13P/Olbers

Last updated
13P/Olbers
Comet 13P Olbers crop2.png
13P/Olbers on 11 August 2024
Discovery
Discovered by Heinrich Olbers
Discovery dateMarch 6, 1815
Designations
1815 E1; 1887 Q1;
1887 V; 1887f;
1956 A1; 1956 IV;
1956a
Orbital characteristics
Epoch 2024-06-19
(JD 2460480.5) [1]
Aphelion 32.56 AU
Perihelion 1.175 AU
Semi-major axis 16.87 AU
Eccentricity 0.9303
Orbital period 69.3 yr
68y 11d (perihelion to perihelion)
Inclination 44.67°
85.8°
Argument of
periapsis
64.4°
Last perihelionJune 30, 2024 [2] [1] [3]
June 19, 1956 [3]
Next perihelionMarch 20, 2094 [4]
Earth MOID 0.466 AU
Jupiter MOID 0.692 AU
Comet total
magnitude
(M1)
6.9 [5]

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. [5] The comet last passed perihelion 30 June 2024 and it was previously seen in 1956. The next perihelion is in 2094.

Contents

Observational history

Discovery

Heinrich Wilhelm Matthias Olbers discovered the comet on 6 March 1815 and described it as small. The comet came to perihelion on 26 April 1815 and reached an apparent magnitude of about 5, [6] and was faintly visible by naked eye. [7] Its orbit was first computed by Carl Friedrich Gauss on March 31 as parabolic, and Friedrich Bessel calculated an orbital period of 73.9 years using observations from June. Calculations by other astronomers during that era resulted anywhere between 72 and 77 years. [6] Modern solutions give an orbital period of 74.9 years for the 1815 epoch. [1]

1887

Orbital period
at different epochs
[8]
Epoch Orbital
period

(years)
188772.37
195669.54
202469.25
209470.72

There were unsuccessful searches for the comet throughout 1887, until it was accidentally found by William Robert Brooks on 25 August 1887. [6] He described as an easy object to see through a 9-inch reflector, with a brightish nucleus and a faint tail; it continued to brighten for a few days after passing perihelion. [9] The comet brightened to an apparent magnitude of about 9. [7] On 28 July 1887 the comet passed 0.081 AU (12.1 million km) from Mars and then passed perihelion on 8 October 1887. [8]

1956

The comet was recovered on 4 January 1956 by Antonín Mrkos. The comet was then located in Eridanus and its apparent magnitude was estimated to be 16. He then found the comet in plates obtained by the McDonald Observatory on 12 November 1955. [7] The comet passed perihelion on 19 June 1956 and reached an apparent magnitude of 6.5, while its tail was about one degree long. [6]

2024

Comet Olbers on 24 June 2024 Comet Olbers 2024-06-24 49f.jpg
Comet Olbers on 24 June 2024

The comet was recovered on 24 August 2023 by Alan Hale with the Las Cumbres Observatory at Siding Spring, and then additional pre-recovery images from August 13 were located. The comet then had an estimated apparent magntitude of about 22. [8] [1] On 16 November 2023 the comet came to opposition 139 degrees from the Sun. On 14 January 2024 the comet had an estimated magnitude of 15.3, was reported to have a strongly condensed coma measuring 0.9 arcminutes across and a faint tail one arcminute. By 10 March 2024 the comet had brightened to a magnitude of 11.4 and the coma was 4 arcminutes across. The comet was observed visually on April 12 to have a magnitude of 9.2, being a magnitude brighter than the ephemeris. [10] It came to perihelion on June 30, 2024, [2] when it was 1.18 AU from the Sun and 1.94 AU from Earth. [2] It was expected to brighten to about apparent magnitude 7−8 but peaked at 6–7. [3]

Earth close approach
DateDistance (AU) Solar
elongation
2024-Jul-20 [11] 1.895 AU (283.5 million km)35°
2094-Jan-09 [12] 0.676 AU (101.1 million km)134°

2094

Before the 2023 recovery, while the last observation was in 1956, Kinoshita calculated that the comet would come to a future perihelion passage (closest approach to the Sun) on 22 March 2094. [13] Accounting for observations in 2023–4, the nominal time of perihelion passage is now calculated to be 20 March 2094. [4]

Meteor showers

There is some speculation that 13P/Olbers has an associated annual meteor shower on Mars coming from the direction of Beta Canis Majoris. [14] The minimum orbit intersection distance of the orbits of comet Olbers and Mars is 0.0266 AU (3.98 million km) and the meteors impact the planet with a velocity of 27 km/s. An intersection distance of less than 0.1 AU and an impact speed high enough for the meteors to become ablaze are considered good predictors for a potential meteor shower. [15]

Related Research Articles

<span class="mw-page-title-main">12P/Pons–Brooks</span> Periodic comet with 71-year orbit

12P/Pons–Brooks is a periodic comet with an orbital period of 71 years. Comets with an orbital period of 20–200 years are referred to as Halley-type comets. It is one of the brightest known periodic comets, reaching an absolute visual magnitude of about 5 in its approach to perihelion. Comet Pons-Brooks was conclusively discovered at Marseilles Observatory in July 1812 by Jean-Louis Pons, and on its next appearance in 1883 by William Robert Brooks. There are ancient records of comets that are suspected of having been apparitions of 12P/Pons–Brooks.

<span class="mw-page-title-main">55P/Tempel–Tuttle</span> Periodic comet with an orbital period of 33 years, parent body of the Leonid meteor shower

55P/Tempel–Tuttle is a retrograde periodic comet with an orbital period of 33 years. It fits the classical definition of a Halley-type comet with a period of between 20 and 200 years. It was independently discovered by Wilhelm Tempel on December 19, 1865, and by Horace Parnell Tuttle on January 6, 1866.

<span class="mw-page-title-main">8P/Tuttle</span> Periodic comet with 13 year orbit

8P/Tuttle is a periodic comet with a 13.6-year orbit. It fits the classical definition of a Jupiter-family comet with an orbital period of less than 20 years, but does not fit the modern definition of. Its last perihelion passage was 27 August 2021 when it had a solar elongation of 26 degrees at approximately apparent magnitude 9. Two weeks later, on September 12, 2021, it was about 1.8 AU (270 million km) from Earth which is about as far from Earth as the comet can get when the comet is near perihelion.

<span class="mw-page-title-main">10P/Tempel</span> Periodic comet with 5 year orbit

10P/Tempel, also known as Tempel 2, is a periodic Jupiter-family comet with a 5-year orbital period. It was discovered on July 4, 1873 by Wilhelm Tempel. At the perihelion passage on 2 August 2026 the solar elongation is calculated at 164 degrees, with apparent magnitude approximately 8, with closest approach to Earth on 3 August 2026 at a distance of 0.414 AU (61.9 million km).

<span class="mw-page-title-main">7P/Pons–Winnecke</span> Periodic comet with 6-year orbit

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.

<span class="mw-page-title-main">15P/Finlay</span> Periodic comet with 6 year orbit

Comet Finlay is a periodic comet with an orbital period of 6 years discovered by William Henry Finlay 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. It last came to perihelion on December 27, 2014, at around magnitude 10. 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). In October 2060 the comet will pass about 5 million km from Earth.

<span class="mw-page-title-main">Comet Holmes</span> Periodic comet with 6-year orbit

Comet Holmes is a periodic comet in the Solar System, discovered by the British amateur astronomer Edwin Holmes on November 6, 1892. Although normally a very faint object, Holmes became notable during its October 2007 return when it temporarily brightened by a factor of a million, in what was the largest known outburst by a comet, and became visible to the naked eye. It also briefly became the largest object in the Solar System, as its coma expanded to a diameter greater than that of the Sun. Between 1857–2106 perihelion remains between 2.05–2.36 AU.

<span class="mw-page-title-main">22P/Kopff</span> Periodic comet with 6 year orbit

Comet Kopff or 22P/Kopff is a periodic comet in the Solar System. Discovered on August 23, 1906, it was named after August Kopff who discovered the comet. The comet was missed on its November 1912 return, but was recovered on its June 1919 return and has been seen at every apparition since. Close approaches to Jupiter in 1938 and 1943 decreased the perihelion distance and orbital period. 22P/Kopff’s last perihelion passage was 18 March 2022. On 13 July 2028 it will pass 0.353 AU (52.8 million km) from Earth.

<span class="mw-page-title-main">23P/Brorsen–Metcalf</span> Periodic comet with 70 year orbit

23P/Brorsen–Metcalf is a periodic comet with an orbital period of 70 years. It fits the classical definition of a Halley-type comet with. It was first discovered by Theodor Brorsen at the Altona Observatory on July 20, 1847, and again by Kaspar Schweizer (Moscow) on August 11, 1847. It was predicted that it would reappear between 1919 and 1922.

Comet Crommelin, also known as Comet Pons-Coggia-Winnecke-Forbes, is a periodic comet with an orbital period of almost 28 years. It fits the classical definition of a Halley-type comet with. It is named after the British astronomer Andrew C. D. Crommelin who calculated its orbit in 1930. It is one of only four comets not named after their discoverer(s), the other three being Comets Halley, Encke, and Lexell. It next comes to perihelion around May 27, 2039 when it will be near a maximum near-perihelion distance from Earth.

<span class="mw-page-title-main">45P/Honda–Mrkos–Pajdušáková</span> Periodic comet with 5 year orbit

45P/Honda–Mrkos–Pajdušáková is a short-period comet discovered by Minoru Honda December 3, 1948. It is named after Minoru Honda, Antonín Mrkos, and Ľudmila Pajdušáková. The object revolves around the Sun on an elliptical orbit with a period of 5.25 years. The nucleus is 1.3 kilometers in diameter. On August 19 and 20, 2011, it became the fifteenth comet detected by ground radar telescope.

255P/Levy, formerly P/2006 T1 and P/2011 Y1, is a periodic comet with an orbital period of 5.25 years. It last came to perihelion on 14 January 2012. During the 2006 passage the comet achieved an apparent magnitude of ~9.5. Levy (PK06T010) was believed to have been recovered on 3 June 2011 at magnitude 19.8, but other observatories were unable to confirm a recovery. It was most likely a false positive because of large residuals. Levy was recovered on 17 December 2011 at magnitude 19.8, and given the second designation 2011 Y1. It was then numbered.

<span class="mw-page-title-main">62P/Tsuchinshan</span> Periodic comet with 6 year orbit

62P/Tsuchinshan, also known as Tsuchinshan 1, is a periodic comet first discovered January 1, 1965 at the Purple Mountain Observatory in Nanking. It last came to perihelion on 25 December 2023 at around apparent magnitude 8, and was then 0.53 AU (79 million km) from Earth and 110 degrees from the Sun.

<span class="mw-page-title-main">209P/LINEAR</span> Periodic comet

209P/LINEAR is a periodic comet with an orbital period of 5.1 years. The comet has extremely low activity for its size and is probably in the process of evolving into an extinct comet.

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.

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.

<span class="mw-page-title-main">C/2021 T4 (Lemmon)</span>

C/2021 T4 (Lemmon) is an inbound long period comet discovered by the Mount Lemmon Observatory on 7 October 2021. This passage through the planetary region of the Solar System will reduce the orbital period from millions of years to thousands of years.

<span class="mw-page-title-main">C/2023 A3 (Tsuchinshan–ATLAS)</span> Comet from the Oort cloud

C/2023 A3 (Tsuchinshan–ATLAS) is a comet from the Oort cloud discovered by the Purple Mountain Observatory in China on 9 January 2023 and independently found by ATLAS South Africa on 22 February 2023. The comet passed perihelion at a distance of 0.39 AU on 27 September 2024, when it became visible to the naked eye. Tsuchinshan-Atlas peaked its brightest magnitude shortly after passing the Sun at 9 October, with a magnitude of −4.9 per reported observations at the Comet Observation Database (COBS).

<span class="mw-page-title-main">C/2023 P1 (Nishimura)</span> Comet in September 2023

C/2023 P1 (Nishimura) is a long-period comet discovered by Hideo Nishimura on 12 August 2023. The comet passed perihelion on 17 September 2023 and reached an apparent magnitude of about 2.5.

References

  1. 1 2 3 4 MPC
  2. 1 2 3 "Horizons Batch for 13P/Olbers (90000226) on 2024-Jun-30" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Archived from the original on 2022-06-15. Retrieved 2023-08-28. (JPL#11 Soln.date: 2023-Aug-28)
  3. 1 2 3 Seiichi Yoshida (2004-07-31). "13P/Olbers". Seiichi Yoshida's Comet Catalog. Retrieved 2010-02-24.
  4. 1 2 "Horizons Batch for 13P/Olbers (90000226) for March 2094" (Perihelion occurs when rdot flips from negative to positive). JPL Horizons. Archived from the original on 2023-08-29. Retrieved 2024-06-25.
  5. 1 2 "JPL Small-Body Database Browser: 13P/Olbers". Jet Propulsion Laboratory. Retrieved 2012-07-26.
  6. 1 2 3 4 Kronk, Gary W. (2001–2005). "13P/Olbers" . Retrieved 2012-02-22. (Cometography Home Page)
  7. 1 2 3 Roemer, Elizabeth (1956). "Comet Notes". Publications of the Astronomical Society of the Pacific. 68 (401): 171–172. Bibcode:1956PASP...68..171R. doi:10.1086/126910. ISSN   0004-6280. JSTOR   40673045.
  8. 1 2 3 "CBET 5289 : COMET 13P/OLBERS". Central Bureau for Astronomical Telegrams. 2023-08-28. Retrieved 2023-08-29.
  9. Brooks, W. R. (1 January 1888). "The Olbers-Brooks Comet". The Observatory. 11: 90–91. Bibcode:1888Obs....11...90B. ISSN   0029-7704.
  10. Green, Daniel (29 April 2024). "COMET 13P/OLBERS". Central Bureau for Astronomical Telegrams. 5389.
  11. "Closest Approach to Earth around 20 July 2024" (Closest Earth approach occurs when deldot flips from negative to positive). JPL Horizons . Retrieved 2023-08-28.
  12. "Closest Approach to Earth around 9 January 2094" (Closest Earth approach occurs when deldot flips from negative to positive). JPL Horizons . Retrieved 2023-08-28.
  13. Kinoshita, Kazuo (2003-02-25). "13P/Olbers past, present and future orbital elements". Comet Orbit. Retrieved 2023-08-28.
  14. "Meteor Showers And Their Parent Bodies". Archived from the original on 2008-10-03. Retrieved 2006-12-30.
  15. Christou, Apostolos A. (December 2004). "Predicting Martian and Venusian Meteor Shower Activity". Earth, Moon, and Planets. 95 (1–4): 425–431. doi:10.1007/s11038-005-9023-0.
Numbered comets
Previous
12P/Pons–Brooks
13P/OlbersNext
14P/Wolf