Accretion disk is indeed overwhelmingly bright. I made some computations using analythic model (alpha-disk model) for accretion disk around Sagittarius A* in the Milky Way center. Using it's mass of 4.2 million solar masses and realistic accretion rate (3 Earth masses per year), I derived this temperature profile:
max temperature at 4.3 Schwarzschild radii - 96,000K
temperautre at 1000 Schwarzschild radii, where SE rendering stops for now - 2600K (still too bright)
temperature at 3600 Schwarzschild radii - 1000K (so rendering radius in SE should be increased 4x times)
Matter at 96,000K have extremely high brightness. According to the Stefan-Bolzmann law, surface brightness is proportional to T4. So 96,000K is 80,000 times brighter than Sun's surface. It will be saturated to white in SE if exposure is more than 0.0001.
Screenshots here showing accretion disk around Sgr A* with different levels of exposure: 1, 0.01, 0.0001:
吸积盘确实是非常明亮的。我做了一些计算使用analythic模型(α盘模型)在银河中心的人马座A*周围的吸积盘。使用它的质量为4200000个太阳质量和现实的吸积率(3地球群众每年),我得出这个温度分布
最高温度在4.3—96000k史瓦西半径
1000史瓦西半径小,其中SE渲染停止目前2600K(还是太亮)
3600史瓦西半径- 1000K温度(所以绘制半径SE应该增加4倍)
无论在96000k具有极高的亮度。根据斯特凡的测量法,表面亮度是成正比的T4。所以96000k比太阳表面的80000倍。如果暴露在0.0001以上,它将是饱和的白色的硒。
截图显示吸积盘Sgr A*不同暴露水平:1,0.01,0.0001:
(楼上的那个是
普通黑洞吸积盘,这个是
超大黑洞的吸积盘)