2002 RN109: Difference between revisions
m removed dup. nav. template |
astronomical. replaced date page looked at by date range of observations |
||
(27 intermediate revisions by 13 users not shown) | |||
Line 1: | Line 1: | ||
{{Use dmy dates|date=November 2018}} |
|||
{{DISPLAYTITLE:{{mp|2002 RN|109}}}} |
{{DISPLAYTITLE:{{mp|2002 RN|109}}}} |
||
{{Infobox planet |
{{Infobox planet |
||
| |
| minorplanet = yes |
||
| name = {{mp|2002 RN|109}} |
|||
| bgcolour=#FFFFC0 |
|||
| background = #C2E0FF |
|||
| name=2002 RN109 |
|||
| |
| 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 AU from the Sun.<ref name=jpldata/> During perihelion passage the object was 2.9 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 [[Astronomical unit|AU]] once every 12,783 years ([[semi-major axis]] of 546.7 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 AU from the Sun.<ref name=jpldata/> During perihelion passage the object was 2.9 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 |
|type = 2002-11-04 last obs. |
||
|title=JPL Small-Body Database Browser: (2002 RN109) |
|title = JPL Small-Body Database Browser: (2002 RN109) |
||
|url= |
|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3221149 |
||
|publisher=Jet Propulsion Laboratory |
|publisher = [[Jet Propulsion Laboratory]] |
||
|accessdate= |
|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
Discovery[1] | |
---|---|
Discovered by | LINEAR |
Discovery site | Lincoln Lab's ETS |
Discovery date | 6 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 arc | 80 days |
Aphelion | 1090.71 AU |
Perihelion | 2.6915 AU |
546.70 AU | |
Eccentricity | 0.9951 |
12,783 yr | |
0.4600° | |
0° 0m 0.36s / day | |
Inclination | 58.137° |
170.50° | |
212.28° | |
TJupiter | 1.0820 |
Physical characteristics | |
4 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]- ^ a b c d e "2002 RN109". Minor Planet Center. 38 total observations over interval: 2002 08 16.36906 – 2002 11 04.41631
- ^ 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.
- ^ a b c d Johnston, Wm. Robert (7 October 2018). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 19 November 2018.
- ^ "List Of Other Unusual Objects". Minor Planet Center. 14 November 2018. Retrieved 20 November 2018.
- ^ "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)