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255P/Levy

From Wikipedia, the free encyclopedia
Periodic comet
For other comets discovered by David H. Levy, seeComet Levy.
255P/Levy
Discovery[1]
Discovered byDavid H. Levy
Discovery siteJarnac Observatory (G92)
Discovery date2 October 2006
Designations
P/2006 T1
P/2011 Y1
PK06T010
Orbital characteristics[4]
Epoch5 July 2021 (JD 2459400.5)
Observation arc5,484 days (15 years)
Number of
observations
590
Aphelion5.04 AU
Perihelion0.846 AU
Semi-major axis2.94 AU
Eccentricity0.7126
Orbital period5.05 years
Inclination13.46°
275.9°
Argument of
periapsis
185.8°
Last perihelion7 September 2022[2]
Next perihelion25 September 2027[3]
TJupiter2.792
EarthMOID0.0088 AU (2007)[5]
JupiterMOID0.1539 AU (2007)
Physical characteristics
Comet total
magnitude
(M1)
11.5
Comet nuclear
magnitude (M2)
15.1
9.5
(2006 apparition)

255P/Levy, formerlyP/2006 T1 andP/2011 Y1, is aJupiter-family comet with an orbital period of 5.25 years.[5] It last came toperihelion (closest approach to the Sun) on 14 January 2012.[6] During the 2006 passage the comet achieved anapparent magnitude of ~9.5.[7] Levy (PK06T010) was believed to have been recovered on 3 June 2011 at magnitude 19.8,[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.[9] It was then numbered.

It came to perihelion on 14 January 2012 at a distance of 1.007 AU (150.6 million km) from the Sun.[6] The comet passed the Earth on 2012-Jan-26 at a distance of 0.2359 AU (35.29×10^6 km).[10] During the 2012 passage the comet was originally expected to reach an apparent magnitude of 7, but the comet had been in outburst in 2006 and was much dimmer than expected when it was recovered in 2011.MPC estimates after the 2011 recovery estimated that it would reach a magnitude of 17, and it had anelongation of 90°. However, CCD images showed it was diffuse[11] and the comet's magnitude was estimated at 14.1 on 30 December 2011.[12] The comet was not observed during the 2017 or 2022 perihelion passage.[13] Atopposition in August 2016 it would have been dimmer than magnitude 19.

255P/Levy (using anepoch of 2007) has a minimum orbit intersection distance with Earth roughly about 0.0088 AU (1.32 million km).[5]

The comet has been associated with α Cepheidsmeteor shower, which peaks on 2 January.[14]

References

[edit]
  1. ^"MPEC 2006-T21: COMET C/2006 T1 (LEVY)".Minor Planet Electronic Circular.Minor Planet Center. 3 October 2006. Retrieved21 November 2024.
  2. ^"Horizons Batch for 255P/Levy on 2022-Sep-07" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons. Retrieved2023-04-30. (JPL#40/Soln.date: 2021-Oct-18)
  3. ^"Horizons Batch for 255P/Levy on 2027-Sep-25" (Perihelion occurs when rdot flips from negative to positive).JPL Horizons. Retrieved2023-04-30. (JPL#40/Soln.date: 2021-Oct-18)
  4. ^"255P/Levy".Minor Planet Center. Retrieved2025-11-01.
  5. ^abc"255P/Levy – JPL Small-Body Database Lookup".ssd.jpl.nasa.gov.Jet Propulsion Laboratory. Retrieved10 January 2016.
  6. ^ab"P/2006 T1 (Levy)" (last observation: 2011-12-17).Minor Planet Center. Retrieved2011-12-18.
  7. ^"P/2006 T1 Comet for Windows apmag graph for 2006". aerith.net. Retrieved2011-04-07.
  8. ^"MPEC 2011-L51: OBSERVATIONS AND ORBITS OF COMETS".Minor Planet Electronic Circular.Minor Planet Center. 12 June 2011. Retrieved13 June 2011.
  9. ^"MPEC 2011-Y07: P/2006 T1 = 2011 Y1 (Levy)".Minor Planet Electronic Circular.Minor Planet Center. 18 December 2011. Retrieved19 December 2011.
  10. ^"JPL Close-Approach Data: P/2006 T1 (Levy)" (last observation: 2011-12-30;arc: 5.24 years). Retrieved2012-01-04.
  11. ^"Weekly Information about Bright Comets (2011 Dec. 24: North)". aerith.net. 2011-12-27. Retrieved2012-01-04.
  12. ^"CCD comet estimates". severastro.narod.ru. 2012-01-01. Archived fromthe original on 2012-04-22. Retrieved2012-01-04.
  13. ^"255P/Levy Orbit".Minor Planet Center. Retrieved2014-06-20.
  14. ^D. Šegon; P. Gural; Z. Andreić; I. Skokić; K. Korlević; et al. (April 2014)."New showers from parent body search across several video meteor databases".WGN, Journal of the International Meteor Organization.42 (2):57–64.Bibcode:2014JIMO...42...57S.ISSN 1016-3115.

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