Mass of the Moon and Gravitational Lensing

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Discussion Overview

The discussion revolves around the effects of gravitational lensing during a solar eclipse, specifically regarding the Moon's mass and its ability to obscure the Sun. Participants explore the implications of lensing on the apparent sizes of celestial bodies and the visibility of light during eclipses.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants question whether the Moon's mass is sufficient to cause noticeable gravitational lensing during an eclipse, suggesting that light from the Sun should still be detectable.
  • Others argue that the effect of lensing is negligible and would consistently make the Moon's apparent angular diameter smaller, not just during eclipses.
  • A participant suggests that the lensing effect should be compared to the Moon's varying angular size due to its elliptical orbit.
  • Some participants express confusion about the relationship between lensing and the angular resolution of telescopes, questioning the relevance of high definition computers in this context.
  • There is a discussion about whether gravitational lensing affects the apparent size of the Sun or the Moon, with differing views on how lensing operates in this scenario.
  • One participant proposes the term "effective angular diameter" to describe how lensing might alter the perception of the Moon's obscuration of light from behind it.

Areas of Agreement / Disagreement

Participants exhibit multiple competing views regarding the effects of gravitational lensing during eclipses, and the discussion remains unresolved with no consensus reached on the implications of lensing on the apparent sizes of the Moon and the Sun.

Contextual Notes

Some participants highlight the need for clarity on the definitions of angular diameter and effective angular diameter, as well as the conditions under which gravitational lensing would be relevant during an eclipse.

Helena Wells
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During an eclipse the Moon covers the Sun.However this shouldn't be happening due to gravitational lensing we should be able to see some light?

Is the mass of the Moon not big enough or photons do reach us but they are so little our eyes can't detect them?
 
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A. Lensing is negligible.
B. The effect of lensing would be to make the moon's apparent angular diameter smaller all the time, not just during eclipses.
C. You would have total and annular eclipses. Just like we do now.
 
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I just told you the formula for the angular deflection of light in the Elon Musk thread! Plug the numbers in and see how much angular deflection you get.
 
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And after plugging in the numbers for the lensing then compare that to the difference in angular size depending on orbital distance to the moon.
 
A high definition computer would be able to understand the difference?
 
What is a " high definition computer"? And what "difference"? The effect of lensing would be to make the moon's apparent angular diameter smaller all the time, not just during eclipses.
 
Helena Wells said:
A high definition computer would be able to understand the difference?
Never anthropomorphize high definition computers. They hate it when you do that. :wink:
 
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Vanadium 50 said:
The effect of lensing would be to make the moon's apparent angular diameter smaller all the time, not just during eclipses.
I think the point he's hoping to make is that it is only during an eclipse that the small amount would make an obvious difference - because of the sun.

But no. Even if it were a non-negligible amount of lensing, the Moon's elliptical orbit means its apparent size changes noticeably from eclipse to eclipse anyway. So you'd get Vanadium's total and annular eclipses anyway.
 
Helena Wells said:
A high definition computer would be able to understand the difference?
Why would a computer have anything to do with the angular resolution of a telescope? Unless you've got one of those magic CSI computers that can zoom-and-enhance and read a license plate from a single pixel reflection in somebody's eyeball?
 
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  • #10
Helena Wells said:
Is the mass of the Moon not big enough or photons do reach us but they are so little our eyes can't detect them?

Neither. During a total solar eclipse the angular size of the Moon is enough larger than the angular size of the Sun that the miniscule gravitational lensing effect of the Moon is not enough to bend any of the Sun's light sufficiently for us to see it.
 
  • #11
Back to the question at hand for a second. I need a little help. I know these are small effects
Vanadium 50 said:
B. The effect of lensing would be to make the moon's apparent angular diameter smaller all the time, not just during eclipses.

It is hard for me to understand that the lensing effect would be the same (or similar) for light from behind being occluded and light being emitted (or reflected).
So the sun (assuming it has a sharp limb) actually looks smaller than its size because of gravity acting on light?
 
  • #12
Vanadium 50 said:
B. The effect of lensing would be to make the moon's apparent angular diameter smaller all the time, not just during eclipses.

I don't think this is correct. Gravitational lensing refers to an object bending light coming from objects behind it. The Moon's apparent angular diameter normally is determined by light reflected from the Sun off the Moon (or from the Earth off the Moon, if you are seeing "the old moon in the new moon's arms"), not by light coming from behind the Moon. Only during an eclipse is there a light source right behind the Moon such that lensing by the Moon could affect the Moon's apparent angular diameter.
 
  • #13
Vanadium 50 said:
The effect of lensing would be to make the moon's apparent angular diameter smaller

Also, the effect of lensing by object A of light coming from object B, behind object A, is not to make object A's apparent angular diameter smaller; it's to make object B's apparent angular diameter larger.
 
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  • #14
Maybe I should have said "effective angular diameter". If lensing moves the direction of light from an object behind the moon so that it is no longer obstructed, that means the moon obscures less of it, i.e. the effective angular diameter is less.
 
  • #15
Vanadium 50 said:
If lensing moves the direction of light from an object behind the moon so that it is no longer obstructed, that means the moon obscures less of it, i.e. the effective angular diameter is less.

I see what you mean; I think a simpler and more intuitive way to describe it is that it makes the apparent angular diameter of the object behind the moon larger.
 
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