Planets revolve in fixed orbits primarily due to the gravitational force exerted by the Sun, which pulls them towards it. This gravitational attraction, combined with the planets' initial velocity, creates a balance that results in stable, elliptical orbits, as described by Kepler's laws of planetary motion. Additionally, the conservation of angular momentum ensures that the planets maintain their orbits over time, preventing them from spiraling into the Sun or drifting away into space.
Because if they were ever going to collide they would have done it at some time in the last 3.5 billion years. Each planet has its own stable orbit which takes it round the Sun regularly at a fixed range of distances that does not overlap with other planets. The planets are understood to follow Kepler's laws in elliptical orbits, under the force of the Sun's gravity.
Constellations do not orbit planets. Constellations are apparent groupings of stars as seen from Earth, and they are fixed in their position relative to each other. They appear to move across the sky due to the Earth's rotation.
The model that illustrates electrons orbiting the nucleus in paths similar to planets orbiting the sun is the Bohr model of the atom. In this model, electrons occupy distinct energy levels or orbits around the nucleus, akin to the layers of an onion. However, it's important to note that this model has been largely replaced by quantum mechanical models, which describe electron behavior in terms of probabilities rather than fixed orbits.
The Bohr's planetary model of the atom was proposed by Danish physicist Niels Bohr in 1913. In this model, electrons orbit the nucleus in fixed circular paths or orbits at specific energy levels, resembling planets orbiting the sun. This model successfully explained the stability of atoms by quantizing the electron orbits.
Ptolemy believed the Earth was stationary primarily due to the observable motion of celestial bodies in the sky, which appeared to revolve around a fixed Earth. He constructed his geocentric model based on the idea that the Earth was at the center of the universe, with planets and stars moving in complex orbits around it. This perspective was further reinforced by the lack of perceived motion of the Earth itself and the philosophical and religious beliefs of his time that placed humans and the Earth at the center of the cosmos.
in fixed orbits
If the planets did not move in their fixed orbits they may dash each other.
Certainly not, they revolve around a star and the star moves as well.
NO. All the planets are in (more or less) fixed orbits.
Because the Earth and all the planets move in orbits round the Sun, while the stars appear to be fixed if we disregard the Earth's daily rotation.
In the Bohr model, electrons circle the nucleus in specific orbits or energy levels, each with a fixed radius and energy value. These orbits are quantized, meaning electrons can only exist in certain stable orbits without radiating energy. The model's main idea is that electrons move in circular orbits at fixed distances from the nucleus, similar to planets orbiting the sun.
In ancient astronomy, epicycles were imaginary circles within orbits used to explain the retrograde motion of planets. The concept was developed to account for the observed movements of planets in the sky.
Because if they were ever going to collide they would have done it at some time in the last 3.5 billion years. Each planet has its own stable orbit which takes it round the Sun regularly at a fixed range of distances that does not overlap with other planets. The planets are understood to follow Kepler's laws in elliptical orbits, under the force of the Sun's gravity.
Electrons moved in fixed orbits around the nucleus in Bohr's model of the atom. These orbits were quantized, meaning they had specific energy levels, and electrons could jump between these orbits by either absorbing or emitting energy.
Constellations do not orbit planets. Constellations are apparent groupings of stars as seen from Earth, and they are fixed in their position relative to each other. They appear to move across the sky due to the Earth's rotation.
They were two theories that were used to predict the positions of the planets as they moved among the fixed stars. They both used planetary orbits based on combinations of circles and they were both pretty accurate. Ptolemy had the Earth at the centre while Copernicus had the Sun at the centre. They were both replaced by Kepler's theory, published in 1609, which had elliptical orbits for the planets and also had the Sun at the centre.
The position of Mars in relation to Earth changes due to their orbits. There is no fixed "left" or "right" side of Earth in relation to Mars. Both planets orbit the Sun, and their positions vary depending on where they are in their respective orbits.