About: 2015 KE172

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http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2F2015_KE172

2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body Planet planet
rdfs:label	2015 KE172 (en) 2015 KE172 (fr)
rdfs:comment	2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist. (en)
foaf:name	(en)
foaf:depiction
dcterms:subject	Astronomical objects discovered in 2015 Discoveries by OSSOS Minor planet object articles (unnumbered) 1:9 resonance
Wikipage page ID	57258942 (xsd:integer)
Wikipage revision ID	1062052183 (xsd:integer)
Link from a Wikipage to another Wikipage	Resonant trans-Neptunian object Degree (angle) Julian day Perihelion Semi-major axis Astronomical objects discovered in 2015 Discoveries by OSSOS Geometric albedo Minor planet object articles (unnumbered) Trans-Neptunian object Distant minor planet Julian year (astronomy) Minor planet Absolute magnitude Ecliptic 1:9 resonance Astronomical albedo Astronomical unit Solar System Neptune (disambiguation) Orbital eccentricity Orbital inclination Mauna Kea Observatories Mean-motion resonance Scattered disc Outer Solar System Origins Survey
Link from a Wikipage to an external page	http://web.gps.caltech.edu/~mbrown/dps.html http://www.johnstonsarchive.net/astro/tnoslist.html https://minorplanetcenter.net/iau/lists/TNOs.html https://www.minorplanetcenter.net/iau/lists/t_centaurs.html
sameAs	2015 KE172 2015 KE172 2015 KE172
dbp:wikiPageUsesTemplate	dbt:Convert dbt:Deg2DMS dbt:Infobox_planet dbt:JPL_small_body dbt:Mp dbt:Reflist dbt:Small dbt:Small_Solar_System_bodies dbt:Use_dmy_dates dbt:Val dbt:·
thumbnail	wiki-commons:Special:FilePath/2015_KE172-orbit.png?width=300
abs magnitude	8.202400 (xsd:double)
albedo	0.090000 (xsd:double)
alt names	372.0 (second)
arg peri	15.428000 (xsd:double)
asc node	227.550000 (xsd:double)
background	#C2E0FF (en)
caption	Orbit of (en)
discovered	2015-05-21 (xsd:date)
discoverer	Outer Solar System Origins Survey
discovery site	Mauna Kea Observatories
earliest precovery date	2014-05-30 (xsd:date)
eccentricity	0.668500 (xsd:double)
epoch	2018-03-23 (xsd:date)
inclination	38.280000 (xsd:double)
mean anomaly	0.106100 (xsd:double)
mean motion	/ day (en)
minorplanet	yes (en)
mp category	Distant minor planet TNO1:9 (en)
observation arc	1.02877776E8 (second)
period	4.84724736E10 (second)
uncertainty	4 (xsd:integer)
has abstract	2015 KE172, internal designation o5m72, is a distant resonant trans-Neptunian object on an eccentric orbit in the outermost region of the Solar System, approximately 100 kilometers (60 miles) in diameter. It was first observed on 21 May 2015 by astronomers with the Outer Solar System Origins Survey at the Mauna Kea Observatories on the island of Hawaii, United States. It came to perihelion (closest approach to the Sun) in October 2017 at a distance of 44.1 AU (6.60 billion km). Its existence was first released in February 2018, and the observations and orbit were announced on 27 April 2018. It belongs to the most distant resonant objects known to exist. (en)
prov:wasDerivedFrom	wikipedia-en:2015_KE172?oldid=1062052183&ns=0
apoapsis (km)	3.3227183061177E10 (kilometre)
orbital period (μ)	1122042.0 (day)
periapsis (km)	6.6028012190859E9 (kilometre)
page length (characters) of wiki page	7836 (xsd:nonNegativeInteger)
absolute magnitude	8.202400 (xsd:double)
albedo	0.090000 (xsd:double)
apoapsis (μ)	33227183061177.000000 (xsd:double)
discovery date	2015-05-21 (xsd:date)
epoch	23 March 2018 (JD2458200.5)
former name	(en) o5m72 (en)

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