About: SN 2014J     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Whole100003553, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FSN_2014J&invfp=IFP_OFF&sas=SAME_AS_OFF

SN 2014J was a type-Ia supernova in Messier 82 (the 'Cigar Galaxy', M82) discovered in mid-January 2014. It was the closest type-Ia supernova discovered for 42 years, and none have been closer as of 2018. The supernova was discovered by chance during an undergraduate teaching session at the University of London Observatory. It peaked on 31 January 2014, reaching an apparent magnitude of 10.5. SN 2014J was the subject of an intense observing campaign by professional astronomers and was bright enough to be seen by amateur astronomers.

AttributesValues
rdf:type
rdfs:label
  • SN 2014J (es)
  • SN 2014J (fr)
  • SN 2014J (ko)
  • SN 2014J (ja)
  • SN 2014J (en)
  • SN 2014J (pt)
  • SN 2014J (pl)
  • SN 2014J (ru)
  • SN 2014J (sv)
  • SN 2014J (zh)
rdfs:comment
  • SN 2014J es una supernova tipo Ia en la Galaxia del Cigarro (Messier 82) descubierta a mediados de enero de 2014.​ Es la supernova de tipo Ia más cercana descubierta en los últimos 42 años. Fue descubierta por accidente durante una sesión de enseñanza de pregrado en el observatorio de la Universidad de Londres. SN 2014J es actualmente objeto de una intensa campaña de observación por astrónomos profesionales, y es lo suficientemente brillante para ser vista por los astrónomos aficionados. (es)
  • SN 2014J was a type-Ia supernova in Messier 82 (the 'Cigar Galaxy', M82) discovered in mid-January 2014. It was the closest type-Ia supernova discovered for 42 years, and none have been closer as of 2018. The supernova was discovered by chance during an undergraduate teaching session at the University of London Observatory. It peaked on 31 January 2014, reaching an apparent magnitude of 10.5. SN 2014J was the subject of an intense observing campaign by professional astronomers and was bright enough to be seen by amateur astronomers. (en)
  • SN 2014J는 지구에서 큰곰자리 방향으로 1,150만 광년 떨어져 있는 시가 은하 내에서 발생한 Ia형 초신성으로, 2014년 1월 21일 영국 런던대 관측소에서 스티브 포세이 교수에게 카메라 사용법을 배우던 학생들에 의해 처음으로 관측되었다.초신성이 가장 밝을 때인 1월 31일, NASA의 허블 우주 망원경이 초신성을 관측했다. 이 초신성의 관측은 Ia형 초신성을 이용한 우주 거리 측정에 도움을 줄 것으로 기대되고 있다. (ko)
  • SN 2014J とは、地球から見ておおぐま座の方向にある M82 内で出現したIa型超新星である。 (ja)
  • SN 2014J – supernowa typu Ia w galaktyce M82. Odkryta 21 stycznia 2014 roku, w chwili odkrycia miała wielkość 11,5m. Maksimum blasku osiągnęła 31 stycznia, przy wielkości 10,5m. Przed potwierdzeniem odkrycia nosiła tymczasowe oznaczenie PSN J09554214+6940260. (pl)
  • SN 2014J é uma supernova em Messier 82 (Cigar Galaxy, M82) descoberta em meados de janeiro de 2014. Foi a supernova tipo Ia mais próxima descoberta por 42 anos, e nenhuma foi mais próxima. A supernova foi descoberta por acaso durante uma sessão de graduação no Observatório da Universidade de Londres. Ele atingiu o pico em 31 de janeiro de 2014, atingindo uma magnitude aparente de 10,5. (pt)
  • SN 2014J — сверхновая типа Iа в галактике Messier 82 («Сигара»), открытая в январе 2014 года. Ближайшая к Земле сверхновая этого типа за последние 40 лет. SN 1993J (Messier 81, галактика Боде) находилась примерно на таком же расстоянии от Земли, как SN 2014J. Прямое восхождение звезды — 9ч 55м 42,217с, склонение — 69° 40′ 26,56″. (ru)
  • SN 2014J, PSN J09554214+6940260, var en supernova i Cigarrgalaxen (Messier 82), ungefär 11,5 miljoner ljusår från jorden. Det var den närmsta supernovan av typ I på 42 år, sedan upptäckten av SN 1972E. Den upptäcktes av Stephen Fossey vid University College London Observatory den 21 januari 2014 och hade då magnitud, 11,7. Sin högsta ljusstyrka nådde supernovan den i början av februari 2014, med en magnitud av 10,1-10,5. (sv)
  • SN 2014J是一颗位于大熊座雪茄星系(M82)的Ia型超新星,发现于2014年,是四十年来爆发的距离地球最近的Ia型超新星。 (zh)
  • SN 2014J, provisoirement PSN J09554214+6940260, est une supernova située dans la galaxie du Cigare (ou Messier 82) découverte par un groupe d'étudiants en astronomie à l'observatoire de l'université de Londres et leur professeur le 21 janvier 2014 à 19 h 20 (GMT). Le télescope utilisé était un télescope de 0,35 m de diamètre automatisé. (fr)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Opo1742a.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Mill_hill_observatory_2009.jpg
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 53 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software