(87269) 2000 OO67

Trans-Neptunian object yes #C2E0FF (87269) 2000 OO 67 Cerro Tololo Obs. Cerro Tololo Obs. 29 July 2000 2000 OO 67 TNOcentaur (DES) 13 January 2016 (JD 2457400.5) 2 2187 days (5.99 yr) 29 July 2000 1.82 AU Tm on(87269) = 2000 OO67 IAU minor planet center https://www.minorplanetcenter.net/db_search/show_object?object_id=87269 https://archive.today/20130626202231/http://www.minorplanetcenter.net/db_search/show_object?object_id=87269 2013-06-26 live 2017-02-22 5.265 531.2369251 AU Tm on 20.7305754 AU Tm on 1041.743 AU Tm on on 0.9609768 11760.29 yr (4295446.2 d) 20.0729° 142.391° 212.345° 0.328967° 0.0000838097 ms / day 0.88 km/s 64 km (est. at 0.09) Asteroid Size Estimator CNEOS NASA/JPL https://cneos.jpl.nasa.gov/tools/ast_size_est.html 3 March 2020 9.2 ~12 K (87269) 2000 OO 67 is a trans-Neptunian object, approximately 64 km mi off 2 us in diameter, on a highly eccentric orbit in the outermost region of the Solar System. It was discovered by astronomers at the Chilean Cerro Tololo Inter-American Observatory on 29 July 2000. Description At aphelion it is over 1,000 AU from the Sun and, with a perihelion of 21 AU, almost crosses the orbit of Uranus at closest approach. Astronomers with the Deep Ecliptic Survey classify it as a centaur rather than a trans-Neptunian object.https://doi.org/10.1007%2Fs11038-006-9095-5 10.1007/s11038-006-9095-5 Structure and Dynamics of the Centaur Population: Constraints on the Origin of Short-Period Comets 2006 Emelʹyanenko V.V. Earth, Moon, and Planets 97 3–4 341–351 122072238 subscription 2000 OO 67 came to perihelion in April 2005.Marc W. Buie Marc W. Buie Orbit Fit and Astrometric record for 87269 2006-07-25 using 33 of 34 obs Deep Ecliptic Survey http://www.boulder.swri.edu/~buie/kbo/astrom/87269.html 2008-05-18JPL Small-Body Database Browser: 87269 (2000 OO67) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=87269 2006-07-25 last obs 12 April 2016 Yeomans Donald K. http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2000OO67 Horizons Online Ephemeris System California Institute of Technology, Jet Propulsion Laboratory 2008-01-25 Comparison June 2026 thumb|left|500px|The orbits of Sedna, 2012 VP 113, Leleākūhonua, and other very distant objects along with the predicted orbit of Planet Nine. The three sednoids (pink) along with the red-colored extreme trans-Neptunian object (eTNO) orbits are suspected to be aligned with the hypothetical Planet Nine while the blue-colored eTNO orbits are anti-aligned. The highly elongated orbits colored brown include centaurs and damocloids with large aphelion distances over 200 AU. See also 2005 VX 3 (308933) 2006 SQ 372 (523622) 2007 TG 422 TAU (spacecraft) (probe designed to go 1000 AU in 50 years) List of Solar System objects by greatest aphelion References External links List Of Centaurs and Scattered-Disk Objects at the Minor Planet Center 87269 87269 87269 (87269) 2000 OO 67 Category:Scattered disc and detached objects Category:Centaurs (small Solar System bodies) Category:Discoveries by CTIO Category:Discoveries by the Deep Ecliptic Survey 20000729 Category:Inner Oort cloud 087269