You must enter the before collision data, such as the mass of the black hole, the radius of the event horizon before the collision, and the details of the hitting object, and then press the calculate button to obtain the after-collision parameters in the blink of an eye.

**Black Hole Collision Calculator:** We hope that by using this calculator, you will learn about the event horizon, what occurs when an item collides with a black hole, and how to compute a black hole's mass from its size. The black hole collision calculator also allows you to generate and experiment with your own black hole collisions. It's astronomically entertaining.

We are sure you've all heard of black holes in some form or another, whether it's in the context of wacky time travel theories or scary space-time manipulation. This may lead you to believe that black holes are strange objects that no one comprehends. Fortunately, reality is not like that.

This event is assumed to represent the most massive stars' final fate (see black hole). The Schwarzschild radius (R_{g}) of a mass M object is calculated using the formula below:

- G is the universal gravitational constant
- c is the speed of light: R
_{g}=2GM/c^{2}.

We must describe what is occurring prior to the collision to continue: a star travelling the Universe, doing its own thing.

We hope you enjoyed all of the preamble, but now it's time to get down to business! You may calculate what occurs when a black hole collides with any other object in the Universe using this black hole collision calculator.

- We can compute what would happen if a black hole collided with any item in the universe using the basic Black Hole Collision Calculator. We need to know the black hole's mass, the mass of the object being eaten, and the radius of the event horizon.
- To find out how much mass the black hole obtained after the collision, the event horizon radius after the collision, the event horizon growth, and the quantity of released energy, enter all of these values in all of the input fields and click the calculate button.

The mass of the object being consumed (M_{falling}) and the mass of the black hole are required to build up the initial conditions of this scenario (M_{black hole}). Because the mass and radius of a black hole are connected, you can also utilise the radius of the event horizon (R_{event horizon}).

Now we're in the following upon the collision, when the object has totally plunged into the black hole and become a part of it. The black hole has developed slightly in this scenario. The black hole's mass is equal to the other object's initial mass minus the mass that was transformed into energy.

There are two sorts of interactions that bring light to the existence of black holes: destructive and non-destructive interactions.

When a star or a relic of a star collapses into a black hole, a massive amount of energy is released into the Universe.

Depending on the parameters of the black hole it falls into, the amount of energy in this flash of light ranges from around 3% to 42% of the mass of the item.

**Specific mass ranges indicated in proportion to our own Sun's mass**

- Super Massive Black Holes: ~1-1000 million M
_{Sun} - Intermediate Black Holes: ~10-1000 M
_{Sun} - Stellar Black Holes: ~1-10 M
_{Sun} - Neutron stars: ~ 1.5 M
_{Sun} - Stars: ~0.5-250 M
_{Sun} - Planets: 0.5 M
_{Sun}

The units utilised are quite unusual because the energies produced in these occurrences are bigger than anything we will ever encounter or can even comprehend in our lifetime. We've made a Bethe (also known as a foe) the default.

You can checkout more concept with physicscalculatorpro.com to get quick answers by using this free tool.

**1. What is the black hole equation?**

This event is assumed to represent the most massive stars' final fate (see black hole). The Schwarzschild radius (R_{g}) of a mass M object is calculated using the formula below.

- Where, G is the universal gravitational constant
- c is the speed of light: 2GM/c
^{2}= R_{g}

**2. What is the definition of a black hole collision?**

Two smaller black holes are embedded in this disc, and they may have merged to generate a new black hole. Gravitational waves are ripples in space and time that can be detected with incredibly sensitive detectors on Earth when two black holes spiral around one other and eventually collide.

**3. What causes a white hole to form?**

When stars far more massive than our Sun perish spectacularly in a supernova, black holes are formed. Astrophysicists generate white holes by analytically exploring the environment surrounding black holes while pretending there is no mass within the event horizon.