Conservation.
The conservation of angular momentum affects the expected spin of planets by causing them to rotate at a relatively constant speed as they orbit the sun. This means that planets are likely to have a consistent spin rate over time due to the conservation of angular momentum.
It is due to the conservation of momentum.
Planets (and stars) were formed out of dust and gas. That had a rotation to it which does not go away (this is known as the Conservation of Angular Momentum).
Planetary condensation is the process by which solid particles in a protoplanetary disk coalesce to form larger bodies, eventually leading to the formation of planets. This process is a key stage in the formation of planetary systems around stars.
The main difference between the nebular and condensation theories is their emphasis on different aspects of planet formation. Nebular theory focuses on the collapse of a rotating nebula to form a star and planets, while condensation theory emphasizes the role of solid particles (dust and gas) in the early stages of planet formation.
Human beings destroy the planets natural resources.
natural recources
The creation of stars and planets into solar systems by condensation, concretion, and gravitational collapse.
it is because of the natral resources
what planet's resources might come close with earth
Planets spin on their axes due to the conservation of angular momentum, which is a fundamental principle in physics. As planets formed from rotating clouds of gas and dust in space, their rotation continued as they condensed and solidified. This spinning motion is what causes planets to rotate on their axes.
Terrestrial planets were formed by:the collapse of the solar nebulathe condensation of grainsthe growth of planetesimalsthe clearing of debrisJovian planets were formed by:the collapse of the solar nebulathe condensation of grainsthe growth of planetesimalsthe capturing of gasthe clearing of debris