Modern Atomic Models Take Shape
Ernest Rutherford completely revolutionised our understanding with his solar system model. Through his famous gold foil experiment, he proved that atoms have a tiny, dense, positively charged nucleus at the centre, with electrons orbiting around it like planets around the sun.
Niels Bohr refined this further by introducing the electron shell model in 1913. Instead of electrons flying around randomly, Bohr showed they occupy specific energy levels or "shells" around the nucleus - a bit like seats in a stadium with different tiers.
The final piece of the puzzle came when James Chadwick discovered the neutron in 1932. This completed our understanding of atomic structure: a nucleus containing positively charged protons and neutral neutrons, surrounded by negatively charged electrons in shells.
Remember This: Each discovery built on the previous one - scientists didn't start from scratch but improved existing models based on new evidence. This is exactly how real science works!