1952 Hesburgh

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1952 Hesburgh
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date3 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 arc77.14 yr (28,177 days)
Aphelion3.5522 AU
Perihelion2.6708 AU
3.1115 AU
Eccentricity0.1416
5.49 yr (2,005 days)
175.77°
0° 10m 46.56s / day
Inclination14.255°
78.149°
339.27°
Physical characteristics
Dimensions32.39±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]

Physical characteristics

Lightcurve

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]

Spectral type

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.

Diameter and albedo

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]

Naming

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]

Notes

References

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