Discovery [1] | |
---|---|
Discovered by |
Indiana University ( Indiana Asteroid Program) |
Discovery site | Goethe Link Obs. |
Discovery date | 3 May 1951 |
Designations | |
(1952) Hesburgh | |
Named after |
Theodore M. Hesburgh (University president) [2] |
1951 JC · 1936 ND 1939 AB · 1940 GQ 1954 XC · 1974 KQ | |
main-belt · ( outer) [3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 77.14 yr (28,177 days) |
Aphelion | 3.5522 AU |
Perihelion | 2.6708 AU |
3.1115 AU | |
Eccentricity | 0.1416 |
5.49 yr (2,005 days) | |
175.77 ° | |
0° 10m 46.56s / day | |
Inclination | 14.255° |
78.149° | |
339.27° | |
Physical characteristics | |
Dimensions | 32.39±8.33 km
[4] 35.55±1.4 km ( IRAS:15) [5] 37.501±0.151 km [6] 39.660±0.381 km [7] 41.27±1.19 km [8] |
47.7±0.1 h [9] [a] | |
0.078±0.005
[8] 0.080±0.012 [6] 0.0837±0.0130 [7] 0.10±0.03 [4] 0.1041±0.009 (IRAS:15) [5] | |
Tholen = CD:
[1] · CD:
[3] B–V = 0.756 [1] U–B = 0.340 [1] | |
10.31±0.33 [10] · 10.32 [1] [3] [5] [8] [7] [4] | |
1952 Hesburgh, provisional designation 1951 JC, is a rare-type carbonaceous asteroid from the outer regions of the asteroid belt, approximately 37 kilometers in diameter.
It was discovered on 3 May 1951, by IU's Indiana Asteroid Program at Goethe Link Observatory near Brooklyn, Indiana, United States. [11] It was named for Father Theodore M. Hesburgh. [2]
Hesburgh orbits the Sun in the outer main-belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,005 days). Its orbit has an eccentricity of 0.14 and an inclination of 14 ° with respect to the ecliptic. [1] It was first identified as 1936 ND at Johannesburg Observatory in 1936. The body's observation arc begins at Goethe, five days after its official discovery observation. [11]
In March 2005, a rotational lightcurve of Hesburgh was obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Lightcurve analysis gave a longer-than average rotation period of 47.7 hours with a brightness variation of at least 0.18 magnitude ( U=2). [9] [a]
In the Tholen taxonomy, Hesburgh is a rare CD: spectral type, [1] an intermediary between the common carbonaceous C-type asteroid and the dark D-type asteroid, which is typical among the Jupiter trojans beyond the main-belt. Another asteroid with a CD:-type is 691 Lehigh.
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Hesburgh measures between 32.39 and 41.27 kilometers in diameter and its surface has an albedo between 0.078 and 0.1041. [4] [5] [6] [7] [8] The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.1041 and a diameter of 35.55 kilometers with an absolute magnitude of 10.32. [3]
This minor planet was named after American Theodore M. Hesburgh (1917–2015), a priest and president of the University of Notre Dame in Notre Dame, Indiana. He was also a member of the National Science Board and played a decisive role for the founding of the Kitt Peak National Observatory, as well as of the Chilean Cerro Tololo Interamerican Observatory during the 1960s. [2] The approved naming citation was published by the Minor Planet Center on 1 January 1981 ( M.P.C. 5688). [12]