A polar orbit would allow a satellite to view any point on the Earth's surface from (nearly) directly overhead. The times for a given location would depend on the altitude and the speed of the orbit. The advantages are a minimal angle to the specific point below the satellite's path, which would benefit direct obsevation (as with military "spy satellites"). Among the disadvantages is increased fuel cost to reach the orbit, and increased shielding in some orbits due to the polar radiation belts around the Earth.
The eclipse effect in satellite communication occurs when the satellite passes into the shadow of the Earth, causing a temporary loss of communication signal. This happens during solar eclipses or when the satellite is behind the Earth in its orbit. To mitigate the impact, satellite operators can use battery power or pointing strategies to maintain connectivity during these periods.
In spaceflight jargon it means when a spacecraft or satellite passes close enough to an object in space (typically a celestial body, such as a planet) to gather scientific data without orbiting or landing on the object.
The three main stages in exploring a planet are: 1. send out a spacecraft that passes one or more bodies in space without orbiting them. 2. study a planet over a long period of time. and finally, 3. land instruments on a planet or to send instruments through its atmosphere.
A geostationary orbit would allow a satellite to see all parts of the globe as it orbits the Earth at the same speed that the Earth rotates. This means the satellite remains fixed above the same point on the equator, providing continuous coverage of that area.
A satellite can stop being visible due to factors such as entering the Earth's shadow, changing its orbit, or switching off its reflective surfaces making it harder to see from the ground. Additionally, atmospheric conditions, like clouds or light pollution, can also obstruct visibility of satellites.
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.
Possibly because it passes into Earth's shadow, though without more detail on exactly what satellite it's hard to be certain.
All satellites pass the equator. Twice every orbit.
The eclipse effect in satellite communication occurs when the satellite passes into the shadow of the Earth, causing a temporary loss of communication signal. This happens during solar eclipses or when the satellite is behind the Earth in its orbit. To mitigate the impact, satellite operators can use battery power or pointing strategies to maintain connectivity during these periods.
In spaceflight jargon it means when a spacecraft or satellite passes close enough to an object in space (typically a celestial body, such as a planet) to gather scientific data without orbiting or landing on the object.
A satellite is a craft in orbit around another body. A probe either passes by another body or goes to that body and lands (an sometimes returns).
It passes through several cities. It is located in the country of Germany.
TLE stands for Two-Line Element Set, which is a data format used by satellites to describe their orbits. It includes information such as the satellite's position, velocity, and time parameters. TLE data is commonly used by satellite trackers and ground stations for predicting satellite passes and orbital analysis.
Absolutely. Hover your cursor/mouse over 'Profile' in the navigation bar and then choose 'My Passes'. From there, you can choose your country, how many passes you would like to buy, and how you would like to pay.
A polar orbit (as opposed to an equatorial orbit) passes over the poles, north and south. A low orbit is relatively close to the Earth (or other object being orbited), it might be a few hundred miles up.
If you are interested in purchasing passes for the Eurail, then you will find several websites available. The Eurail official website offers online purchasing options.
Two stars orbiting each other so that one regularly passes in front of the other blocking out some or all of light of the hidden star. See related link for an animation.