Freethinker,
you said "One answer to what would we SEE if we were traveling at the speed of light would be "nothing". We would not survive the acceleration"
you are quite right of course, that's why I said "IF" it were possible.
Thanks for your explanation of color, this is also how I understand it. I was baffled by the idea Alex gave about looping linear spectrum over 360 degrees. I thought maybe I was misinterpreting what he was trying to say or just lacked knowledge on some aspect of light. (there's much in science/physics that go way over my head). Anyway...
I have found a site with an answer.
But bare in mind the main page states "Its purpose is to provide good answers to questions that have been discussed often in sci.physics and related usenet newsgroups. The articles in this FAQ are based on those discussions and on information from good reference sources. That does not mean that they are always perfect and complete."
This following link gives a brief overview with images of what you would see, according to the theory of special relativity.
http://math.ucr.edu/home/baez/physic...spaceship.html
It is (according to the above site) a mix of effects: Doppler shift (or red shift), Aberration (the tunnel effect, as I poorly explained it) also "Beaming" (brightening of light due to increased flux intensity.
Here's an excerpt -
"Starlight consists of light in a wide range of wavelengths, so while it is true that an approaching star will have its light Doppler shifted into shorter wavelengths (except for very high and inclined velocities), it is not necessarily true in general that the star will show a bluer colour. The reason is that the whole spectral energy distribution is shifted, so that a previously invisible infrared part may contribute considerably to a redder colour, and similarly, light from the blue part of the spectrum may be shifted out to the invisible UV."
"Considerations of the flux lead to what is generally called beaming. Beaming is related to aberration in that flux intensity is increased in the forward direction due to the squeezing of the total flux. In addition, if we consider a steady stream of photons, they tend to arrive more often if one travels towards the source, and less often if one recedes. This results in higher flux intensity, and causes stars in front to get brighter, and from rear to get fainter."
Well I was on the right track it seems, although I had not thought about the stars getting brighter. Well I am only a lay person striving to get a better concept of these things
Anyone else have a different (or additional) idea of what you might see?
I'd just like to say Thank you to Tormod for hosting these forums. There's some fascinating topics here. Much food for thought.
Thanks
sundog