Yes, there is a relationship between the distance from the sun and the length of the year for the planets. The greater the distance from the sun, the longer the year. The reasons are explained in Newton's Laws of Gravity and Einstein's Theory of Relativity.
A planets year is known as the distance a planet takes to travel around the Sun in a complete orbit. For example, in 365 days time, or one year, the Earth will have traveled around the Sun and be back in the position it is in right now. When compared to Earth, the closer a planet is to the the Sun, the shorter its years are (Mercury, Venus). Planets further away from the Sun have longer years when compared to an Earth year (Mars, Saturn, Jupiter, Uranus, Neptune, Pluto). So we say that a year on Mercury compared to ours only lasts 88 Earth days, whereas a year on Neptune takes about 60000 Earth days (nearly 165 Earth years).
The cube of the distance is proportional to the square of the length of the year or orbital period.
For example, Jupiter is about 5.2 times as far from the Sun as the Earth is. Cube 5.2. Now take the square root of the result. That's how many times longer Jupiter's year is than Earth's year.
Distance (in AU's) cubed equals orbit time (in earth years) squared. For example, Mars is 1.52 AU with an orbit time of 1.88 Earth years. 1.52^3 == 1.88^2 (�= 3.54) Neptune is 30.11 AU and orbit time of 164.79 Earth years. 30.11^3 == 164.79^2 (�=27295.25)
The length of the planet's year is equal to the distance to the power 1.5. So for a planet at 4 times the distance, the rotation period would be 8 times longer (Kepler's 2nd law).
The Earth and other planets of the solar system move in orbits around the sun.
A satellite is any mass that orbits a larger mass. A satellite may be a planet, moon, asteroid, or comet. The word 'satellite' is also used to refer to any man-made object launched to orbit Earth or another planetary body. Artificial satellites may be spacecraft or orbiting telescopes.
This is true if the angular velocity is not a variable. That being said this is the reason why the outer planets such as Saturn and Jupiter have such long Solar orbits as opposed to Earth,
Really, the best way to differ between a dwarf and regular planet is by looking at their size, and comparing it to Mercury's size, which is our smallest Planet. The size difference is usually obvious, but in some cases, you may need to refer to an actual chart because of how big that small dwarf planet may be.See the related link for definition
That depends on what it orbits. If it orbits the Sun or another star, it may be called a planet, a dwarf planet, or an asteroid (or planetoid), depending on the size. If it orbits a planet, it is called a Moon. It is also possible for two stars to orbit each other (orbit their center of mass, actually).
Different planets have different length orbits because they are at varying distances from the sun. The farther a planet is from the sun, the longer it takes to complete an orbit. This is due to the gravitational pull of the sun, which affects the speed at which planets travel around it.
If two planets are in orbits with radii of R1 and R2, the distance between them varies from R2-R1 to R2+R1.
Keplar showed that there is a relationship between the planets distance from the sun and the time taken for one orbit (planets year). This is described in Keplars third law; the square root of the time taken to orbit the sun is proportional to the cube of the average distance between the sun.
Unfortunately there is no simple answer to that. The distance is constantly changing as the planets move in their orbits.
To some extent the question is meaningless because you would have to define where in the orbits the planets are to work out the instantaneous distance between them (Saturn could be on one side of the Sun and Uranus on the other) It would be more meaningful to ask the distance between the orbits of the orbital paths of the planets not the planets themselves.
The length of a planet's orbit around the Sun varies depending on the distance from the Sun. For example, Mercury has an orbit of about 88 Earth days, while Neptune's orbit is around 165 Earth years.
The force of gravity between the planets and the sun keeps them in their respective orbits, maintaining their approximate distances from each other. This gravitational force acts as a centripetal force, balancing the planets' inertia and keeping them in stable orbits around the sun.
YES. However the relationship is not quite that simple. This is Kepler's third law. I'll give you a simplified version which assumes the planets orbits are circular, instead of being ellipses : The square of the length of the year is proportional to the cube of the planet's distance from the Sun.
The planets in our solar system orbit around the Sun in elliptical paths. Each planet follows its own unique orbit based on its distance from the Sun and gravitational interactions with other celestial bodies. The orbits are roughly aligned along the same plane known as the ecliptic.
No. No two planets have the same size orbit. Mars orbits the sun at more than twice the distance that Venus does.
The main difference between the orbits of inner and outer planets is their distance from the Sun. Inner planets (Mercury, Venus, Earth, Mars) have shorter orbits and are closer to the Sun, while outer planets (Jupiter, Saturn, Uranus, Neptune) have longer orbits and are farther away from the Sun. Additionally, outer planets are larger and predominantly composed of gas and ice, while inner planets are smaller and have rocky surfaces.
Gravitational force is what holds all the planets in their orbits around the sun. This force is determined by the mass of the objects and the distance between them. The gravitational pull of the sun keeps the planets in their respective orbits.