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originally posted by: teamcommander
a reply to: JadeStar
I really appreciate your reply. It is always pleasing to have someone with a grasp of the subject respond.
I will say, I would suppose you'll agree, that the 10 parsecs (33.6 light years) from our sun looks like a short strol compared to the vast distances shown in the picture.
originally posted by: Aleister
a reply to: JadeStar
I for two must say how much I've missed your posts and threads lately. Said it before before I say it again, ATS is lucky to have you wandering the halls.
originally posted by: JadeStar
originally posted by: Snarl
originally posted by: teamcommander
originally posted by: Snarl
a reply to: teamcommander
I wonder what that picture will look like taken a hundred years from now.
A hundred years is less than the blink of an eye in real universal time.
The perspective won't even change very much by then.
I'd wager the resolution improves by a factor of a thousand. I'd wager we'd be seeing objects well beyond the accepted 13.8B LY limit.
Not really. At least not with a visible/near-IR telescope like Hubble.
Due to the redshift, they'd have to keep looking at lower and lower wavelengths of light, deep into the infrared, then millimeter radiation before ending up in radio.
See Cosmic Microwave Background Radiation.
originally posted by: Snarl
originally posted by: JadeStar
originally posted by: Snarl
originally posted by: teamcommander
originally posted by: Snarl
a reply to: teamcommander
I wonder what that picture will look like taken a hundred years from now.
A hundred years is less than the blink of an eye in real universal time.
The perspective won't even change very much by then.
I'd wager the resolution improves by a factor of a thousand. I'd wager we'd be seeing objects well beyond the accepted 13.8B LY limit.
Not really. At least not with a visible/near-IR telescope like Hubble.
Due to the redshift, they'd have to keep looking at lower and lower wavelengths of light, deep into the infrared, then millimeter radiation before ending up in radio.
See Cosmic Microwave Background Radiation.
Ooh, I don't know. There's something else out there and all around us. Measurements of what can be seen and what can be detected with current technologies aren't filling out the equation. Think DM and DE. What'll happen when we can 'see' them?
We've extended our abilities of perception farther than anyone would have anticipated 200 years ago. The Hubble deep field image surprised a lot of folks in your field too, didn't it?
Good to see you back and active on the boards.