What is the Velocity of a Person at the Equator?

In summary, the conversation is about calculating the speed of a 97.4kg person at the equator given the values of r(Earth), m(Earth), r(moon), g, and G. The formula used to solve for v is v=((GM/r^2 - g)*r)^1/2, where r is the radius of the Earth's equator. The conversation also discusses the importance of understanding the formula and the values used in order to solve the problem correctly.
  • #1
nrc_8706
70
0
:confused: Given: r(Earth)=6.37*10^6 m
m(earth)=5.98*10^24 kg
r(moon)=1.74*10^6m
g=9.8 m/s^2
G=6.67259*10^-11 Nm^2/kg^2

Calculate the speed of a 97.4kg person at the equator.
do u use a=v^2/r v=sqr root (a*r) ?
 
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  • #2
Hello?!

Can Anybody Help Me?!
 
  • #3
[tex] \Sigma F = ma_c [/tex]

... you know that gravity is the force acting towards the center, you know the radius, so you can find the v.
 
  • #4
...

ok, taking what you said i got that Gravity=m*v^2/r

v=(gr/m)^1/2 correct?
 
  • #5
which radius do u use? the Earth's or the moon's?
 
  • #6
where is the person?
 
  • #7
equartor

he is at the equator
 
  • #8
of which? the Earth or the moon? which radius does it make sense to use?
 
  • #9
at the Earth's equator
 
  • #10
yeah, so use the Earth's equator..
 
  • #11
do u use 9.8m/s^2 or 6.67*10^-11
 
  • #12
those are two different things... you can use either, if you know what you're doing.
 
Last edited:
  • #13
[tex] F_g - N = m \times \frac {v^2}{r} [/tex]
[tex] \frac{GMm}{r^2} - mg = \frac {mv^2}{r} [/tex]
[tex] \frac{GM}{r^2} - g = \frac{v^2}{r} [/tex]

now solve for v.

do you understand what i did?
 
Last edited:
  • #14
v=(GM/r^2-g)^1/2


=(((6.67*10^-11*5.98*10^24)/(6.37*10^6)^2)-9.8)^1/2 correct?
 
  • #15
nrc_8706 said:
v=(GM/r^2-g)^1/2
=(((6.67*10^-11*5.98*10^24)/(6.37*10^6)^2)-9.8)^1/2 correct?

there should be an "r"

v=((GM/r^2 - g)*r)^1/2more importantly, do you understand how i got that?
 
Last edited:
  • #16
yes thank you. i knew it had something to do with F=GMm/R^2 i just didnt know what to do. thank for all your help and your patience.
 

What is centripetal acceleration?

Centripetal acceleration is the acceleration of an object moving in a circular path towards the center of the circle. It is a result of the centripetal force acting on the object, which is responsible for keeping the object in its circular path.

What is the formula for calculating centripetal acceleration?

The formula for centripetal acceleration is a = v²/r, where "a" is the centripetal acceleration in meters per second squared, "v" is the velocity of the object in meters per second, and "r" is the radius of the circular path in meters.

How does centripetal acceleration differ from tangential acceleration?

Centripetal acceleration is the acceleration towards the center of a circle, while tangential acceleration is the acceleration along the tangent of a circle. Centripetal acceleration changes the direction of an object's velocity, while tangential acceleration changes the magnitude of its velocity.

What are some real-life examples of centripetal acceleration?

Some examples of centripetal acceleration include the motion of a car around a curve, the rotation of a Ferris wheel, and the orbit of a satellite around a planet. Any circular motion involves centripetal acceleration.

How does centripetal acceleration relate to centripetal force?

Centripetal acceleration and centripetal force are directly related. Centripetal acceleration is the result of the centripetal force, which is responsible for keeping an object in a circular path. The greater the centripetal force, the greater the centripetal acceleration will be.

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