Discovery | |
---|---|
Discovered by | Theodor Brorsen |
Discovery site | Holstein, Germany |
Discovery date | 26 February 1846 |
Designations | |
P/1846 D2 P/1857 F1 | |
1846 III; 1857 II; 1868 I; 1873 VI; 1879 I | |
Orbital characteristics [1] | |
Epoch | 1 April 1879 (JD 2407440.5) |
Aphelion | 5.612 AU |
Perihelion | 0.5898 AU |
Semi-major axis | 3.101 AU |
Eccentricity | 0.8098 |
Orbital period | 5.461 years |
Inclination | 29.382° |
Last perihelion | 31 March 1879 (last observation) 17 April 2023 [2] (calculated) |
Next perihelion | 28 November 2028 [2] (calculated) |
TJupiter | 2.467 |
Earth MOID | 0.367 AU |
Comet total magnitude (M1) | 8.3 |
5D/Brorsen (also known as Brorsen's Comet or Comet 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.
The comet was discovered on February 26, 1846, by Danish astronomer Theodor Brorsen. The perihelion of 5D/Brorsen was February 25, just a day before its discovery, and it passed closest to Earth on March 27, at a distance of 0.52 AU (78 million km). [3] As a result of this close encounter to Earth, the comet's coma diameter increased. Johann Friedrich Julius Schmidt estimated it as 3 to 4 arcminutes across on March 9, and 8 to 10 arcminutes across on the 22nd of that same month. [3] On April 22, it was about 20 degrees from the north celestial pole. By the end of this first apparition the orbital period was calculated as 5.5 years. [3] J. Russell Hind later calculated that this comet had a close approach to Jupiter on 20 May 1842, placing it to the initial orbit from which it was discovered. [4]
The comet's 5.5-year period would mean that apparitions would alternate between good and poor. [3] As expected, the comet was missed in its 1851 apparition, when it only came as close as 1.5 AU to Earth. The comet's orbit was still relatively uncertain, made worse by its approach to Jupiter in 1854. Karl Christian Bruhns found a comet on 18 March 1857. [3] Soon an orbit was computed and it was found to be 5D/Brorsen, although predictions were three months off. [3] The comet was followed until June 1857, and the orbit was then well established. [3] Observers reported that the comet had a bright, almost star-like nucleus. [5]
The comet was missed in 1862, and the next recovery was in 1868. A close approach to Jupiter shortened the period enough to make the comet visible in 1873. [6] [7] A very favorable apparition followed in 1879, allowing the comet to be observed for the longest time to date – four months. [8] The comet was missed in 1884, due to observing circumstances, but was also missed in 1890, a favorable apparition. The next favorable apparition occurred in 1901, but searches did not locate the comet.
The next serious search was started by Brian G. Marsden in 1963, who believed the comet had faded out of existence, but computed the orbit for a very favorable 1973 apparition. [9] Takuo Kojima made intensive searches for the comet on January 1973, but nothing turned up, which finally led Marsden to conclude that the comet was lost. [10]
Zdenek Sekanina suggested that the comet underwent a change in the rotation axis of the nucleus in mid 19th century, resulting to non-gravitational changes in the orbit, while also mentioned that there are some evidence that the comet may have disintegrating. [11] These evidence are the accounts of the large expansion of the coma after perihelion at the 1868 and 1879 apparitions, the presence of condensations in the inner coma during the 1857 and 1868 apparitions and the account by Johann Friedrich Julius Schmidt that on 20 May 1879 the comet was very faint and lacked a nucleus. [11]
In 2001, Lubos Neslusan tentatively identified the asteroid (297274) 1996 SK as the possible extinct nucleus of 5D/Brorsen based on the similarity of their respective orbits. [12] [13]
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.
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 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.
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.
14P/Wolf is a periodic comet in the Solar System.
D/1770 L1, popularly known as Lexell's Comet after its orbit computer Anders Johan Lexell, was a comet discovered by astronomer Charles Messier in June 1770. It is notable for having passed closer to Earth than any other comet in recorded history, approaching to a distance of only 0.015 astronomical units, or six times the distance from the Earth to the Moon. The comet has not been seen since 1770 and is considered a lost comet.
A lost comet is one which was not detected during its most recent perihelion passage. This generally happens when data is insufficient to reliably calculate the comet's location or if the solar elongation is unfavorable near perihelion passage. The D/ designation is used for a periodic comet that no longer exists or is deemed to have disappeared.
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.
93P/Lovas, also called Comet Lovas 1, is a Jupiter-family comet with an orbital period of 9.2 years. It was discovered in 1980 by Hungarian astronomer Miklós Lovas.
Comet 252P/LINEAR is a periodic comet and near-Earth object discovered by the LINEAR survey on April 7, 2000. The comet is a Jupiter family comet, meaning that it passes quite close to the orbit of Jupiter.
104P/Kowal, also known as Kowal 2, is a periodic Jupiter-family comet discovered by Charles T. Kowal in 1979. The orbit was confirmed after new sightings in 1991 and 1998.
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.
126P/IRAS is a periodic comet with an orbital period of 13.4 years. It was discovered in images taken by the Infrared Astronomical Satellite (IRAS) on 28 July 1983 by J. Davies. The discovery was confirmed with images taken with the 1.2-m Schmidt telescope at Palomar Observatory.
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.
205P/Giacobini is a periodic Jupiter-family comet with an orbital period of 6.68 years. It was discovered by Michel Giacobini on 4 September 1896 and then it was lost until it was recovered by Koichi Itagaki on 10 September 2008. The comet was then found to have fragmented into three pieces.
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.
C/1975 T2 (Suzuki–Saigusa–Mori) is a long-period comet discovered on 5 October 1975. The comet approached Earth at a distance of 0.1 AU on 31 October 1975 and became visible with naked eye. The comet has been associated with the lambda Ursae Majorids meteor shower.
C/1991 L3 (Levy) is a periodic comet discovered by David H. Levy on 14 June 1991. The comet has an orbital period of 51 years and thus fits the definition of Halley-type comets, which have orbital periods between 20 and 200 years.
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).
489P/Denning is a Jupiter-family comet with an orbital period of 9.4 years. It was discovered by William Frederick Denning on 26 March 1894 but was subsequently lost until 2024, when asteroid 2007 HE4 was identified as the same object.