David C. Jewitt

Jewitt was born in London, England, in 1958. His mother was a telephonist, and his father worked on an assembly line making industrial steel cutters. ==Education==

Jewitt was educated at local authority primary and secondary schools. He was also an autodidact, borrowing books from a travelling library to supplement the few that his parents could afford to buy for him. His interest in physics began when a teacher introduced him to the subject, of which he had never previously heard, when he was twelve or thirteen. In 1976, supported by a local authority grant, Jewitt enrolled at University College London to take courses in astronomy, physics, mathematics, computing, electronics, metalwork and technical drawing, studying both at UCL's Gower Street campus and at the UCL Observatory (then called the University of London Observatory) in Mill Hill. The module that he enjoyed most was a panoramic survey of physics delivered by the Christian, Rolls-Royce-driving space scientist Professor Sir Robert Boyd. Together with his friend, the future poet and environmental activist Roly Drower, Jewitt graduated with a first class honours B.Sc. in astronomy in 1979. Following the advice of UCL's Professor Michael Dworetsky, Jewitt decided to pursue his postgraduate studies at the California Institute of Technology in Pasadena. He became an Anthony Fellow at Caltech in 1979, achieving an M.S. in planetary science in 1980. After investigating planetary nebulae and comets with the 200 inch Hale Telescope of the Mount Palomar Observatory, working with Ed Danielson and Gerry Neugebauer under the supervision of Professor James Westphal, he was awarded a Ph.D. in planetary science and astronomy in 1983. He has recalled his adventures in the Hale's vertiginous prime focus cage as occasionally a risk to life and limb. ==Career==

In 1983, Jewitt became an assistant professor at the Massachusetts Institute of Technology in Cambridge, Massachusetts. In 1988, attracted by the powerful telescopes sited on Mauna Kea, he moved to the University of Hawaiʻi, becoming an Associate Astronomer in its Institute of Astronomy and an associate professor in its Department of Physics and Astronomy. In 1993, the Institute promoted him to the rank of Astronomer tout court. In 2009, Jewitt returned to the American mainland to work at the University of California, Los Angeles, becoming a Member of UCLA's Institute of Geophysics and Planetary Physics and a professor in what was then its Department of Earth and Space Sciences. In 2010 he was given a second chair, becoming a professor in UCLA's Department of Physics and Astronomy. In 2011, he became the Director of UCLA's Institute for Planets and Exoplanets. ==Research==

Jewitt's research interests have embraced many topics in planetary science, including the Kuiper belt, circumstellar discs, planetary ring systems, the physical properties of comets, frozen volatiles in asteroids, the moons of the gas giant planets and the formation and evolution of the Solar System. In 1992, after five years of searching, Jewitt and the Vietnamese-American astronomer Jane X. Luu discovered 15760 Albion, the first Kuiper belt object (other than Pluto and its largest moon Charon) to be detected. Jewitt and Luu named the object after a character who features in the mythological poetry of William Blake, a writer whom Jewitt admires. (Blake in turn took the name from an ancient poetic term for Jewitt's native England.) Jewitt and Luu would have preferred to name the object Smiley after the protagonist of John le Carré's novel Tinker, Tailor, Soldier, Spy, a favourite book of both of theirs, but they were unable to do so because the name had already been allocated to the asteroid 1613 Smiley in honour of Charles Hugh Smiley, an American astronomer. Since discovering 15760 Albion, Jewitt has identified dozens of other objects in the Kuiper belt in a series of pioneering wide field surveys. Thanks to his work and the efforts of other astronomers, it is now known that the Kuiper belt objects are divided into four distinct populations. In what is called the dynamically cold classical Kuiper belt, of which 15760 Albion is the prototypical member, objects have orbits that are almost circular and only slightly tilted with respect to the orbits of the major planets. In the dynamically hot classical Kuiper belt, objects have orbits that are more elongated and that are tilted at steeper angles. In the scattered disc, also called the scattered Kuiper belt, discovered in 1997, bodies move in large orbits that are more elongated and more tilted still. The Resonant Kuiper belt objects move in orbits that are harmonically related to that of Neptune: the ratio of the orbital period of a resonant object to the Neptunian year is equal to one small integer divided by another. (The resonant objects in the 3:2 mean-motion resonance Jewitt has named plutinos, in recognition of Pluto's being the first of them to be discovered.) Mathematical models of the formation and evolution of the Solar System have indicated that in order for the Kuiper belt to have developed the structure that has been observed, the Kuiper belt objects and the gas giant planets must have come to their present orbits after migrating to them from elsewhere, pulled away from their earlier paths by their gravitational interactions with one another and with the disc of material that had coalesced around the juvenile Sun. In particular, it seems that Neptune long ago moved outward from an earlier orbit that was much closer to the Sun, and that the Kuiper belt objects, also originally closer to the Sun, were drawn outward with it. In 1979, in his first months as a graduate student, Jewitt discovered the Jovian moon Adrastea on images taken by Voyager 2. He has since discovered more than seventy further moons of Jupiter, Saturn, Uranus and Neptune. In 1982, he achieved worldwide fame as the first astronomer to recover Halley's Comet as it approached its 1986 perihelion, detecting it with the Hale telescope using an early CCD. He is credited by the Minor Planet Center with the discovery of more than forty asteroids. The inner main-belt asteroid 6434 Jewitt, discovered by Edward Bowell in 1981, was named in his honour. In the naming citation, published on 1 July 1996, Jane Luu described Jewitt as "the consummate astronomer" (). ==Controversies==

When Pluto was first discovered, it was added to the canonical list of major planets. After Jewitt and Luu's discovery of 15760 Albion and the subsequent finding of many more Kuiper belt objects, it became apparent that Pluto had more in common with these objects than it did with its supposed planetary peers. Some astronomers suggested that Pluto should be demoted. Jewitt thought that the question of whether Pluto was a planet was "essentially bogus" and "scientifically [...] a non-issue", but ultimately agreed with the International Astronomical Union's 2006 decision to reclassify Pluto as a dwarf planet. With the development of ever better telescopes and detectors, astronomers have been able to find moons that are ever smaller and smaller. Some astronomers have argued that moons smaller than some arbitrary size are unworthy of their title. Jewitt has dissented, asking "Is a small dog not a dog because it is small?" ==Outreach==

In October 1982, Patrick Moore interviewed Jewitt about his recovery of Halley's Comet in a special episode of BBC TV's The Sky at Night. A quarter of a century later, Horizon returned to Jewitt to interview him for Asteroids: the Good, the Bad and the Ugly (Season 47, Episode 6). Jewitt told viewers that he had found it difficult to secure enough telescope time for his trans-Neptunian research, and had only been able to achieve his celebrated breakthrough by looking for Kuiper belt objects on nights when he was supposed to be working on other projects. Jewitt has also explained his work to non-specialists in articles in Scientific American, Sky and Telescope and The Sky at Night BBC Magazine. ==Honours==

In 1994, Jewitt was awarded the University of Hawaiʻi's Regent's Medal for excellence in research. ==Personal life==

In 1991, Jewitt met Jing Li (a Chinese-American born in Beijing, China), a Ph.D. student of solar physics at the University of Paris, while she was visiting the University of Hawaiʻi. ==Select bibliography==

} || 27 February 1995 • with J. X. Luu • with J. Chen • with C. A. Trujillo • with K. Berney • with D. J. Tholen • with S. S. Sheppard • with J. T. Kleyna • credited to Mauna Kea Observatories A complete, up to date list of Jewitt's more than two hundred academic publications is available via his UCLA website. His magazine articles for general readers are: • J. Luu and D. Jewitt: The Kuiper belt; Scientific American, May 1996 • D. Jewitt, S. Sheppard and J. Kleyna: The strangest satellites in the Solar System; Scientific American, August 2006 • D. Jewitt: What else is out there?; Sky and Telescope, March 2010 • D. Jewitt: Mysterious travelers; Sky and Telescope. December 2013 • D. Jewitt and E. Young: Oceans from the skies; Scientific American, March 2015 • D. Jewitt: The Kuiper belt; The Sky at Night BBC Magazine, November 2015 ==References==