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The Force Exerted on the Moon In FIGURE $5-37$ we show the Earth,Moon, and Sun (not to scale) in their relative positions at thetime when the Moon is in its third-quarter phase. Though fewpeople realize it, the force exerted on the Moon by the Sun isactually greater than the force exerted on the Moon by theEarth. In fact, the force exerted on the Moon by the Sun has a magnitude of $F_{\mathrm{sM}}=4.34 \times 10^{20} \mathrm{N},$ whereas the force exerted bythe Earth has a magnitude of only $F_{\mathrm{EM}}=1.98 \times 10^{20} \mathrm{N}$ . Theseforces are indicated to scale in Figure $5-37 .$ Find (a) the directionand (b) the magnitude of the net force acting on the Moon.(c) Given that the mass of the Moon is $M_{M}=7.35 \times 10^{22} \mathrm{kg}$ ,find the magnitude of its acceleration at the time of the third-quarter phase.

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$24.5^{\circ}$$4.77 \times 10^{20} \mathrm{N}$0.00649 $\mathrm{m} / \mathrm{s}^{2}$

Physics 101 Mechanics

Chapter 5

Newton's Laws of Motion

University of Michigan - Ann Arbor

Hope College

University of Winnipeg

Lectures

03:28

Newton's Laws of Motion are three physical laws that, laid the foundation for classical mechanics. They describe the relationship between a body and the forces acting upon it, and its motion in response to those forces. These three laws have been expressed in several ways, over nearly three centuries, and can be summarised as follows: In his 1687 "Philosophiæ Naturalis Principia Mathematica" ("Mathematical Principles of Natural Philosophy"), Isaac Newton set out three laws of motion. The first law defines the force F, the second law defines the mass m, and the third law defines the acceleration a. The first law states that if the net force acting upon a body is zero, its velocity will not change; the second law states that the acceleration of a body is proportional to the net force acting upon it, and the third law states that for every action there is an equal and opposite reaction.

09:37

Isaac Newton (4 January 1643 – 31 March 1727) was an English mathematician, physicist, astronomer, theologian, and author (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time and a key figure in the scientific revolution. His book Philosophiæ Naturalis Principia Mathematica ("Mathematical Principles of Natural Philosophy"), first published in 1687, laid the foundations of classical mechanics. Newton also made seminal contributions to optics, and he shares credit with Gottfried Wilhelm Leibniz for developing the infinitesimal calculus.

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The Force Exerted on the M…

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E; The Force Exerted on th…

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Force on the Moon due to S…

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When the Moon is directly …

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Cravitational Fields The M…

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Calculate the magnitude an…

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(II) Find the net force on…

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The drawing (not to scale)…

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The Moon, whose mass is $7…

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When the Earth, Moon, and …

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Okay, So for this problem, we're giving different vectors of force as it pertains to moon, To the earth and moon to the sun were us to find the direction in the magnitude of the net force acting on the moon between parts and be now to find our I'm going to start with part B where we're finding our net force. Because then I can also use that along with some triggered trigonometry, to find the angle off our direction. So starting with part B, I'm just gonna use notice here. We have a right triangle, so I can just use Pythagorean theorem to soften this. So let's just call this side. C C. Squared equals 1.98 times 10 of 20 news squared, plus my poor point 34 times 10 to the 20 news squared. So once you plug that into a calculator and you ah, use algebra to solve for C, we come out Teoh an answer of four point for hope for for 4.77 times 10 to the 20 Newtons. So that is the answer to party. This is our net force that is acting on the moon. So for part A. You just write this up here for C 4.77 We rounded to the hundreds place because we have three significant figures that we're looking at here. Okay, so I need to figure out the angle along this my here because we always want to find it according to a horizontal. So if I were to draw it out like this, I'm going to take all right, the co sign and it's called Angle Theta, and it's gonna be our near side. So we're gonna be doing this side here, which just happens to be the same as 4.34 times 10 to the 10 to the 20th Power. So we have 4.34 times 10 or 20 divided by what we just found, which was 4.77 Because we always do by the hypotheses. Now, once you divide these numbers and take the coast sine inverse of both sides using your calculator, we're finding that it's gonna be a angle of about 24.5 degrees, and that's just straight out of trigonometry. That's where that angle comes from. So this angle here, this is our data and That's the direction that the moon is going. Okay. Now, for the last part, it's asking that given that the mass of the moon is equal to 7.35 times 10 of the 22 kilograms we need to find the magnitude of its acceleration at the time of the third quarter fits. So given our mass here, we also need to remember that our equation for force mass and acceleration is force equals mass times acceleration. Now, we just found that Arnett, Matt or our net force is 4.77 times 10 to the 20 news, and that is equal to our mass of 7.35 times 10 to 22 kilograms. And we're solving for acceleration. So using algebra, just a viable sides by the 7.35 times 10 of the 22 that cancels out the kilograms in the Newton's. So we're left with nothing but meters per second squared. So that works out and we're going to get an answer off 0.649 And we rounded to this place because we have three significant figures. Three here, three here. So we have to have three here. And don't forget our units, and that's how you solve it.

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