![]() Shape of Hopmann modeled from its
lightcurve | |
Discovery [1] | |
---|---|
Discovered by | K. Reinmuth |
Discovery site | Heidelberg Obs. |
Discovery date | 13 January 1929 |
Designations | |
(1985) Hopmann | |
Named after |
Josef Hopmann (German astronomer) [2] |
1929 AE · 1951 CA2 1951 CP · 1952 KE 1964 PJ · 1973 AA4 | |
main-belt · ( outer) [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 88.16 yr (32,201 days) |
Aphelion | 3.6021 AU |
Perihelion | 2.6408 AU |
3.1214 AU | |
Eccentricity | 0.1540 |
5.51 yr (2,014 days) | |
334.27 ° | |
0° 10m 43.32s / day | |
Inclination | 17.159° |
305.15° | |
234.25° | |
Physical characteristics | |
35.47 km (derived)
[3] 35.51±3.1 km ( IRAS:6) [1] 44.33±3.53 km [4] | |
17.476±0.003
h
[5] 17.478±0.004 h [6] 17.4787±0.0001 h [7] 17.480±0.002 h [8] | |
0.039±0.007 (IRAS:6)
[4] 0.0613 (derived) [3] | |
C [3] | |
10.75±0.19 [9] · 10.9 [1] [3] · 10.91 [4] | |
1985 Hopmann ( prov. designation: 1929 AE) is a dark background asteroid in the outer regions of the asteroid belt. It was discovered on 13 January 1929, by astronomer Karl Reinmuth at Landessternwarte Heidelberg-Königstuhl in southern Germany. [10] The asteroid has a rotation period of 17.5 hours and measures approximately 36 kilometers (22 miles) in diameter. It was later named after German astronomer Josef Hopmann (1890–1975). [2]
Hopmann is a dark C-type asteroid that orbits the Sun in the outer main-belt at a distance of 2.6–3.6 AU once every 5 years and 6 months (2,014 days). Its orbit has an eccentricity of 0.15 and an inclination of 17 ° with respect to the ecliptic. [1] The first observation used for the body's observation arc was taken at the discovering observatory on 4 February 1926, or 22 days after its official discovering observation. [10]
This minor planet was named in memory of German astronomer Josef Hopmann (1890–1975), a director of Vienna Observatory between 1951 and 1962, a productive observer of variable and binary stars, and a participant in the international program to observe near-Earth asteroid 433 Eros in the early 1930s. The lunar crater Hopmann is also named in his honour. [2] The official naming citation was published by the Minor Planet Center on 15 October 1977 ( M.P.C. 4237). [11]
According to the survey carried out by the Infrared Astronomical Satellite IRAS, Hopmann measures 35.51 kilometers in diameter. [1] The Collaborative Asteroid Lightcurve Link agrees with the Supplemental IRAS Minor Planet Survey (SIMPS) data and derives an albedo of 0.039 and a diameter of 35.47 kilometers, [3] while observations with NASA's Wide-field Infrared Survey Explorer and its subsequent NEOWISE mission gave an albedo of 0.06 and a diameter of 44.33 kilometers. [4]
In January and February 2012, three rotational lightcurves were obtained by Robert Stephens at Santana Observatory ( 646), California, Josep Maria Aymami at Carmelita Observatory ( B20), Barcelona, and Patricia Moravec at Oakley Southern Sky Observatory ( E09), Australia. The lightcurves gave a well-defined rotation period of 17.476, 17.478 and 17.480 hours, respectively, with a brightness variation between 0.36 and 0.44 magnitude ( U=3/3/3-). [5] [6] [8] In 2016, a re-modeled lightcurve, constructed from data compiled in the Lowell Photometric Database, also gave a concurring period. [7]