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Black.Hole,Extremal.Kerr.Newman,Raytracing.png (800 × 430 pixels, file size: 262 KB, MIME type: image/png)
English: Extremal Kerr-Newman black hole with spin a/M=√½ and charge Q/M=√½, in natural units of G=K=c=1. Therefore a²+Q²=M². The observer is at r=50M and views the black hole from the equatorial plane (edge on). FOV: 77.4°×38.7°. The equations that were used to raytrace the image can be found here.
|Author||Yukterez (Simon Tyran, Vienna). Source material for the Milky way background (also available on Commons): ESO/S.Brunier. Code for the relativistic raytracer: yukterez.net|
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|current||02:00, 21 April 2018||800 × 430 (262 KB)||Yukterez||display the distance and angle of view in the right upper corner|
|20:13, 11 April 2018||800 × 430 (262 KB)||Yukterez||reduced width to 800px to avoid rescaling|
|19:59, 11 April 2018||860 × 430 (285 KB)||Yukterez||User created page with UploadWizard|
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