solution] tallpaul | 184_notes:examples:week9_earth_field [2021/07/05 21:55] (current) – [Solution] schram45 | ||
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=====Using the Earth' | =====Using the Earth' | ||
- | You have spotted an unidentified flying object! Naturally, you wish to find its charge. You have a compass, a good sense of direction, and keen eyesight. You notice that it is flying due south on a course that will pass directly overhead, and it is $30 \text{ m}aboveyou,travellingat200 \text{ m/s}$. You observe the dial on your properly aligned compass as the object passes overhead. As a function of time, this is what you see: | + | You have spotted an unidentified flying object! Naturally, you wish to find its charge. You have a compass, a good sense of direction, and keen eyesight. You notice that it is flying due south on a course that will pass directly overhead, and it is $15 \text{ m}aboveyou,travellingat200 \text{ m/s}$. You observe the dial on your properly aligned compass as the object passes overhead. As a function of time, this is what you see: |
- | {{ 184_notes: | + | [{{ 184_notes: |
===Facts=== | ===Facts=== | ||
- | * We know $|\vec{B}_{\text{earth}}| = 32 \mu\text{T}$. | + | * We know $B_{\text{earth}} = 32 \mu\text{T}$. |
- | * If we align our coordinate axes, according to the represention | + | * If we align our coordinate axes according to the representation |
- | * $h = 30 \text{ m}$. | + | * $h = 15 \text{ m}$. |
* →v=−200 m/s ˆy. | * →v=−200 m/s ˆy. | ||
* You have the graph of θ versus t. | * You have the graph of θ versus t. | ||
===Lacking=== | ===Lacking=== | ||
- | * →BtextUFO | + | * $\vec{B}_{\text{UFO}}$ |
+ | * $q$ | ||
===Approximations & Assumptions=== | ===Approximations & Assumptions=== | ||
- | | + | * q, →v, h, and →Bearth are all constants: All these variable could easily be changing in this problem. However, to simplify down the model to better analyze the situation we will assume all these things are constant. This could be an accurate assumption if the UFO were cruising steadily over us at the given height. |
- | | + | |
* Your sense of direction and eyesight can be trusted. | * Your sense of direction and eyesight can be trusted. | ||
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* We represent the Biot-Savart Law for the magnetic field from a moving point charge as | * We represent the Biot-Savart Law for the magnetic field from a moving point charge as | ||
→B=μ04πq→v×→rr3 | →B=μ04πq→v×→rr3 | ||
+ | <WRAP TIP> | ||
+ | ===Approximation=== | ||
+ | We will approximate the UFO as a point charge. This may not be the most accurate assumption since the UFO is most likely a large object, but it is an approximation that must be made in order to apply our knowledge to the problem. Since the problem doesn' | ||
+ | </ | ||
* We represent the situation with the following pictures. Coordinate axes and cardinal directions are specified. | * We represent the situation with the following pictures. Coordinate axes and cardinal directions are specified. | ||
- | {{picture}} | + | |
- | {{picture}} | + | [{{ 184_notes: |
+ | |||
+ | |||
+ | |||
+ | [{{ 184_notes: | ||
====Solution==== | ====Solution==== | ||
We can find the magnetic field from the UFO based on the compass measurement. Below we show the geometric argument. | We can find the magnetic field from the UFO based on the compass measurement. Below we show the geometric argument. | ||
- | {{picture}} | + | [{{ 184_notes: |
+ | |||
+ | We know that the UFO is closest when it is directly overhead, which is also when it will have the largest contribution to the magnetic field at our observation point, resulting in the largest displacement of the compass needle. On our graph, this would be 20∘. We can also reason that the magnetic field of the UFO at our observation point will point in the +x-direction, | ||
+ | |||
+ | →BUFO=Bearthtanθˆx | ||
+ | |||
+ | Now we only have to relate the B-field from the UFO to the charge, which we'll do with the Biot-Savart law we just learned about. When the UFO is directly overhead, it should not be hard to see (pictured below) that the separation vector is →r=−hˆz and the velocity of the UFO is →v=−vˆy. Their cross product is then →v×→r=hvˆx | ||
+ | |||
+ | [{{ 184_notes: | ||
+ | |||
+ | Then plugging these into the Biot-Savart law, we can find another expression for the B-field. | ||
+ | |||
+ | →BUFO=μ04πq→v×→rr3 | ||
+ | →BUFO=μ04πqhvh3ˆx | ||
+ | |||
+ | At this point, we have two ways to express the magnetic field of the UFO, which should help us find an expression for q, the charge of the UFO. Setting these two expressions equal to one another, we find: | ||
+ | Bearthtanθˆx=μ04πqhvh3ˆx | ||
+ | |||
+ | Solving for q, we have | ||
- | We know that the UFO is closest when it is directly overhead, which is also when it will have the largest contribution to the magnetic field at our observation point, resulting in the largest displacement of the compass needle. On our graph, this would be $20^\circ.WecanalsoreasonthatthemagneticfieldoftheUFOatourobservationpointwillpointinthe+x$-direction, | + | $$q=\frac{4 \pi h^2 B_{\text{earth}} \tan \theta}{\mu_0 v} = 131 \text{ C}$$ |
- | $$\$$ | + | This is a lot of charge. Since magnetic fields are very small in magnitude, and this can be seen in the magnetic constant, it makes sense that we would need such a large amount of charge to have a noticeable effect on our compass. Uf we were to compare the magnetic field of a moving charge to the electric field from that charge, the electric field would be much larger. |