The mathematical expression for the gravitational Gauss law is: gdA -4Gm, where g is the gravitational field, dA is the area element, G is the gravitational constant, and m is the mass enclosed by the surface.
This law is used to calculate the gravitational field around a massive object by integrating the gravitational field over a closed surface surrounding the object. The result of the integration gives the total gravitational flux through the surface, which is related to the mass enclosed by the surface.
The more massive the objects, the greater the gravitational force between them. The gravitational force is affected by mass and distance. The closer two bodies are, the greater the gravitational force also.
Gravitational force depends on mass, so larger objects like planets and stars have a stronger gravitational pull. This is why we tend to notice the gravitational force of massive objects more, as their effects are more pronounced on smaller objects like us on Earth.
No, they don't. They "curve" around massive objects, but this is a function of the photon following the "bend" in spacetime that objects with massive gravity create. Photons have a mass equal to zero.
If the product of the two masses increases, then the gravitational force in both directions between them increases.
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.
The more massive the objects, the greater the gravitational force between them. The gravitational force is affected by mass and distance. The closer two bodies are, the greater the gravitational force also.
The space surrounding a massive object subject to the body's force of attraction is the gravitational field. This field is responsible for exerting a force on any other object within its influence, causing it to experience gravitational acceleration towards the massive object.
no
Gravitational force depends on mass, so larger objects like planets and stars have a stronger gravitational pull. This is why we tend to notice the gravitational force of massive objects more, as their effects are more pronounced on smaller objects like us on Earth.
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Gravitational waves are created when massive objects accelerate, such as when two black holes merge or when a massive star explodes in a supernova. As these objects move, they cause ripples in the fabric of spacetime, which propagate outward as gravitational waves at the speed of light. Detection of gravitational waves provides valuable insights into the behavior and interactions of massive objects in the universe.
Everywhere in the universe. Gravitational fields are steeper and more intense around very massive objects such as stars and planets.
Gravitational lensing is the bending of light around a massive object due to gravity.
On Earth, not much ; it is pretty far away, and not very massive.
Jupiter is the largest and most massive planet.
No, they don't. They "curve" around massive objects, but this is a function of the photon following the "bend" in spacetime that objects with massive gravity create. Photons have a mass equal to zero.
black hole