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118401 LINEAR

Asteroid and main-belt comet


Asteroid and main-belt comet

FieldValue
minorplanetyes
background#D6D6D6
name118401 LINEAR
176P/LINEAR
imageGemini North (GMOS) imaging of Asteroid 118401 (geminiann06008a).jpg
discovererLINEAR
discovered7 September 1999
mpc_name(118401) LINEAR
alt_names176P/LINEAR
named_afterLINEAR
mp_categorymain-beltThemis
MBC
orbit_ref{{cite web
type2010-11-02 last obs
titleJPL Small-Body Database Browser: 118401 LINEAR (1999 RE70)
urlhttps://ssd.jpl.nasa.gov/sbdb.cgi?sstr=118401
access-date26 March 2016}}
epoch13 January 2016 (JD 2457400.5)
T_jup = 3.166
uncertainty0
observation_arc5808 days (15.90 yr)
moid1.58057 AU
jupiter_moid1.6475 AU
semimajor3.1951 AU
perihelion2.5793 AU
aphelion3.8110 AU
eccentricity0.19276
period5.71 yr (2086.1 d)
inclination0.23477°
asc_node345.96°
arg_peri35.460°
mean_anomaly286.74°
avg_speed16.51 km/s
dimensions4.0±0.4 km (Spitzer){{cite journal
lastHsiehfirst=Henry H.
author2Jewitt, David C.
author3Fernández, Yanga R.
titleAlbedos of Main-Belt Comets 133P/ELST-PIZARRO and 176P/LINEAR
journalThe Astrophysical Journal Letters
volume694issue=2pages=L111–L114date=2009
doi10.1088/0004-637X/694/2/L111
arxiv0902.3682bibcode=2009ApJ...694L.111Hs2cid=17438376
mass4.3? kg
density1.3? g/cm3 (assumed)
surface_grav2
escape_velocity
rotation? d
spectral_type?
magnitude18.19 to 21.91
abs_magnitude15.1
albedo0.06±0.02R
single_temperature~156 K
mean_motion0.17257°/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

  1. Using a spherical radius of 2 km; [[Volume#Formulas
  2. [https://minorplanetcenter.net/iau/ECS/MPCArchive/2021/MPC_20210920.pdf M.P.C. 133823]
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