Ah, M42 is a testament to the huge dynamic range (difference between the brightest and darkest parts of the nebula) of the human eye and the limited dynamic range of even 16-bit cameras and the even more limited dynamic range of most monitors we would use to view our results.
With a big scope the naked eye can see lots of nebulosity in M42 and the stars of the Trapezium.
The camera cannot capture both. When you see a good astrophoto of M42 it is usually 2 photos blended together, with the Trapezum area shot with very short exposures and the nebulosity with much longer exposures. Otherwise the whole Trapezium will just blow out (all the pixels r3cord at their highest level, which is pure white), and no amount of histogram manipulation can bring it back.
Moreover, when you see many astro photos on your PC, the image dynamic range is seriously compressed to brighten the shadows and darken the brightest areas. That is because your typical monitor clips far too much of the dynamic range in an image. That is why, even for daylight photography with a DSLR, you often have to brighten shadows to see what is in them. It is in the image, just not on the screen.
So, as the old saying goes: you cannot get there from here, at least not with respect to M42. M51 is a great target to see what you can capture, as it has no really bright bits. M33 is a challenging target as, while large, it has only faint bits. Even M31 (Andromeda) is a bit of a challenge as it is easy to blow out the bright core while trying to capture more of the arms and dust lanes.