Orbits are shaped like an ellipse, with the star at the focus. An ellipse does not have a constant radius.
gravity is that keeping the orbital speed from falling or breaking loose. and the distance away = time
57,909,100 km
A planet's orbital period is related to its distance from the Sun by Kepler's third law, which states that the square of the orbital period is proportional to the cube of the semi-major axis of the orbit. For an orbital period of 3 million years, the planet would need to be located at a distance of approximately 367 AU from the Sun.
The distance of a planet from the sun affects its orbital period. Generally, the farther a planet is from the sun, the longer its orbital period will be. This relationship is described by Kepler's third law of planetary motion, which states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun.
Because Venus has less distance to travel than the Earth and is travelling faster. With an orbital speed of 35.02 km/s and an orbital period of 224.70069 days gives an orbital distance of 679,883,169.35km The Earth has an orbital speed of 29.78 km/s (Slower than Venus) and an orbital period of 365.256 days gives an orbital distance of 939,800,765.95km
The primary factors affecting orbital time are the mass of the objects involved, the distance between them, and the gravitational force between them. Orbital time increases with greater mass or distance, and decreases with stronger gravitational forces. The velocity of the objects also plays a role in determining the orbital time.
No because the distance between them are always changing. If you were trying to ask if the orbital paths of all the planets about the same distance apart then the answer is still no. The distance from each orbital path varies from each planet to the next. The orbital path of Neptune and Pluto cross one another so this also answers the question, no.
Sub-orbital space flight reaches space while low orbital spaceflight attain sufficient velocity to go to space.
In an s orbital, the probability of finding an electron at a particular distance from the nucleus does not depend on the direction in which the distance is measured or the orientation of the orbital. This is because s orbitals are spherically symmetric, meaning the electron has an equal likelihood of being found at any distance from the nucleus in all directions.
The approximate orbital period of an object at a distance of 65 AU from the sun would be around 177 years. This corresponds to Kepler's third law of planetary motion, which relates the orbital period of a planet to its distance from the sun.
Kepler's third law of planetary motion states that the square of a planet's orbital period is directly proportional to the cube of its average distance from the sun. This relationship allows us to predict the orbital period of a planet based on its distance from the sun, and vice versa.
The distance between the sun and a planet determines its orbital period, its orbital speed, and the amount of insolation. Other factors such as composition and albedo are required to determine other variables.