请输入您要查询的百科知识:

 

词条 (19308) 1996 TO66
释义

  1. Origin

  2. References

  3. External links

{{DISPLAYTITLE:{{mp|(19308) 1996 TO|66}}}}{{Infobox planet
| minorplanet = yes
| background = #C2E0FF
| image = (19308) 1996 TO66 imaged by NTT cut out.jpg
| image_size = 265
| image_alt = (19308) 1996 TO66 imaged by NTT cut out
| caption = {{longitem|{{mp|1996 TO|66}} (center top) imaged by the NTT at La Silla in 1998. Other objects are elongated due to the 4-hour-exposure. The horizontal streak is from a geostationary satellite.|style=padding:6px 0;}}
| name = {{mp|(19308) 1996 TO|66}}
| discoverer = Chadwick Trujillo
David Jewitt
Jane Luu
| discovered = 12 October 1996
| mpc_name = {{mp|(19308) 1996 TO|66}}
| alt_names =
| mp_category = TNO
weak eighth-order 11:19 resonance? 
| orbit_ref =  [2]
| epoch = 13 January 2016 (JD 2457400.5)
| semimajor = {{Convert|43.157|AU|Tm|abbr=on}}
| perihelion = {{Convert|37.939|AU|Tm|abbr=on}}
| aphelion = {{Convert|48.375|AU|Tm|abbr=on|lk=on}}
| eccentricity = 0.12090
| period = 283.52 yr (103555 d)
| inclination = 27.4948°
| asc_node = 355.2889°
| arg_peri = 239.07°
| mean_anomaly = 137.16°
| avg_speed =
| dimensions = 200 km (assuming a {{nowrap|Haumea-like albedo of 0.7) [3]}}
(<902km) [4]
| radius =
| mass =
| density =
| surface_grav =
| escape_velocity =
| sidereal_day = 7.92 h [2]
| spectral_type = (Neutral)
B−V=0.68, V−R=0.39 [6]
B−V=0.74; V−R=0.38 [7]
| abs_magnitude = 4.5
| albedo = 0.7 (assumed)
| single_temperature = ~ 43 K
| mean_motion = {{Deg2DMS|0.0034764|sup=ms}} / day
| rotation = {{Convert|7.92|h|d|abbr=on|lk=on}}
| observation_arc = 7322 days (20.05 yr)
| uncertainty = 3
| moid = {{Convert|37.0117|AU|Tm|abbr=on}}
| jupiter_moid = {{Convert|33.0091|AU|Tm|abbr=on}}
}}

{{mp|(19308) 1996 TO|66}} (also written (19308) 1996 TO66) is a trans-Neptunian object that was discovered in 1996 by Chadwick Trujillo, David Jewitt and Jane Luu. Until 20000 Varuna was discovered, it was the second-largest known object in the Kuiper belt, after Pluto.

Origin

{{main|Haumea family}}

Based on their common pattern of IR water-ice absorptions, neutral visible spectrum[8] and the clustering of their orbital elements, the other KBOs {{mpl|(24835) 1995 SM|55}}, {{mpl|(55636) 2002 TX|300}}, {{mpl|(120178) 2003 OP|32}} and {{mpl|(145453) 2005 RR|43}} all appear to be collisional fragments broken off of the dwarf planet {{dp|Haumea}}.

{{clear|left}}

References

1. ^{{cite web |type=2003-10-18 last obs |title=JPL Small-Body Database Browser: 19308 (1996 TO66) |url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1996TO66 |accessdate=5 April 2016}}
2. ^{{cite web |title=Conversion of Absolute Magnitude to Diameter for Minor Planets |publisher=Department of Physics & Astronomy (Stephen F. Austin State University) |author=Dan Bruton |url=http://www.physics.sfasu.edu/astro/asteroids/sizemagnitude.html |accessdate=2009-12-27 |archiveurl= https://web.archive.org/web/20100323180835/http://www.physics.sfasu.edu/astro/asteroids/sizemagnitude.html |archivedate= 23 March 2010}}
3. ^{{cite journal |arxiv=astro-ph/0502229 |title=Diverse albedos of small trans-neptunian objects |last=Grundy |first=W. M. |date=2004 |journal=Icarus |volume=176 |pages=22 |bibcode=2005Icar..176..184G |doi = 10.1016/j.icarus.2005.01.007}}
4. ^{{cite journal |author=Snodgrass, Carry |author2=Dumas, Hainaut |title=Characterisation of candidate members of (136108) Haumea's family |doi=10.1051/0004-6361/200913031 |journal=Astronomy and Astrophysics |date=16 December 2009 |arxiv=0912.3171 |bibcode = 2010A&A...511A..72S}}
5. ^{{cite web |url=http://www.physics.nau.edu/~tegler/research/survey.htm |archive-url=https://archive.is/20060901063349/http://www.physics.nau.edu/~tegler/research/survey.htm |dead-url=yes |archive-date=2006-09-01 |title=Kuiper Belt Object Magnitudes and Surface Colors |accessdate=2006-11-07 |last=Tegler |first=Stephen C. |date=2007-02-01 }}
6. ^{{cite journal |title=The water ice rich surface of (145453) 2005 RR43: a case for a carbon-depleted population of TNOs? |author=Pinilla-Alonso, N. |author2=Licandro, J. |author3=Gil-Hutton, R. |author4=Brunetto, R. |journal=Astronomy and Astrophysics |date=June 2007 |volume=468 |issue=1 |bibcode=2007A&A...468L..25P |doi= 10.1051/0004-6361:20077294 |page=L25|arxiv= astro-ph/0703098}}

|author=D. Ragozzine
|author2=M. E. Brown
|journal=The Astronomical Journal
|volume=134 |issue=6 |pages= 2160–2167
|date=2007-09-04
|bibcode=2007AJ....134.2160R
|doi=10.1086/522334
|arxiv=0709.0328}}
[1][2][3][4][5][6]

}}

External links

  • First Rotation Period of a Kuiper Belt Object Measured – ESO, 5 November 1998
  • {{JPL small body|id=19308}}
{{Haumea}}{{Minor planets navigator| |number=19308|PageName={{mp|(19308) 1996 TO|66}}| }}{{Small Solar System bodies}}{{Trans-Neptunian objects}}{{DEFAULTSORT:019308}}{{centaurTNO-stub}}

6 : Haumea family|Kuiper belt objects|Discoveries by David C. Jewitt|Discoveries by Jane Luu|Discoveries by Chad Trujillo|Astronomical objects discovered in 1996

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/9/27 23:26:22