Pickering-Fleming system
Quick Summary
The Pickering-Fleming system, developed by Edward Charles Pickering and Williamina Paton Stevens Fleming, was a pioneering method for classifying stellar spectra. Pickering, a physicist and astronomer, established the Harvard College Observatory and introduced the meridian photometer for measuring star brightness. Fleming, working at the observatory, used tens of thousands of celestial photographs to classify stellar spectra, which are patterns of lines formed by dispersing a star's light. This system allowed for the categorization of stars based on their spectral characteristics and was foundational for future astronomical work, including the discovery of numerous celestial objects and the establishment of photographic standards for measuring stellar brightness.12
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