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Originally posted by mb2591
reply to post by ErtaiNaGia
Why's it gotta be dark...racist
On a more serious note.. I'm not quite sure what your question isedit on 5-7-2011 by mb2591 because: (no reason given)
On a more serious note.. I'm not quite sure what your question is
Originally posted by ErtaiNaGia
Bueler?edit on 5-7-2011 by ErtaiNaGia because: smaller picture
The kind of lensing you're talking about, no, it hasn't been factored into distance and mass calculations.
Astrophysicists know about gravitational lensing, but it's only considering significant around black holes.
To introduce a second source of lensing would require a revision of all accepted masses and distances.
Though, if such lensing does exist, then it's a revision that must be done.
You're also not the only one here with this idea. I think it's XPLodER who has a similar lensing theory. And, personally, I like the idea.
Originally posted by Phage
Gravitational lensing occurs when light which originated beyond a massive object (galaxy, cluster, etc.) passes that object. Light from the galaxy itself is not "bent".
minerva.union.edu...
The effects are readily apparent, producing distorted and multiple images of the galaxy from which the light is being lensed.
www.sciencedaily.com...
edit on 7/5/2011 by Phage because: (no reason given)
It's pretty arrogant of us to think that we've "seen it all". 99.9% of what we "know" about our Universe is based on extrapolation of information that we have observed directly. Considering we are missing about 96% of the matter out there, I'd say those extrapolations are simply way off base.
No such thing as dark matter.
I posted it to show that the effects of gravitational lensing are well understood and unless every galaxy observed is to be precisely located "behind" a large mass in order to produce an "enlarged" image, their sizes are not being incorrectly calculated.
Originally posted by Phage
The Sun has far too little mass to produce such an effect
but as I pointed out, only the light passing directly by the Sun (or other massive object) on its way to Earth is affected perceptibly.
Only galaxies on the dayside of Earth would have any chance of being affected and only when they were directly opposite the Sun.
If this were not the case all of the stars in the sky would be "displaced" by the Sun's gravity, depending on the season.
What if there was some sort of "Lensing" effect around massive objects like stars... maybe caused by "Gravity" that bent light towards the center of the star system?
Now, keep in mind, our knowledge of galactic mass, is based on our estimations of stellar masses, and our observation of their average separation distance.
So, what if the galaxy is actually more dense than we have observed it to be?
What if there was some sort of "Lensing" effect around massive objects like stars... maybe caused by "Gravity" that bent light towards the center of the star system?
But, I believe that this is actually a fairly solid hypothesis that could account for the "Missing Mass" of the galaxy... that being our incorrect calculations of the density of the galaxy, by seeing stars and such as farther away than they actually are.
I don’t think a galaxy can cause a gravitational lensing effect on its own light.
This only works from the point of the gravitational lensing effect and beyond. It has nothing to do with the distance of the object to our Sun.
This means that the further an object is from the sun, the more important the gravitational lensing effect will be, until you get objects that are SO distant, that the gravitational lensing effect is constituting the BULK of the parallax angle measurement.
Gravity follows the inverse square law. It is effected by the mass of an object and the distance between two masses. Figure out the radius of our Sun and its gravitational force and inversely square that force by the distance to Earth. This, I think, will show an insignificant amount of force to create a gravitational lensing effect as seen from Earth in the night sky (looking away from the Sun).
you are assuming that gravity has a definite cut off distance to interact with light, and this is not the case.
Originally posted by ErtaiNaGia
So, I plugged this one into Google's handy dandy calculator equation, and I got this:
0.0000000394671664 degrees, which is 0.000142081799 arc seconds
I say this because a parsec (astronomical unit of measurement) is the parallax of one arc second.
Now, the difference that this could make, would not seem like much, but it actually would be quite huge....
Because the parallax of one arc second, is a measurement of some 4.3 light years.
So, being off by one ten-thousandth, would put your star several solar radii distance closer than you originally calculated.
And when you get into measurements of Kiloparsecs, Megaparsecs, and such, this can REALLY add up