Edward Emerson Barnard

Edward Emerson Barnard studied at Vanderbilt University. The recorded working language is English. The field of work recorded is astronomy. Employment is recorded with University of Chicago, Lick Observatory and Vanderbilt University. Work by Edward Emerson Barnard is recorded in the collections of Museum of New Zealand Te Papa Tongarewa. Distinctions recorded are Prix Jules Janssen, Gold Medal of the Royal Astronomical Society, Lalande Prize and Bruce Medal.

• Name — Edward Emerson Barnard • Born — 16 December 1857 • Birthplace — Nashville, Tennessee, U.S. • Died — 6 February 1923 • Place of death — Williams Bay, Wisconsin, U.S. • Field — Astronomy • Workplaces — Lick Observatory, University of Chicago • Known for — * Barnard's Star • Barnard's Loop • astrophotography • Awards — * Lalande Prize (1892) • Gold Medal of the Royal Astronomical Society (1897) • Janssen Medal (1900) • Prix Jules Janssen (1906) • Bruce Medal (1917)

Barnard was born in Nashville, Tennessee, on December 16, 1857, to Reuben Barnard and Elizabeth Jane Barnard (née Haywood), and had one brother. His father died three months before his birth, so he grew up in an impoverished family and did not receive much in the way of formal education. His first interest was in the field of photography, and he became a photographer's assistant at the age of nine. He later developed an interest in astronomy. In 1876 he purchased a 5 in refractor telescope, and in 1881 he discovered his first comet, but failed to announce his discovery. He found his second comet later the same year and a third in 1882. While he was still working at a photography studio he was married to the British-born Rhoda Calvert in 1881. In the 1880s, Hulbert Harrington Warner offered per discovery of a new comet. Barnard discovered a total of five, and used the money to build a house for himself and his wife, Rhoda Barnard (née Calvert). With his name being brought to the attention of amateur astronomers in Nashville, they collectively raised enough money to give Barnard a fellowship to Vanderbilt University. He never graduated from the school, but did receive the only honorary degree Vanderbilt has ever awarded. He joined the staff of the Lick Observatory in California in 1887, though he later clashed with the director, Edward S. Holden, over access to observing time on the larger instruments and other issues of research and management.

• Illustration — Barnard at the Fourth Conference International Union for Cooperation in Solar Research at Mount Wilson Observatory, 1910 Barnard observed the gegenschein in 1882, not aware of earlier papers by Theodor Brorsen and T. W. Backhouse. In 1889, he observed the moon Iapetus pass behind Saturn's rings. As he watched Iapetus pass through the space between Saturn's innermost rings and the planet itself, he saw a shadow pass over the moon. Although he did not realize it at the time, he had discovered proof of the "spokes" of Saturn, dark shadows running perpendicular to the circular paths of the rings. These spokes were doubted at first, but confirmed by the spacecraft Voyager 1. In 1892, he made observations of a nova and was the first to notice the gaseous emissions, thus correctly deducing that it was a stellar explosion. The same year he also discovered Amalthea, the fifth moon of Jupiter. He was the first to discover a new moon of Jupiter since Galileo Galilei in 1609. This was the last satellite discovered by direct visual observation (rather than by examining photographic plates or other recorded images). In 1895, he joined the University of Chicago as professor of astronomy. There he was able to use the 40 in telescope at Yerkes Observatory. Much of his work during this period was taking photographs of the Milky Way. Together with Max Wolf, he discovered that certain dark regions of the galaxy were actually clouds of gas and dust that obscured the more distant stars in the background. From 1905, his niece Mary R. Calvert worked as his assistant and computer. The faint Barnard's Star is named for Edward Barnard after he discovered in 1916 that it had a large proper motion relative to other stars. This is the second nearest star system to the Sun, second only to the Alpha Centauri system. He was also a pioneering astrophotographer. His Barnard Catalogue lists a series of dark nebulae, known as Barnard objects, giving them numerical designations akin to the Messier catalog. They begin with Barnard 1 and end with Barnard 370. He published his initial list in a 1919 paper published in the Astrophysical Journal, titled "On the Dark Markings of the Sky with a Catalogue of 182 such Objects". He died on February 6, 1923, in Williams Bay, Wisconsin, and was buried in Nashville. After his death, many examples from his exceptional collection of astronomical photographs were published in 1927 as A Photographic Atlas of Selected Regions of the Milky Way, this work having been finished by Mary R. Calvert and Edwin B. Frost, then director of Yerkes Observatory.

Between 1881 and 1892, he discovered 15 comets, three of which were periodic, and co-discovered two others: • C/1881 did not announce • C/1881 S1 • C/1882 R2 • D/1884 O1 (Barnard 1) • C/1885 N1 • C/1885 X2 • C/1886 T1 (Barnard–Hartwig) • C/1887 B3 • C/1887 D1 • C/1887 J1 • C/1888 U1 • C/1888 R1 • C/1889 G1 • 177P/Barnard (P/1889 M1, P/2006 M3, Barnard 2) • C/1891 F1 (Barnard–Denning) • C/1891 T1 • D/1892 T1 (Barnard 3) – First comet to be discovered by photography; recovered in late 2008 as 206P/Barnard–Boattini

Edward Emerson Barnard worked in astronomy. He was employed by University of Chicago, Lick Observatory and Vanderbilt University.