🚀 go-pugleaf

"Pentcho Valev" <pvalev@yahoo.com> wrote in message 
news:2cb3c011-b9c9-4d76-997d-2ef54a62a5c8@d10g2000yqh.googlegroups.com...
> http://www.pitt.edu/~jdnorton/teaching/HPS_0410/chapters/big_bang/index.html
> John Norton: "Here's a light wave and an observer. If the observer
> were to hurry towards the source of the light, the observer would now
> pass wavecrests more frequently than the resting observer. That would
> mean that moving observer would find the frequency of the light to
> have increased (AND CORRESPONDINGLY FOR THE WAVELENGTH - THE DISTANCE
> BETWEEN CRESTS - TO HAVE DECREASED)."
>

====================

  The source is observed to be 200 light seconds out and away from the 
observer (0) before the observer's "hurry towards the source of the 
light..." The observer hurries toward the source and observes the source to 
be 190, 180........., 100........., 50........, 10, 9, 8....., 4, 3, 2 light 
seconds out and away from him until the attainment of 0 (until 0 = 0). From 
the source's history observed -200 seconds relative to the observer (0), the 
observer observes for the source -- during his hurry toward the source -- a 
progressive RUSH forward in history from the source's past observed (to mean 
a RUSH forward in space and time, that is) to -190 seconds relative..., -180 
seconds relative..., -100 seconds relative..., -50 seconds relative..., -10 
sec..., -9 sec..., -8 sec..., -4 sec..., -3 sec..., -2 seconds relative to 
himself until the attainment of 0 (until 0 = 0). The traveling observer 
contracted, then expanded, space-time in RUSHING from the observed 
historical past of the source (-200 seconds to the observer's 0) to the 
distantly unobserved present of the source (0) (0 = 0) via observably 
speeding up through an intervening future of the source (-200 seconds to 0 
(the universe horizon to be observed directly-in-line beyond the source's 
horizon of -200 seconds to 0 being -13.7 billion years to 0. The traveling 
observer's point of original departure is now an horizon -200 seconds to 
0...with the universe horizon still to be observed -13.7 billion years to 0 
directly-in-line beyond that point's now historical horizon of -200 seconds 
to 0....or it observably being 200 light seconds of distance from the 
observer (0) (from 0 to -- observably -- 200 light seconds in distance) 
(from 0 to -- observably -- minus 200 seconds into the past relative to the 
observer (0)))).

Light>>>>>>>>>>>>>>>
     ()<------traveler-----()
<<<<<<<<<<<<<<<Light

Light<><><><><><>Light
------t-t-t-t-t-t-t-t-t-t------

---------------------

(()-0-1-2-3-4-5-6>())
(()<----traveler-----())
(()<6-5-4-3-2-1-0-())

---------------------

(observable universe horizon)
 ***
   ||

() < * (() = destination point)
0 ^ 6 (^ < = hurrying observer))
1 ^ 5
2 ^ 4
3 ^ 3
4 ^ 2
5 ^ 1
6 ^ 0  (< ^ = hurrying observer)
* < () (() = departure point)

   ||

 ***
(observable universe horizon)

---------------------

GLB

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