Early Calculations
It is believed that the accretion of Earth began after the formation of the calcium-aluminum-rich inclusions and the meteorites. It is also estimated that these calcium-aluminum-rich inclusions are approximately 4.567 billion years old. The oldest terrestrial materials that the scientists have analyzed are the tiny zircon crystals collected from the Jack Hills in Western Australia, which are about 4.404 billion years old.
Nevertheless, the British mathematical physicist William Thomson, 1st Baron Kelvin, published his calculations in 1862, which placed the Earth’s age between 20 to 400 million years. Thomson assumed that the Earth formed as a molten object and determined the time the molten object would take to cool to the current temperature. Therefore, Thomson’s calculations did not consider the amount of heat produced by radioactive decay and mantle convection. Besides this, Thomson’s estimates of the Sun’s age were also very constraining since the calculations were based on the sun’s thermal output. However, many scientists, including Charles Lyell and Thomas Henry Huxley, found it difficult to accept such a short age of the Earth as estimated by Thomson. In the later years, the German physicist Hermann von Helmholtz and the Canadian-American astronomer Simon Newcomb published their own calculations that placed the age of the Earth about 22 and 18 million years, respectively.
Modern Concepts
Before the discovery of radioactive dating in the early 20th century, many scientists used relative dating to determine the age of the materials. The study of strata or the different rock layers gave many researchers the idea about the series of changes that the Earth had undergone since its existence. Besides this, the various rock layers also contained fossilized remains of many unknown creatures, which helped the scientists study the organism’s progression from one rock layer to another. In the 17th century, the observations made by the Danish scientist Nicolas Steno led to the formulation of the stratigraphic concept, and Steno became the first person to find a connection between the fossil remains and the rock strata. However, even though this Stratigraphic technique did not tell the exact age of the different rock layers, it primarily suggested the Earth was billions of years old and not millions of years as were predicted earlier.
The discovery of radioactive dating introduced a critical factor that helped calculate the Earth’s age. The pioneers of radioactivity were the American chemist Bertram B. Boltwood and the British physicist Ernest Rutherford, while Arthur Holmes discovered radiometric dating. In 1927, Arthur Holmes published “The Age of the Earth, an Introduction to Geological Ideas,” where he placed the age of the Earth in the range of 1.6 to 3.0 billion years. Arthur Holmes was also a part of the committee set up by the National Research Council of the US Academy of Sciences in 1931 to find out the age of the Earth. The committee’s final report concluded that radioactive dating was the sole reliable method to date the geologic timescales. In 1956, after performing uranium-lead isotope dating on many meteorites, the American geochemist Clair Cameron Patterson determined the Earth’s age to be 4.55 ± 0.07 billion years. The ancient Archean lead ores of Galena were also used to determine the planet’s age as they represented the earliest formed lead-only minerals on Earth. These rocks have determined the Earth’s age to be 4.54 billion years with an error margin of 1%.