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{{Use dmy dates|date=November 2018}}
{{DISPLAYTITLE:{{mp|2002 RN|109}}}}
{{DISPLAYTITLE:{{mp|2002 RN|109}}}}
{{Infobox planet
{{Infobox planet
| physical_characteristics = yes
| minorplanet = yes
| name = {{mp|2002 RN|109}}
| bgcolour=#FFFFC0
| background = #C2E0FF
| name=2002 RN109
| discovery = yes
| image =
| image_size =
| discovery_ref = <ref name=mpc/>
| caption =
| discoverer = [[LINEAR]]
| discovery_ref = <ref name="MPC-object" />
| discovered=2002-08-16
| discoverer = [[Lincoln Near-Earth Asteroid Research|LINEAR]]
| alt_names=
| discovery_site = [[Lincoln Laboratory's Experimental Test Site|Lincoln Lab's ETS]]
| mp_category=[[List of Jupiter-crossing minor planets|Jupiter crosser]],<br>[[List of Saturn-crossing minor planets|Saturn crosser]],<br>[[List of Uranus-crossing minor planets|Uranus crosser]],<br>[[List of Neptune-crossing minor planets|Neptune crosser]],<br>[[Damocloid]],<br>[[Trans-Neptunian object]]
| discovered = 6 September 2002
| orbit_ref =<ref name="jpldata"/>
| mpc_name = {{mp|2002 RN|109}}
| epoch=2456800.5 (2014-May-23.0)
| alt_names =
| semimajor=715 AU ±40
| pronounced =
| perihelion=2.7056 AU ±0.0002
| named_after =
| aphelion=1428 [[Astronomical unit|AU]] ±80
| mp_category = {{nowrap|[[Trans-Neptunian object|TNO]]<ref name="jpldata" />{{·}}[[damocloid]]<ref name="johnstonsarchive-TNO-list" />}}<br />[[Unusual minor planet|unusual]]<ref name="MPC-Unusual-list" />{{·}}[[Distant minor planet|distant]]<ref name="MPC-object" />
| eccentricity=0.99622 ±0.0002
| orbit_ref = <ref name="jpldata" />
| period=19130 [[Julian year (astronomy)|a]] (6980000 d) ±1600 (584000)
| epoch = 27 April 2019 ([[Julian day|JD]] 2458600.5)
| inclination=57.94° ±0.005
| uncertainty = 4
| asc_node=170.50° ±0.000065
| observation_arc = 80 days
| arg_peri=212.48° ±0.006
| aphelion = 1090.71 [[Astronomical unit|AU]]
| mean_anomaly=0.21° ±0.018
| perihelion = 2.6915 AU
| dimensions=4 km (assumed)<ref name="johnston"/>
| semimajor = 546.70 AU
| escape_velocity=
| eccentricity = 0.9951
| rotation=
| period = 12,783 [[Julian year (astronomy)|yr]]
| spectral_type=
| mean_anomaly = 0.4600[[Degree (angle)|°]]
| abs_magnitude=15.3
| mean_motion = {{Deg2DMS|0.0001|sup=ms}} / day
| inclination = 58.137°
| asc_node = 170.50°
| arg_peri = 212.28°
| tisserand = 1.0820
| mean_diameter = {{val|4|ul=km}} {{small|(est.)}}<ref name="johnstonsarchive-TNO-list" />
| rotation =
| albedo = 0.09 {{small|(assumed)}}<ref name="johnstonsarchive-TNO-list" />
| spectral_type =
| abs_magnitude = 15.3<ref name="MPC-object" /><ref name="jpldata" />
}}
}}


'''{{mp|2002 RN|109}}''' is a [[Trans-Neptunian object|trans-Neptunian astronomical object]] and [[damocloid]] on a highly eccentric, [[comet]]ary-like orbit. It was first observed on 6 September 2002, by astronomers of the [[Lincoln Near-Earth Asteroid Research]] project at [[Lincoln Laboratory's Experimental Test Site|its ETS]] near Socorro, New Mexico, United States.<ref name="MPC-object" /> The [[Unusual minor planet|unusual object]] is approximately {{convert|4|km|mi|abbr=off|sigfig=1|sp=us}} in diameter.<ref name="johnstonsarchive-TNO-list" /> It has the second-highest [[orbital eccentricity]] of any known minor planet, after {{mpl|2005 VX|3}}.<ref name="jpl-search"/>
'''{{mp|2002 RN|109}}''' is a [[minor planet]] with the second highest [[orbital eccentricity]] of any known minor planet, after {{mpl|2005 VX|3}}.<ref name="jpl-search"/> It also has the sixth-largest heliocentric [[semi-major axis]] and [[aphelion]] of all known minor planets, while its extreme eccentricity brings it well within the orbit of [[Jupiter]] when at [[perihelion]].


== Description ==
{{mp|2002 RN|109}} has an [[observation arc]] 80 days and has not been observed since November 2002 about 2 months before it came to perihelion 2.7&nbsp;AU from the Sun.<ref name=jpldata/> During perihelion passage the object was 2.9&nbsp;AU from Earth.


''{{mp|2002 RN|109}}'' may be a [[dormant comet]] that has not been seen [[outgassing]]. In the past it may have made closer approaches to the Sun that could have removed most near-surface [[Volatile (astrogeology)|volatiles]]. It orbits the Sun at a distance of 2.7–1,091&nbsp;[[Astronomical unit|AU]] once every 12,783 years ([[semi-major axis]] of 546.7&nbsp;AU). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.9951 and an [[orbital inclination|inclination]] of 58[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" /> The body's [[observation arc]] began with a [[precovery]] observation at [[Lincoln Laboratory's Experimental Test Site]] on 16 August 2002, or three weeks prior to its first observation.<ref name="MPC-object" /> The observation arc is only 80 days long. The object has not been observed since November 2002, about 2 months before it came to perihelion 2.7&nbsp;AU from the Sun.<ref name=jpldata/> During perihelion passage the object was 2.9&nbsp;AU from Earth.
It may be a [[dormant comet]] that has not been seen [[outgassing]]. In the past it may have made closer approaches to the Sun that could have removed most near-surface [[volatiles]].


''{{mp|2002 RN|109}}'' belongs to the dynamical group of [[damocloid]]s due to its low [[Tisserand's parameter|Tisserand parameter]] (T<sub>Jupiter</sub> of 1.0820).<ref name="jpldata" /> It is also a [[List of Jupiter-crossing minor planets|Jupiter-]], [[List of Saturn-crossing minor planets|Saturn-]], [[List of Uranus-crossing minor planets|Uranus-]], and [[List of Neptune-crossing minor planets|Neptune-crosser]]. The object has the seventh-largest heliocentric semi-major axis and [[aphelion]] of all known minor planets, while its extreme eccentricity brings it well within the orbit of [[Jupiter]] when at [[perihelion]].

== See also ==
* [[List of Solar System objects by greatest aphelion]]


== References ==
== References ==
{{reflist
{{reflist|30em|refs=
| refs =


<ref name="jpldata">{{cite web
<ref name="jpldata">{{cite web
|type=last observation: 2002-11-04; [[Observation arc|arc]]: 80 days
|type = 2002-11-04 last obs.
|title=JPL Small-Body Database Browser: (2002 RN109)
|title = JPL Small-Body Database Browser: (2002 RN109)
|url=http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002RN109
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3221149
|publisher=Jet Propulsion Laboratory
|publisher = [[Jet Propulsion Laboratory]]
|accessdate=2014-03-07}}</ref>
|accessdate = 20 November 2018}}</ref>

<ref name="MPC-object">{{cite web
|title = 2002 RN109
|work = Minor Planet Center
|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=2002+RN109
}} 38 total observations over interval: 2002 08 16.36906 – 2002 11 04.41631</ref>

<ref name="MPC-Unusual-list">{{cite web
|title = List Of Other Unusual Objects
|work = Minor Planet Center
|date = 14 November 2018
|url = https://www.minorplanetcenter.net/iau/lists/t_others.html
|accessdate = 20 November 2018}}</ref>

<ref name="johnstonsarchive-TNO-list">{{cite web
|title = List of Known Trans-Neptunian Objects
|work = Johnston's Archive
|date = 7 October 2018
|last = Johnston |first= Wm. Robert
|url = http://www.johnstonsarchive.net/astro/tnoslist.html
|accessdate = 19 November 2018}}</ref>


<ref name="jpl-search">{{cite web
<ref name="jpl-search">{{cite web
|title=JPL Small-Body Database Search Engine: Asteroids and a > 100 (AU)
|title=JPL Small-Body Database Search Engine: Asteroids and a > 100 (AU)
|publisher=JPL Solar System Dynamics
|publisher=[[JPL Solar System Dynamics]]
|url=http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=ast;obj_numbered=all;OBJ_field=0;ORB_field=0;c1_group=ORB;c1_item=Bh;c1_op=%3E;c1_value=100;table_format=HTML;max_rows=100;format_option=comp;c_fields=AcBhBgBjBiBnBsCjCpAiCkBe;.cgifields=format_option;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=com_orbit_class&query=1&c_sort=BhD
|url=http://ssd.jpl.nasa.gov/sbdb_query.cgi?obj_group=all;obj_kind=ast;obj_numbered=all;OBJ_field=0;ORB_field=0;c1_group=ORB;c1_item=Bh;c1_op=%3E;c1_value=100;table_format=HTML;max_rows=100;format_option=comp;c_fields=AcBhBgBjBiBnBsCjCpAiCkBe;.cgifields=format_option;.cgifields=ast_orbit_class;.cgifields=table_format;.cgifields=obj_kind;.cgifields=obj_group;.cgifields=obj_numbered;.cgifields=com_orbit_class&query=1&c_sort=BhD
|accessdate=2014-10-15}} (Epoch defined at will change every 6 months or so)</ref>
|accessdate=2014-10-15}} (Epoch defined at will change every 6 months or so)</ref>


}} <!-- end of reflist -->
<ref name=mpc>{{Cite web
|title=MPEC: 2002 RN109
|publisher=IAU Minor Planet Center
|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=2002+RN109
|accessdate=2014-03-07}})</ref>


== External links ==
<ref name="johnston">{{Cite web
* {{JPL small body|id=3221149}}
|title=List of Known Trans-Neptunian Objects
|publisher=Johnston's Archive
|date=2005-11-08
|url=http://www.johnstonsarchive.net/astro/tnoslist.html
|accessdate=2014-03-05}}</ref>


}}

{{Small Solar System bodies}}
{{Trans-Neptunian objects}}
{{Trans-Neptunian objects}}
<!--use upon numbering: {{Minor planets navigator | |number=? |PageName={{mp|(?) 2002 RN|109}} | }} -->
{{Small Solar System bodies}}
{{Authority control}}


{{DEFAULTSORT:2002 RN109}}
[[Category:Astronomical objects discovered in 2002]]
[[Category:Damocloids]]
[[Category:Damocloids]]
[[Category:Trans-Neptunian objects]]
[[Category:Trans-Neptunian objects]]
[[Category:Unusual minor planets|#]]
[[Category:Minor planet object articles (unnumbered)]]
[[Category:Astronomical objects discovered in 2002|20020816]]

Latest revision as of 11:55, 18 December 2023

2002 RN109
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date6 September 2002
Designations
2002 RN109
TNO[2] · damocloid[3]
unusual[4] · distant[1]
Orbital characteristics[2]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 4
Observation arc80 days
Aphelion1090.71 AU
Perihelion2.6915 AU
546.70 AU
Eccentricity0.9951
12,783 yr
0.4600°
0° 0m 0.36s / day
Inclination58.137°
170.50°
212.28°
TJupiter1.0820
Physical characteristics
km (est.)[3]
0.09 (assumed)[3]
15.3[1][2]

2002 RN109 is a trans-Neptunian astronomical object and damocloid on a highly eccentric, cometary-like orbit. It was first observed on 6 September 2002, by astronomers of the Lincoln Near-Earth Asteroid Research project at its ETS near Socorro, New Mexico, United States.[1] The unusual object is approximately 4 kilometers (2 miles) in diameter.[3] It has the second-highest orbital eccentricity of any known minor planet, after 2005 VX3.[5]

Description

[edit]

2002 RN109 may be a dormant comet that has not been seen outgassing. In the past it may have made closer approaches to the Sun that could have removed most near-surface volatiles. It orbits the Sun at a distance of 2.7–1,091 AU once every 12,783 years (semi-major axis of 546.7 AU). Its orbit has an eccentricity of 0.9951 and an inclination of 58° with respect to the ecliptic.[2] The body's observation arc began with a precovery observation at Lincoln Laboratory's Experimental Test Site on 16 August 2002, or three weeks prior to its first observation.[1] The observation arc is only 80 days long. The object has not been observed since November 2002, about 2 months before it came to perihelion 2.7 AU from the Sun.[2] During perihelion passage the object was 2.9 AU from Earth.

2002 RN109 belongs to the dynamical group of damocloids due to its low Tisserand parameter (TJupiter of 1.0820).[2] It is also a Jupiter-, Saturn-, Uranus-, and Neptune-crosser. The object has the seventh-largest heliocentric semi-major axis and aphelion of all known minor planets, while its extreme eccentricity brings it well within the orbit of Jupiter when at perihelion.

See also

[edit]

References

[edit]
  1. ^ a b c d e "2002 RN109". Minor Planet Center. 38 total observations over interval: 2002 08 16.36906 – 2002 11 04.41631
  2. ^ a b c d e f "JPL Small-Body Database Browser: (2002 RN109)" (2002-11-04 last obs.). Jet Propulsion Laboratory. Retrieved 20 November 2018.
  3. ^ a b c d Johnston, Wm. Robert (7 October 2018). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 19 November 2018.
  4. ^ "List Of Other Unusual Objects". Minor Planet Center. 14 November 2018. Retrieved 20 November 2018.
  5. ^ "JPL Small-Body Database Search Engine: Asteroids and a > 100 (AU)". JPL Solar System Dynamics. Retrieved 15 October 2014. (Epoch defined at will change every 6 months or so)
[edit]