Matter tells spacetime how to curve, and spacetime tells matter how to move. This was the recipe that finally explained why Mercury’s orbit was so weird—the sun is so heavy that it curves the space around it in a way that Newton’s old rules couldn't see.
The one idea behind Einstein's relativity

The central idea behind Einstein's relativity is the realization that space and time are not separate, rigid entities as previously believed in Newtonian physics. Instead, they form a single, stretchy fabric known as spacetime. This shift in understanding suggests that our reality is far more flexible than the predictable, clockwork universe described by Isaac Newton, where time was thought to be a steady beat that never changed regardless of motion.
Isaac Newton viewed the universe as a giant, ticking clock where space was an empty box and time was absolute and unchanging. In this Newtonian world, gravity was seen as a simple pull between objects, like a magnet and a paperclip. Einstein's relativity challenged this by proposing that the universe is not a rigid mechanism but a flexible fabric where space and time are interconnected, fundamentally changing our common sense about how the cosmos works.
Mercury's orbit presented a mysterious flaw that Newton's math could not explain, acting like a slipping gear in the universal clock. This tiny, nagging problem revealed that the path of the planet around the sun didn't fit the predictable rules of Newtonian physics. This discrepancy served as the first hint that our basic understanding of the world was incomplete, eventually leading to the groundbreaking insights of Einstein's relativity and the concept of spacetime.
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