Discovery image of comet 103P?Hartley at 1986 03 15.59361 Anglo-Australian Observatory (AAO) with the UK Schmidt Telescope |
Subsequent observations in April 1986 by Oak Ridge Observatory and Palomar Observatory were submitted and the orbit refined confirming that the comet was had an elliptical orbit, e < 1, and was periodic with a short period (P < 200 years).
Perihelion Date T = 1985 June 5.053 ET
Perihelion distance q = 0.96099 AUeccentricty e = 0.71563
inclination i = 9.181 degrees
Period 6.21 years
Peri. = 174.670
Node = 226.609
semi-major axis a = 3.37933 AU
Daily orbital motion n = 0.158657 degrees/day
The 1986 computed orbit shows that comet 103P/Hartley passed close to Jupiter on November 1982 and again in December 1993
Kazuo Kinoshita Comet Orbit Page for 103P shows close approach to Jupiter:
Jupiter 0.3255 AU on 19821102.5
Jupiter 0.3743 AU on 19931219.3
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MPC observatory code 413Code Long. cos sin Name
413 149.06608 0.855595 -0.516262 Siding Spring Observatory
The UK Schmidt Telescope (UKST) has an aperture of 1.2 metres and a very wide-angle field of view. The telescope was commissioned in 1973. The telescope was designed to photograph 6.6 x 6.6 degree areas of the night sky on plates 356 x 356 mm (14 x 14 inches) square.
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Using MPCOBS on the Minor Planet Center web site
1986 observations of comet 103P:
0103PJ86E020 A1986 03 15.59361 11 25 25.15 -07 44 15.6 17.5 T 10592413
0103PJ86E020 A1986 03 17.67951 11 23 26.88 -07 27 42.7 10592413
0103PJ86E020 A1986 03 20.60691 11 20 45.41 -07 04 21.9 10592413
0103PJ86E020 A1986 04 04.12772 11 09 13.39 -05 11 29.2 10592801
0103PJ86E020 A1986 04 05.16007 11 08 32.84 -05 03 52.1 10592801
0103PJ86E020 A1986 04 05.20583 11 08 30.96 -05 03 31.3 18 T 10592675
0103PJ86E020 A1986 04 05.21069 11 08 30.75 -05 03 28.7 10592675
0103PJ86E020 A1986 04 05.21750 11 08 30.50 -05 03 26.0 10592675
0103PJ86E020 A1986 04 08.15569 11 06 41.19 -04 42 22.9 10592675
0103PJ86E020 A1986 04 08.16097 11 06 40.99 -04 42 20.5 10592675
0103PJ86E020 A1986 04 08.17083 11 06 40.64 -04 42 16.4 10592675
0103PJ86E020 A1986 05 10.15791 10 58 11.07 -01 59 12.5 10794691
0103PJ86E020 A1986 05 10.17935 10 58 11.11 -01 59 08.3 10794691
0103PJ86E020 A1986 05 10.19726 10 58 11.16 -01 59 04.9 10794691
0103PJ86E020 A1986 05 12.08925 10 58 17.95 -01 53 34.6 10794801
0103PJ86E020 A1986 06 07.15793 11 05 31.14 -01 23 08.0 10892691
0103PJ86E020 A1986 06 07.16865 11 05 31.41 -01 23 08.9 10892691
0103PJ86E020 A1986 06 07.22340 11 05 32.86 -01 23 09.9 10892691
IAUC 4197 1986 March 24
COMET HARTLEY (1986c) Malcolm Hartley, U.K. Schmidt Telescope Unit, Siding Spring, reports his discovery of a comet of magnitude ~ 17-18 with a faint tail evident: 1986 UT R.A. (1950.0) Decl. Mar. 15.59361 11 22 52.78 - 7 27 45.7 17.67951 11 20 54.53 - 7 11 14.2 20.60691 11 18 13.08 - 6 47 55.4 The following parabolic orbital elements are very uncertain. A low-inclination, short-period orbit gives similar residuals. T = 1985 June 20.07 ET Peri. = 185.39 Node = 179.23 1950.0 q = 0.0759 AU Incl. = 59.76 1986 ET R.A. (1950.0) Decl. p r m1 Mar. 11 11 27.33 - 8 04.2 3.476 4.452 17.2 21 11 17.86 - 6 44.8 31 11 09.42 - 5 27.2 3.733 4.678 17.6 Apr. 10 11 02.34 - 4 15.0 20 10 56.79 - 3 11.1 4.118 4.898 18.0 30 10 52.84 - 2 17.0 May 10 10 50.41 - 1 33.4 4.594 5.114 18.4 20 10 49.40 - 1 00.2 30 10 49.65 - 0 36.8 5.120 5.325 18.8 1986 March 24 (4197) Daniel W. E. Green
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IAUC 4200: 1986c;
References:
UK Schmidt Telescope (UKST): http://www.aao.gov.au/ukst/
IAUC 4197: http://www.cfa.harvard.edu/iauc/04100/04197.html
IAUC 4200: http://www.cfa.harvard.edu/iauc/04200/04200.html
Seiichi Yoshida Comet Page: http://www.aerith.net/comet/catalog/0103P/index.html
IAUC 4200: 1986c;
PERIODIC COMET HARTLEY 2 (1986c) The following precise positions have been reported: 1986 UT R.A. (1950.0) Decl. m1 Observer Apr. 5.16007 11 06 00.40 - 4 47 36.4 Schwartz 5.20583 11 05 58.52 - 4 47 15.6 18 Gibson 5.21069 11 05 58.31 - 4 47 13.0 " 5.21750 11 05 58.06 - 4 47 10.3 " G. Schwartz (Oak Ridge Observatory). 1.5-m reflector. Weak image. Measurer: C.-Y. Shao. J. Gibson (Palomar Observatory). 1.5-m reflector + CCD. A computation from the observations Mar. 15-Apr. 5 confirms this to be a short-period comet (cf. IAUC 4197). The solar elongation would have been too small to permit observations near perihelion. The revolution period is somewhat uncertain, but the comet evidently made a rather close approach to Jupiter in 1982. T = 1985 June 5.053 ET Peri. = 174.670 e = 0.71563 Node = 226.609 1950.0 a = 3.37933 AU Incl. = 9.181 n = 0.158657 q = 0.96099 AU P = 6.21 years 1986 ET R.A. (1950.0) Decl. p r m1 Mar. 31 11 09.61 - 5 26.2 2.362 3.312 17.6 Apr. 10 11 03.09 - 4 13.4 20 10 58.59 - 3 10.7 2.641 3.446 18.0 30 10 56.16 - 2 20.6 May 10 10 55.68 - 1 43.8 3.001 3.575 18.4 20 10 56.98 - 1 20.1 30 10 59.81 - 1 08.7 3.407 3.699 18.8 June 9 11 03.96 - 1 08.3 19 11 09.21 - 1 17.7 3.825 3.818 19.2 29 11 15.36 - 1 35.7 July 9 11 22.25 - 2 01.1 4.230 3.932 19.6
1986 April 8 (4200) Brian G. Marsden
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Comet 103P/Hartley 2 (1986c) on November 2, 1982 near Jupiter |
Comet 103P/Hartley 2 (1986c) on June 5, 1985 at perihelion. Comet elongation low |
Comet 103P/Hartley 2 (1986c) on March 15, 1986 at discovery. Comet near earth opposition. |
Comet 103P/Hartley 2 (1986c) on December 19, 1993 near Jupiter |
References:
UK Schmidt Telescope (UKST): http://www.aao.gov.au/ukst/
IAUC 4197: http://www.cfa.harvard.edu/iauc/04100/04197.html
IAUC 4200: http://www.cfa.harvard.edu/iauc/04200/04200.html
Seiichi Yoshida Comet Page: http://www.aerith.net/comet/catalog/0103P/index.html
Kazuo Kinoshita Comet Orbit Home Page: http://jcometobs.web.fc2.com/pcmtn/0103p.htm
Cometary Orbit Viewer: http://www.astroarts.com/simulation/cometary-orbit.php
CDS Image Server discovery image of comet 103P from the "Second Epoch Survey" of the southern sky was made by the Anglo-Australian Observatory (AAO) with the UK Schmidt Telescope digitized and compressed by the SScI: http://aladin.u-strasbg.fr/java/alapre-ok.pl?-c=11+25+25.15+-07+44+15.6&out=image&fmt=FITS&resolution=FULL&qual=SERC+ER+DSS2
CDS Image Server discovery image of comet 103P from the "Second Epoch Survey" of the southern sky was made by the Anglo-Australian Observatory (AAO) with the UK Schmidt Telescope digitized and compressed by the SScI: http://aladin.u-strasbg.fr/java/alapre-ok.pl?-c=11+25+25.15+-07+44+15.6&out=image&fmt=FITS&resolution=FULL&qual=SERC+ER+DSS2