87P/Bus

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87P/Bus
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Comet 87P/Bus photographed by the Hubble Space Telescope on 7 June 2001
Discovery[1]Template:R/superscript
Discovered bySchelte J. Bus
Discovery siteSiding Spring Observatory
(UK Schmidt Telescope)
Discovery date2 March 1981
Designations
P/1981 E1, P/1987 B4
Template:Unbulleted
Orbital characteristics[3]Template:R/superscript[4]Template:R/superscript
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]Template:R/superscript
TJupiter3.009
Earth MOID1.098 AU
Jupiter MOID0.181 AU
Physical characteristics[5]Template:R/superscript
Mean radius
0.27±0.01 km
32.0±9.0 hours
(V–R) = 0.545±0.02[6]Template:R/superscript
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

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]Template:R/superscript 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]Template:R/superscript Preliminary orbital calculations in 9 March 1981 had Brian G. Marsden to conclude that the comet may be a short-periodic one,[8]Template:R/superscript which was later confirmed after Bus was able to find precovery images as early as 9–13 February 1981.[9]Template:R/superscript

It has been observed on each of its subsequent apparitions, most recently in 2020.[10]Template:R/superscript

Physical characteristics

Preliminary CCD photometry from the La Palma Observatory in December 1998 obtained an upper limit value of around Template:Cvt for the comet's nuclear radius.[11]Template:R/superscript 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]Template:R/superscript Hubble data also showed the comet to be elongated in shape, with an a/b ratio greater than 2.2.[5]Template:R/superscript Its rotational period is estimated to be around 32.0±9.0 hours in length.[5]Template:R/superscript

Orbit

Perihelion distance
at different epochs
[12]Template:R/superscript
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]Template:R/superscript

References

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  1. ^ a b Page Module:Citation/CS1/styles.css has no content.S. J. Bus; K. S. Russell (4 March 1981). D. W. Green (ed.). "Comet Bus (1981b)". IAU Circular. 3578 (1). Bibcode:1981IAUC.3578....1B. ISSN 0081-0304.
  2. ^ Page Module:Citation/CS1/styles.css has no content."Horizons Batch for 87P/Bus (90000883) on 2029-Jun-07" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Retrieved 27 June 2022. (JPL#K203/18 Soln.date: 2020-Sep-28)
  3. ^ Page Module:Citation/CS1/styles.css has no content."87P/Bus – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 20 March 2016.
  4. ^ Page Module:Citation/CS1/styles.css has no content."87P/Bus Orbit". Minor Planet Center. Retrieved 16 June 2014.
  5. ^ a b c d Page Module:Citation/CS1/styles.css has no content.P. L. Lamy; I. Toth; H. A. Weaver; M. F. A'Hearn; L. Jorda (2011). "Properties of the nuclei and comae of 10 ecliptic comets from Hubble Space Telescope multi-orbit observations" (PDF). Monthly Notices of the Royal Astronomical Society. 412 (3): 1573–1590. doi:10.1111/j.1365-2966.2010.17934.x.
  6. ^ Page Module:Citation/CS1/styles.css has no content.K. J. Meech; O. R. Hainaut; B. G. Marsden (2004). "Comet nucleus size distributions from HST and Keck telescopes". Icarus. 170 (2): 463–491. Bibcode:2004Icar..170..463M. doi:10.1016/j.icarus.2004.03.014.
  7. ^ Page Module:Citation/CS1/styles.css has no content.S. J. Bus; K. S. Russell (5 March 1981). B. G. Marsden (ed.). "Comet Bus (1981b)". IAU Circular. 3579 (1). Bibcode:1981IAUC.3579....1B. ISSN 0081-0304.
  8. ^ Page Module:Citation/CS1/styles.css has no content.C. Y. Shao; G. Schwartz; T. Seki (9 March 1981). B. G. Marsden (ed.). "Comet Bus (1981b)". IAU Circular. 3581 (2). Bibcode:1981IAUC.3581....2S. ISSN 0081-0304.
  9. ^ Page Module:Citation/CS1/styles.css has no content.S. J. Bus; K. S. Russell; M. Hartley (10 March 1981). B. G. Marsden (ed.). "Periodic Comet Bus (1981b)". IAU Circular. 3582 (1). Bibcode:1981IAUC.3582....1B. ISSN 0081-0304.
  10. ^ Page Module:Citation/CS1/styles.css has no content.S. Yoshida. "87P/Bus". www.aerith.net. Retrieved 15 May 2015.
  11. ^ Page Module:Citation/CS1/styles.css has no content.S. C. Lowry; A. Fitzsimmons (1999). "CCD photometry of distant comets II" (PDF). Astronomy & Astrophysics. 365: 204–213. Bibcode:1999A&A...349..649L. doi:10.1051/0004-6361:20000180.
  12. ^ a b Page Module:Citation/CS1/styles.css has no content.K. Kinoshita (13 February 2014). "87P/Bus: Past, Present and Future orbital elements". Comet Orbit. Retrieved 13 November 2024.

Bibliography


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