File:HR 6819.jpg

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Captions

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orbits of the HR 6819 hierarchical triple star system: an inner binary with one star (orbit in blue) and a newly discovered black hole (orbit in red), as well as another star in a wider orbit (also in blue).

Summary

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Description
العربية: تصويرٌ لِمدار الأجرام الفلكيَّة التابعة لِنظام HR 6819 ثُلاثي النُجُوم. يتكوَّن هذا النظام من ثُنائي داخلي بنجمٍ وحيدٍ (المدار الأزرق) وثُقبٌ أسود حديث الاكتشاف (المدار الأحمر)، إضافةً إلى جرمٍ ثالثِ، ونجمٌ آخر، في مدارٍ أوسع (بِالأزرق أيضًا). اعتقد الفريق بدايةً أنَّ هُناك جرمان فقط، وهُما النجمان. لكن مع استمرار تحليلهم لِلمعلومات المُرصدة، فوجئوا بِاكتشافهم جرمًا ثالثًا، لم يكن ظاهرًا قبلًا، في نظام HR 6819، وهو ثُقبٌ أسود، الأقرب إلى الأرض حتَّى تاريخ اكتشافه. والثقب الأسود المذكور غير مرئي، لكن يؤكَّد وُجُوده بِفعل قُوَّاه الجاذبة، التي تدفع النجم المُشع الداخلي إلى التحرُّك ضمن مدار. للأجرام الواقعة ضمن النظام الثُنائي الداخلي ذات الكُتلة والمدار تقريبًا. أظهرت عمليَّات الرصد أنَّ النجم الداخلي المرئي يدُورُ حول الثُقب الأسود كُل 40 يوم، بينما النجمُ الآخر يقع على مسافةٍ بعيدةٍ من الثُنائي الداخلي.
English: This artist’s impression shows the orbits of the objects in the HR 6819 triple system. This system is made up of an inner binary with one star (orbit in blue) and a newly discovered black hole (orbit in red), as well as a third object, another star, in a wider orbit (also in blue). The team originally believed there were only two objects, the two stars, in the system. However, as they analysed their observations, they were stunned when they revealed a third, previously undiscovered body in HR 6819: a black hole, the closest ever found to Earth. The black hole is invisible, but it makes its presence known by its gravitational pull, which forces the luminous inner star into an orbit. The objects in this inner pair have roughly the same mass and circular orbits. The observations, with the FEROS spectrograph on the 2.2-metre telescope at ESO’s La Silla, showed that the inner visible star orbits the black hole every 40 days, while the second star is at a large distance from this inner pair.
Date
Source https://www.eso.org/public/images/eso2007a/
Author ESO/L. Calçada

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