[Extra Quality] Download Orbits 5
Deidra Mehis
IGS orbit combination solutions are available in three forms: ultra-rapid, rapid, and final. The ultra-rapid product, useful for real-time and near real-time applications, is archived at regular intervals four times per day; the ultra-rapid solution includes both observed and predicted satellite orbits. The rapid orbit combination is a daily solution available approximately 17 hours after the end of the previous UTC day. The final, and most consistent and highest quality IGS solutions, consists of daily orbit files, generated on a weekly basis approximately 13 days after the end of the solution week. All orbit solution files utilize the Extended Standard Product- 3 (SP3c) format.
All operational IGS GNSS products (i.e., orbits, station positions, EOP, clock solutions) are available in subdirectories by GPS week. Solution summary files are provided by the analysis centers in which they describe their analysis methods and strategies and list processing statistics. Descriptions of AC analysis procedures and models used are available from the IGS website.
Orbits come in different shapes. All orbits are elliptical, which means they are an ellipse, similar to an oval. For the planets, the orbits are almost circular. The orbits of comets have a different shape. They look like a "squashed" circle. They look more like thin ellipses than circles.
Satellites that stay above a location on Earth are in geosynchronous Earth orbit, or GEO. These satellites orbit about 23,000 miles above the equator and complete one revolution around Earth precisely every 24 hours. Geosynchronous orbits are also called geostationary.
Any satellite with an orbital path going over or near the poles has a polar orbit. Polar orbits are usually low Earth orbits. Eventually, Earth's entire surface passes under a satellite in polar orbit.
We describe the use of radical craniofacial osteotomies, to improve the correction of exorbitism and to obtain better esthetic results in children with Crouzon's syndrome. We suggest some minor modifications to improve the fixation and the mechanical stability of the mobilized segments of the skull. Our procedure consists, essentially, of advancement of both orbits and the midface in one piece, plus advancement and reshaping of the frontal area. The results obtained by this technique, in children with a Crouzon's deformity without open bite, have been most satisfactory. We believe the satisfactory resultant appearance will be maintained during and after growth of the face, although these children have not been followed long enough yet to ascertain this with certainty.
One example of a highly elliptical orbit is a Molniya orbit. Molniya orbits have an inclination of 63.4 degrees, an apogee of about 40,000 km and a perigee of about 1,000 km. For the majority of their periods, satellites in Molniya orbit are primarily observing the northern hemisphere of the Earth. Since both the United States and Russia are in the northern hemisphere, Molniya orbits were ideal for reconnaissance in the Cold War Era.
Instead, these satellites perform one final fuel burn, sending them into graveyard orbits. Current U.S. guidelines require a spacecraft to be raised to an orbit at least 300 km higher, well out of the way of the busier operational orbits below.
An orbit is a regular, repeating path that one object takes around another object or center of gravity. Orbiting objects, which are called satellites, include planets, moons, asteroids, and manmade devices.
Objects orbit each other because of gravity. Gravity is the force that exists between any two objects with mass. Every object, from the smallest subatomic particle to the largest star, has mass. The more massive the object, the larger its gravitational pull. Gravitational pull is the amount of force one object exerts on another object.
The sun is the most massive object in our solar system. All of the other objects in the solar system are subject to the gravitational pull of the sun.
Many satellites orbit on orbital planes. An orbital plane is a flat, disk-shaped space that connects the center of the object being orbited with the center of orbiting objects. Because all planets in our solar system share a similar orbital plane, planets dont run in to each other.
All the planets in our solar system line up with each other on the same general orbital plane. However, sometimes orbital paths of other objects in the solar system intersect, and the objects can collide. Comet Tempel-Tuttle, for instance, passes through Earths orbit. The debris from the tail of this comet passes through Earths atmosphere as meteors, or falling stars, at a specific time every year. The debris from the comet's orbit is called the Leonid meteor shower.
The time it takes for an object to orbit around another object is called its orbital period. Earth completes its orbital period around the sun every 365 days. The further away a planet is from the sun, the longer its orbital period. The planet Neptune, for example, takes almost 165 years to orbit the sun.
Each orbit has its own eccentricity. Eccentricity is the amount an orbits path differs from a perfect circle. A perfect circle has an eccentricity of zero. Earths eccentricity is .017. Mercury has the largest eccentricity of all the planets in the solar system, at .206.
Types of Orbits
Moons orbit planets, while planets orbit the sun. Our entire solar system orbits around the black hole at the center of our galaxy, the Milky Way. There are three major types of orbits: galactocentric orbits, heliocentric orbits, and geocentric orbits. Objects with geocentric orbits have their own types.
A galactocentric orbit is an orbit that goes around the center of a galaxy. Our solar system follows this type of orbit around the Milky Way.
A heliocentric orbit is one that goes around the sun. All the planets in our solar system, along with all the asteroids in the Asteroid Belt and all comets, follow this kind of orbit. Each planet's orbit is regular: they follow certain paths and take a certain amount of time to make one complete orbit. The planet Mercury completes its short heliocentric orbit every 88 days. Comet Kohoutek may take 100,000 years to complete its long heliocentric orbit.
A geocentric orbit is one that goes around the Earth. Our moon follows a geocentric orbit, and so do most manmade satellites. The Moon is Earth's only natural satellite. It takes about 27 days for the moon to complete its orbital period around the Earth. There are three major types of geocentric orbits: low-Earth orbit (LEO), medium-Earth orbit (MEO), and geostationary orbit.
Low-Earth orbit exists between 160 kilometers (100 miles) and 2,000 kilometers (1,240 miles) above Earth's surface. Most artificial satellites with human crews are in low-Earth orbit. The orbital period for objects in LEO is about 90 minutes.
Medium-Earth orbit exists between 2,000 kilometers (1,243 miles) and 36,000 kilometers (23,000 miles) above the Earths surface. Satellites in MEO are at greater risk for damage, because they are exposed to powerful radiation from the sun. Satellites in MEO include global positioning system (GPS) and communication satellites. MEO satellites can orbit the Earth in about two hours.
Satellites in geostationary orbit circle the Earth directly above the Equator. These satellites have geosynchronous orbits, or move at the same rotation of the Earth. Therefore, the orbital period of geosynchronous satellites is 24 hours.
Geostationary satellites are useful because they appear as a fixed point in the sky. Antennae pointed toward the geostationary satellite will have a clear signal unless objects in the atmosphere (such as storm clouds) between Earth and the satellite interfere. Most weather satellites are geostationary and provide images of Earths atmosphere.
Satellite Orbits
Manmade satellites are sent to orbit the Earth to collect information we can only assemble from above the atmosphere. The first satellite, Sputnik, was launched by the Soviet Union in 1957. Today, thousands of satellites orbit the Earth. Weather satellites provide images of weather patterns for meteorologists to study. Communication satellites connect cell phone users and GPS receivers. Military satellites track movement of weapons and troops from different countries.
Sometimes, manmade satellites have people on them. The most famous manmade satellite is the International Space Station (ISS). Astronauts from all over the world stay on the ISS for months at a time as it orbits the Earth. Astronomers and stargazers can see the ISS and other satellites as they orbit through telescopes and even powerful binoculars.
Not all artificial satellites orbit the Earth. Some orbit other planets. The Cassini-Huygens mission, for instance, is studying the planet Saturn. The project has a spacecraft, Cassini, in orbit around Saturn.
Putting satellites into orbit is complex and costly. Few governments can afford large space programs. Manmade satellites from the United States are sent into orbit by the National Aeronautics and Space Administration, or NASA. The European Space Agency (ESA) sends up satellites from countries in the European Union. The Russian Federal Space Agency (Roscosmos), the Japanese Space Agency (JSA), and the Iranian Space Agency (ISA) have all successfully put satellites into orbit.
Satellites are put into orbit from spaceports, which are carefully constructed for that purpose. The Baikonur Cosmodrome in Kazakhstan and the Kennedy Space Center in the U.S. state of Florida are both well-known spaceports.