on Mars: Before leaving the surface of the planet aboard the shuttle, it is useful for astronauts to estimate the escape velocity. What does escape velocity mean? Calculate the escape velocity for the shuttle (mass of 6500 kg). Show your steps.
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on Mars:
Before leaving the surface of the planet aboard the shuttle, it is useful for astronauts to estimate the escape velocity.
What does escape velocity mean?
Calculate the escape velocity for the shuttle (mass of 6500 kg). Show your steps.

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- Calculate the escape velocity to an orbit of 457 km height from a planet with the radius of 2000 km and the density of 3400 kg⋅m-³. Give your answer in Sl units.What is satellites? Name and explain various types of satellites.Answer the question in full details, thank you very much, Answer on the correct significant figures: Suppose you are a space traveler, and you land on the surface of a strange new planet. As stated in yourStarfleet Manual, your first job is to measure the acceleration due to gravity, g, on this planet. You construct an"Atwood machine”, which consists of two masses connected to a pulley by a string of negligible mass, asshown in the figure. One of the masses is m1 = 54.1 kg and the other is m2 = 44.0 kg. The pulley is auniform disk of mass M = 108.0 kg and radius r = 67.0 cm; it is mounted on frictionless bearings. Whenreleased from rest, the heavier mass moves down 21.1 cm in 0.57 s, and there is no slippage of the string onthe pulley. What is the magnitude of the acceleration of the blocks, in m/s^2 What is the acceleration due to gravity gg on this planet? Give the answer in m/s^2
- Given the CRP attitude description B/N = (0.1, 0.2, 0.3) what is the equivalent DCM value? 1 1234567 # adjust the return matrix values as needed def result(): dcm = [0, 0, 0, 0, 0, 0, 0, 0, 0] return dcmDescribe your approach to calculation of the gravitational field strength on a planet with a given size (e.g. diameter) and known escape velocity. O a. Use Newton's law of universal gravitation. O b. Use Newton's 3rd law. O c. Use Newton's 1st law. O d Use Newton's 2nd law. O e. Use law of conservation of energy.a. Calculate the surface temperature of Pluto and Charon at perihelion, assuming both bodies are rapid rotators and in equilibrium with the solar radiation field. b. Calculate the escape velocity from Pluto and Charon, and compare these numbers with the velocity of N2, CH4, and H2O molecules. c. Given your answers in (a) and (b), explain qualitatively the differences in surface ice coverage for Pluto and Charon.