Alight Motion: Black Hole v2 ⚫ Animation ✨ & VFX PART 1 ✨ - by Priyam Kashyap 🪐
Hello, It's Priyam here, BLACK HOLES are awesome. You can Animate a #blackhole in #AlightMotion in easy-peasy way. Just copy my effect data (or details) of element in yours and you'll see the magic.
⭐ MUST READ THIS ⭐
IN #AlightMotion, I created this #blackhole on the basis of it's Luminosity, Rotational Motion and Heat Radiating Capabilities.
⚠️ I am using #AlightMotion v4.0.3 ⚠️
Can a black hole cause gravitational lensing?
While isolated black holes do not produce detectable emission, their gravity can bend and focus light from background objects. This bending and focusing of light through gravity is known as gravitational lensing.
Do you know?:
• A black hole is called a black hole because of it’s color, especially since light can’t escape. What we can see, though, is the effects of a black hole. Analyzing the surrounding area of a black hole, we can see its effects upon its environment. For example, a star that’s close enough to a black hole can be seen being ripped apart.
• There are four types of black holes: stellar, intermediate, supermassive, and miniature. The most commonly known way a black hole forms is by stellar death. As stars reach the ends of their lives, most will inflate, lose mass, and then cool to form white dwarfs.
🌟 Read about #blackhole : https://en.wikipedia.org/wiki/Black_hole
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Little Details:
A black hole is a region of spacetime where gravity is so strong that nothing – no particles or even electromagnetic radiation such as light – can escape from it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of no escape is called the event horizon. Although it has a great effect on the fate and circumstances of an object crossing it, it has no locally detectable features according to general relativity. In many ways, a black hole acts like an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is of the order of billionths of a kelvin for stellar black holes, making it essentially impossible to observe directly.
Black holes of stellar mass form when massive stars collapse at the end of their life cycle. After a black hole has formed, it can grow by absorbing mass from its surroundings. Supermassive black holes of millions of solar masses (M☉) may form by absorbing other stars and merging with other black holes. There is consensus that supermassive black holes exist in the centres of most galaxies.
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