Discovery | |
---|---|
Discovered by | William Henry Finlay |
Discovery date | September 26, 1886 |
Designations | |
1886 S1; 1886 VII; 1886e; 1893 K1; 1893 III; 1893a; 1906 V; 1906d; 1919 II; 1919d; 1926 V; 1926d; 1953 VII; 1953i; 1960 VIII; 1960d; 1967 IX; 1967g; 1974 X; 1974d; 1981 XII; 1981e; 1988 IX; 1988f | |
Orbital characteristics | |
Epoch | 2014-Dec-09 (JD 2457000.5) |
Aphelion | 6.019 AU |
Perihelion | 0.976 AU |
Semi-major axis | 3.488 AU |
Eccentricity | 0.7202 |
Orbital period | 6.51 a |
Inclination | 6.799° |
Last perihelion | July 13, 2021 [1] December 27, 2014 [1] [2] June 22, 2008 |
Next perihelion | 2028-Feb-09 [3] 2034-Sep-08 2041-Apr-03 2047-Oct-25 2054-May-02 2060-Oct-03 [4] |
Earth MOID | 0.009 AU (1.3 million km) [5] |
Jupiter MOID | 0.16 AU (24 million km) [5] |
Physical characteristics | |
Dimensions | 1.8 km (uncertain) [6] |
Comet Finlay is a periodic comet with an orbital period of 6 years discovered by William Henry Finlay (Royal Observatory, Cape of Good Hope, South Africa) on September 26, 1886. The next perihelion passage is July 13, 2021 when the comet will have a solar elongation of 54 degrees at approximately apparent magnitude 10. [7] It last came to perihelion on December 27, 2014, [2] at around magnitude 10. [7] Of the numbered periodic comets, the orbit of 15P/Finlay has one of the smallest minimum orbit intersection distances with the orbit of Earth (E-MOID). [8] In October 2060 the comet will pass about 5 million km from Earth.
Perihelion distance at different epochs [1] | |||||||
Epoch | Perihelion (AU) | ||||||
---|---|---|---|---|---|---|---|
1866 | 1.0 | ||||||
1906 | 0.96 | ||||||
1919 | 1.0 | ||||||
1981 | 1.1 | ||||||
2008 | 0.97 | ||||||
2021 | 0.99 | ||||||
2028 | 1.0 [3] |
When the first orbit calculations were made in 1886, there was a similarity between this orbit and that of Francesco de Vico's lost periodic comet of 1844 (54P/de Vico-Swift-NEAT). Lewis Boss (Dudley Observatory, Schenectady, United States) noted large discrepancies between the orbits and after further observations concluded that de Vico's comet could not be the same as Finlay's. [9]
During the 1906 apparition the comet brightened to magnitude 6. In 1910 a close pass with Jupiter increased the orbital period, in 1919 the path was off predictions and a new comet discovered by Sasaki (Kyoto Observatory, Japan) on October 25, 1919, was discovered to be Finlay's.
The magnitude of the comet declined after 1926, and it was not until 1953 that it has been observed on every return.
During the 2014 perihelion passage the comet outburst on 16 December 2014 from magnitude 11 to magnitude 9 becoming bright enough to be seen in common binoculars with a 50 mm objective lens. [10] On December 23, 2014, 15P and Mars were only 1/6 of a degree apart in the sky after sunset. [10] But by December 23, 2014, the comet had dimmed considerably since the outburst. On 16 January 2015, the comet outburst to magnitude 8. [11]
15P/Finlay currently has an Earth-MOID of 0.009 AU (1,300,000 km ; 840,000 mi ). [5] The comet will come to perihelion six more times and then on October 22, 2060, the comet will pass roughly 0.0334 AU (5.00 million km; 3.10 million mi) from Earth with an uncertainty region of about ±2300 km. [5] [12] This will be one of the closest comet approaches to Earth. [13]
Debris ejected during the 1995 perihelion passage generated a meteor shower on 29–30 September 2021 radiating from the southern constellation of Ara. [14] More outbursts are expected on 7 October 2021 from the 2008 and 2014 streams.
Comet 4P/Faye is a periodic Jupiter-family comet discovered in November 1843 by Hervé Faye at the Royal Observatory in Paris. Its most recent perihelia were on November 15, 2006; May 29, 2014; and September 8, 2021.
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7P/Pons–Winnecke is a periodic Jupiter-family comet with a six-year orbit. Early calculations for the 1921 apparition suggested that the orbit of the comet might collide with Earth in June, but observations on 10 April ruled out an impact. It made a very close approach to Earth in June 1927. The outward migration of perihelion created impressive meteor showers in 1916, 1921 and 1927.
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54P/de Vico–Swift–NEAT is a periodic comet in the Solar System first discovered by Father Francesco de Vico on August 23, 1844. It has become a lost comet several times after its discovery. The comet makes many close approaches to Jupiter. The comet was last observed on 20 December 2009 by Ageo Observatory.
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62P/Tsuchinshan, also known as Tsuchinshan 1, is a periodic comet discovered on 1965 January 1 at Purple Mountain Observatory, Nanking. It will next come to perihelion on 25 December 2023 at around apparent magnitude 8, and will be 0.53 AU (79 million km) from Earth and 110 degrees from the Sun.
51P/Harrington is a periodic comet in the Solar System.
72P/Denning–Fujikawa is a periodic comet discovered on 4 October 1881 by William Frederick Denning. The comet was not seen at another apparition until recovered by Shigehisa Fujikawa in 1978. From 29 December 1978 until 17 June 2014, the comet was lost. On 17 June 2014 the comet was recovered by Hidetaka Sato at apparent magnitude 16 when it was 50 degrees from the Sun. The comet came to perihelion in June 2023, and will next come to perihelion in May 2032.
66P/du Toit is a periodic comet in the Solar System with a current orbital period of 14.78 years. It came to perihelion on 2018 May 19 at roughly apparent magnitude 12.
79P/du Toit–Hartley or du Toit 2 is a periodic comet, now divided into two parts, in the Solar System with an orbital period of 5.06 years. It next comes to perihelion in September 2023 but is only expected to reach about apparent magnitude 18. It will be less than 90 degrees from the Sun from February 2023 until June 2024. On 26 May 2024 it will be 2.7 AU from the Sun and Earth.