Lubang hitam: Perbedaan antara revisi

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Kita tidak dapat melihat lubang hitam akan tetapi kita bisa mendeteksi materi yang tertarik / tersedot ke arahnya. Dengan cara inilah, para astronom mempelajari dan mengidentifikasikan banyak lubang hitam di angkasa lewat observasi yang sangat hati-hati sehingga diperkirakan di angkasa dihiasi oleh jutaan lubang hitam.
 
Black holes are predicted by [[general relativity]]. According to [[general relativity|classical general relativity]], neither matter nor [[information]] can flow from thet[pop[he interior of a black hole to an outside observer. For example, one cannot bring out any of its mass, or receive a reflection back by shining a light source such as a flashlight, or retrieve any information about the material that has entered the black hole. [[Quantum mechanics|Quantum mechanical]] effects may allow [[matter]] and [[energy]] to [[Hawking radiation|radiate]] from black holes; however, it is thought that the nature of the radiation does not depend on what has fallen into the black hole in the past.
 
The existence of black holes in the universe is well supported by astronomical observation, particularly from studying [[supernova|supernovae]] and [[X-ray]] emissions from [[active galactic nuclei]].