Skip to main content

  | मौसम…

411 समाचार
Public archive edition · Attributed source reporting with original dates · AI drafts are excluded

411 REFERENCE · Wikipedia

(153201) 2000 WO107

Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.

Sub-kilometer asteroid October 2019 yes (153201) 2000 WO 107 #FFC2E0 2000WO107-20201128.jpg Goldstone radar images showing the two lobes of contact binary 2000 WO 107. LINEAR Lincoln Lab's ETS 29 November 2000 (153201) 2000 WO 107 AtenNEOPHA 2020-May-31 (JD 2459000.5) 0 20.0 yr (7,304 days) 1.6231 AU 0.2000 AU 13 October 2020 0.9115 AU 0.7807 0.87 yr (318 days) 206.45° 1.1327 ms / day 7.7703° 69.252° 213.72° 0.0031 AU e3km LD unit on 0.510 0.083 km 4.8 hours 0.129 0.058 SMASS X 19.3 (153201) 2000 WO 107 is a sub-kilometer asteroid, classified as a near-Earth object and potentially hazardous asteroid of the Aten group with a very well determined orbit. It was discovered on 29 November 2000, by astronomers of the Lincoln Near-Earth Asteroid Research (LINEAR) at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. It is a contact binary. Orbit The orbit of this potentially hazardous asteroid (PHA) has been well-established with 20 years of observations. It orbits from inside the orbit of Mercury out to the orbit of Mars. It makes close approaches to all of the inner planets. 2020 The asteroid came to perihelion on 13 October 2020 when it passed the Sun going 88 km/s km/h off us.speed The asteroid was not more than 60 degrees from the Sun until 26 November 2020 and was observed by Goldstone radar on 27 November 2020. On 29 November 2020 the asteroid passed 0.02876 AU e6km LD unit on from Earth. Even the 2018 orbit solution had a known accuracy of roughly ±150 km for the close approach. With the radar observations the close approach distance is known with an accuracy of roughly ±5 km. 2140 This asteroid will pass 0.00162 AU e3km LD unit on from Earth on 1 December 2140. The 2140 close approach distance is known with an accuracy of roughly ±1000 km. For comparison, the distance to the Moon is about 0.0026 AU (384,400 km). The Jupiter Tisserand invariant, used to distinguish different kinds of orbits, is 6.228. Physical characteristics In the SMASS classification, the object's spectral type is that of an X-type. According to the space-based survey by NASA's NEOWISE mission, the asteroid measures 510 meters in diameter and its surface has an albedo of 0.129. Numbering and naming This minor planet was numbered by the Minor Planet Center on 2 April 2007. As of 2018, it has not been named. __NOTOC__ See also 2002 NY 40 2014 HQ 124 (388188) 2006 DP 14 (53319) 1999 JM 8 Notes speed v = 42.1219 1/r − 0.5/a, where r is the distance from the Sun, and a is the major semi-axis. Objects move fastest at perihelion and slowest at aphelion. References 30em 2020-11-28 last obs. JPL Small-Body Database Browser: 153201 (2000 WO107) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2153201;cad=1 Jet Propulsion Laboratory https://web.archive.org/web/20201106120852/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2153201;cad=1 2020-11-06 live 29 November 2020 153201 (2000 WO107) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=153201 13 January 2018 Goldstone Radar Observations Planning: (7753) 1988 XB, 2017 WJ16, and 2000 WO107 Asteroid Radar Research https://echo.jpl.nasa.gov/asteroids/1988XB/1988xb.2020.goldstone.planning.html 29 November 2020 MPC/MPO/MPS Archive Minor Planet Center https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html 24 February 2018 6 A. Mainzer T. Grav J. Bauer J. Masiero R. S. McMillan R. M. Cutri R. Walker E. Wright P. Eisenhardt D. J. Tholen T. Spahr R. Jedicke L. Denneau E. DeBaun D. Elsbury T. Gautier S. Gomillion E. Hand W. Mo J. Watkins A. Wilkins G. L. Bryngelson A. Del Pino Molina S. Desai M. Gómez Camus S. L. Hidalgo I. Konstantopoulos J. A. Larsen C. Maleszewski M. A. Malkan J.-C. Mauduit B. L. Mullan E. W. Olszewski J. Pforr A. Saro J. V. Scotti L. H. Wasserman December 2011 NEOWISE Observations of Near-Earth Objects: Preliminary Results http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...743..156M The Astrophysical Journal 743 2 17 2011ApJ...743..156M 10.1088/0004-637X/743/2/156 1109.6400 13 January 2018 Richard P. Binzel Andrew S. Rivkin J. Scott Stuart Alan W. Harris Schelte J. Bus Thomas H. Burbine Observed spectral properties of near-Earth objects: results for population distribution, source regions, and space weathering processes http://www.mtholyoke.edu/~tburbine/binzel.icarus.2004.pdf Icarus 170 2 20 March 2004 259–294 2004Icar..170..259B 10.1016/j.icarus.2004.04.004 October 2026 InternetArchiveBot External links List Of The Potentially Hazardous Asteroids (PHAs), Minor Planet Center 153201 153201 2000WO107 2007 UW 1 Large NEO Earth close approach(inside the orbit of the Moon) 1 December 2140 (85640) 1998 OX 4 153201 (153201) 2000 WO 107 153201 153201 153201 153201 20001129 153201 153201