A sun-synchronous orbit (SSO) is a specific type of low Earth orbit that allows satellites to maintain a consistent angle with respect to the Sun as the Earth rotates. The orbital speed required for a satellite in SSO is approximately 7.4 kilometers per second (about 26,640 kilometers per hour or 16,600 miles per hour). This speed enables the satellite to complete an orbit roughly every 90 to 100 minutes, ensuring it passes over the same point on Earth at the same solar time each day. This characteristic is particularly useful for Earth observation and remote sensing applications.
Orbital velocity refers to the speed at which a planet travels in its orbit.
The radius of an orbit is directly related to the average speed of the orbiting body. As the radius of the orbit increases, the average speed of the orbiting body decreases. This is because at a larger distance from the center of mass, the gravitational force decreases, requiring a lower speed to maintain the orbit.
No, a rock cannot speed up on its own to reach a higher orbit. A change in orbit requires an external force, such as propulsion or gravity assists.
Depending on the direction in which your speed was pointed, and at what stage of the launch it was faster, any of these could happen: -- you would get to orbit sooner -- you would settle into a smaller, more circular orbit -- you would settle into a larger, more eccentric orbit -- you would not orbit at all, but escape the Earth completely and never return
Yes, the speed of a planet changes during its orbit due to the elliptical shape of the orbit, as described by Kepler's laws of planetary motion. A planet moves faster when it is closer to the Sun (at perihelion) and slower when it is farther away (at aphelion). This variation in speed occurs because of the gravitational pull the Sun exerts on the planet, which is stronger when they are closer together. Overall, the planet's orbital speed is not constant throughout its orbit.
Geostationary satellites are the ones used for GPS satellites.
The orbit of objects that approach the Sun, or Earth, from far away, above a certain critical speed.At a certain critical speed, the orbit will be a parabola. Above the critical speed, the orbit will be a hyperbola. (In both cases, the object will go away, never to come back.) Below the critical speed, the orbit is an elipse or a circle.The orbit of objects that approach the Sun, or Earth, from far away, above a certain critical speed.At a certain critical speed, the orbit will be a parabola. Above the critical speed, the orbit will be a hyperbola. (In both cases, the object will go away, never to come back.) Below the critical speed, the orbit is an elipse or a circle.The orbit of objects that approach the Sun, or Earth, from far away, above a certain critical speed.At a certain critical speed, the orbit will be a parabola. Above the critical speed, the orbit will be a hyperbola. (In both cases, the object will go away, never to come back.) Below the critical speed, the orbit is an elipse or a circle.The orbit of objects that approach the Sun, or Earth, from far away, above a certain critical speed.At a certain critical speed, the orbit will be a parabola. Above the critical speed, the orbit will be a hyperbola. (In both cases, the object will go away, never to come back.) Below the critical speed, the orbit is an elipse or a circle.
speed of electrons varies from shell to shell . it increases from inner orbit to outer orbit
Orbital velocity refers to the speed at which a planet travels in its orbit.
The speed of an electron in its orbit around an atom is approximately 2.18 million meters per second.
A satellite in a closed orbit has the greatest speed when it's closest to the planet, and the lowest speed when it's farthest from the planet.
The speed of the planet Uranus at every point in its orbit is lessthan the speed of the planet Jupiter at every point in its orbit.
If something is in orbit it's orbital speed is independent of its mass. Be it a gram or a tonne, it's speed depends only on its orbit; if it had a different speed it would be in a different orbit ( or none at all).
The radius of an orbit is directly related to the average speed of the orbiting body. As the radius of the orbit increases, the average speed of the orbiting body decreases. This is because at a larger distance from the center of mass, the gravitational force decreases, requiring a lower speed to maintain the orbit.
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The speed of an electron in its orbit around the nucleus is approximately 2.18 million meters per second.
No, a rock cannot speed up on its own to reach a higher orbit. A change in orbit requires an external force, such as propulsion or gravity assists.