Summertime means it's time to play ball! But what would it be like to play ball on various locations across our Solar System?
Planetary scientist Dr. James O'Donoghue has put together a fun animation of how quickly an object falls on to the surfaces of places like the Sun, Earth, Ceres, Jupiter, the Moon, and Pluto.
The animation shows a ball dropping from 1 kilometer (0.6 miles) to the surface of each object, assuming no air resistance. You can compare, for example, that it takes 2.7 seconds for a ball to drop that distance on the Sun, while it takes 14.3 seconds Earth.
"This should give an idea for the pull you would feel on each object," O'Donoghue said.
But what about the pull of gravity on the big planets vs. Earth? Interestingly enough, it takes and 13.8 seconds for the ball to drop on Saturn, and 15 seconds on Uranus.
"It might be surprising to see large planets have a pull comparable to smaller ones at the surface," O'Donoghue explains on YouTube.
"For example Uranus pulls the ball down slower than at Earth! Why? Because the low average density of Uranus puts the surface far away from the majority of the mass. Similarly, Mars is nearly twice the mass of Mercury, but you can see the surface gravity is actually the same… this indicates that Mercury is much denser than Mars."
Ceres comes in at the pokiest place to play ball, with a ball dropping 1 km (0.6 miles) in 84.3 seconds.
O'Donoghue, along with input from astronomer Rami Mandow, used a NASA planetary fact sheet for reference to create the video.
O'Donoghue also referenced one of the most famous gravity experiments ever conducted, the one by astronaut Dave Scott on the Moon:
If you drop a feather and a hammer on the Moon from the same height at the same time, both land simultaneously. This is because without significant air resistance, all objects fall at the same rate (regardless of mass)
🔊 Apollo 15 Commander David Scott pic.twitter.com/wC6dg8QgdL
— Dr. James O'Donoghue (@physicsJ) July 11, 2021
O'Donoghue has a number of great videos on his YouTube channel, including a visualization of the velocities required to escape the pull of gravity from various bodies in the Solar System.
This article was originally published by Universe Today. Read the original article.
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