The orbital speed of a body with negligible mass compared to the central one,
in a circular orbit, is
v = square root of ( G M/R ) G = the universal gravitational constant = 6.67 x 10-11nt-m2 / kg2
M = mass of the central body; Venus' mass = 4.8676 x 1024 kg (0.815 of Earth)
R = radius of the orbit; Venus' mean radius = 6,051.8 km
The distance around a surface-skimming orbit is the planet's circumference.
C = (2 pi R); Venus's circumference = 12,103.6 x 103 pi
The period is 12,103.6 x 103 pi/v
The whole mess, all in one, is
T = C sqrt(R/G M)
T = (12,103.6 x 103 pi) sqrt(6051.8 x 103/6.67 x 4.8676 x 1013) . From that, I get T = 5,296.7 seconds = 1hr 28min 17sec
To check it, the only thing I have to compare it with is that, from my half-vast
trove of useless knowledge, I know the corrresponding period for Earth to be
86 minutes = 1hr 26min. I learned that when Sputnik-1 launched while I was in
high school.
Being at a radius 0.95 as large, around 0.815 as much central mass, the
1:28 that I got seems reasonable, at least within an order of magnitude.
You can use Kepler's Third Law to calculate this.
This question cannot be answered because:the total energy of the satellite includes its kinetic energy and that depends on its orbital speed. This is not specified;it is not clear what you mean by "potational": is it a typo for rotational or potential?what is R? The radius of the earth or the height of the satellite or some other measure?
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.
Since the distance from the Earth's center is doubled, the force will be reduced by a factor of 4.
The sine wave represents 360 degrees or a full circle. As the satellite revolves 360 degrees around the earth in its orbit this is how it is represented on a flat surface.
Scientists must carefully set the right orbital speed for a satellite that will be orbiting Earth, so that it will orbit correctly. The wrong speed will have the satellite move too fast, or too slow, skewing information and possibly causing the satellite to fall out of orbit and back to the planet's surface.
The orbital speed would be approximately 7.63 km/s and the period would be approximately 95.59 minutes for a satellite orbiting Earth at an altitude of 1.44 x 10^3 m. These values can be calculated using the formula for orbital speed (v = √(GM/r)) and the formula for orbital period (T = 2π√(r^3/GM)), where G is the gravitational constant, M is the mass of Earth, and r is the altitude of the satellite above Earth's surface.
Venus has two artificial satellites orbiting it, radar-mapping the surface and gathering other useful information about its surface.
60 cm diameter sphere area = pi x 602 cm2 = 11310 cm2 = 1.131 m2
The speed of the satellite is dependant on its distance from the surface of the planet. the greater the altitude, the greater the speed, or velocity. I would think that Velocity Equation would be a simple linear equation of the form; y=kx, where k is a constant. What that constant is for Mars, I do not know as I did not do Astronomy at Uni, only Physics subjects.
You can use Kepler's Third Law to calculate this.
A satellite is orbiting the Earth and taking pictures of it. Satellites are equipped with cameras that capture images of Earth's surface for various purposes, such as weather monitoring, environmental analysis, and mapping.
Mimas is a large moon of Saturn. Metis is a moon around Jupiter.
Among one of many differences is that Landsat is Polar-orbiting while GOES is geostationary. This also means that GOES is much further above the surface, so the resolution is poorer.
Mercury has no known moons (or natural satellites) and has no manmade satellites orbiting it either. It was visited in the 1970s buy a man made probe called mariner 10, which made three passes to observe and map it's surface.
The Lunar Reconnaissance Orbiter (LRO) is a satellite that has been orbiting the Moon since 2009, collecting valuable data and images of the lunar surface. It is part of NASA's ongoing exploration of the Moon.
The orbital time period of a geostationary satellite is approximately 24 hours, specifically about 23 hours, 56 minutes, and 4 seconds. This allows the satellite to maintain a fixed position relative to a point on the Earth's surface, as it orbits the Earth at the same rotational speed. Geostationary satellites are positioned at an altitude of about 35,786 kilometers (22,236 miles) above the equator.