The densest gas planetary nebulae are presumed to be about 100 to 10,000 particles per cc. (Osterbrook & Ferland, 2005). Larger particles may be multi-molecular, up to several microns across. (
http://www-ssg.sr.unh.edu/ism/what1.html)
The Interstellar medium runs 1 atom per cc... (
http://www-ssg.sr.unh.edu/ism/what1.html)... some 100 to 10,000 times the density.
The Interplanetary medium is around 5 particles per CC in orbit 3 of a G2V... inverse square applies. But note also solar wind runs 10 particles per cc ±10%, so the lower density is practically only in shadows behind planets and solar weather events. CME's run 1000 to 100,000 particles per CC, again inverse square applies, and typically it's around 1000 particles per cc at earth, but can easily top 5x that for the biggest ones, IIRC.
Surface air on earth runs 3e19 particles per cc...
A CME is supposedly naked-eye visible for the first couple hours... if one can block out the glare from the sun.
The temperature is FAR more important than the density for visibility. Looking at the blackbody graph, get that stuff up to about 1500° K, and you've got visibility.
Likewise, a lot of the visibility is reflective - you might actually see the nebula as a slightly dark blue shell (for dust)... rather than the black we see.
Visible, but not highly visible...