James Keeler stood at the edge of a new scientific era in 1895. He helped establish The Astrophysical Journal to bridge the gap between astronomy and physics. Before this moment, astronomers measured positions and motions of stars while physicists studied matter on Earth. Keeler declared that astrophysics seeks to ascertain the nature of heavenly bodies rather than their locations. This shift changed how humanity understood the universe. Scientists began asking what stars were made of instead of just tracking where they moved. The field applied principles from classical mechanics, electromagnetism, and thermodynamics to celestial objects. Researchers examined luminosity, density, temperature, and chemical composition across all parts of the electromagnetic spectrum. They studied the Sun, other stars, galaxies, and the cosmic microwave background. These investigations required concepts from quantum mechanics, relativity, and nuclear physics.
Spectroscopy And Chemical Discovery
William Hyde Wollaston and Joseph von Fraunhofer independently discovered dark lines in the solar spectrum during the nineteenth century. These regions showed less or no light when decomposing sunlight. By 1860 Gustav Kirchhoff and Robert Bunsen demonstrated that these dark lines corresponded to bright lines in known gases. Each line represented a unique chemical element found in the Solar atmosphere. Norman Lockyer detected radiant and dark lines in 1868 while working with chemist Edward Frankland. He could not associate a yellow line in the solar spectrum with any known elements at that time. Lockyer claimed this line represented a new element called helium after Helios personified the Sun. Edward C. Pickering undertook an ambitious program of stellar spectral classification at Harvard College Observatory starting in 1885. A team of women computers including Williamina Fleming, Antonia Maury, and Annie Jump Cannon classified spectra recorded on photographic plates. By 1890 they prepared a catalog of over 10,000 stars grouped into thirteen spectral types. Cannon expanded this work by 1924 into nine volumes containing over a quarter of a million stars.