Using planetary motion, prove that the planet always being bound to the attracting solar center and never escapes from it
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Using planetary motion, prove that the planet always being bound to the attracting solar center and never escapes from it. (need proper math equation and big answer)
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- Question #13 (attached) using the solution template (also attached)2Read Revolution and Chang X E Unthled document-Google Docs X Apex Leaming - Courses .com/public/activity/3003002/assessment Zearn Math: A Com. G Google Redirecting... M Mail G Images Wrigley.com :: Or L 3.3.2 Test (CST): Forces Question 2 of 14 Which of the four fundamental forces acts over very long distances but does not cause planets in the solar system to pull on each other? A. Weak nuclear B. Electromagnetic C. Strong nuclear D. Gravitational SUBMIT + PREVIOUSPlease solve and show solution. Please include ILLUSTRATION TOO. Thanks
- 4) Science fiction movies often portray asteroid belts as crowded, dense regions that require spaceships to maneuver quickly to get through them. In this problem, we will calculate the fraction of volume in an asteroid belt that is actually occupied by asteroids. a) If there are 300,000 large asteroids between 2 and 3 AU from the Sun, and each asteroid is assumed to be spherical with a radius of 100 km, determine the total volume occupied by asteroids in this region. Recall that the volume of a sphere is given by the equation V = 4TR³ /3. b) Let's assume the region in which these asteroids orbit is an annulus with an inner radius of 2 AU, an outer radius of 3 AU, and a thickness of 2Ro. Determine the volume of this region. Recall that the area of a circle is given by the equation A = TR². Here are two conversions that you'll need: 1 AU = 1.496 × 108 km and 1 Ro = 6.955 × 105 km. c) What is the ratio of the volume occupied by asteroids to the volume of the asteroid belt (i.e., the…As a consequence of conservation of ............., the 2nd Law of Planetary Motion also implies that a planet will move ............ when farther away from its host star.Explain why a massive, cool planet is more likely to have a thick atmosphere than is a less massive, hot planet.
- Derive the of the time period of rerolution T ot the satellite around the plant. State clearly the assumptions Jou have taken calculate this expression.wether this formela is applícable for jupiter? Give a expression to reason for r your aunswer.Scale 0.7707346 AU Period= 2.41495 Years Kepler's Laws: Using the orbit shown below and a ruler, measure the scale bar in the top left corner in centimeters. The length of the bar is equal to the distance in AU shown below the bar. Measure the aphelion and perihelion distance of the orbit inPlease help