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(523731) 2014 OK394

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(523731) 2014 OK394
Discovery[1]
Discovered byPan-STARRS 1
Discovery siteHaleakalā Obs.
Discovery date8 October 2010
Designations
1995 SN55[2]
3:5 resonant[3] · TNO[4] · distant[2]
Orbital characteristics[4]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 2
Observation arc25.14 yr (9,181 days)
Earliest precovery date20 September 1995 (Spacewatch)[5]
Aphelion49.153 AU
Perihelion35.351 AU
42.252 AU
Eccentricity0.16333
274.65 yr
30.889°
0° 0m 12.919s / day
Inclination4.140°
128.384°
≈ 4 January 1997[6]
247.580°
Known satellites0
Physical characteristics
160–280 km (est. 0.08–0.20)[7][8]
6.2[2][4]

(523731) 2014 OK394 is a trans-Neptunian object that orbits in the outer Solar System beyond the orbit of Neptune. Once thought to be a centaur crossing the orbits of the gas giants,[9] 2014 OK394 is now known to be a trans-Neptunian object in a 3:5 orbital resonance with Neptune.[4] With an estimated diameter between 160–280 kilometers (99–170 miles), it was formerly thought to be one of the largest centaurs.[7][10][11]

Discovery

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The object was discovered twice and therefore has two provisional designations. It was near perihelion 35.4 AU from the Sun when it was first observed on 20 September 1995 by astronomers Nichole Danzl and Arianna Gleason of the Spacewatch survey at Kitt Peak Observatory in Arizona, United States.[5] It was given the designation 1995 SN55.[1] However, it was only observed 14 times over 36 days, from 20 September to 26 October 1995.[9] The discovery observations were published by the Minor Planet Center on 11 June 1999.[5] By then the uncertainty in the original orbit solution was too great for easy recovery.

On 8 October 2010, it was unknowingly rediscovered by the Pan-STARRS 1 survey and in July 2016 it was announced as 2014 OK394.[12] When its orbit was secure, it was assigned the permanent designation (523731). Ten years later, on 30 November 2020, amateur astronomers S. Deen and K. Ly identified 2014 OK394 as being the same object as 1995 SN55.[12] This identification was published by the Minor Planet Center on 27 January 2021.[13]

Classification and orbit

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2014 OK394 orbits the Sun at an average distance of 42.33 AU once every 275 years. Its orbit has an eccentricity of 0.16 and an inclination of 4° with respect to the ecliptic plane. Over the course of its orbit, its distance from the Sun ranges from 35.4 AU at perihelion to 49.3 AU at aphelion. 2014 OK394 is in a 3:5 mean-motion orbital resonance with Neptune; for every three orbits it makes, Neptune orbits five times.[3] Its orbit has a minimum orbit intersection distance approximately 5.6 AU (840 million km; 520 million mi) from Neptune's orbital path.[4]

Numbering and naming

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2014 OK394 was numbered by the Minor Planet Center on 25 September 2018 and received the number 523731 in the minor planet catalog.[14] The provisional designation 1995 SN55 was added by the Minor Planet Center on 27 January 2021 after the two discoveries were linked.[13] As of 2026, it has not been named.[2]

See also

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References

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  1. ^ a b Gibson, B.; Goggia, T.; Primak, N.; Schultz, A.; Willman, M.; Chambers, K.; Chastel, S.; Chen, Y. -T.; Denneau, L.; Flewelling, H.; Holman, M.; Huber, M.; Jedicke, R.; Lackner, M.; Lilly, E.; Lin, H. -W.; Magnier, E.; Micheli, M.; Payne, M.; Veres, P.; Wainscoat, R.; Waters, C.; Weryk, R. (17 July 2016). "MPEC 2016-O154 : 2014 OK394". Minor Planet Electronic Circular. 2016-O154. Minor Planet Center. Bibcode:2016MPEC....O..154G. Retrieved 23 February 2021.
  2. ^ a b c d "(523731) = 1995 SN55 = 2014 OK394". Minor Planet Center. International Astronomical Union. Archived from the original on 30 November 2020. Retrieved 23 February 2021.
  3. ^ a b Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 24 February 2021.
  4. ^ a b c d e "JPL Small-Body Database Browser: 523731 (2014 OK394 = 1995 SN55)" (2020-11-19 last obs.). Jet Propulsion Laboratory. Archived from the original on 30 November 2020. Retrieved 23 February 2021.
  5. ^ a b c Marsden, Brian G. (11 June 1999). "MPEC 1999-L25 : 1995 SN55, 1998 TF35". Minor Planet Electronic Circular. 1999-L25. Minor Planet Center. Bibcode:1999MPEC....L...25D. Retrieved 30 November 2020.
  6. ^ "JPL Horizons On-Line Ephemeris for 523731 (2014 OK394 = 1995 SN55)". JPL Horizons On-Line Ephemeris System. Jet Propulsion Laboratory. Retrieved 10 February 2021.
    Ephemeris Type: OBSERVER, Target Body: 523731 (2014 OK394), Observer Location: Sun (body center) [500@10], Table Settings: QUANTITIES=20. Observer range
    (Perihelion occurs when deldot changes from negative to positive.)
  7. ^ a b Brown, Michael E. (23 February 2021). "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 24 February 2021.
  8. ^ Bruton, Dan. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics, Engineering, and Astronomy. Stephen F. Austin State University. Archived from the original on 23 July 2011. Retrieved 24 February 2021.
  9. ^ a b "JPL Small-Body Database Browser: (1995 SN55)" (1995-10-26 last obs.). Jet Propulsion Laboratory. Archived from the original on 30 November 2020. Retrieved 24 February 2021.
    (Archive of 36 day observation arc of 1995 SN55)
  10. ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. International Astronomical Union. Archived from the original on 18 November 2020. Retrieved 24 February 2021. (Archived list of centaurs including 1995 SN55)
  11. ^ Sokol, Joshua (25 October 2017). "A 300-kilometre space rock has vanished since we saw it in 1995". New Scientist. Retrieved 24 February 2021.
  12. ^ a b Deen, Sam (30 November 2020). "1995 SN55". groups.io. Retrieved 23 February 2021.
  13. ^ a b "M.P.C. 127300" (PDF). Minor Planet Circular. Minor Planet Center. 27 January 2021. Retrieved 23 February 2021.
  14. ^ "M.P.C. 111781" (PDF). Minor Planet Circular. Minor Planet Center. 25 September 2018. Retrieved 23 February 2021.
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