DESCRIBE THE SOLAR SYSTEM
Q: Calculate the Sun's orbital period.
A: Sun is part of the Milkyway galaxy and follows an orbit around the center of the galaxy. Sun is…
Q: 110. Which graph best represents the relationship between the mass of an object and its distance…
A: For an object as big as a planet, the distance considered in the inverse square law must be measured…
Q: Match Kepler Laws with the correct description. * Kepler's First Law Kepler's Second Law…
A: Given:-matching statements of keplers law
Q: Like many other space objects, Earth travels in a predictable path through space. Which of the…
A: Like many other objects. Earth travels in a predictable path through space. -(b) The Earth is…
Q: How is Kepler's law different from Newton's law of motion
A: Newton’s law describe every motion you will ever experience. You can use them to calculate anything…
Q: The moon's Prometheus and Pandora orbit Saturn at 139,350 and 141,700kilometers. 1) Use Newton's…
A: 1) According to kepler third law, time period is given as,T=4π2 r3GMWhere G=Universal gravitaional…
Q: Which space station was the first to involve several countries working together?
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Q: Select all of the following that describe an AU. OThe average distance between Earth and our Sun…
A: Astronomical unit is a unit of distance commonly known as AU.
Q: Find the mass of the earth, given that g = 9.29 m/s and radius of earth is 6,378,0002, and G has…
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Q: The proves that the Earth revolves around the Sun. All of these prove the Earth revolves around the…
A: This problem can be answered by having basic knowledge about the terms given in the options. In the…
Q: What is the sun's mass?
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Q: The radius of the Earth's orbit is 1.50 1011 m and that of Mars is 2.28 1011 m. The star that this…
A: The expression for the orbital period,
Q: 2. On August 27, 2003, the planet Mars was at a distance of 0.373 AU from Earth. The diameter of…
A: The final answer is attached below Explanation:
Q: 4) Asteroid A and asteroid B come to a distance of 3,210 km from each other. Calculate the…
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Q: In Kepler's laws, the focus of the ellipse is an important point. What color in this diagram is the…
A: In the given figure, we have to discuss the color of focus of elliptical trajectory of planet…
Q: Our solar system is approximately 10 billion km across. This diameter can be also be expressed as:…
A: Diameter of our solar systemD= 10 billion km
Q: A particle of mass m that is confined in a one-dimensional box of length L, i.e. x € (0, L), is…
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Q: 9.) Find the time it takes Saturn to orbit the sun . Show all work a.) in terms of seconds b.) in…
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Q: It is important to have an idea about the distances between and relative sizes of celestial objects…
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Q: The planet Jupiter orbits the Sun once every 12 Earth years. The Earth orbits the Sun at an average…
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Q: You have a pendulum that is 2.0 m long and has a period of 2.98 s. What planet are you on? If the…
A: The value of g is different for different planets
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- 12 Which of the following is not a characteristic of an object in our solar system that allows life to exist? F Diameter of the object G Distance from the Sun Presence of liquid water J Composition of the atmosphereDefine Tidal energy.Please use the info to answer the question. Please circle your answer.
- A planet orbits a star in a different stellar system The mass of the planet is 2 times Jupiter's mass and 5 times the distance from the star than Jupiter is from the sun How does the force of gravity change for this new system if the star is 4 Solar Mass?Astronomy help What does each number (16-20) represent? Semi-major axis Focus point Center Focus offset EccentricityDownload Edits will not be automatically saved. Save now BI U A - 三= Scientific Knowledge PLUTO To what change in scientific knowledge does the cartoon above refer? SC.6.N.2.2(SC.8.N.1.5), SC.7.N.2.1(SC.7.N.1.7) Created by: R. Hallett-Njuguna, SCPS
- f) Assume that the space station orbits the Earth with uniform circular motion. This means that the magnitude of the acceleration of the space station is given by a = v²/r. In addition, the net force on the space station is equal to m,tation*a (Newton's Second Law, as always), and the force on the space station is F = - G*m,tation*Mearth/r?. Using these equations, we can derive a formula for the speed of the space station as it orbits Earth: Fnet = m*a (towards centre of earth for uniform circular motion) Inserting Newton's Law of Universal Gravitation and the formula for centripetal acceleration, G*mstation *mearth/r² = mstation*Vstation/r, and dividing both sides by mstation and multiplying both sides by r, we get: G*marth/r = v, and finally we arrive at our formula for the speed of the station, Vstation = V(G*mearth/r), ...note that this is meant to be a square root symbol. Use this equation to calculate the approximate speed of the space station given the distance between the…I need help with physics and it's about converging and diverging , I need help with the two bullet points mentioned below the questionA Toming oom earning.com/public/activity/5000001/assessment Google Docs A aeries Pretest: Unit 5 Apex Leaming - Courses Google Slides music X Ganent fa nonton for hlegim-2 Question 8 of 32 Imagine that scientists placed a satellite at the Earth-Moon L1 Lagrangian point, which is a point between Earth and the Moon where the gravitational pulls from the two bodies are equal and opposite. What would happen if a satellite at this position drifted slightly closer to Earth? ← PREVIOUS chstv m hbo 6 library A. The satellite would continue to drift toward Earth as Earth's pull became stronger than that of the Moon. B. The gravitational pull from the Sun would eventually pull the satellite from this point and cause it to directly orbit the Sun. C. The gravitational pull from the Moon would correct the satellite and bring it back to the Lagrangian point. D. The satellite would stop drifting and would remain fixed in this position because of its tangential velocity. hip bell schedule ut