This HTML5 document contains 90 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

Namespace Prefixes

PrefixIRI
n3http://dbpedia.org/ontology/Planet/
dctermshttp://purl.org/dc/terms/
yago-reshttp://yago-knowledge.org/resource/
dbohttp://dbpedia.org/ontology/
foafhttp://xmlns.com/foaf/0.1/
n18http://su.dbpedia.org/resource/
n5https://global.dbpedia.org/id/
schemahttp://schema.org/
dbthttp://dbpedia.org/resource/Template:
rdfshttp://www.w3.org/2000/01/rdf-schema#
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
owlhttp://www.w3.org/2002/07/owl#
wikipedia-enhttp://en.wikipedia.org/wiki/
dbchttp://dbpedia.org/resource/Category:
dbphttp://dbpedia.org/property/
provhttp://www.w3.org/ns/prov#
xsdhhttp://www.w3.org/2001/XMLSchema#
wikidatahttp://www.wikidata.org/entity/
dbrhttp://dbpedia.org/resource/

Statements

Subject Item
dbr:2015_TC25
rdf:type
dbo:Location wikidata:Q634 dbo:CelestialBody schema:Place dbo:Place dbo:Planet owl:Thing
rdfs:label
2015 TC25
rdfs:comment
2015 TC25 is a near-Earth asteroid, and at only 6 feet (2 meters) across and absolute magnitude 29.34 mag, it is thought to be the second smallest asteroid observed over multiple years, the smallest being 2006 RH120 with 29.5 mag. The asteroid is notable for reflecting about 60% of the light that hits it, making it one of the brightest near-earth asteroids ever seen.
foaf:name
dcterms:subject
dbc:Astronomical_objects_discovered_in_2015 dbc:Minor_planet_object_articles_(unnumbered) dbc:Fast_rotating_minor_planets dbc:Apollo_asteroids
dbo:wikiPageID
53199218
dbo:wikiPageRevisionID
1068533317
dbo:wikiPageWikiLink
dbc:Astronomical_objects_discovered_in_2015 dbc:Minor_planet_object_articles_(unnumbered) dbr:Degree_(angle) dbr:Julian_date dbr:Albedo dbr:Asteroid dbr:Polarization_(waves) dbr:Astronomical_unit dbr:2006_RH120 dbr:Near-Earth_asteroid dbr:Rotation_period dbc:Fast_rotating_minor_planets dbr:Regolith dbc:Apollo_asteroids dbr:Aubrite dbr:44_Nysa dbr:Arecibo_Observatory dbr:Radar dbr:Surface_gravity dbr:Celestial_mechanics dbr:Apollo_asteroid dbr:Asteroid_spectral_types dbr:E-type_asteroid dbr:Catalina_Sky_Survey dbr:Planetary_differentiation
owl:sameAs
n5:2qYcR yago-res:2015_TC25 wikidata:Q30591909 n18:2015_TC25
dbp:wikiPageUsesTemplate
dbt:Convert dbt:Mp dbt:JPL_small_body dbt:Reflist dbt:NeoDys dbt:ESA-SSA dbt:Use_dmy_dates dbt:Infobox_planet dbt:Deg2DMS dbt:Small_Solar_System_bodies
dbp:absMagnitude
29.5
dbp:aphelion
1.1504
dbp:argPeri
80.5784
dbp:ascNode
19.6544
dbp:background
#FFC2E0
dbp:discovered
2015-10-12
dbp:discoverer
dbr:Catalina_Sky_Survey
dbp:eccentricity
0.1177
dbp:epoch
JD 2457607.5
dbp:inclination
3.6383
dbp:meanAnomaly
214.2377
dbp:meanMotion
/ day
dbp:minorplanet
yes
dbp:mpCategory
dbr:Apollo_asteroid
dbp:perihelion
0.9081
dbp:period
3.2819904000000004E7
dbp:semimajor
1.0292
dbp:spectralType
dbr:E-type_asteroid
dbo:abstract
2015 TC25 is a near-Earth asteroid, and at only 6 feet (2 meters) across and absolute magnitude 29.34 mag, it is thought to be the second smallest asteroid observed over multiple years, the smallest being 2006 RH120 with 29.5 mag. The asteroid is notable for reflecting about 60% of the light that hits it, making it one of the brightest near-earth asteroids ever seen. Discovered by the Catalina Sky Survey on 12 October 2015, it was observed with several ground-based telescopes. Radar observations were also made using the Arecibo Observatory as it passed 128,000 kilometers (79,500 miles) from the Earth. Observations suggest its surface composition is similar to Aubrite meteorites, a rare class of high-albedo differentiated meteorites. The albedo and radar polarization ratio suggest 2015 TC25 belongs to the E-type asteroids, and comparison of its spectral and dynamical properties suggest it may have broke off of the 70-kilometer diameter E-type asteroid 44 Nysa. 2015 TC25 is also notable for its rather short rotation period of only about 2 minutes, which, combined with its low surface gravity makes it very difficult for 2015 TC25 to retain a regolith layer. Its surface therefore most likely resembles a bare rock.
prov:wasDerivedFrom
wikipedia-en:2015_TC25?oldid=1068533317&ns=0
n3:apoapsis
1.7209739045328E8
n3:meanRadius
0.002
n3:orbitalPeriod
379.86000000000007
n3:periapsis
1.3584982638267E8
dbo:wikiPageLength
4264
dbo:absoluteMagnitude
29.5
dbo:apoapsis
172097390453.28
dbo:discovered
2015-10-12
dbo:epoch
JD2457607.5 (2016 August 7)
dbo:meanRadius
2.0
dbo:orbitalPeriod
32819904.0
dbo:periapsis
135849826382.67
dbo:rotationPeriod
133.74
dbo:discoverer
dbr:Catalina_Sky_Survey
foaf:isPrimaryTopicOf
wikipedia-en:2015_TC25