Centripetal and Tangitial Accelerations: Some Help please

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Homework Help Overview

The problem involves calculating various aspects of the Earth's orbit around the sun, specifically focusing on angular speed, tangential speed, and centripetal acceleration. The context is centered around circular motion in physics.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss methods for calculating angular speed, tangential speed, and centripetal acceleration, with some questioning the assumptions made regarding the Earth's orbit. There is also a focus on the correct interpretation of angular speed and its relationship to angular displacement.

Discussion Status

Some participants have provided calculations and expressed uncertainty about the correctness of their approaches. Questions regarding the calculation of angular speed and the definitions involved are being explored, indicating an ongoing dialogue without a clear consensus.

Contextual Notes

Participants note the need for clarification on the definitions of angular speed and the formulas used, as well as the implications of assuming a constant orbit. There is mention of the "Big 3" equations, suggesting a search for appropriate methods to apply in this context.

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Problem: The Earth orbits the sun once a year (3.16 x 10^7 s) in a nearly circular orbit of radius 1.5 x 10^11 m. With respect to the sun, determine (a) the angular speed of the earth, (b) the tangential speed of the earth, and (c) the magnitude and direction of the Earth's center centripetal acceleration.

My Approach:

(a) Finding Velocity:

V = (1.5 x 10^11 m)/(3.16 x 10^7 s) = 4747 m/s

--I did this because I'm assuming the Earth's orbit of the sun is constant

(b) Tangential Speed:

V = rw = (1.5 x 10^11 m) (4747 m/s) = 7^14 .12 x 10m/s

(c) Find Centripetal Acceleration:

a(centripetal) = (V tangential)^2 / (radius) = (7.12 x 10^14 m/s)^2 / (1.5 x 10^11 m) = 3.38 x 10^18 m/s^2

Please check my work and point out a quick way to fix something. I know this can be easy for any physics expert, but I am just a beginner-so help me in simple terms :smile:
 
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cheechnchong said:
My Approach:

(a) Finding Velocity:

V = (1.5 x 10^11 m)/(3.16 x 10^7 s) = 4747 m/s

--I did this because I'm assuming the Earth's orbit of the sun is constant
Wasn't the first question about angular speed?

(b) Tangential Speed:

V = rw = (1.5 x 10^11 m) (4747 m/s) = 7^14 .12 x 10m/s
This answer will be modified based on (a)...



(c) Find Centripetal Acceleration:

a(centripetal) = (V tangential)^2 / (radius) = (7.12 x 10^14 m/s)^2 / (1.5 x 10^11 m) = 3.38 x 10^18 m/s^2

...and so will this (and don't forget the direction). The formulae for b and c are correct.
 
How Would Angular Speed be Calculated in this problem? we are only given the time and radius...Should i use one of the Big 3 equations?
 
^^^bump!
 
cheechnchong said:
How Would Angular Speed be Calculated in this problem? we are only given the time and radius...Should i use one of the Big 3 equations?
Angular speed is not distance divided by time. It is the angular displacement divided by the time. Angular displacement is measured in radians.
 

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