This HTML5 document contains 75 embedded RDF statements represented using HTML+Microdata notation.

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

Namespace Prefixes

PrefixIRI
dctermshttp://purl.org/dc/terms/
yago-reshttp://yago-knowledge.org/resource/
dbohttp://dbpedia.org/ontology/
foafhttp://xmlns.com/foaf/0.1/
n4http://dbpedia.org/resource/File:
n14https://global.dbpedia.org/id/
schemahttp://schema.org/
dbthttp://dbpedia.org/resource/Template:
rdfshttp://www.w3.org/2000/01/rdf-schema#
freebasehttp://rdf.freebase.com/ns/
n15http://commons.wikimedia.org/wiki/Special:FilePath/
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
owlhttp://www.w3.org/2002/07/owl#
wikipedia-enhttp://en.wikipedia.org/wiki/
dbphttp://dbpedia.org/property/
dbchttp://dbpedia.org/resource/Category:
provhttp://www.w3.org/ns/prov#
xsdhhttp://www.w3.org/2001/XMLSchema#
wikidatahttp://www.wikidata.org/entity/
goldhttp://purl.org/linguistics/gold/
dbrhttp://dbpedia.org/resource/

Statements

Subject Item
dbr:V1017_Sagitarii
dbo:wikiPageWikiLink
dbr:V1017_Sagittarii
dbo:wikiPageRedirects
dbr:V1017_Sagittarii
Subject Item
dbr:V1017_Sagittarii
rdf:type
dbo:CelestialBody dbo:Star dbo:Location schema:Place owl:Thing dbo:Place
rdfs:label
V1017 Sagittarii
rdfs:comment
V1017 Sagittarii is a cataclysmic variable star system in the constellation Sagittarius. It first erupted in 1919, reaching magnitude 7. Its other eruptions in 1901, 1973 and 1991 only reached magnitude 10, leading it to be reclassified from a recurrent nova to a dwarf nova. After the eruption of 1919, the orbital period of the binary system has decreased by 0.0273±0.0061%, to the 5.786290±0.000032 days. Physical models cannot explain the orbital change of such sign and magnitude as in 2019.
foaf:name
V1017 Sagittarii
foaf:depiction
n15:V1017SgrLightCurve.png
dcterms:subject
dbc:White_dwarfs dbc:Dwarf_novae dbc:2MASS_objects dbc:Objects_with_variable_star_designations dbc:Eclipsing_binaries dbc:G-type_giants dbc:Sagittarius_(constellation)
dbo:wikiPageID
46526679
dbo:wikiPageRevisionID
1075683759
dbo:wikiPageWikiLink
n4:V1017SgrLightCurve.png dbc:2MASS_objects dbr:Photometric_system dbr:Sagittarius_(constellation) dbr:White_dwarf dbc:Objects_with_variable_star_designations dbr:Cataclysmic_variable dbr:Dwarf_nova dbr:AAVSO dbc:Eclipsing_binaries dbr:Recurrent_nova dbr:Light_curve dbc:Sagittarius_(constellation) dbc:G-type_giants dbc:White_dwarfs dbc:Dwarf_novae
owl:sameAs
yago-res:V1017_Sagittarii n14:26DeQ wikidata:Q22086967 freebase:m.0134tvnx
dbp:wikiPageUsesTemplate
dbt:DEC dbt:Starbox_image dbt:Starbox_observe dbt:Multi-star-stub dbt:Odlist dbt:Stars_of_Sagittarius dbt:Reflist dbt:Val dbt:Starbox_reference dbt:RA dbt:± dbt:Short_description dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_end dbt:Var-star-stub dbt:Starbox_character
dbo:thumbnail
n15:V1017SgrLightCurve.png?width=300
dbp:appmagV
(Max.) 13.5
dbp:class
G5IIIp / white dwarf
dbp:constell
dbr:Sagittarius_(constellation)
dbp:epoch
J2000
dbp:pError
0.0437
dbp:parallax
0.7892
dbp:radialV
15
dbp:variable
eclipsing recurrent nova
dbo:abstract
V1017 Sagittarii is a cataclysmic variable star system in the constellation Sagittarius. It first erupted in 1919, reaching magnitude 7. Its other eruptions in 1901, 1973 and 1991 only reached magnitude 10, leading it to be reclassified from a recurrent nova to a dwarf nova. After the eruption of 1919, the orbital period of the binary system has decreased by 0.0273±0.0061%, to the 5.786290±0.000032 days. Physical models cannot explain the orbital change of such sign and magnitude as in 2019.
gold:hypernym
dbr:System
prov:wasDerivedFrom
wikipedia-en:V1017_Sagittarii?oldid=1075683759&ns=0
dbo:wikiPageLength
4071
foaf:isPrimaryTopicOf
wikipedia-en:V1017_Sagittarii
Subject Item
wikipedia-en:V1017_Sagittarii
foaf:primaryTopic
dbr:V1017_Sagittarii