About: PSR J1141−6545

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PSR J1141−6545 is a pulsar in the constellation of Musca (the fly). Located at 11h 41m 07.02s −65° 45′ 19.1″, it is a binary pair composed of a white dwarf star orbiting a pulsar. Because of this unusual configuration and the close proximity of the two stars it has been used to test several of Einstein's theories.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body star
rdfs:label	PSR J1141−6545 (en) PSR J1141-6545 (sv)
rdfs:comment	PSR J1141−6545 is a pulsar in the constellation of Musca (the fly). Located at 11h 41m 07.02s −65° 45′ 19.1″, it is a binary pair composed of a white dwarf star orbiting a pulsar. Because of this unusual configuration and the close proximity of the two stars it has been used to test several of Einstein's theories. (en)
foaf:name	PSR J1141-6545 (en)
name	B (en)
dcterms:subject	Binary stars White dwarfs Pulsars Musca (constellation)
Wikipage page ID	63035486 (xsd:integer)
Wikipage revision ID	1018574120 (xsd:integer)
Link from a Wikipage to another Wikipage	Binary star Binary stars White dwarfs Gravitational wave Musca Pulsar White dwarf Albert Einstein Pulsars Musca (constellation) Time dilation Spacetime Musca (constellation) Lense-Thirring effect White dwarf star
sameAs	PSR J1141−6545 PSR J1141−6545 PSR J1141−6545
dbp:wikiPageUsesTemplate	dbt:Reflist dbt:Short_description dbt:Starbox_begin dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_observe dbt:Starbox_orbit dbt:Starbox_reference dbt:DEC dbt:RA dbt:Musca
age	1.400000 (xsd:double)
component	A (en) B (en)
constell	Musca (constellation)
eccentricity	0.171876 (xsd:double)
epoch	J2000 (en)
inclination	>75 (en)
mass	0.986000 (xsd:double) 1.300000 (xsd:double)
periarg	42.457000 (xsd:double)
periastron	MJD 51369.854553 (en)
period unitless	17077.04283168 (second)
primary	A (en)
rotation	393.8978340370 ms (en)
has abstract	PSR J1141−6545 is a pulsar in the constellation of Musca (the fly). Located at 11h 41m 07.02s −65° 45′ 19.1″, it is a binary pair composed of a white dwarf star orbiting a pulsar. Because of this unusual configuration and the close proximity of the two stars it has been used to test several of Einstein's theories. PSR J1141−6545 is notable because it has shown several relativistic theories to have real-world results. The star is emitting gravitational waves and the process of time dilation appears to be affecting the orbit of the white dwarf. In January 2020 it was announced that the stars were also showing the Lense-Thirring effect, whereby a rotating mass drags the surrounding spacetime with it. (en)
prov:wasDerivedFrom	wikipedia-en:PSR_J1141−6545?oldid=1018574120&ns=0
page length (characters) of wiki page	5026 (xsd:nonNegativeInteger)
foaf:isPrimaryTopicOf	wikipedia-en:PSR_J1141−6545
is Link from a Wikipage to another Wikipage of	PSR J1141-6545
is Wikipage redirect of	PSR J1141-6545
is foaf:primaryTopic of	wikipedia-en:PSR_J1141−6545

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