I Visible light Over Large Distances

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Visible light Over Large Distances
How does light maintain enough energy in the visible part of the spectrum for the naked eye to see in the night sky. Also, how did it start of in the visible frequency part of the spectrum. Was it, for example, photons being ejected at that frequency after high energy particle interaction. Or does the light become visible (spectrum) after hitting our atmosphere or space dust or something?

EDIT: Actually I just thought. Maybe the EM starts off as very high energy (outside the visible spectrum) But then over distance it loses energy and then becomes visisble as it's frequency reduces. Can anyone confirm
 
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Light from stars is emitted as visible light and reaches us as visible light (ditto the other frequencies stars emit). No energy is lost on the way except if there are dust clouds or other stuff in the way that absorbs light, but that doesn't change light into microwaves or something - it mostly just makes it dimmer.

Light from distant galaxies is redshifted in flight, but only really sensitive telescopes can see those.
 
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Ibix said:
Light from stars is emitted as visible light and reaches us as visible light (ditto the other frequencies stars emit). No energy is lost on the way except if there are dust clouds or other stuff in the way that absorbs light, but that doesn't change light into microwaves or something - it mostly just makes it dimmer.

Light from distant galaxies is redshifted in flight, but only really sensitive telescopes can see those.
Thanks.
So I guess also that light emitted in the non visible (higher frequencies) could interact with, say, dust clouds (as you mention) and then continue their journey to the naked eye in the visible spectrum having been absorbed (lost some energy) and re-emitted as visible?
 
RobbyQ said:
So I guess also that light emitted in the non visible (higher frequencies) could interact with, say, dust clouds (as you mention) and then continue their journey to the naked eye in the visible spectrum having been absorbed (lost some energy) and re-emitted as visible?
Mostly it's just dimmer, not at different frequencies. There are absorption and re-emission processes, which is why things like nebulae glow at all, but if you're looking at a star (even through a dust cloud) then you're seeing the spectrum the star emits, not some shifted version of it.
 
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Is a homemade radio telescope realistic? There seems to be a confluence of multiple technologies that makes the situation better than when I was a wee lad: software-defined radio (SDR), the easy availability of satellite dishes, surveillance drives, and fast CPUs. Let's take a step back - it is trivial to see the sun in radio. An old analog TV, a set of "rabbit ears" antenna, and you're good to go. Point the antenna at the sun (i.e. the ears are perpendicular to it) and there is...
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