Understanding Our Universe
Understanding Our Universe
3rd Edition
ISBN: 9780393614428
Author: PALEN, Stacy, Kay, Laura, Blumenthal, George (george Ray)
Publisher: W.w. Norton & Company,
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Chapter 5.4, Problem 5.4CYU
To determine

The reason for the absence of the water ice at the distance of the orbit of Mars.

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We think the terrestrial planets formed around solid “seeds” that later grew over time through the accretion of rocks and metals. a)  Suppose the Earth grew to its present size in 1 million years through the accretion of particles averaging 100 grams each. On average, how many particles did the Earth capture per second, given that the mass of the Earth is = 5.972 × 10 ^24 kg ? b)  If you stood on Earth during its formation and watched a region covering 100 m^2, how many impacts would you expect to see in one hour. Use the impact rate you calculated in part a. You’ll need the following as well: the radius of the Earth is = 6.371 × 10 ^6 m and the surface area of the Earth is 4??^2Earth
What is the range of density for the outer planets (in g/cm3)? 1.2 to 5.5 2.2 to 5.5 2.2 to 6.5 3.3 to 7.2 none of these
The table to the right gives size and distance data for the planets at a certain point in time. Calculate the scaled size and distance for each planet using a 1 to 10 billion scale model solar system. Planet Diameter Distance from Sun Mercury 4880 km   65.1 million km   Venus 12,100 km   108.8 million km   Earth 12,760 km   147.5 million km   Mars 6790 km   244.6 million km   Jupiter 143,000 km   807.2 million km   Saturn 120,000 km   1406 million km   Uranus 52,000 km   2938 million km   Neptune 48,400 km   4508 million km
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