Discovery [1] [2] | |
---|---|
Discovered by | Michael P. Candy |
Discovery date | 26 December 1960 |
Designations | |
1960n [3] 1961 II | |
Orbital characteristics [4] [5] | |
Epoch | 9 January 1961 (JD 2437308.5) |
Observation arc | 8 days |
Earliest precovery date | 17 December 1960 |
Number of observations | 8 |
Aphelion | 29.004 AU |
Perihelion | 0.9899 AU |
Semi-major axis | 15.025 AU |
Eccentricity | 0.93034 |
Orbital period | 932 years (inbound) 1,032 years (outbound) |
Inclination | 151.175° |
177.293° | |
Argument of periapsis | 138.765° |
Last perihelion | 8 February 1961 |
TJupiter | –0.746 |
Earth MOID | 0.1522 AU |
Jupiter MOID | 0.1628 AU |
Physical characteristics [4] [6] | |
Comet total magnitude (M1) | 7.9 |
Comet nuclear magnitude (M2) | 16.5 |
8.0 (1961 apparition) |
Candy's Comet, also known as C/1960 Y1 by its modern nomenclature, is a non-periodic comet in retrograde orbit around the Sun. It is the first comet to have its orbit calculated by its own discoverer. [7]
The comet was first imaged unnoticed in three prediscovery images taken from the Sonneberg Observatory on December 17, [6] however it wasn't discovered until Michael Philip Candy spotted it when he was testing an eyepiece of his 5 in (13 cm) comet seeker on December 26. [2] At the time of discovery, it was a magnitude 8.0 object about 3 degrees southeast of the star Kappa Cephei. The subsequent two nights were clear, which helped Candy and G. E. Taylor to calculate its orbit and ephemeris right away. [2] Precovery ephemerides of the comet showed that it should be only 5 degrees from Comet Borrelly on October 1960.
The comet made its closest approach to Earth of 26 December 1960, the day it was discovered, at a distance of 0.645 AU. [6] The comet moved quickly southwards and faded while approaching perihelion. [8] Observations from 13 January 1961 show a very sharp nuclear condensation of magnitude 15.0. [2] Throughout January, the comet did not produce a discernible tail, however photometric analysis show the comet emitting an intense far-red emission of activity. [9] A faint tail about 15–20 arcminutes long was observed in January and February. The comet throughout February was a 9th magnitude object. The comet was last detected on 14 May 1961. [6]
An orbit calculated based on a short observation arc of only 8 days, [4] indicated the comet as a Halley-type periodic comet with an orbit lasting 58 years. The very small minimum orbit intersection distance with Earth of 0.152 AU (22.7 million km) has led JPL to classify it as a near-Earth comet, although orbital simulations conducted by CNEOS do not show any close approaches to Earth. [4] [10] An orbit calculated by Brian G. Marsden, Zdenek Sekanina, and E. Everhart from positions obtained from 30 December 1960 to 14 May 1961 indicates that eccentricity of the comet is 0.9899, that corresponds to an orbital period of 932 years inbound and 1,057 years outbound. [5]
Comet Ikeya–Seki, formally designated C/1965 S1, 1965 VIII, and 1965f, was a long-period comet discovered independently by Kaoru Ikeya and Tsutomu Seki. First observed as a faint telescopic object on 18 September 1965, the first calculations of its orbit suggested that on October 21, it would pass just 450,000 km (280,000 mi) above the Sun's surface, and would probably become extremely bright.
Comet Encke, or Encke's Comet, is a periodic comet that completes an orbit of the Sun once every 3.3 years. Encke was first recorded by Pierre Méchain on 17 January 1786, but it was not recognized as a periodic comet until 1819 when its orbit was computed by Johann Franz Encke. Like Halley's Comet, it is unusual in its being named after the calculator of its orbit rather than its discoverer. Like most comets, it has a very low albedo, reflecting only 4.6% of the light its nucleus receives, although comets generate a large coma and tail that can make them much more visible during their perihelion. The diameter of the nucleus of Encke's Comet is 4.8 km.
The Great Comet of 1882, formally designated as C/1882 R1, 1882 II, and 1882b, was a comet which became very bright in September 1882. It was a member of the Kreutz Sungrazers, a family of comets which pass within 1 R☉ of the Sun's photosphere at perihelion.
Comet Arend–Roland was discovered on November 6, 1956, by Belgian astronomers Sylvain Arend and Georges Roland on photographic plates. As the eighth comet found in 1956, it was named Arend–Roland 1956h after its discoverers. Because it was the third comet to pass through perihelion during 1957, it was then renamed 1957 III. Finally, it received the standard IAU designation C/1956 R1 (Arend–Roland), with the "C/" indicating that it was a non-periodic comet and the "R1" showing that it was the first comet reported as discovered in the half-month designated by "R". The last is equivalent to the period September 1–15.
Comet White–Ortiz–Bolelli was a bright comet which appeared in 1970. It was a member of the Kreutz sungrazers, a family of comets which resulted from the break-up of a large parent comet several centuries ago. It was already easily visible to the naked eye when first discovered, and reached a maximum apparent magnitude of +1.
5D/Brorsen was a periodic Jupiter-family comet discovered on February 26, 1846, by Danish astronomer Theodor Brorsen. The comet was last seen in 1879 and is now considered lost.
65P/Gunn is a periodic comet in the Solar System which has a current orbital period of 6.79 years. The comet is a short-period comet, orbiting the Sun every 6.79 years inside the main asteroid belt between the orbits of the planets Mars and Jupiter.
Comet Bennett, formally known as C/1969 Y1, was one of the two bright comets observed in the 1970s, along with Comet West and is considered a great comet. The name is also borne by an altogether different comet, C/1974 V2. Discovered by John Caister Bennett on December 28, 1969, while still almost two AUs from the Sun, it reached perihelion on March 20, passing closest to Earth on 26 March 1970, as it receded, peaking at magnitude 0. It was last observed on 27 February 1971.
13P/Olbers is a periodic comet with an orbital period of 69 years. It fits the classical definition of a Halley-type comet with a period between 20 and 200 years. The comet last passed perihelion 30 June 2024 and it was previously seen in 1956. The next perihelion is in 2094.
Comet Arend or 50P/Arend is a periodic comet in the Solar System which was discovered on October 4, 1951. It was discovered by astronomer Sylvain Julien Victor Arend at the Royal Observatory of Belgium located in the municipality of Uccle. The comet was illustrated at approximately a magnitude of 14 and also exhibited a nucleus within a coma 14 arc seconds across. From its discovery, the comet has had 7 perihelions with its last return of Earth recorded on November 1, 2007. The comet's next perihelion will be in the year 2024.
The Great Southern Comet of 1887, or C/1887 B1 using its International Astronomical Union (IAU) designation, was a bright comet seen from the Southern Hemisphere during January 1887. Later calculations indicated it to be part of the Kreutz Sungrazing group. It came to perihelion on 11 January 1877 at a distance of 0.00483 AU (723 thousand km) with a velocity of 606.1 km/s. Since the Sun has a radius of 696000 km, the comet passed about 27000 km from the surface of the Sun.
63P/Wild is a periodic comet in the Solar System with a current orbital period of 13.21 years.
Comet 141P/Machholz or 141P/Machholz 2 is a periodic Jupiter family comet with an orbital period of 5.3 years. It was discovered by Donald Machholz on 13 August 1994. A few days after the discovery a number of condensations were found near the main component of the comet, indicating that the comet had fragmented between 1987 and 1989, during its previous perihelion.
C/2001 A2 (LINEAR) is a non-periodic comet from the Oort cloud discovered by LINEAR on 15 January 2001. The nucleus of comet split in multiPLe fragments during its perihelion passage. The comet brightened to an apparent magnitude of about 3.
Comet Tago–Sato–Kosaka, formally designated as C/1969 T1, is a non-periodic comet that became visible in the naked eye between late 1969 and early 1970. It was the first comet ever observed by an artificial satellite.
Comet Ikeya-Seki, formally designated as C/1967 Y1, is a retrograde non-periodic comet discovered by Kaoru Ikeya and Tsutomu Seki on 1967. It is the second comet discovered together by the two Japanese astronomers after C/1965 S1.
Comet du Toit, formal designation C/1945 X1, is a sungrazing comet that was observed four times by South African astronomer, Daniel du Toit, on December 1945. The comet is a member of the Kreutz sungrazer family.
Comet Alcock, formally designated as C/1963 F1 is a non-periodic comet that became barely visible to the naked eye in May 1963. It is the third of five comets discovered by English astronomer, George Alcock.
C/1983 J1 (Sugano–Saigusa–Fujikawa) is a non-periodic comet discovered by Matsuo Sugano, Yoshikazu Saigusa, and Shigehisa Fujikawa on 8 May 1983. The comet approached Earth at a distance of 0.063 AU on 12 June 1983.
C/1988 A1 (Liller) is a non-periodic comet discovered on 11 January 1988 by William Liller. The comet is part of a family of comets, known as the Liller family, which also includes the comets C/1996 Q1 (Tabur), C/2015 F3 (SWAN), C/2019 Y1 (ATLAS), and C/2023 V5 (Leonard).