From Surf Wiki (app.surf) — the open knowledge base
118401 LINEAR
Asteroid and main-belt comet
Asteroid and main-belt comet
| Field | Value | |||
|---|---|---|---|---|
| minorplanet | yes | |||
| background | #D6D6D6 | |||
| name | 118401 LINEAR | |||
| 176P/LINEAR | ||||
| image | Gemini North (GMOS) imaging of Asteroid 118401 (geminiann06008a).jpg | |||
| discoverer | LINEAR | |||
| discovered | 7 September 1999 | |||
| mpc_name | (118401) LINEAR | |||
| alt_names | 176P/LINEAR | |||
| named_after | LINEAR | |||
| mp_category | main-beltThemis | |||
| MBC | ||||
| orbit_ref | {{cite web | |||
| type | 2010-11-02 last obs | |||
| title | JPL Small-Body Database Browser: 118401 LINEAR (1999 RE70) | |||
| url | https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=118401 | |||
| access-date | 26 March 2016}} | |||
| epoch | 13 January 2016 (JD 2457400.5) | |||
| T_jup = 3.166 | ||||
| uncertainty | 0 | |||
| observation_arc | 5808 days (15.90 yr) | |||
| moid | 1.58057 AU | |||
| jupiter_moid | 1.6475 AU | |||
| semimajor | 3.1951 AU | |||
| perihelion | 2.5793 AU | |||
| aphelion | 3.8110 AU | |||
| eccentricity | 0.19276 | |||
| period | 5.71 yr (2086.1 d) | |||
| inclination | 0.23477° | |||
| asc_node | 345.96° | |||
| arg_peri | 35.460° | |||
| mean_anomaly | 286.74° | |||
| avg_speed | 16.51 km/s | |||
| dimensions | 4.0±0.4 km (Spitzer){{cite journal | |||
| last | Hsieh | first=Henry H. | ||
| author2 | Jewitt, David C. | |||
| author3 | Fernández, Yanga R. | |||
| title | Albedos of Main-Belt Comets 133P/ELST-PIZARRO and 176P/LINEAR | |||
| journal | The Astrophysical Journal Letters | |||
| volume | 694 | issue=2 | pages=L111–L114 | date=2009 |
| doi | 10.1088/0004-637X/694/2/L111 | |||
| arxiv | 0902.3682 | bibcode=2009ApJ...694L.111H | s2cid=17438376 | |
| mass | 4.3? kg | |||
| density | 1.3? g/cm3 (assumed) | |||
| surface_grav | 2 | |||
| escape_velocity | ||||
| rotation | ? d | |||
| spectral_type | ? | |||
| magnitude | 18.19 to 21.91 | |||
| abs_magnitude | 15.1 | |||
| albedo | 0.06±0.02R | |||
| single_temperature | ~156 K | |||
| mean_motion | 0.17257°/day |
176P/LINEAR MBC |access-date=26 March 2016}} T_jup = 3.166 |access-date=2017-04-09}} 2017 March 12 June 30, 2011{{cite web |author-link=Syuichi Nakano |access-date=2012-02-25}} October 18, 2005
118401 LINEAR (provisional designation ****, comet designation 176P/LINEAR) is an active asteroid and main-belt comet{{cite web |archive-url=https://web.archive.org/web/20110806021852/http://www.ifa.hawaii.edu/~hsieh/mbcs.shtml |url-status=dead |archive-date=2011-08-06 |access-date=2010-12-15 |access-date=2010-12-15 |author-link=David C. Jewitt}} that was discovered by the Lincoln Near-Earth Asteroid Research (LINEAR) 1-metre telescopes in Socorro, New Mexico on September 7, 1999. (118401) LINEAR was discovered to be cometary on November 26, 2005, by Henry H. Hsieh and David C. Jewitt as part of the Hawaii Trails project using the Gemini North 8-m telescope on Mauna Kea and was confirmed by the University of Hawaii's 2.2-m (88-in) telescope on December 24–27, 2005, and Gemini on December 29, 2005. Observations using the Spitzer Space Telescope have resulted in an estimate of 4.0±0.4 km for the diameter of (118401) LINEAR.
The main-belt comets are unique in that they have flat (within the plane of the planets' orbits), approximately circular (small eccentricity), asteroid-like orbits, and not the elongated, often tilted orbits characteristic of all other comets. Because (118401) LINEAR can generate a coma (produced by vapour boiled off the comet), it must be an icy asteroid. When a typical comet approaches the Sun, its ice heats up and sublimates (changes directly from ice to gas), venting gas and dust into space, creating a tail and giving the object a fuzzy appearance. Far from the Sun, sublimation stops, and the remaining ice stays frozen until the comet's next pass close to the Sun. In contrast, objects in the asteroid belt have essentially circular orbits and are expected to be mostly baked dry of ice by their confinement to the inner Solar System (see extinct comet).
It is suggested that these main-belt asteroid-comets are evidence of a recent impact exposing an icy interior to solar radiation. It is estimated short-period comets remain active for about 10,000 years before having most of their ice sublimated away and going dormant.
Eight other objects are classified as both periodic comets and numbered asteroids: 2060 Chiron (95P/Chiron), 4015 Wilson–Harrington (107P/Wilson–Harrington), 7968 Elst–Pizarro (133P/Elst–Pizarro), 60558 Echeclus (174P/Echeclus), (282P/2003 BM80), (288P/2006 VW139), (362P/2008 GO98),{{cite web |access-date=2018-02-13}} and (433P/2005 QN173). As a dual-status object, astrometric observations of 118401 LINEAR should be reported under the minor planet designation.
118401 LINEAR last came to perihelion on 2017 March 12.
References
References
- Using a spherical radius of 2 km; [[Volume#Formulas
- [https://minorplanetcenter.net/iau/ECS/MPCArchive/2021/MPC_20210920.pdf M.P.C. 133823]
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 118401 LINEAR — 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