Minorplanet: | yes |
1824 Haworth | |
Background: |
|
Discovered: | 30 March 1952 |
Discoverer: | Indiana University |
Mpc Name: | (1824) Haworth |
Alt Names: | 1952 FM1942 GC 1951 CA1952 HW 1957 HQ1957 LA 1974 XA |
Named After: | Leland J. Haworth |
Epoch: | 4 September 2017 (JD 2458000.5) |
Uncertainty: | 0 |
Observation Arc: | 110.25 yr (40,268 days) |
Perihelion: | 2.7603 AU |
Semimajor: | 2.8837 AU |
Eccentricity: | 0.0428 |
Period: | 4.90 yr (1,789 days) |
Mean Motion: | / day |
Inclination: | 1.9299° |
Asc Node: | 15.034° |
Arg Peri: | 69.949° |
Dimensions: | km |
Abs Magnitude: | 11.4 |
1824 Haworth (prov. designation:) is an asteroid from the outer region of the asteroid belt, approximately 14 kilometers in diameter. It was discovered on 30 March 1952, by Indiana University's Indiana Asteroid Program at its Goethe Link Observatory near Brooklyn, Indiana, United States, and named after physicist Leland John Haworth.
Haworth orbits the Sun in the outer main-belt at a distance of 2.8–3.0 AU once every 4 years and 11 months (1,789 days). Its orbit has an eccentricity of 0.04 and an inclination of 2° with respect to the ecliptic.
Its first precovery was taken at Lowell Observatory in 1906, extending the body's observation arc by 46 years prior to its official discovery observation at Goethe Link.
It was named in honor of American particle physicist Leland John Haworth (1904–1979), a graduate of Indiana University and second director of the National Science Foundation.
His long and varied career included teaching and serving as member of the Atomic Energy Commission, as vice-president and president of Associated Universities, Inc., and as director of the Brookhaven National Laboratory. His negotiations were instrumental for the funding of a 4-meter telescope at the Cerro Tololo Interamerican Observatory. The official was published by the Minor Planet Center on 18 April 1977 .
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Haworth measures 14.17 kilometers in diameter and its surface has an albedo of 0.266. As of 2017, its composition, rotation period and shape remain unknown.