High School Gravitational Lensing: Magnification of Galaxies

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The discussion on gravitational lensing highlights the complexity of magnifying galaxies, particularly those the size of the Milky Way. It emphasizes that the effectiveness of a galaxy as a lens depends on its mass and the distance of the light source, rather than just its size. Light bending around such galaxies can lead to multiple distorted images rather than a single magnified view. The conversation references Hartle's work on light deflection, noting that calculations for the Milky Way would require advanced modeling due to its irregular shape. Overall, the topic reveals that there is no straightforward answer to the magnification of galaxies.
Mikael17
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How many time does a galaxy (same size as our milkyway) magnified the background ?
How many time does a galaxy (same size as our milkyway) magnified the background ?
 
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Um...once?

This is impossible to answer. "How strong is a glass lens"?
 
It doesn't magnify at all, because it's an absolutely terrible lens. It's not even circularly symmetric, so you usually get up to four distorted and displaced copies of whatever is in the background.
 
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OK, how much would light then bend , when passing nearby a milkyway size galaxy ?
 
Depends how far away the light is and it depends how massive the galaxy is more than its size. There isn't really a single answer to this question.

Why are you asking? Perhaps if you have a less general question we can be more helpful.
 
Mikael17 said:
OK, how much would light then bend , when passing nearby a milkyway size galaxy ?
In Hartle's Introduction to General Relativity, he studies the deflection of light for a spherical mass in chapter 9. The estimate is ##1.7## seconds of arc for a light ray grazing the Sun. There would be less deflection for a light ray further from the Sun. In other words, it depends on the mass of the Sun and the impact parameter.

The calculation for the Milky Way would be considerably more complex, as it is not a neat spherical mass. A good project for a computer model, perhaps.
 
MOVING CLOCKS In this section, we show that clocks moving at high speeds run slowly. We construct a clock, called a light clock, using a stick of proper lenght ##L_0##, and two mirrors. The two mirrors face each other, and a pulse of light bounces back and forth betweem them. Each time the light pulse strikes one of the mirrors, say the lower mirror, the clock is said to tick. Between successive ticks the light pulse travels a distance ##2L_0## in the proper reference of frame of the clock...

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