The orbits of the planets and the cosmic balance

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The orbits of the planets are more like ovals than perfect circles, as Johannes Kepler discovered in his first law, this means that a planet's distance from the sun changes as it moves along its orbit: it gets closer at a point called perihelion and farther away at aphelion. This elliptical orbit explains why we have seasons on Earth and helps us understand why planets like Mars have more noticeable changes in their distance from the sun.
What keeps these orbits in check is gravity, Isaac Newton discovered that the pull of the sun keeps the planets moving in a loop, preventing them from drifting away into space or crashing into the sun. This delicate balance between the inertia of motion and gravitational attraction is what keeps the solar system in harmony—an order that has been stable for billions of years.
But even the paths of the planets around the sun aren't set in stone, the way the planets pull on each other, along with tiny nudges from asteroids or comets, causes slight variations. These changes, though barely noticeable at first glance, are measured with high precision by modern astronomy. Thanks to this, we can predict eclipses, planetary alignments, and the paths of objects near Earth with accuracy.
So, in short, planetary orbits are like a super-organized system where physics and geometry just perfectly mesh, their studies have given us a better understanding of our cosmic neighborhood and have even helped map out safe paths for spacecraft, not to mention their remarkable ability to predict the movements of stars and planets. Orbits are essentially the mathematical patterns that keep the universe in order.
Reference
Solar Systems: Planets, Stars and Orbits by Nadia Higgins, 2019.
Physics for Science and Technology. II by Paul Allen Tipler, Gene Mosca, 2004.