Very interesting article came up in my feed today: http://io9.com/the-truth-behind-interstellars-scientifically-accurate-1686120318
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Turns out the original Wired article about Kip Thorne's work was a little - overexcited - about "new discoveries". Bit in reading that, this article was also linked to:
http://dneg.com/dneg_vfx/blackhole/
What was fascinating are the videos and how close Frontier HAVE got the black holes, but that there is still work that can be done to make them more accurate (and prettier)
[video=youtube;CbW2jKXq3gE]https://www.youtube.com/watch?v=CbW2jKXq3gE[/video]
[video=youtube;mKmHD7v9Qt8]https://www.youtube.com/watch?v=mKmHD7v9Qt8[/video]
At the moment, as far as I can tell they are merely rendered as spheres with an environment mapping from the background, and does not capture any "foreground" objects such as nearby stars - nor does looking through lensing effect have any effect on bending these around. They also don't appear to be of any particular genus - rather all static and no spinning ones, so they have no accretion disks, which should also surely be visible from nearby systems in the background images.
Anyway just thought it might be of interest to some of you and a nice discussion point instead of constantly bickering about community goals.
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The second and third images show what the accretion disk would look like, given the increasingly intense color-changing effects of Doppler and gravitational frequency shifts. (I'm simplifying, but these shifts characterize how light moving quickly toward and away from an observer affect the perceived color and intensity of that light.) The third and final image, write Thorne and his colleagues "is what the disk would truly look like to an observer near the black hole."
Turns out the original Wired article about Kip Thorne's work was a little - overexcited - about "new discoveries". Bit in reading that, this article was also linked to:
http://dneg.com/dneg_vfx/blackhole/
What was fascinating are the videos and how close Frontier HAVE got the black holes, but that there is still work that can be done to make them more accurate (and prettier)
All these movies entail a black hole with spin 0.999 of maximum and a camera at radii 6.03 GM/c2 or 2.6 GM/c2, where M is the black hole’s mass, and G and c are Newton’s gravitational constant and the speed of light. The observer is moving in a circular geodesic orbit.
View of a starfield under the influence of gravitational lensing. The camera is at radius r=2.6 GM/c2
[video=youtube;CbW2jKXq3gE]https://www.youtube.com/watch?v=CbW2jKXq3gE[/video]
View of a starfield under the influence of gravitational lensing. The camera is at radius r=6.03 GM/c2. The primary and secondary critical curves are overlaid in purple and the path of a star at polar angle 0.608 pi is overlaid in red.
[video=youtube;mKmHD7v9Qt8]https://www.youtube.com/watch?v=mKmHD7v9Qt8[/video]
At the moment, as far as I can tell they are merely rendered as spheres with an environment mapping from the background, and does not capture any "foreground" objects such as nearby stars - nor does looking through lensing effect have any effect on bending these around. They also don't appear to be of any particular genus - rather all static and no spinning ones, so they have no accretion disks, which should also surely be visible from nearby systems in the background images.
Anyway just thought it might be of interest to some of you and a nice discussion point instead of constantly bickering about community goals.