Currently, 1983 Bok has gained great relevance in different areas of society. Its impact has been felt in the economy, politics, culture and people's daily lives. This phenomenon has aroused great interest and has generated controversy in various sectors, who seek to understand the implications and consequences that 1983 Bok has in today's society. This is why it is crucial to explore this issue in depth, analyzing its causes, effects and possible solutions to address the challenges it poses. In this article, the impact of 1983 Bok on different aspects of modern life will be comprehensively addressed, with the aim of providing the reader with a complete and detailed vision of this issue that is so relevant today.
![]() Modelled shape of Bok from its lightcurve | |
Discovery[1] | |
---|---|
Discovered by | E. Roemer |
Discovery site | Catalina Stn. |
Discovery date | 9 June 1975 |
Designations | |
(1983) Bok | |
Named after | Bart Bok and Priscilla Fairfield Bok[2] |
1975 LB · 1950 RV 1963 UJ | |
main-belt · (middle)[3] | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 66.73 yr (24,372 days) |
Aphelion | 2.8796 AU |
Perihelion | 2.3632 AU |
2.6214 AU | |
Eccentricity | 0.0985 |
4.24 yr (1,550 days) | |
260.33° | |
0° 13m 55.92s / day | |
Inclination | 9.4133° |
23.557° | |
346.78° | |
Physical characteristics | |
10.08 km (calculated)[3] 15±3 km[4] 15.70±0.24 km[5] | |
10.70±0.01 h[4] | |
0.034±0.015[5] 0.06±0.02[4] 0.10 (assumed)[3] | |
C[4] · S/C[3] | |
12.83±0.10[4] · 13.1[1][3] · 13.10±0.22[6] · 13.32[5] | |
1983 Bok (prov. designation: 1975 LB) is a dark background asteroid from the central region of the asteroid belt. It was discovered on 9 June 1975, by American astronomer Elizabeth Roemer at the Catalina Station of the UA's Steward Observatory in Tucson, Arizona, and named for Bart Bok and Priscilla Fairfield Bok.[2][7] The carbonaceous C-type asteroid has a rotation period of 10.7 hours and measures approximately 15 kilometers (9.3 miles) in diameter.
Bok orbits the Sun in the central main-belt at a distance of 2.4–2.9 AU once every 4 years and 3 months (1,550 days). Its orbit has an eccentricity of 0.10 and an inclination of 9° with respect to the ecliptic.[1] The first observation was taken at the Argentinian La Plata Astronomical Observatory in 1950, extending the asteroid's observation arc by 25 years prior to its discovery.[7]
This minor planet was named after the astronomer couple Bart Bok (1906–1983) and Priscilla Fairfield Bok (1896–1975), in recognition for their contribution to astrometry of small Solar System bodies. Both astronomers studied the structure of the southern Milky Way and fostered astronomy in the Southern Hemisphere.
Bok was the first numbered discovery made with the Stewart Observatory's 90-inch Bok Telescope. The body's name was proposed by the discovering astronomer and by Alan C. Gilmore from New Zealand.[2] The official naming citation was published by the Minor Planet Center on 18 April 1977 (M.P.C. 4158).[8]
Bok has been characterized as a C-type asteroid.[4]
In October 2014, the first rotational lightcurve for this body was obtained by Italian astronomer Giovanni Battitsa Casalnuovo at the Eurac Observatory (C62) in Bolzano, Italy. Lightcurve analysis gave a well-defined rotation period of 10.70±0.01 hours with a relatively high brightness variation of 0.46 magnitude (U=3-).[4]
The Italian astronomer also calculated an albedo of 0.06 for its surface and a diameter of 15±3 kilometers, in agreement with the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer which gave a diameter of 15.7 kilometers and an albedo of 0.034.[5]
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.10, a compromise value between the stony (0.20) and carbonaceous (0.057) asteroids with a semi-major axis between 2.6 and 2.7 AU, and consequently calculates a much smaller diameter of 10.08 kilometers using an absolute magnitude of 13.1.[3]