Updated 2022 September 8
When observing a comet please try to forget how bright you think the comet should be, what it was when you last viewed it, what other observers think it is or what the ephemeris says it should be.
The equations for the light curves of comets that are currently visible use only the raw observations and should give a reasonable prediction for the current brightness. If the comet has not yet been observed or has gone from view a correction for aperture is included, so that telescopic observers should expect the comet to be fainter than given by the equation. The correction is about 0.033 per centimetre. Values for the r parameter given in square brackets [ ] are assumed. The form of the light curve is either the standard m = H0 + 5 log d + K0 log r or the linear brightening m = H0 + 5 log d + L0 abs(t - T + D0) where T is the date of perihelion, t the present and D0 an offset, if L0 is +ve the comet brightens towards perihelion and if D0 is +ve the comet is brightest prior to perihelion.
The order given here is provisional and based on the logical sequence of linked orbits. The final numbering scheme does not seem to follow this logical pattern.
This should have been numbered 405 if given in sequential order.
Erwin Schwab recovered the comet in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain. on 2020 September 11.09. The indicated delta-T correction to the prediction, by Gareth Williams, on MPC 58118 is -0.15 days. [CBET 4847, MPEC 2020-R159, 2020 September 14]
This should have been numbered 406 if given in sequential order.
The comet is a distant object and reached perihelion at the end of June 2003. The period is 18.5 years and the perihelion distance 3.93 au. Observers contributing to the preliminary orbit included BAA Member Peter Birtwhistle.
Erwin Schwab recovered the comet in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain. on 2020 August 18.11. The comet was some 5' from the expected position. [CBET 4835, 2020 August 19] It was finally given a designation for the return in MPEC 2020-S155 [2020 September 23].
This should have been numbered 403 if given in sequential order.
The Mt Lemmon Survey discovered a comet on 2020 October 15.45, which was placed on the PCCP as C3HU5C2. Hirohisa Sato subsequently realised that this was a return of 2007 VQ11 and it was withdrawn from the PCCP. CBET 4869 and MPEC 2020-U169 were issued on October 22. The comet was some 22' from the expected position, corresponding to a delta T of around -1.9 days.
Syuichi Nakano found images of the comet in PanSTARRS 1 data taken with the 1.8m Ritchey-Chretien on 2020 June 17.55 and on July 17 and 20. The comet was close to the expected position. The comet passed 0.97 au from Jupiter in 2020 February in an encounter that reduced the perihelion distance from 4.8 to 4.1 au and the period from 12.7 to 10.3 years. [CBET 4831, 2020 August 16] It was finally given a designation for the return in MPEC 2020-U182 [2020 October 23]. It was numbered 404 in CBET 4898 [2020 December 18], though it should have been 400.
An object briefly appeared on the PCCP as P218YG3 before being transferred to the "Previous NEOCP Objects" page having been identified as a return of comet 2013 TL117, though it was given on the page as 2013 TL17. The PCCP recovery was by by PanSTARRS 2 on 2020 October 25.6. Shortly afterwards further details were given in MPEC 2020-U231 and CBET 4874 [2020 October 25/26]. These reveal the continuing tensions between the MPC and CBET. Erwin Schwab had recovered the comet on October 17.13 with the Calar Alto 0.8m Schmidt (not Calar Alto-Schmidt as given in the MPEC). Additional independent recoveries were made at the Dominion Astrophysical Observatory on October 22 and by T. Ikemura and Hirohisa Sato on October 23/24.
Comet 2007 R2 was recovered during observations with the Korea Microlensing Telescope Network-SSO 1.6m reflector on 2020 September 11.64, when it was around 22nd magnitude. PanSTARRS 2 recorded it two days later and the Korean group made further observations on September 15. All these observations were published in MPEC 2020-S188 as observations of 2007 R2, though none of the observers realised that it was a recovery. [2020 September 25] Syuichi Nakano of the CBAT later noticed the observations and drew attention to the recovery. T. Ikemura and Hirohisa Sato made follow-up observations on October 10 and 12, with PanSTARRS 1 observing it on October 20. The comet was missed at the 2014 return and passed 0.74 au from Jupiter in 2016 March. The encounter increased the perihelion distance to 1.6 au and the period to 6.8 years. The comet was at perihelion in September. [CBET 4884, MPEC 2020-U269, 2020 October 30/31]. The CBET yet again hints at the tensions between the CBAT and MPC.
D Carson Fuls discovered a comet of 19th magnitude in Mt Lemmon Survey images taken with the 1.5m reflector on 2019 December 21.53. It was placed on the PCCP as C1N4PQ2 and confirmed by other observers including Michael Jaeger and Eric Bryssinck. [CBET 4709, MPEC 2020-A91, 2020 January 7/8]. The comet was at perihelion at 2.1 au in 2020 January and has a period of around 6 years.
Sam Deen has shown that the two comets are identical. The comet passed 0.34 au from Jupiter in 2010 in an encounter that significantly changed the orbit. [CBET 4792, 2020 June 8].
The comet should have been numbered 397, but the MPC have ignored the convention of numbering in order of orbit determination and returns. An MPEC announcing the identity was finally published on 2020 November 11 [MPEC 2020-V67].
Only the name Novichonok was originally given to the comet, however the discoverer was clear that it was a team effort with Gerke, and the name was later amended.
Denis Denisenko noted
As usual, there's a whole story behind the new discovery. This comet was caught just 63 (!!!) pixels from the edge of 1330x890 CCD image in 3x3 binning mode in the first night. Upon posting at NEO Confirmation Page most people (including myself) originally thought it to be identical to 111P (whose predicted position was less than 5' away, yet the magnitude was almost identical to the new object). But the direction of motion of the Comet Novichonok was totally different from Comet Helin-Roman-Crockett, and the new object was about twice slower.
Congratulations to Artyom with the first Russian periodic comet since the breakup of USSR! If you remember, two Comets Elenin were discovered on the telescope installed in USA. This time the observation was made in southern Russia, in the Republic of Karachay-Cherkessia in northern Caucasus, not far away from the 6-meter BTA telescope.
Syuichi Nakano found images of 2011 R3 in PanSTARRS 1 data taken with the 1.8m Ritchey-Chretien on 2020 June 20.49 and July 18.36. The comet was close to the expected position. The comet was put into its present orbit during a series of encounters with Jupiter: 0.87 au in 1992 October, 0.11 au in 1993 August and 0.45 au in 2005 April. Prior to these encounters the comet was in a more distant orbit with perihelion at 5.2 au and a period of 19.4 years. [CBET 4833, 2020 August 17] It was finally given a designation for the return in 2020 November [MPEC 2020-V78, 2020 November 12].
According to the MPEC the comet was recovered on 2020 November 3.49 by the Zwicky Transient Facility with the 1.2m Oschin Schmidt and by the Mt Lemmon Survey with the 1.5m reflector on November 16.51. The indicated delta-T correction to the prediction by G. V. Williams on MPC 75706 is -1.08 days and it was some 30' from the expected position. The CBET gives priority to the Mt Lemon Survey for reporting a new comet and then drawing attention to the likely identity with 2005 XA54. [CBET 4885, MPEC 2020-W25, 2020 November 17] The comet has perihelion at 1.8 au in 2021 January and a period of 14.9 years.
Erwin Schwab recovered comet 2007 B1 as a stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on November 17.13. The comet was some 20' from the predicted position, requiring a Delta(T) of -0.89 day. [CBET 4903, MPEC 2021-A66, 2021 January 7/9]
Brian Marsden noted on MPEC 2010-F69 [2010 March 23] that further [astrometric] observations of this comet were desirable.
The comet is one of those suspected to have undergone nuclear splitting according to the list of Marcos & Marcos [Dynamically correlated minor bodies in the outer solar system, MNRAS, 474, 838, 2018 February]. They note that it appears to be related to the multiple fragments of 332P/Ikeya-Murakami.
Quanzhi Ye recovered comet 2010 B2 in images taken with the 4.3 m Lowell Discovery Telescope on December 19.46. The recovery confirms the identification made by Sam Deen of a single observation made by the DECam on the Cerro Tololo 4 m reflector in 2015 June. [CBET 4904, MPEC 2021-A76, 2021 January 8/9] The comet passed 0.075 au from Mars on 1999 February 18. It passed 0.44 au from Jupiter on 1962 November 12 and 0.72 au on 1974 October 11. The comet will pass 0.51 au from Jupiter on 2045 September 12
Erwin Schwab recovered the comet as a stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2020 November 25.17. [CBET 4910, MPEC 2021-A147, 2021 January 11/12]
An object was discovered by the Zwicky Transient Factory on January 5.1 and posted on the PCCP as ZTF01on. It was summarily removed on January 8 and noted to be P/2016 J3. The previous evening Maik Meyer had discovered the identity, computed a linked orbit and informed the MPC and CBAT. Maik's linked orbit shows that the period is 4.67 years, with perihelion at 0.53 au on January 25. Despite this it was not designated 2021 A1. Michael Jaeger has imaged it, finding it to be around 14th magnitude.
Sam Dean notes:
It's caught in a Kozai resonance with Jupiter that it's currently on the higher-e, lower-i leg of. I think that'll peak around 2400-2500 before cycling back. Like plenty of Earth-crossing Kozai oscillating objects, its orbit also crosses Earth sometimes, creating a potential for meteor showers. It last crossed Earth's orbit within 0.1 au in the 1300s, coming as close as 0.07 au - and it will next do so in the 2200s/2300s, coming less than 0.01 au around 2300, where it should create a fairly regular and impressive meteor shower considering that it would be even more active than it is now.Sam also suggests that the absolute magnitude is very faint, around 23 and that it brightens rapidly, perhaps at 20 log r.
Rather belatedly the CBAT issued CBET 4911 on January 11, with a revision
coming 15 minutes later. This gives a similar account to that given above
and notes that the comet will pass Jupiter at 0.9 au in 2031 December. It
also hints that either the comet shows strong non-gravitational forces or that
the 2016 positions are somewhat out. The MPC finally issued MPEC 2021-A157 on January 12.
This does not give elements for 2016, although the published elements for 2021
and 2025 do use observations from 2016, so it may
just be an oversight.
J J Gonzalez made a visual observation of the comet on 2021 January 16.78 from his mountain observing site, estimating it at 9.7 in his 20 cm SCT.
The comet was acccidently recovered in astrometry taken by PanSTARRS on 2020 December 25.57. It was independently deliberately recovered by Erwin Schwab as a stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 January 13.01. The comet will pass 0.5 au from Jupiter in 2033 December in an encounter that will increase the perihelion distance to 3.8 au. [CBET 4918, MPEC 2021-B17, 2021 January 16/17]
Erwin Schwab recovered the comet as a nearly stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 January 14.01. [CBET 4919, MPEC 2021-B21, 2021 January 17]
Erwin Schwab recovered the comet as a nearly stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 January 17.23. The comet passed 0.48 au from Jupiter in 1952 August and will pass 0.43 au from the planet in 2024 September in an encounter that will increase the perihelion distance from 1.49 to 1.57 au. [CBET 4920, MPEC 2021-B118, 2021 January 22/23]
An object recorded at 22nd magnitude in astrometry taken by PanSTARRS 2 on December 23.49 was subsequently identified as as a return of 2010 A5 by the MPC. It was also detected by PanSTARRS 1 and Mt Lemmon later in 2021 January. [CBET 4928, MPEC 2021-B140, 2021 January 29]
Erwin Schwab recovered comet 2015 F1 as an apparently stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 January 13.06. Additional observations were made on February 10, 13 and 14. The comet was some 4' from the predicted position, implying a delta T of -0.2 days. The comet passed 0.46 au from Jupiter in 1975 December in an encounter that substantially reduced the perihelion distance. The comet is significantly fainter at this return than it was at the discovery return. [CBET 4933, MPEC 2021-D104, 2021 February 16/25]. In what seems to be competition between the CBET and MPC the MPEC was issued nine days after the CBET.
In 2009 October Rob Matson found images of the comet on three Heleakala-NEAT images from 1996, which in turn allowed him to find it in two more nights from 1998. It was very bright in the 1996 images showing obvious coma, but barely detectable in 1998.
Erwin Schwab recovered the comet as a stellar object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 March 11.13. The recovery was confirmed by Diana Abreu using the 1.0m reflector at the ESA Optical Ground Station, Tenerife on March 14. The comet was some 9' from the expected position and does not reach perihelion until 2022 May. When Syuichi Nakano computed a linked orbit the observations showed that non-gravitiational parameters were required. When these were included it was found that the 1996 observations reported by Rob Matson were of the comet, though his 1998 measurements did not fit so well. [CBET 4943, MPEC 2021-F07, 2021 March 16/17]
Brian Marsden noted on MPEC 2009-Y57 [2009 December 29] that further [astrometric] observations of this comet were desirable.
In 2021 May the MPC linked isolated tracklets from PanSTARRS and Mt Lemmon made in 2020 April and May to 2009 U4 (P/McNaught). [CBET 4971, MPEC 2021-K101, 2021 May 31] The comet was at perihelion at 1.6 au in 2021 January, about 6 days earlier than predicted, and has a period of 11.4 years.
Cristovao Jacques recovered the comet at the SONEAR observatory on 2021 June 5.32. Taras Prystavski independently recovered the comet on 2021 June 15.75 using the 0.5 m iTelescope at Siding Spring, some 9' from the ephemeris position. The recovery was reported on the comets-ml on June 15/16, with Jacques noting that he had sent the observations to the MPC 10 days previously. The MPC is a bit behind with processing comet observations and did not announce the recovery until June 17 [MPEC 2021-M34, CBET 4979]
The comet was recovered in astrometry taken with the Gemini North 8.1 m telescope at Mauna Kea on January 9.27 and January 15. The comet passed 0.7 au from Jupiter in 1921 and 0.9 au from the planet in 1986. These encounters modified the elements, but kept the perihelion distance between 5.2 and 5.6 au. [MPEC 2021-M89 CBET 4992, 2021 June 26]. The MPEC does not say why there was such a long gap between the observations and announcement.
Images of the comet were found in incidental PanSTARRS 1 asrometry taken with the 1.8m Ritchey-Chretien on 2021 June 6.53. It was independently found later in images from ATLAS at Mauna Loa. [CBET 49xx, MPEC 2021-N47, 2021 July 8] The comet is at perihelion at 1.4 au in 2021 October and has a period of 9.3 years.
PanSTARRS 1 discovered a 20th magnitude comet in images taken with the 1.8m Ritchey-Chretien on July 20.60. It was identified as a return of 2005 W3 by the MPC. There were prediscovery PanSTARRS observations from 2020 September, October, November and December. The comet was some 13' from the predicted position, corresponding to a delta T of around -1.0 days. [CBET 4506, MPEC 2021-O66, 2021 July 30] At this return the comet is at perihelion at 2.9 au in 2021 September and has a period of 15.9 years. It made a distant encounter (1.1 au) with Saturn in 2014 July.
Marco Micheli recovered 2019 A7 in images taken by other observers with the 8.1m Gemini South telescope on May 17.17. He found confirmatory images of the comet in data from the Canada-France-Hawaii at Mauna Kea taken on June 13. [MPEC 2021-P78, CBET 5010, 2021 August 8] It reaches perihelion in 2023 September.
Marco Micheli recovered 2017 S5 in images taken by other observers with the 8.1m Gemini South telescope on June 9.07. [MPEC 2021-P79, CBET 5011, 2021 August 8]. It reaches perihelion in 2023 March.
Erwin Schwab recovered comet 2014 W12 as a 20th magnitude object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 August 16.13. It was a long way from the predicted position, with a delta T of -37.6 days, putting the comet at perihelion in 2021 May rather than June. Hirohisa Sato then reported the comet in images taken on August 7, with Syuichi Nakano then able to find images from the Catalina Sky Survey from 2008 November. There have been no close encounters with any major planets. [MPEC 2021-Q47, CBET 5025, 2021 August 22/23]
In 2020 Sam Deen found images of the comet in DECam data taken with the 4.0m reflector at Cerro Tololo on 2016 January 15.26 and 2016 March 1.14. These were identified by Syuichi Nakano as being a return of 2008 QP20. The comet was close to the expected position. [CBET 4832, 2020 August 17] It was not given a designation for the return, nor was it numbered at the time, though it should have been 410P.
PanSTARRS found a 23rd magnitude image of 2008 QP20 in data taken with the PanSTARRS 1 1.8m Ritchey-Chretien on June 18.59, with additional images from July and August. Despite having been identified at the 2015 return it was given a year identifier. The CBET suggests that it should have been designated as 2016 [A]10 at that return. [MPEC 2021-Q68, 2021 August 28, CBET 5040, 2021 September 18] The comet is at perihelion at 1.8 au in 2022 January and now has a period of 6.7 years following a distant encounter with Jupiter in 2017 July.
Gareth Williams noted on MPEC 2011-A65 [2011 January 14] that it was probable that this was a short-period comet and that further [astrometric] observations of the comet were desirable.
Further observations confirmed the short period orbit, and Hirohisa Sato gave a period of around 5.5 years with perihelion at 1.6 au in 2010 December.
The comet was recovered on 2021 August 20.50 in images taken by the Zwicky Transient Factory with the 1.2m Oschin Schmidt. It was also present in images taken on August 23, 24 and 25. The comet is at perihelion at 1.6 au in December and has a period of 5.5 years. It was some 17' from the predicted position, corresponding to a delta T of +0.79 days. The comet passed 0.41 au from Jupiter in 1986. [MPEC 2021-Q69, CBET 5026, 2021 August 28/31]
Francois Kugel recovered 2015 Q1 in images taken on August 2.96 at his observatory "Chante-Perdrix" (Dauban, France) with his 0.4-m f/2.8 reflector. This was confirmed in follow up observations on August 7 and 16 and by other amateurs Jean-Francois Soulier and John J Maikner. [MPEC 2021-Q75, 2021 August 29, CBET 5038, 2021 September 17] Rob Matson then found prediscovery observations made with the 1.2-m Palomar Schmidt in 2002, but no designation has yet been assigned for that return. The comet passed 0.6 au from Jupiter in 2005 December in an encounter that reduced the perihelion distance, whilst it passed 1.5 au in 2017 December, which increased the perihelion distance. The comet is next at perihelion at 1.8 au in 2022 February and has a period of 6.5 years.
As the orbit improved it became possible to search for earlier observations and PanSTARRS found images of the comet in data taken on 2016 October 25.47 and November 15. It was designated 2016 U2 for this return, though the MPEC does not give elements for that epoch. The CBET confirms the comet name as PanSTARRS. [MPEC 2021-Q96, 2021 August 31, CBET 5041, 2021 September 19]
A paper by Hsieh et al characterises the object as a Main Belt Comet, with activity driven by sublimation around perihelion. They note that archival observations also show activity at the last perihelion in 2016 and estimate a nuclear radius of around 1.6 km. They suggest that it might be a fast rotator.
Erwin Schwab recovered comet 2012 TK8 as a 20th magnitude object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 September 30.16. The comet was some 6' from the predicted position, indicating a Delta(T) of -0.38 day. [MPEC 2021-T44, CBET 5048, 2021 October 4] The comet was at perihelion at 3.0 au in 2021 October and now has a period of 8.4 years.
Taras Prystavski recovered 2007 R4 in images taken with the 0.51m iTelescope at Siding Spring on October 24.43. Confirmation came from John Drummond who had imaged the comet on September 5.47. The MPEC gives additional positions from John taken on August 15.61 but does not mention the September observations. The CBET does include these observations, along with additional ones by Filipp Romanov on August 13.61. The comet was some 7' east of the ephemeris position, corresponding to a delta-T of -0.2 days. [MPEC 2021-U108, CBET 5061, 2021 October 27]
Alessandro Odasso identified an object given the minor planet designation of 2020 OV62, found by the Mt Lemmon Survey on 2020 July 31.42, as being a return of 2005 T2. The MPC then found detections by PanSTARRS on 2012 November 5.21 at which return it was given the designation 2012 V5. Sam Deen then found additional PanSTARRS detections from 2012 August, in images taken with the CFH telescope at Mauna Kea in 2013 October and with DECam in 2019 June. The 2012 positions were over a degree from that expected from published predictions. [MPEC 2021-W47, CBET 5073, 2021 November 24/26] The comet will pass 0.40 au from Jupiter in 2037 November, although the 2012 Jupiter MOID was 0.45 au.
Erwin Schwab recovered the comet as a 20th magnitude object in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2021 November 30.03. The position was close to that previously predicted, although it was missed at the 2015 return. The MPC then found an isolated tracklet from PanSTARRS 1 from August 8. [MPEC 2021-X81, CBET 5078, 2021 December 3] The comet passed 0.81 au from Jupiter in 2017 October in an encounter that has increased the perihelion distance to 1.85 au. The next close Jupiter encounter is in 2077, when the comet passes within 0.3 au.
The Purple Mountain Observatory discovered a potential 20th magnitude NEO at their XuYi station with their 1.04m Schmidt on 2022 January 11.67. The MPC identified this as a return of 1997 B1 and then found isolated tracklets from 2021 November 29 taken with the Bok 2.25m reflector at Kitt Peak. PanSTARRS then found the comet in images taken earlier in November. This sequence suggests that the comet should have been designated 2022 A2 as this was the discovery. The comet was some 0.5 degrees from the prediction based on observations in 1997. [MPEC 2022 A164, CBET 5091, 2022 January 11/12] The comet is at perihelion at 2.0 au in March and has a period of 25 years. The comet was close to 67P/ in the sky and Nick James subsequently discovered that he had imaged it on January 9, as did Peter Carson.
The MPC identified a 21st magnitude object found in incidental astrometry from Mt Lemmon on January 25.51 and PanSTARRS 2 on February 10.50 as being a return of 2017 R1. [CBET 5100, MPEC 2022-D03, 2022 February 16] The comet is at perihelion at 3.3 au in 2025 September and has a period of 8.4 years.
The comet is one of those suspected to have undergone nuclear splitting according to the list of Marcos & Marcos [Dynamically correlated minor bodies in the outer solar system, MNRAS, 474, 838, 2018 February]. They link it to 208P/McMillan.
Hirohisa Sato recovered 2011 Q3 at 20th magnitude in images taken with the 0.51-m f/6.8 iTelescope astrograph at Siding Spring on 2022 April 5.79, with confirming images taken with the same telescope five days later. [MPEC 2022-H01, CBET 5115, 2022 April 16/19]. The comet is at perihelion at 2.3 au in August. Following the recovery Syuichi Nakano was able to link isolated observations made on 2000 November 28.21 by Spacewatch to the comet. He notes that the comet passed 0.75 au from Jupiter in 1990 and 0.53 au in 2002, in encounters that made changes mostly to the angular elements.
It appeared on the PCCP as 2F61M11 on 2022 June 7.65, so was presumably recovered, though confirmation had to wait a month. Following the recovery additional tracklets from 1998 and 2006 were identified. The comet is at perihelion at 2.4 au in 2022 August and has a period of 8.2 years. [MPEC 2022-N51, CBET 5149, 2022 July 8]
PanSTARRS 2 discovered a new object on June 28.58, which the MPEC automatically identified as a return of 2012 O3. Hirohisa Sato was then able to find the comet in images taken with the 0.51-m f/6.8 iTelescope astrograph at Siding Spring on April 10.80. PanSTARRS checked their images and confirmed that they did show cometary activity. [MPEC 2022-N81, CBET 5150, 2022 July 12]. The comet was at perihelion at 1.6 au in May. It is not clear why the MPEC did not designate the comet as 2022 M2 (or M1) as would be expected from the discovery date.
The comet orbit has a Jupiter MOID of 0.65 au and the comet approached to 0.74 au in 1933 June.
Erwin Schwab recovered comet 2015 X1 at 21st magnitude and essentially stellar, in images taken with the 0.8-m f/3 Schmidt reflector at Calar Alto, Spain, on 2022 August 23.09. Additional confirming observations were made on August 24. Following recovery, Syuichi Nakano was able to link MPC ITF positions from 2008 October 1.38 and 2008 December 31 taken by the Catalina Sky Survey to the comet. [MPEC 2022-Q153, CBET 5164, 2022 August 28]. The comet is at perihelion at 2.1 au in September and has a period of 6.9 years. The comet passed 0.6 au from Jupiter in 2005 January; the orbit has a Jupiter MOID of 0.54 au.
Following the discovery, Syuichi Nakano was able to link an asteroid discovered by LONEOS on 2000 July 29.36 and designated 2000 OZ21, but only observed over a five day arc, with the comet. [CBET 5166, 2022 September 3]
Published by Jonathan Shanklin. Jon Shanklin - firstname.lastname@example.org