2004 TG10: Difference between revisions
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{{DISPLAYTITLE:2004 TG<sub>10</sub>}} |
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{{DISPLAYTITLE:{{mp|2004 TG|10}}}} |
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{{Infobox Comet |
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{{Infobox planet |
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| name=2004 TG<sub>10</sub> |
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| minorplanet = yes |
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| image= |
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| name = {{mp|2004 TG|10}} |
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| discoverer= |
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| background = #FFC2E0 |
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| discovery_date= |
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| image = |
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| designations= |
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| image_size = |
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| epoch=June 18, 2009 (2455000.5) |
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| caption = |
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| semimajor=2.2427 [[Astronomical Unit|AU]] |
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| discovery_ref = <ref name="jpldata" /><ref name="MPC-2004TG10" /> |
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| perihelion=0.31399 AU |
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| discovered = 8 October 2004<br />{{nowrap|{{small|(discovery: first observed only)}}}} |
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| aphelion=4.1715 AU |
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| discoverer = [[Spacewatch]] |
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| eccentricity=0.85999 |
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| discovery_site = [[Kitt Peak National Observatory|Kitt Peak Obs.]] |
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| period=3.36 [[Julian year (astronomy)|yr]] |
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| mpc_name = {{mp|2004 TG|10}} |
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| inclination=3.707° |
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| alt_names = |
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| last_p=October 4, 2011<ref name=jpldata/><br>May 21, 2008 |
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| pronounced = |
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| next_p=February 4, 2015 |
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| named_after = |
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| mp_category = [[Near-Earth object|NEO]]{{·}}[[Apollo asteroid|Apollo]]{{·}}[[Potentially hazardous object|PHA]]<ref name="jpldata" /> |
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| orbit_ref = <ref name="jpldata" /> |
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| epoch = 4 September 2017 ([[Julian day|JD]] 2458000.5) |
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| uncertainty = 0 |
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| observation_arc = 10.16 yr (3,712 days) |
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| aphelion = 4.1597 [[Astronomical unit|AU]] |
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| perihelion = 0.3086 AU |
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| semimajor = 2.2341 AU |
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| eccentricity = 0.8619 |
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| period = 3.34 [[Julian year (astronomy)|yr]] (1,220 days) |
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| mean_anomaly = 278.07[[Degree (angle)|°]] |
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| mean_motion = {{Deg2DMS|0.2951|sup=ms}} / day |
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| inclination = 4.1802° |
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| asc_node = 205.10° |
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| arg_peri = 317.37° |
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| moid = 0.0225 AU{{·}}8.8 [[Lunar distance (astronomy)|LD]] |
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| jupiter_moid = 0.8877 AU |
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| dimensions = 0.35–0.78 km<ref name="Porubcan-2006" /><br />{{val|1.316|0.605}} km<ref name="Nugent-2015" /> |
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| rotation = |
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| albedo = {{val|0.018|0.037}}<ref name="Nugent-2015" /> |
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| spectral_type = |
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| abs_magnitude = 19.4<ref name="jpldata" /><ref name="Porubcan-2006" /> |
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}} |
}} |
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'''{{mp|2004 TG|10}}''', is an eccentric [[asteroid]], classified as [[near-Earth object]] and [[potentially hazardous asteroid]] of the [[Apollo asteroid|Apollo group]]. First observed by the [[Spacewatch]] survey on 8 October 2004,<ref name="MPC-2004TG10" /> it may be a fragment of [[Comet Encke]] and is the source of the [[Northern Taurids]] [[meteor shower]] seen annually in November<ref name="Porubcan-2006" /><ref name="Taurids 2017">{{cite web|url=https://patch.com/us/across-america/taurids-meteor-shower-fireballs-peak-dates-what-expect|title=Taurids Meteor Shower Fireballs: Peak Dates, What To Expect|author=Beth Dalbey|date=24 October 2017|access-date=11 November 2017}}</ref> and the June [[Beta Taurids]].<ref name=Jenniskens>Meteor showers and their parent comets [https://books.google.com/books?id=QpajMuyXG8AC&pg=PA470&dq=TG10 pg 470] by [[Peter Jenniskens]]</ref> The asteroid may be larger than one kilometer in diameter. |
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'''{{mp|2004 TG|10}}''', also written as '''2004 TG10''', is a [[near-Earth object]].<ref name=jpldata>{{cite web |
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|type=last observation: 2008-07-17; [[Observation arc|arc]]: 3.78 years |
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|title=JPL Small-Body Database Browser: (2004 TG10) |
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|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004TG10 |
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|accessdate=2009-05-19}}</ref> It may be a fragment of [[Comet Encke]].<ref name=Porub2006> |
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{{cite journal |
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|last=Porubčan |first=V. |
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|author2=Kornoš; Williams |
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|title=The Taurid complex meteor showers and asteroids |
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|journal=Contributions of the Astronomical Observatory Skalnaté Pleso |
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|volume=36 |pages=103–117 |year=2006 |
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|arxiv=0905.1639 |
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|bibcode = 2006CoSka..36..103P }}</ref> Depending on its [[albedo]] it is estimated to be 350 to 780 meters in diameter.<ref name=Porub2006/> It may be the source of the [[Northern Taurids]] [[meteor shower]] in November. |
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== Orbit == |
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<div style="float:right; margin:2px;"> |
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{| class=wikitable style="text-align:center" |
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{{mp|2004 TG|10}} orbits the Sun at a distance of 0.3–4.2 [[Astronomical unit|AU]] once every 3 years and 4 months (1,220 days). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.86 and an [[orbital inclination|inclination]] of 4[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" /> |
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It has an ''Earth [[minimum orbital intersection distance]]'' of {{convert |0.0225 |AU |km |abbr=on |sigfig=3}}, which corresponds to 8.8 [[Lunar distance (astronomy)|lunar distances]].<ref name="jpldata" /> |
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== Physical characteristics == |
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According to the survey carried out by the [[NEOWISE]] mission of NASA's [[Wide-field Infrared Survey Explorer]], the asteroid measures 1.316 kilometers in diameter and its surface has an exceptionally low [[astronomical albedo|albedo]] of 0.018,<ref name="Nugent-2015" /> while Porubcan estimates a diameter of 350 to 780 meters, based on an albedo of 0.25 to 0.05, which typically covers most [[S-type asteroid|S-type]] and [[C-type asteroids]].<ref name="Porubcan-2006" /> |
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{| class=wikitable style="text-align: center;" |
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|+ TG10 compared to Comet Encke |
|+ TG10 compared to Comet Encke |
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![[Astronomical unit|AU]]!!TG |
! [[Astronomical unit|AU]] !! {{mp|2004 TG|10}} !![[Comet Encke|Encke]]<ref name="jpl-Encke" /> |
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|type=last observation: 2008-09-30 |
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|title=JPL Small-Body Database Browser: 2P/Encke |
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|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2P |
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|accessdate=2009-05-19}}</ref> |
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|- |
|- |
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|[[Semi-major axis]] || 2.24 || 2.21 |
| [[Semi-major axis]] || 2.24 || 2.21 |
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|- |
|- |
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|[[Apsis|Perihelion]] || 0.313 || 0.338 |
| [[Apsis|Perihelion]] || 0.313 || 0.338 |
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|- |
|- |
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|Aphelion || 4.17 || 4.09 |
| Aphelion || 4.17 || 4.09 |
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|- |
|- |
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|[[Orbital eccentricity|Eccentricity]] || 0.859 || 0.847 |
|[[Orbital eccentricity|Eccentricity]] || 0.859 || 0.847 |
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|- |
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|}</div> |
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| [[Longitude of perihelion]] || 162.455° || 161.113° |
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{{-}} |
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|} |
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== References == |
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{{reflist|refs= |
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<ref name="jpldata">{{cite web |
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|type = 2014-12-04 last obs. |
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|title = JPL Small-Body Database Browser: (2004 TG10) |
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|url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3256324 |
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|publisher = [[Jet Propulsion Laboratory]] |
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|accessdate = 29 July 2017}}</ref> |
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<ref name="MPC-2004TG10">{{cite web |
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|title = 2004 TG10 |
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|work = Minor Planet Center |
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|url = http://www.minorplanetcenter.net/db_search/show_object?object_id=2004+TG10 |
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|accessdate = 29 July 2017}}</ref> |
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<ref name="Nugent-2015">{{Cite journal |
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|display-authors = 6 |
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|first1 = C. R. |last1 = Nugent |
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|first2 = A. |last2 = Mainzer |
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|first3 = J. |last3 = Masiero |
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|first4 = J. |last4 = Bauer |
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|first5 = R. M. |last5 = Cutri |
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|first6 = T. |last6 = Grav |
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|first7 = E. |last7 = Kramer |
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|first8 = S. |last8 = Sonnett |
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|first9 = R. |last9 = Stevenson |
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|first10 = E. L. |last10 = Wright |
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|date = December 2015 |
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|title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N |
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|journal = The Astrophysical Journal |
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|volume = 814 |
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|issue = 2 |
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|page = 13 |
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|bibcode = 2015ApJ...814..117N |
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|doi = 10.1088/0004-637X/814/2/117 |
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|arxiv = 1509.02522 |
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|access-date= 29 July 2017}}</ref> |
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<ref name="Porubcan-2006">{{Cite journal |
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|first1 = V. |last1 = Porubčan |
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|first2 = L. |last2 = Kornoš |
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|first3 = I. P. |last3 = Williams |
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|date = June 2006 |
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|title = The Taurid complex meteor showers and asteroids |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2006CoSka..36..103P |
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|journal = Contributions of the Astronomical Observatory Skalnaté Pleso |
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|volume = 36 |
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|pages = 103–117 |
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|bibcode = 2006CoSka..36..103P |
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|arxiv = 0905.1639 |
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|access-date= 29 July 2017}}</ref> |
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<ref name="jpl-Encke">{{cite web |
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|type = last observation: 2008-09-30 |
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|title = JPL Small-Body Database Browser: 2P/Encke |
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|url = http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2P |
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|accessdate = 2009-05-19}}</ref> |
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}} <!-- end of reflist --> |
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== External links == |
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==References== |
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* {{NeoDys|2004TG10}} |
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<references/> |
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* {{ESA-SSA|2004TG10}} |
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* {{JPL small body}} |
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<!--use upon numbering: {{Minor planets navigator | |number=? |PageName={{mp|(?) 2004 TG|10}} | }} --> |
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==External links== |
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{{Small Solar System bodies}} |
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*[http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2004TG10;orb=1;view=Far Orbital simulation] from JPL (Java) / [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2004TG10 Ephemeris] |
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{{Authority control}} |
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{{DEFAULTSORT:2004 |
{{DEFAULTSORT:2004 TG10}} |
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[[Category:Apollo asteroids]] |
[[Category:Apollo asteroids|#]] |
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[[Category: |
[[Category:Meteor shower progenitors|*]] |
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[[Category:Discoveries by the Spacewatch project]] |
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[[Category:Minor planet object articles (unnumbered)]] |
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[[Category:Potentially hazardous asteroids|#]] |
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[[Category:Astronomical objects discovered in 2004|20041008]] |
Latest revision as of 20:52, 28 December 2024
Discovery[1][2] | |
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Discovered by | Spacewatch |
Discovery site | Kitt Peak Obs. |
Discovery date | 8 October 2004 (discovery: first observed only) |
Designations | |
2004 TG10 | |
NEO · Apollo · PHA[1] | |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 10.16 yr (3,712 days) |
Aphelion | 4.1597 AU |
Perihelion | 0.3086 AU |
2.2341 AU | |
Eccentricity | 0.8619 |
3.34 yr (1,220 days) | |
278.07° | |
0° 17m 42.36s / day | |
Inclination | 4.1802° |
205.10° | |
317.37° | |
Earth MOID | 0.0225 AU · 8.8 LD |
Jupiter MOID | 0.8877 AU |
Physical characteristics | |
Dimensions | 0.35–0.78 km[3] 1.316±0.605 km[4] |
0.018±0.037[4] | |
19.4[1][3] | |
2004 TG10, is an eccentric asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group. First observed by the Spacewatch survey on 8 October 2004,[2] it may be a fragment of Comet Encke and is the source of the Northern Taurids meteor shower seen annually in November[3][5] and the June Beta Taurids.[6] The asteroid may be larger than one kilometer in diameter.
Orbit
[edit]2004 TG10 orbits the Sun at a distance of 0.3–4.2 AU once every 3 years and 4 months (1,220 days). Its orbit has an eccentricity of 0.86 and an inclination of 4° with respect to the ecliptic.[1]
It has an Earth minimum orbital intersection distance of 0.0225 AU (3,370,000 km), which corresponds to 8.8 lunar distances.[1]
Physical characteristics
[edit]According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, the asteroid measures 1.316 kilometers in diameter and its surface has an exceptionally low albedo of 0.018,[4] while Porubcan estimates a diameter of 350 to 780 meters, based on an albedo of 0.25 to 0.05, which typically covers most S-type and C-type asteroids.[3]
AU | 2004 TG10 | Encke[7] |
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Semi-major axis | 2.24 | 2.21 |
Perihelion | 0.313 | 0.338 |
Aphelion | 4.17 | 4.09 |
Eccentricity | 0.859 | 0.847 |
Longitude of perihelion | 162.455° | 161.113° |
References
[edit]- ^ a b c d e f "JPL Small-Body Database Browser: (2004 TG10)" (2014-12-04 last obs.). Jet Propulsion Laboratory. Retrieved 29 July 2017.
- ^ a b "2004 TG10". Minor Planet Center. Retrieved 29 July 2017.
- ^ a b c d Porubčan, V.; Kornoš, L.; Williams, I. P. (June 2006). "The Taurid complex meteor showers and asteroids". Contributions of the Astronomical Observatory Skalnaté Pleso. 36: 103–117. arXiv:0905.1639. Bibcode:2006CoSka..36..103P. Retrieved 29 July 2017.
- ^ a b c Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. Retrieved 29 July 2017.
- ^ Beth Dalbey (24 October 2017). "Taurids Meteor Shower Fireballs: Peak Dates, What To Expect". Retrieved 11 November 2017.
- ^ Meteor showers and their parent comets pg 470 by Peter Jenniskens
- ^ "JPL Small-Body Database Browser: 2P/Encke" (last observation: 2008-09-30). Retrieved 19 May 2009.
External links
[edit]- 2004 TG10 at NeoDyS-2, Near Earth Objects—Dynamic Site
- 2004 TG10 at ESA–space situational awareness
- 2004 TG10 at the JPL Small-Body Database