The Great Red Spot is a massive, oval, ruddy spot that is prominent in photographs of Jupiter. How may this main characteristic be applied to predict the planet's rotation period?
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The Great Red Spot is a massive, oval, ruddy spot that is prominent in photographs of Jupiter.
How may this main characteristic be applied to predict the planet's rotation period?
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- Calculate the escape velocity to an orbit of 243 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. Answer: Choose...The asteroid Pallas has a mass of 2.11 x 10^20 kg and an average radius of about 2.6 km (2.56 x 10^2 km) What is the escape velocity in (m/s). (Hint: use the formula for escape velocity; remember to concert units to m, kg, & s). ________ m/s could you jump off the asteroid? -yes -noAfter Ceres was promoted to a dwarf planet, we now recognize the largest known asteroid to be Vesta, with a mass of 2.67 × 1020 kg and a diameter ranging from 578 km to 458 km. Assuming that Vesta is spherical with radius 520 km, find the approximate escape velocity from its surface.
- Calculate the weight of a 75.6 kg astronaut on the surface of Mars at the equator. See p. 273 of your textbook for Mars' mass and equatorial radius. 75 Clu m UWhy is pluto not considered a major planet? Explain.Explain why a massive, cool planet is more likely to have a thick atmosphere than is a less massive, hot planet.
- Imagine that Earth had two identical Moons, following the same orbit but staying 90° apart. What effects would this have on the ocean tides experienced on Earth?Two large asteroids start with an initial separation of r0, at which time they each exert a gravitational force on the other of strength F0. After they have fallen toward each other for a period of time, their separation has decreased to 0.38r0. At that moment, what is the strength of the new gravitational force that each asteroid feels, in terms of F0? Blank 1. Calculate the answer by read surrounding text. times F0. Express your final answer to at least 3 significant figures.Assuming a spherical shape and a uniform density of 2000 kg/m³, calculate how small an icy moon of one of the outer planets would have to be before a 40 m/s (about 90 mph) fast- ball could escape.