87P/Bus

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87P/Bus
File:Comet 87P Bus u65z1f02r.fits.gz sci.jpg
Comet 87P/Bus photographed by the Hubble Space Telescope on 7 June 2001
Discovery[1]
Discovered bySchelte J. Bus
Discovery siteSiding Spring Observatory
(UK Schmidt Telescope)
Discovery date2 March 1981
Designations
P/1981 E1, P/1987 B4
  • 1981 XI, 1987 XXXIV
  • 1994 XVI
  • 1981b, 1987f, 1993b
Orbital characteristics[3][4]
Epoch31 May 2025 (JD 2459000.5)
Observation arc39.57 years
Earliest precovery date9 February 1981
Number of
observations
801
Aphelion4.776 AU
Perihelion2.099 AU
Semi-major axis3.438 AU
Eccentricity0.38918
Orbital period6.374 years
Inclination2.603°
181.87°
Argument of
periapsis
24.932°
Mean anomaly3.356°
Last perihelion9 May 2020
Next perihelion7 June 2029[2]
TJupiter3.009
Earth MOID1.098 AU
Jupiter MOID0.181 AU
Physical characteristics[5]
Mean radius
0.27±0.01 km
32.0±9.0 hours
(V–R) = 0.545±0.02[6]
Comet total
magnitude
(M1)
12.7
Comet nuclear
magnitude (M2)
16.1

87P/Bus is an Encke-type comet with a current orbital period of 6.37 years around the Sun. It is the only comet discovered by Australian astronomer, Schelte J. Bus.

Observational history

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It was discovered by Schelte J. Bus on the night of 2 March 1981 from a photographic plate taken with the 1.2m UK Schmidt telescope at the Siding Spring Observatory.[1] Additional observations by Kenneth S. Russell noticed a faint tail about 20 arcseconds in length to the northwest, estimated to be 17.5 in apparent magnitude.[7] Preliminary orbital calculations in 9 March 1981 had Brian G. Marsden to conclude that the comet may be a short-periodic one,[8] which was later confirmed after Bus was able to find precovery images as early as 9–13 February 1981.[9]

It has been observed on each of its subsequent apparitions, most recently in 2020.[10]

Physical characteristics

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Preliminary CCD photometry from the La Palma Observatory in December 1998 obtained an upper limit value of around 0.6–0.8 km (0.37–0.50 mi) for the comet's nuclear radius.[11] Later observations from the Hubble Space Telescope in 2009 revised the size of its nucleus, which is now estimated to be 0.27±0.01 km in radius.[5] Hubble data also showed the comet to be elongated in shape, with an a/b ratio greater than 2.2.[5] Its rotational period is estimated to be around 32.0±9.0 hours in length.[5]

Orbit

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Perihelion distance
at different epochs
[12]
Epoch Perihelion
(AU)
1942 4.43
1955 2.13
2029 3.69

A close approach to Jupiter on 13 May 1952, at a distance of 0.0668 AU (9.99 million km), lowered the orbital period from 12.46 years and the perihelion distance from 4.43 AU to 6.43 years and 2.13 AU respectively. Another close approach to Jupiter on 24 February 2023, at a distance of 0.182 AU (27.2 million km), raised the perihelion to 3.62 AU and the orbital period to 9.58 years.[12]

References

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  1. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  2. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). (JPL#K203/18 Soln.date: 2020-Sep-28)
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  12. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).

Bibliography

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  • Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
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