CXC: Famous Black Hole Has Jet Pushing Cosmic Speed Limit
Posted: Tue Jan 07, 2020 5:21 pm
Famous Black Hole Has Jet Pushing Cosmic Speed Limit
NASA | MSFC | SAO | Chandra X-ray Observatory | 2020 Jan 06
Detection of Superluminal Motion in the X-Ray Jet of M87 ~ Bradford Snios et al
NASA | MSFC | SAO | Chandra X-ray Observatory | 2020 Jan 06
These images show evidence from NASA's Chandra X-ray Observatory that the black hole in the galaxy Messier 87 (M87) is blasting particles out at over 99% the speed of light, as described in our latest press release. While astronomers have observed features in the M87 jet blasting away from its black hole this quickly at radio and optical wavelengths for many years, this provides the strongest evidence yet that actual particles are traveling this fast. Astronomers required the sharp X-ray vision from Chandra in order to make these precise measurements.
The main panel of the graphic shows the entire length of M87's jet seen by Chandra, stretching for about 18,000 light years. "Knots" of X-ray emission seen here are created when material falls onto the M87 sporadically, creating bursts of X-ray light that travel along the jet and away from the black hole. The insets show Chandra observations taken in 2012 and 2017 of a small region near the base of the jet. The source in the lower left is X-ray emission from material around the black hole, and the other source is a knot in the jet about 900 light years from the black hole. This knot moves away from the black hole between 2012 and 2017 and also fades by 70%.
The researchers carefully studied this knot, and another one about 2,500 light years along the jet. By comparing how far these knots moved over the five-year interval, the team of astronomers was able to determine the closer knot has an apparent speed of 6.3 times the speed of light for the X-ray knot, while the other looks like it is moving at 2.4 times the speed of light. ...
Detection of Superluminal Motion in the X-Ray Jet of M87 ~ Bradford Snios et al
- Astrophysical Journal 879(1):8 (2019 Jul 01) DOI: 10.3847/1538-4357/ab2119
- arXiv.org > astro-ph > arXiv:1905.04330 > 10 May 2019 (v1), 12 Jun 2019 (v2)