How Fast Does Mars Travel Around the Sun?

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Mars orbits the sun in approximately 1.88 Earth years, with an orbital radius of about 2.28 x 10^8 km. The orbital speed of Mars can be calculated using the formula V = d/T, where d is the circumference of the orbit and T is the orbital period. The correct calculation yields a speed of approximately 2.4 x 10^4 m/s. An alternative method involving centripetal acceleration is more complex but ultimately leads to the same result. The initial method of calculating velocity directly from distance and time is the most straightforward and accurate.
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Mars travels around the sun in 1.88 {Earth} yrs,in an approximately circular orbit with a radius of 2.28 * 10^8km.Determine
{a}The orbital speed of Mars {relative to the sun}Answer {a}:
period {T} = 1.88 * 365 *24 * 3600 sec , R = 2.28 * 10^8 * 10^2 = 2.28 * 10^11
d = 2 pie R ------> 2 * 3.14 * 2.28 * 10^11
V=d / T -------> { 2 * 3.14 * 2.28 * 10^11 } / { 1.88 * 365 *24 * 3600 }
=2.4 * 10^4m/sIs that correct?or do I use

acceleration of centripetal motion = (4)(pi^2)(r)(f^2)

then use the acceleration and find velocity in

V = √(acceleration x radius)

which method is correct? if any...
 
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You did this correctly, though longishly.

And the second way is the same thing just with with extra steps. Notice that your initial solution was to find v=d/t, where d is the circumference, 2 pi r , and t is the period, T.

so v=(2 pi r)/T (all done right there)

and since f= 1/T , v=2 pi r f

Your second solution takes the square of this, divides by radius, then multiplies by radius, then square roots it.
 
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