Originally posted by chroot
No, sorry, russ is correct.
Well, now, let’s see. Russ said:
“The speed of light is constant. It is always measured by all observers, everywhere, to be C.”
That’s not quite the same as what you said.
You said:
”Every observer who builds an apparatus at rest with respect to him, and allows light to go through it, will always measure the speed of light as c.”
And that’s pretty much what I said earlier:
”So, when local photon speed is measured in a certain gravitational potential by an atomic clock in that same gravitational potential, the speed is measured as being “c”.”
See? You are referring to a “local” observer observing the photons’ speed “locally”, and that is also what I was referring to. I added a specific kind of clock which we can use to time the local speed of the local photons. But Russ’ less specific statement could include “local” observers observing the motion of distant photons moving from one distant place to another.
Originally posted by chroot
If you built an apparatus near the sun, the apparatus would indicate that the light is traveling at c. Light always travels at c locally.
That's what I said, but you've got to specify what type of clock you are using for the measurement, and to get "c", an atomic clock is requried.
Originally posted by chroot
When you say "light slows down near the Sun," you mean that an Earth-bound observer would say it took longer than it would've on Earth. A Sun-bound observer, however, would say it took just as long as it should've.
Right, if both observers are using resting atomic clocks where they are located.
So, Russ’ statement is not quite correct, and it's misleading:
“The speed of light is constant. It is always measured by all observers, everywhere, to be C.”
Because a local observer at the Earth will measure a slowdown in the speed of light as it passes near the sun, so we can’t say “It is always measured by all observers,
everywhere, to be C”, since the Earth observer would tell the sun observer, “The light slowed down when it passed near to you,” while the sun observer would say to the Earth observer, “It traveled at ‘c’ when it passed me, but now it’s on the way to you traveling faster than ‘c’, relative to me.”