Gravitational Lensing: Exploring Light in Space

In summary, gravitational lensing occurs when an object with mass causes space to bend, leading to distorted images of objects behind it. The strength of the gravitational pull is represented by the lines in the image, which cause light to bend as it passes by the object. The light is bent more strongly where the lines are bent more, creating a curved path. The net effect is that the light enters at a 90 degree angle and exits at a lesser angle, resulting in a curved trajectory.
  • #1
shadytriba
2
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Hi Everyone,

This is my very first post here.. :)

My question is regarding the gravitational lensing.. i understand that any object with mass in space causes the space to bend more like in the image here.. so imaginig a star behind the planet how would the light of it form gravitational lensing because the space around the planet is not bulging out but instead bulging inside...
 

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  • #2
Light that would have passed by the planet, and the observer in the shadow of the planet, is pulled inward towards the planet. If the gravitational pull is strong enough the path of the light is changed enough for it to be seen by the observer behind the planet, and it then forms an image. (Usually heavily distorted however)

The lines on your image simply represent the strength of the gravitational pull. As the lines approach the planet they are bent further and further from their straight paths by gravity. As they recede gravity is reduced and the lines go back to their straight paths. The lines DO NOT represent something passing by such as light. Light will not bend inwards and then come back out. Imagine a beam of light traveling parallel to one of the top lines. The further the line is bent inward, the greater the strength of gravity is, so the more the path of the light is bent. The greatest bending will occur when the light is at its closest approach to the planet, where the pull is strongest, which is represented by the lines being bent towards the planet the most.

Does that make sense?
 
  • #3
so what you are trying to say is that the bending of light is opposite to those gravity liness... iam i right?
 
  • #4
shadytriba said:
so what you are trying to say is that the bending of light is opposite to those gravity liness... iam i right?

No, the light is bent more strongly where the lines are bent more. When the lines recede from the planet and straighten back out the light is bent less while traveling through that area. If we were to exaggerate this, you would draw a light beam initially parallel to the top line, and as it approached the planet it would start to bend inwards towards it, similar to the line. But, as the line starts to straighten back out, the light beam DOES NOT. It is still bending towards the planet, but less and less at it moves away. The net effect is the light enters from the left side at a 90 degree angle from the edge, bends, and leaves the right side at an angle LESS than 90 degrees from the right edge. So it isn't a straight beam of light, it's a curve.
 
  • #5


Hello there!

Gravitational lensing is a fascinating phenomenon that occurs when the path of light from a distant object is bent by the gravitational pull of a massive object, such as a planet or galaxy. This bending of light can create distorted or magnified images of the distant object, allowing us to study it in more detail than would otherwise be possible.

In the scenario you described, with a star behind a planet, the light from the star would indeed be bent by the planet's gravitational field. The space around the planet is not bulging out, but rather it is the curvature of space itself that causes the bending of light. This is due to Einstein's theory of general relativity, which states that mass and energy can warp the fabric of space-time.

The amount of bending in the light's path depends on the mass and distance of the object causing the gravitational lensing effect. In the case of a planet, the effect would be relatively small compared to a massive galaxy. However, with advanced telescopes and techniques, scientists are able to detect and study even the subtlest effects of gravitational lensing.

Gravitational lensing has been a valuable tool in studying the universe and has helped us to discover and understand many distant objects, such as exoplanets, galaxies, and even dark matter. It also has practical applications, such as in the study of gravitational waves and in the search for distant supernovae.

I hope this helps to answer your question. Let's continue to explore the wonders of gravitational lensing and the mysteries of space together!
 

Related to Gravitational Lensing: Exploring Light in Space

What is gravitational lensing?

Gravitational lensing is a phenomenon in which the gravitational field of a massive object, such as a galaxy or a cluster of galaxies, bends the path of light from a distant object. This can result in the appearance of multiple images or distorted images of the distant object.

How does gravitational lensing occur?

Gravitational lensing occurs because of Einstein's theory of general relativity, which states that massive objects can bend the fabric of space-time. When light travels through this curved space-time, its path becomes bent, just like a ball rolling on a curved surface.

What can we learn from studying gravitational lensing?

Studying gravitational lensing can provide valuable insight into the distribution of mass in the universe. By observing how light is bent and distorted by massive objects, scientists can map out the location of dark matter, which makes up a significant portion of the mass in the universe.

What is the difference between strong and weak gravitational lensing?

Strong gravitational lensing occurs when the mass of the foreground object is strong enough to produce clearly visible multiple images of the background object. Weak gravitational lensing, on the other hand, occurs when the bending of light is subtle and produces only slight distortions in the image of the background object.

How is gravitational lensing used to discover new objects in space?

Gravitational lensing can magnify and amplify the light from distant objects, making them easier to detect and study. By looking for distortions in the light from background objects, scientists can identify and study new objects, such as distant galaxies or stars, that would otherwise be too faint to observe directly.

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