For objects in orbit around the sun, it's the aphelion.
For objects in Earth orbit, it's the 'apogee', and in orbit
around the moon, it's the 'apolune'.
The orbital far point, or aphelion, is the point in an object's orbit around the sun where it is farthest away from the sun. This is in contrast to the perihelion, which is the point in the orbit where the object is closest to the sun.
The closest point in an orbit is called the perigee, for objects orbiting Earth, or periapsis for objects orbiting other celestial bodies.
The rotation of an object around a fixed point is called "revolution" or "orbital motion".
That point is called apogee and it rotates round the orbital plane every 19 years.
The orbital high point, or apogee, is the farthest point in an object's orbit around another body, such as a planet or star. It is the point in the orbit where the object is at its maximum distance from the body it is orbiting.
The orbital far point, or aphelion, is the point in an object's orbit around the sun where it is farthest away from the sun. This is in contrast to the perihelion, which is the point in the orbit where the object is closest to the sun.
The closest point in an orbit is called the perigee, for objects orbiting Earth, or periapsis for objects orbiting other celestial bodies.
The rotation of an object around a fixed point is called "revolution" or "orbital motion".
far point far point
That point is called apogee and it rotates round the orbital plane every 19 years.
That point is called apogee and it rotates round the orbital plane every 19 years.
The lowest point of an orbit is called the "perigee" in the context of Earth orbits, or "periapsis" in general orbital mechanics. At this point, the orbiting object is closest to the body it is orbiting, resulting in the highest speed due to gravitational attraction. Conversely, the highest point of the orbit is called "apogee" (or "apoapsis"). These points are critical for understanding orbital dynamics and the behavior of satellites and celestial bodies.
Perigee
Orbital speed is the velocity (speed) of an object as it travels an orbital path around a reference point.
Orbital radiography
The orbital high point, or apogee, is the farthest point in an object's orbit around another body, such as a planet or star. It is the point in the orbit where the object is at its maximum distance from the body it is orbiting.
Aphelion is the point in a planet's orbit where it is farthest from the sun. This is when the planet is at its greatest distance from the sun in its orbital path.