2013 SY99
The orbits of 2013 SY99 (left; light blue) and other detached objects, along with the hypothetical Planet Nine's orbit (right; green)
Discovery[1]
Discovered byOSSOS
Discovery siteCFHT
Discovery date29 September 2013
Designations
2013 SY99
uo3L91[2] (OSSOS survey designation)
TNO · detached
Orbital characteristics
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 4[3]
Observation arc4.30 yr[3]
Earliest precovery date5 September 2013
Aphelion
Perihelion50.029 ± 0.056 AU[3]
(7.48 ± 0.01 billion km; 4.65 ± 0.01 billion mi)
  • Barycentric: 730 AU[4][n 1]
    (109 billion km; 68 billion mi)
  • Heliocentric: 690.4 ± 22.5 AU[3]
    (103.3 ± 3.4 billion km; 64.2 ± 2.1 billion mi)
Eccentricity0.9274±0.0024[3]
359.292°±0.034°[3]
0.203±0.010 arcsec/day[3]
Inclination4.228°±0.001°[3]
29.493°±0.005°[3]
≈ 4 December 2054[6]
±1 month
32.037°±0.114°[3]
Jupiter MOID45.00 AU[3]
(6.7 billion km; 4.2 billion mi)
Physical characteristics
Mean diameter
≈250 km (160 mi)[7]
0.05±0.03[7]
moderately red[7]
24.5 (V)[8]
23.67 (peak 2055)[3]
6.7[3][8]

    2013 SY99, also known by its OSSOS survey designation uo3L91, is a trans-Neptunian object discovered on September 29, 2013 by the Outer Solar System Origins Survey using the Canada–France–Hawaii Telescope at Mauna Kea Observatory. This object orbits the Sun between 50 and 1,300 AU (7.5 and 190 billion km), and has a barycentric orbital period of nearly 20,000 years.[4][5][1] It has the fourth largest semi-major axis for an orbit with perihelion beyond 38 AU.[9][10] 2013 SY99 has one of highest perihelia of any known extreme trans-Neptunian object, behind sednoids including Sedna (76 AU), 2012 VP113 (80 AU), and Leleākūhonua (65 AU).

    Discovery

    According to astronomers Mike Brown and Konstantin Batygin, the discovery of 2013 SY99 provides additional evidence for the existence of Planet Nine, but Michele Bannister (see 10463), one of the astronomers who reported the discovery of this object, disputes this due to the orientation of the orbit.[1][11]

    Its existence was announced in 2016, but the observations were kept private until 2017. It was listed at the Minor Planet Center and the JPL Small-Body Database on 6 April 2017[8] with a three-year observation arc and an epoch 2017 heliocentric orbital period of 17,500 years.[3] Barycentric orbital solutions, however, are more stable for objects on multi-thousand year orbits, and the barycentric period for 2013 SY99 is 19,700 years.[4][n 1]

    As of April 2019, its perihelion distance of q=50.029±0.056 AU and semi-major axis a=690±22 AU make 2013 SY99 a possible sednoid, according to the most common definition of the term (q>50 AU, a>150 AU). It is listed as a sednoid by some.[12] However, 2013 SY99 is usually considered to be an extreme trans-Neptunian object and not a sednoid, due to its high eccentricity which makes the heliocentric orbit unstable.[13][n 1] In the heliocentric reference frame, the perihelion is currently rising, and the nominal orbit has a perihelion distance above 50 AU only since October 2018.[14]

    2013 SY99 is estimated to be about 250 km (160 mi) in diameter and moderately red in color.[7] In 2052 it will be roughly 20.3 AU (3.04 billion km) from Neptune. It will come to perihelion (closest approach to the Sun) around 2055 when it will be 50 AU (7.5 billion km) from the Sun.[3]

    See also

    Notes

    1. 1 2 3 4 5 Heliocentric solutions are unstable due to the changing position of Jupiter over Jupiter's 12 year orbit which perturbs the eccentricity of the two-body solution of the Sun+asteroid. Barycentric solutions are more stable for objects that take thousands of years to orbit the Sun. Between epoch 2017 and epoch 2029, the heliocentric orbital period varies from a low of 17400 years "PR= 6.364×106 d (epoch 2017-Nov-16)" to a high of 26100 years "PR= 9.538×106 d (epoch 2023-Nov-16)".

    References

    1. 1 2 3 Witze, Alexandra (18 October 2016). "Astronomers spot distant world in Solar System's far reaches". Nature. doi:10.1038/nature.2016.20831.
    2. ↑ Shankman, Cory; et al. (2017). "OSSOS. VI. Striking Biases in the Detection of Large Semimajor Axis Trans-Neptunian Objects". The Astronomical Journal. 154 (2): 50. arXiv:1706.05348. Bibcode:2017AJ....154...50S. doi:10.3847/1538-3881/aa7aed. hdl:10150/625487. S2CID 3535702.
    3. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 "JPL Small-Body Database Browser: (2013 SY99)" (last observation: 4 November 2016; arc: 3.16 years). Jet Propulsion Laboratory. Retrieved 15 October 2018.
    4. 1 2 3 4 5 Horizons output. "Barycentric Osculating Orbital Elements for 2013 SY99". Retrieved 6 April 2017. (Ephemeris Type:Elements and Center:@0)
    5. 1 2 Mann, Adam (17 October 2016). "New icy world with 20,000-year orbit could point to Planet Nine". Science. doi:10.1126/science.aal0270.
    6. ↑ JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)
    7. 1 2 3 4 Bannister, Michele; Shankman, Cory; Volk, Katherine (2017). "OSSOS: V. Diffusion in the orbit of a high-perihelion distant Solar System object". The Astronomical Journal. 153 (6): 262. arXiv:1704.01952. Bibcode:2017AJ....153..262B. doi:10.3847/1538-3881/aa6db5. S2CID 3502267.
    8. 1 2 3 "MPEC 2017-G55 : 2013 SY99". IAU Minor Planet Center. 6 April 2017. Retrieved 15 October 2018. (K13S99Y)
    9. ↑ "Objects with q > 38 & a > 250". Minor Planet Center. International Astronomical Union. Retrieved 24 October 2016.
    10. ↑ Bannister, Michele T.; Chen, Ying-Tung; Jakubik, Marian; et al. (October 2016). A new high-perihelion a ~ 700 AU object in the distant Solar System. 48th Meeting of the Division for Planetary Sciences. 16–21 October 2016. Pasadena, California. Bibcode:2016DPS....4811308B. 113.08.
    11. ↑ Brown, Mike (24 March 2016). "the new one is uo3L91..." Twitter.com.
    12. ↑ Johnston, W. R. (7 October 2018). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 15 October 2018.
    13. ↑ Scott Sheppard; Chadwick Trujillo; David Tholen; Nathan Kaib (2 October 2018). "A New High Perihelion Inner Oort Cloud Object". arXiv:1810.00013. doi:10.3847/1538-3881/ab0895. S2CID 119071596. {{cite journal}}: Cite journal requires |journal= (help)
    14. ↑ JPL Horizons On-Line Ephemeris System. "Ephemeris Type: ELEMENTS, Target Body: Asteroid (2013 SY99), Center: Sun (body center) [500@10], Time Span: Start=2018-10-01, Stop=2018-10-15, Step=1 d, Table Settings: defaults, Display/Output: default (formatted HTML)". Retrieved 4 October 2018.
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