Light, though it travels in a straight line in a vacuum, must follow any curves in spacetime. Recall that the volume of the universe is called spacetime, and spacetime itself is distorted or "bent" by gravity. Light, though it travels in a straight line in a vacuum, will follow any gravity-induced curves in spacetime. An example might be the deformation of spacetime around a black hole, and the resultant gravitational lensing that can occur because of it.
Light particles (photons) have no rest mass. They have an equivalent mass worked out using any of several equations or combinations
m = E/c2 or E=mc2
and since E = fxh
m = fh/c 2
m = h/Lc or L=h/mc (de Broglie wavelength for light)
where m is the mass, E is the energy of the photon, c is the speed of light in a vacuum, f is the frequency, h is Plank's constant (6.626 x 10-34 joules/sec) and L is the wavelength (usually greek lambda).
Under relativity theory, it's not strictly required for photons to have mass in order to be affected by a gravitational field. Space itself is bent by gravity, and light takes the straightest possible path through bent spacetime.
Gravitational lensing does not depend on a the state of matter of light, rather it is an expression of the geometric curvature of space/time due to mass.
Dark matter may be invisible to light, but it can still be detected, through its gravitational interactions. Specifically, it can be detected: * By the fact that galaxies rotate way too fast, for the amount of known matter. * By gravitational lensing.
Einstein's cross is located about 8 billion light-years away from Earth. It is a gravitational lensing phenomenon where the light from a distant quasar is bent by the gravitational field of a foreground galaxy, creating multiple images of the quasar.
Its real (absolute) magnitude; its distance from Earth; the amount of light that's absorbed by matter between the star and us (extinction); distortions due to gravitational lensing.
Einstein says that he could prove the effect of gravitational lensing by looking at the moon during a solar eclipse and you will see stars behind the sun. Im not sure of the formula.
Gravitational lensing does not depend on a the state of matter of light, rather it is an expression of the geometric curvature of space/time due to mass.
Gravitational lensing
Gravitational lensing is a phenomenon where light from a distant object is bent and distorted by the gravitational field of a massive object, such as a galaxy or a cluster of galaxies, that lies in between the distant object and the observer. This bending of light can create multiple images of the distant object, distort its appearance, or even magnify it. Gravitational lensing is a powerful tool for studying the distribution of dark matter in the universe and for discovering distant galaxies and objects.
Yes. It is an adjective meaning "of, relating to, or involving gravitation." It is used terms such as "gravitational acceleration" and "gravitational lensing."
Gravitational lensing is the bending of light around a massive object due to gravity.
Dark matter is estimated to be responsible for about 27% of the total mass-energy in the universe (normal matter is a bit under 5%)."Gravity-lensing" is essentially a meaningless phrase here; all mass causes gravitational lensing, so there's no such thing as "non-gravity-lensing" dark matter.
Gravitational lensing.
The gravitational effects. For example, gravitational lensing; also, galaxies spin way too fast for the amount of known matter.
Christopher R. Burns has written: 'Gravitational lensing of polarized sources'
Gravitational lensing can create multiple images due to the bending of light rays around a massive object, like a galaxy or galaxy cluster. The light from the source gets bent at different angles, leading to multiple paths the light can take towards the observer. This results in multiple images of the same object being seen from different angles.
Gravitational lensing occurs when the gravity of massive objects, like dark matter, bends and distorts light from distant sources. By studying these lensing effects, scientists can map the distribution of dark matter in the universe. This helps us understand the role of dark matter in shaping the large-scale structure of the cosmos.
Yes. Lensing magnifies the image of galaxies behind distant galaxy clusters but also greatly distorts the image.