You can help expand this article with text translated from the corresponding article in French. (December 2017) Click for important translation instructions. View a machine-translated version of the French article. Machine translation, like DeepL or Google Translate, is a useful starting point for translations, but translators must revise errors as necessary and confirm that the translation is accurate, rather than simply copy-pasting machine-translated text into the English Wikipedia. Consider adding a topic to this template: there are already 1,470 articles in the main category, and specifying|topic= will aid in categorization. Do not translate text that appears unreliable or low-quality. If possible, verify the text with references provided in the foreign-language article. You must provide copyright attribution in the edit summary accompanying your translation by providing an interlanguage link to the source of your translation. A model attribution edit summary is Content in this edit is translated from the existing French Wikipedia article at :fr:PSR_J2032%2B4127; see its history for attribution. You may also add the template {{Translated|fr|PSR_J2032%2B4127}} to the talk page. For more guidance, see Wikipedia:Translation.

PSR J2032+4127, sometimes abbreviated as J2032, is a pulsar. It is accompanied by a massive Be star named MT91 213 (also 2MASS J20321312+4127243). The system is located in the constellation Cygnus (constellation) at a distance of about 1.4 kpc (~ 4570 al ) from the Sun. The system is part of the Cygnus OB2 association.

It is expected that the coming together of the two stars in early 2018 will generate high-energy phenomena.^[1]

The System has an orbital period of around 45-50 yr.^[2]

Referencesedit

External linksedit

• Astronomers Predict Fireworks from Rare Stellar Encounter in 2018 NASA
• Coming Soon: Closest Approach - movie-style "preview" video from NASA about the far-ranging explorations expected during close encounter in 2018

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