From Surf Wiki (app.surf) — the open knowledge base
(179806) 2002 TD66
Near-Earth asteroid
Near-Earth asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #FFC2E0 |
| name | |
| discoverer | LINEAR |
| discovery_site | Lincoln Lab ETS |
| discovered | 5 October 2002 |
| mp_category | NEOApollo |
| orbit_ref | |
| epoch | 13 January 2016 (JD 2457400.5) |
| observation_arc | 2017 days (5.52 yr) |
| uncertainty | 0 |
| semimajor | 1.8580 AU |
| perihelion | 0.86543 AU |
| aphelion | 2.8505 AU |
| eccentricity | 0.53421 |
| period | 2.53 yr (925.03 d) |
| inclination | 4.9211° |
| asc_node | 335.73° |
| arg_peri | 125.66° |
| mean_motion | / day |
| mean_anomaly | 55.037° |
| moid | 0.00603808 AU |
| jupiter_moid | 2.35661 AU |
| dimensions | 300 meters |
| 270–590 meters [H](https://web.archive.org/web/20010302182040/http://neo.jpl.nasa.gov/glossary/h.html) | |
| rotation | 9.455 h |
| abs_magnitude | 20.2 |
270–590 meters H
**(179806) ** (also written 2002 TD66) is a sub-kilometer asteroid, classified as near-Earth object of the Apollo group. It was discovered on 5 October 2002, by the LINEAR project at Lincoln Laboratory's ETS in Socorro, New Mexico. It was announced on 7 October 2002 and appeared later that day on the JPL current risk page.
Description
Due to the proximity of its orbit to Earth and its estimated size, this object has been classified as a potentially hazardous asteroid (PHA) by the Minor Planet Center in Cambridge, Massachusetts. In November 2006 there were 823 PHAs known. , there are 1261 PHAs known. was removed from the Sentry Risk Table on October 10, 2002. A Doppler observation has helped produce a well known trajectory with a condition code (Uncertainty Parameter U) of 0.
Based on an absolute magnitude (H) of 20.2, the asteroid is estimated to be between 270 and 590 meters in diameter. Radar astronomy shows it is a contact binary asteroid with a diameter of 300 meters and a rotation period of 9.5 hours.
On February 26, 2008, passed 0.04282 AU from Earth. The asteroid also comes close to Venus, Mars, and dwarf planet Ceres.
References
|archive-url=https://web.archive.org/web/20020602101400/http://neo.jpl.nasa.gov/risk/removed.html |url-status=dead |archive-date=2002-06-02
|archive-url=https://web.archive.org/web/20020202160655/http://neo.jpl.nasa.gov/neo/groups.html |url-status=dead |archive-date=2002-02-02
|archive-url=https://web.archive.org/web/20040608071121/http://echo.jpl.nasa.gov/~lance/binary.neas.html |url-status=dead |archive-date=2004-06-08
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about (179806) 2002 TD66 — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report