tashja
Registered Senior Member
QuarkHead, you've got mail:
QuarkHead: Assume a light-emitting celestial body - a star. Assume further that light is emitted from this body in all directions.
Disregarding atmospheric scattering, I observe my star to be discrete - i.e. not "fuzzy" at the perimeter (is this true? If so why? I believe that R. Feynman has an answer, related to why light appears to always travels in straight line)
If it is, this seems to suggest to me that the only light from this star that I see consists on "more-or-less" parallel photon beams.
Question: If these parallel photon beams interact via self-gravity, is my image of the diameter of a star at, say, 1 million light years distance, and assuming I can calculate the "image shrinking" over this sort of distance, different from the "true" diameter of the star?
Granted that this "true diameter" may not be possible to determine, do astrophysicists take this into account when making such measurements?
Prof. Jensen:
Yes, for all practical purposes, star light reaches us in parallel beams. Even solar radiation is almost parallel; it is how Eratosthenes measured the radius of the Earth in 240 BC. But the light is only parallel to an approximation. So you should get some aberration due to gravitational effects but I think it should be negligible. The farther the star is, the more time is allowed for gravitation to take effect between the approximately parallel photons, but at the same time the photons become more sparse and this tends to cancel out the effect. It would seem their escape velocity from one another is negligible compared to their relative velocity, no matter the angle.
Ray