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Problem 117 Easy Difficulty

As a spacecraft approaches the planet Jupiter, it releases a probe which is to enter the planet's atmosphere at point $B$ at an altitude of $280 \mathrm{mi}$ above the surface of the planet. The trajectory of the probe is a hyperbola of eccentricity $e=1.031$. Knowing that the radius and the mass of Jupiter are $44,423 \mathrm{mi}$ and $1.30 \times 10^{26}$ slug, respectively, and that the velocity $\mathbf{v}_{B}$ of the probe at $B$ forms an angle of $82.9^{\circ}$ with the direction of $O A$, determine $(a)$ the angle $A O B,(b)$ the speed $v_{B}$ of the probe at $B$


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Newton's Laws Basics - Overview

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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Video Transcript

everyone here is giving as the spacecraft approaching the planet Jupiter Italy's approach which is to enter the planet's atmosphere at point B having that altitude. So I'll take you off. The point is to 80 might at the surface of the planet. That project Lee off the book is hyperba with eccentricity 1.0 Stephen or release of the deputies 44 What did he on my end? Moss is 130 Look, the velocity off the probe at the former ended 82 condemned with direction off or a yeah, big or a actually angle. It will be Onda. We speed up broke at me Quite you hear? Are we having developed four people Quite 4 to 3. Yeah, 10 to the power three plus 2 80 My 44 quite even the road three bon upon our culture, gm upon at square one plus eccentricity for sapyta at 0.8. Peter is zero. Really? So one upon our aid skull toe gm upon at square one. Plus I cause off you. So at the square upon GM can be written it are a into one plus Okay, at three point Victor is it'll be via calling on Get a or B. So born upon RV sculpture, GM upon 80 square cars off Peter B at the square Appall GM can build on it. Are we in tow? One plus a simplicity into cars. Off It'll be from Equation Bannon, Toe beacon, Right? Our A plus one plus a Centris City. Yeah. So from here, yes. Substituting the toe find anger. A simplicity is given 1.3 bucks are a RV 44.703 miles. Mhm. One plus yeah, 1.31 minus one toe on. Solving it, you told me, will be 14.2 nights it degree hands angle a O. B. That's all for it. Thanks for watching it.

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Video Thumbnail

03:28

Newton's Laws - Intro

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.

Video Thumbnail

09:37

Newton's Laws Basics - Overview

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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