- reproduced with permission from Gary Kronk (personal communication,2024)
1P/760 K1 (Halley)
- Discovered: 760 May 15.8 (A=0.94 AU, r=0.59 AU, Elong.=35°)
- Last seen: 760 July
- Closest to the Earth: 760 June 2 (0.4105 AU)
- Calculated path: ARI (Disc), PER (May 22), AUR (May 29), LYN (Jun. 3), CNC (Jun. 6), LEO (Jun. 8), VIR (Jul. 10)
The Chiu T'ang shu (945), T'ang hui yao (961), and Hsin T'ang shu (1060) provide virtually identical details of this appearance of
1P/Halley. The comet is referred to as a "broom star" when it was first seen on 760 May 16 "in the east between Lou
[α, β, and γ Arietis] and Wei [35, 39, and 41 Arietis]." The date and location indicate a morning observation, implying a UT of May 15.8.
The comet is described as white and about 4° long. The details acquired from the Chiu T'ang shu and Hsin T'ang shu were obtained from
the astronomical chapters. It is interesting that the annals of these two texts say the comet was first seen on May 17.
The Chinese accounts say that it moved rapidly toward the northeast. It passed the Mao [the Pleiades], the Pi [α and ε Tauri],
the Tsui-Hsi [γ and φ
1 Orionis], the Shen [α, β, γ, δ, ζ, and κ Orionis], the Tung-Ching [γ, ε, ζ, λ, μ, ν, ξ, and 36 Geminorum),
the Yu-Kuei [γ, δ, η, and θ Cancri] the Liu [δ, ε, ζ, η, θ, ρ, σ, and ω Hydrae], and Hsien-Yuan [α, γ, ε, ζ, η, κ, λ, μ, o, ρ, and 15
Leonis, and α and 38 Lyncis]. It finally moved to the west of the T'ai-wei Enclosure, 7° to the west of Yu-chih-fa [β Virginis], and was extinguished.
It lasted for a total of more than 50 days.
The details of the comet's final observation are interesting to examine. First, the statement that the comet remained visible for over 50 days
indicates it was still under observation following July 5. Second, although the T'ang hui yao and Hsin T'ang shu say the comet passed within
7° of β Virginis, the Chiu T'ang shu says it passed only 0.7° away. Calculations using the orbit below indicate the comet never passed closer
than 3.7° from that star and that this occurred on July 13.
The Byzantine monk Theophanes the Confessor wrote Chronographia around 813 and noted that during Annus Mundi 6252 (759-60),
"a very bright comet appeared for ten days in the east and another twenty-one days in the west.".
The Arabic historian Agapius of Manbij (10th century) reported, "In this year the star with a tail appeared, and it was in Aries before the Sun,
and the Sun was in Leo. It proceeded until it was under the rays of the sun, then went behind it and stayed 40 days."
David Cook (1998) has suggested the observation was actually made by Theophilus of Edessa.
The first person to suggest that this comet was 1P/Halley was P. A. E. Laugier (1846). Although he did not compute an orbit, he said the orbit of
that comet could fit the available Chinese observations if the perihelion date was estimated as 760 June 11. J. R. Hind (1850) investigated this
apparition and agreed with Laugier's conclusion, right down to the date of perihelion. He said, "The return of the comet in 760 appears to me little short of a
certainty." P. H. Cowell and A. C. D. Crommelin (1908) were the first to investigate the long-term orbital motion of 1P/Halley and concluded the
perihelion date was 760 June 15. The modern orbital investigations of D. K. Yeomans and T. Kiang (1981), Werner Landgraf (1986), and G. Sitarski (1988)
have included the effects of nongravitational forces and have almost unanimously determined the perihelion date as 760 May 20. Calculations using the
Yeomans-Kiang orbit below indicate the comet reached at a minimum solar elongation of 2° on April 3 and a maximum solar elongation of 35° on May 17.
On June 1 the comet reached another minimum solar elongation (18°), and on June 2, it attained its most northerly declination of +41° (apparent).
It reached a maximum solar elongation of 54° on June 22.
| T |
ω |
Ω (2000.0) |
i |
q |
e |
| 760 May 20.671 (UT) |
99.997 |
44.687 |
163.443 |
0.58184 |
0.96785 |
- ABSOLUTE MAGNITUDE: H10=2 (Vsekhsvyatskij, 1964), 4.0 (Kronk)
- FULL MOON: April 5, May 4, June 3, July 3
Sources
Chronographia (813), p. 597
Chin Tang situ (945), p. 171
T'ang hui yao (961), p.
171
Agapius of Manbij (10th century), p. 542
Hsin T'ang situ (1060), p. 171
Synopsis
Istorion (1100), p. 464
A. G. Pingre (1783), pp. 336-7, 610-11
CR, 15 (1842 Nov. 21),
pp. 952-3
CR, 23 (1846), pp. 186-7
MNRAS, 10 (1850 Jan. 11), p. 56
PMJS (3rd Series),
36 (1850 Jun.), pp. 471, 474
J. Williams (1871), p. 44
G. F. Chambers (1889), pp. 512-13
MNRAS, 68 (May 1908), pp. 510-14
PA, 42 (1934 Apr.), p. 196
Ho Peng Yoke (1962), p. 171
S. K. Vsekhsvyatskij (1964), p. 48
MRAS, 76 (1972), pp. 35, 53
R. R. Newton (1972), p. 683
CAA, 3 (1979), p. 122
D. K. Yeomans and T. Kiang (1981), p. 643
J. L. Brady (1982), p. 210
IBIS, 38 (1985), pp. 205-6
W. Landgraf (1986), p. 258
G. Sitarski (1988), p. 263
personal
correspondence from David Cook (1998).
References
Kronk, Gary W. (1999) Cometography A Catalog of Comets Vol. 1 Ancient-1799: A Catalog of Comets 1
Cambridge University Press - not open access - Cambridge University Press