Finding Acceleration for Object on Equator

AI Thread Summary
An object on Earth's equator experiences acceleration in three directions: toward the center of Earth due to rotation, toward the Sun because of Earth's revolution, and toward the center of the galaxy as the Sun orbits the galactic center. To calculate these accelerations as multiples of g (9.8 m/s²), one must find the centripetal acceleration for each case. For the first two accelerations, the period and radius are essential; the Earth's radius is used for the first, while the distance to the Sun is used for the second. The centripetal acceleration can be calculated using the formula a = v²/r, where velocity is derived from the period equation T = 2(pi)r/v. Understanding these calculations simplifies the process of determining the required accelerations.
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An object lying on Earth's equator is accelerated in the following three directions.
(a) toward the center of Earth because Earth rotates
(b) toward the Sun because Earth revolves around the Sun in an almost circular orbit
(c) toward the center of our galaxy because the Sun moves about the galactic center
For the latter, the period is 2.5 * 10^8 y and the radius is 2.2 * 10^20 m. Calculate these three accelerations as multiples of g = 9.8 m/s2.

Ok so this shouldn't be hard, I'm probably making it harder than it really is, I'm having trouble working with gravity and circular motion for some odd reason. So any help?
 
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Find the centripetal acceleration and then divide by g.
 
well I found part C but I can't figure out teh answers to part a and b. :blushing: This should be easy!
 
A and B work exactly the same way as C. Just use the period eqn (T=2(pi)r/v) to find velocity and then plug into the centripetal accel. eqn and divide by g. For A, you'll use the Earth's radius for r and 24 hours for the period, but convert it to seconds. For B, you'll use the distance from the Earth to the sun for r and a period of 365 days, once again converted to seconds.
 
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