Re = Radius of earth (6.38EE6)
H = Height of satellite (780km => 780,000m)
Me = Mass of earth (5.98EE24)
Ms = Mass of satellite
G = Universal Gravity (6.67EE-11)
V = Orbital Speed
Fg= Force of gravity
Fc= Centripetal force
Use the formula Fg=Fc
(((G)(Me)(Ms))/ (Re+H)^2)= (Ms)(V^2)/(Re+H)
Ms cancel out
((G*Me)/ ((Re+H)^2)) = (V^2)/(Re+H)
Solve for V
V = sqrt( ((G*Me)/((Re+H)^2)) * (Re+H) )
= sqrt( ((6.73EE-11*5.98EE24)/((6.38EE6+780,000)^2)) * (6.38EE6+780,000) )
= 7465.426831 m/s
26,836 Km/h
Solution:To calculate speed, we need to divide the distance travelled by the time. We are given the time of one orbit, so we now must calculate the distance the satellite travels in one orbit. To do that, we need one more piece of information: the Earth's radius, which is 6,378 Km.
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The satellite scribes a circle around the earth as it orbits, and the circumference of that circle is the distance the satellite travels in one orbit. We know that the circumference of a circle is obtained from the following equation:
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C = 2 * PI * r
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where 'r' is the radius of the circle. In the case of the satellite's orbit, the radius is 755 + 6378 Km in our problem, yielding a circumference of 44,817 Km.
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Let's assume we are calculating the speed in Km/h, not m/s. 99.7 minutes is 1.67 hours, so the speed of our satellite is:
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S = D / t
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where D is distance (44,817 Km)
t is time (1.67 h)
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So Speed (S) is calculated at 26, 836 Km/h.
You can use the the formula Fgravity=ma to derive v2=(GM/R) where G is Newton's universal gravity constant, M is the mass of the Earth and R is measured from the center of the earth.
Using this formula you obtain:
v=sqrt(GM/R)
=sqrt((6.67E-11m3/(kg*s2))(5.98E24kg)/(631*1000m+6.37E6m)
remember to convert to meters and add the radius of the earth
=7.548*103m/s
formula:
s=d/t
solution:
s=400km/89.5mins
answer:
s=4.47km/mins
During the devonian time period most of land was under water.
A geosynchronous satellite is a satellite in geosynchronous orbit, with an orbital period the same as the Earth's rotation period.
It is not, because the altitude of the orbit is related to the period. If two satellites have the same orbital period, then they have the same altitude.
the time it takes the satellite to travel around the earth once
Lower. The higher a satellite is, the more stationary it appears. for a satellite close to Earth, the period is a matter of hours, but for a satellite farther away, days.
hot ,wet,
Type your answer here... it was wet and the surface was covered with a thin layer of warm water.
During the devonian time period most of land was under water.
The angle of the satellite period, depends on where the satellite is positioned. When you figure out where the satellite is you position the angle to be where and what you need.
Here we will use the following formula velocity of the satellite v = 2πr/T here r is the radius of the circular path travelled by the satellite = 42250 km and T is the time period = 24 hrs. here, the distance travelled by the satellite in 24 hrs would be the circumference of the circular path of radius 42050 . so, v = (2 X 3.14 X 42050) / 24 = 264074 / 24 :)
A geosynchronous satellite is a satellite in geosynchronous orbit, with an orbital period the same as the Earth's rotation period.
During the Tertiary Period, the surface of the earth looked much like it does today. It was quite warm with periods of cold much like today.
You can use Kepler's Third Law to calculate this.
It is not, because the altitude of the orbit is related to the period. If two satellites have the same orbital period, then they have the same altitude.
the time it takes the satellite to travel around the earth once
Its period increases
A geostationary orbit is an orbit of the Earth that is circular, over the equator, and at the right distance to have a period of 24 hours. A satellite in such an orbit appears to hang motionless, always at the same point in the sky Anything else is a non-geostationary orbit. A satellite in one of those appears to move in the sky, so that if you want to communicate with it, you need a movable dish.