About: (470599) 2008 OG19

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(470599) 2008 OG19 is a trans-Neptunian object located in the scattered disc. It was discovered on 30 July 2008 through the Palomar Observatory. It displays a large light curve amplitude of 0.437±0.011 magnitudes, implying that it is highly elongated in shape, similar to 20000 Varuna. Based on models for its light curve amplitude, they obtained an approximate density of 0.609 g/cm3 and aspect ratios of b/a = 0.513 and c/a = 0.39.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body Planet planet
rdfs:label	(470599) 2008 OG19 (de) (470599) 2008 OG19 (en) (470599) 2008 OG19 (fr) (470599) 2008 OG19 (pt)
rdfs:comment	(470599) 2008 OG19 is a trans-Neptunian object located in the scattered disc. It was discovered on 30 July 2008 through the Palomar Observatory. It displays a large light curve amplitude of 0.437±0.011 magnitudes, implying that it is highly elongated in shape, similar to 20000 Varuna. Based on models for its light curve amplitude, they obtained an approximate density of 0.609 g/cm3 and aspect ratios of b/a = 0.513 and c/a = 0.39. (en) (470599) 2008 OG19 ist ein großes transneptunisches Objekt, das bahndynamisch als Scattered Disk Object (SDO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de) (470599) 2008 OG19, est un objet transneptunien (OTN) de la famille des objets épars découvert le 30 juillet 2008 à l'observatoire Palomar. (fr) (470599) 2008 OG19, também escrito como (470599) 2008 OG19, é um corpo menor que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,6 e tem um diâmetro com cerca de 529 km. 2008 OG19 é um candidato com possível chance de aumentar a lista oficial de planetas anões. (pt)
foaf:name	(en) (470599) (en)
dcterms:subject	Astronomical objects discovered in 2008 Discoveries by the Palomar Observatory Possible dwarf planets Scattered disc and detached objects
Wikipage page ID	46390888 (xsd:integer)
Wikipage revision ID	1051722487 (xsd:integer)
Link from a Wikipage to another Wikipage	Degree (angle) Julian day Light curve Astronomical objects discovered in 2008 Discoveries by the Palomar Observatory Possible dwarf planets Scattered disc and detached objects Palomar Observatory Trans-Neptunian object 20000 Varuna Julian year (astronomy) Amplitude Aspect ratio Magnitude (astronomy) Scattered disc
sameAs	(470599) 2008 OG19 (470599) 2008 OG19 (470599) 2008 OG19 (470599) 2008 OG19 (470599) 2008 OG19
dbp:wikiPageUsesTemplate	dbt:CentaurTNO-stub dbt:Convert dbt:Deg2DMS dbt:Dwarf_planets dbt:Infobox_planet dbt:JPL_small_body dbt:Minor_planets_navigator dbt:Mp dbt:Reflist dbt:Small_Solar_System_bodies dbt:Val
albedo	0.081000 (xsd:double) 0.199000 (xsd:double)
arg peri	140.530000 (xsd:double)
asc node	164.020000 (xsd:double)
background	#C2E0FF (en)
discovered	2008-07-30 (xsd:date)
discoverer	Palomar Observatory team (en)
discovery site	Palomar Observatory
eccentricity	0.418070 (xsd:double)
epoch	2016-01-13 (xsd:date)
inclination	13.167000 (xsd:double)
mean anomaly	1.568100 (xsd:double)
mean motion	/day (en)
minorplanet	yes (en)
mp category	Scattered disc
observation arc	2.242944E8 (second)
period	1.7032583448000002E10 (second)
sidereal day	h (en)
spectral type	V–R=0.64 (en)
uncertainty	3 (xsd:integer)
has abstract	(470599) 2008 OG19 is a trans-Neptunian object located in the scattered disc. It was discovered on 30 July 2008 through the Palomar Observatory. It displays a large light curve amplitude of 0.437±0.011 magnitudes, implying that it is highly elongated in shape, similar to 20000 Varuna. Based on models for its light curve amplitude, they obtained an approximate density of 0.609 g/cm3 and aspect ratios of b/a = 0.513 and c/a = 0.39. (en) (470599) 2008 OG19 ist ein großes transneptunisches Objekt, das bahndynamisch als Scattered Disk Object (SDO) eingestuft wird. Aufgrund seiner Größe ist der Asteroid ein Zwergplanetenkandidat. (de) (470599) 2008 OG19, est un objet transneptunien (OTN) de la famille des objets épars découvert le 30 juillet 2008 à l'observatoire Palomar. (fr) (470599) 2008 OG19, também escrito como (470599) 2008 OG19, é um corpo menor que está localizado no disco disperso, uma região do Sistema Solar. Ele possui uma magnitude absoluta de 4,6 e tem um diâmetro com cerca de 529 km. 2008 OG19 é um candidato com possível chance de aumentar a lista oficial de planetas anões. (pt)
prov:wasDerivedFrom	wikipedia-en:(470599)_2008_OG19?oldid=1051722487&ns=0
apoapsis (km)	1.40627982372828E10 (kilometre)
orbital period (μ)	197137.0 (day)
periapsis (km)	5.7708874601232E9 (kilometre)
page length (characters) of wiki page	4412 (xsd:nonNegativeInteger)
albedo	0.081000 (xsd:double) 0.199000 (xsd:double)
apoapsis (μ)	14062798237282.800781 (xsd:double)
discovery date	2008-07-30 (xsd:date)
epoch	13 January 2016 (JD2457400.5)
orbital period (s)	17032636800.000000 (xsd:double)
periapsis (μ)	5770887460123.200195 (xsd:double)
discoverer	Palomar Observatory
foaf:isPrimaryTopicOf	wikipedia-en:(470599)_2008_OG19
is Link from a Wikipage to another Wikipage of	List of minor planets: 470001–471000 2008 OG19
is Wikipage redirect of	2008 OG19
is foaf:primaryTopic of	wikipedia-en:(470599)_2008_OG19

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