description R. Paul Butler Overview
R. Paul Butler is an American astronomer known for developing highly precise radial-velocity methods used to detect planets outside the Solar System. Working with collaborators including Geoffrey Marcy, he contributed to the discovery and characterization of numerous exoplanets by measuring the small Doppler shifts produced as orbiting planets tug on their host stars. His work included the detection of a multiplanet system around Upsilon Andromedae and helped establish radial velocity as a central exoplanet-search technique.
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How did R. Paul Butler and Geoffrey Marcy discover the first extrasolar planets?
R. Paul Butler and Geoffrey Marcy revolutionized astronomy in the 1990s by developing highly precise radial-velocity techniques to detect the gravitational wobble of distant stars. Their method led to the discovery of numerous exoplanets, including those orbiting 70 Virginis and 47 Ursae Majoris.
Did R. Paul Butler work at the Carnegie Institution for Science?
Yes, following his pioneering work at San Francisco State University, Butler became a staff astronomer at the Carnegie Institution for Science's Department of Terrestrial Magnetism. At Carnegie, he continued to lead planet-hunting surveys using telescopes at the Las Campanas Observatory in Chile.
What awards did R. Paul Butler receive for his exoplanet research?
For his groundbreaking discoveries in the mid-1990s, Butler received numerous major astronomical accolades, including the Henry Draper Medal from the National Academy of Sciences. He was also named a co-recipient of the inaugural Peter Gruber Foundation Cosmology Prize.
How does R. Paul Butler's radial velocity method actually detect a planet?
Instead of seeing the planet directly, the radial velocity method detects the tiny Doppler shift in the star's light caused by the planet's gravitational pull as it orbits. Butler refined the computer algorithms and iodine vapor absorption cells needed to measure these minute shifts in stellar light spectra.
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