PSR J2007+2722
ObjectBlack Holes and Neutron Stars
An isolated pulsar in Vulpecula, identified through Einstein@Home analysis.
1.00Common
Common
PSR J2007+2722
- Black Holes and Neutron Stars
PSR J2007+2722 is an isolated pulsar in the constellation Vulpecula. It rotates at 40.82 hertz, with a period of 24.497 milliseconds, and lies 5.3 kiloparsecs from Earth in the plane of the Galaxy. It is considered most likely to be a disrupted recycled pulsar. The object was found in Arecibo radio telescope data taken in February 2007 and analyzed through the Einstein@Home distributed computing project.
The picture on this card was made with AI. It is an illustration, not a real photo of the subject.
- Type
- Isolated pulsar, most likely a disrupted recycled pulsar
- Location
- Vulpecula constellation, 5.3 kpc distant
- Discovery data
- Found in Arecibo data taken in February 2007
Sources and credits
Sources and credits
- Article
- PSR J2007+2722 (English Wikipedia)
- Wikidata
- Q1558495
- Text
- Card text is adapted from the English Wikipedia article by an automated summary. Wikipedia content is available under CC BY-SA 4.0; see the article history for its contributors. CC BY-SA 4.0 · Article history and contributors
- Illustration
- AI-generated illustration. Not a photograph or documentary image. (model: gpt-image-2)
- Popularity
- 2 median daily views (Wikimedia Pageviews API (all-access, user agent))
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