Calculating The Event Horizon of a Supermassive Black Hole

In summary, The diameter of the largest black hole, with a mass equivalent to 100 billion galaxies, each with an average of 200 billion solar masses, can be calculated using the formula 2GM/c^2. This results in a diameter of approximately 3*10^25 meters or 1.1*10^27 inches. This calculation can be easily done using Google's calculator.
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Ok, let's say we wanted to know the diameter of the largest black hole. (Its event horizon) Let's say the universe had contracted and all the galaxies had been consumed by black holes and all merged into one single massive hole.

Say there were approximately 100 billion galaxies, all relatively the same size, and each had an average of 200 billion solar masses. 1 solar mass = 1.9891 × 10^30 kilograms

I believe the formula to calculate the radius of the event horizon is 2GM/c^2

Not being very good with math, perhaps someone would be able to calculate this? Thanks in advance…
 
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  • #2
I don't know much about black holes, but that equation you gave can be determined by knowing the mass of the black hole, since G and c are both constants. That bothers me a little, that you can calculate length from mass.
 
  • #3
Welcome to the wonderful world of geometric units, where time, length, mass, and even charge can all be expessed in terms of the same unit - usually, cm.

G/c^2 is the conversion between mass and distance, this is most convenient in a unit system where G=c=1 :smile:

The answer to the specific question asked previously is most easily found with Google's calculator. Just go to http://www.google.com and type in

G*(100*10^9*200*10^9*2*10^30 kg)/c^2

and the answer pops out, 3*10^25 meters

If you want that in inches, you can say "in inches" at the end, and it will convert the answer to inches (1.1*10^27 inches).

The "more about calculator" link gives more info on the calculator, if you type in any recognized mathematical expression (the above, or if you're having trouble, type in a simple mathematical expression, 2+2 will do it).
 

1. What is the event horizon of a supermassive black hole?

The event horizon of a supermassive black hole is the point of no return for anything that enters it. This is the boundary at which the gravitational pull of the black hole becomes so strong that not even light can escape.

2. How is the event horizon of a supermassive black hole calculated?

The event horizon of a supermassive black hole is calculated using the Schwarzschild radius formula, which takes into account the mass of the black hole and the speed of light. The equation is: Rs = 2GM/c2, where Rs is the Schwarzschild radius, G is the gravitational constant, M is the mass of the black hole, and c is the speed of light.

3. What factors can affect the size of the event horizon of a supermassive black hole?

The size of the event horizon of a supermassive black hole is primarily determined by its mass. The greater the mass, the larger the event horizon. Other factors that can affect the size of the event horizon include the rotation of the black hole and the presence of other nearby objects that may influence its gravitational pull.

4. Can the event horizon of a supermassive black hole change over time?

Yes, the event horizon of a supermassive black hole can change over time as the black hole gains or loses mass. If the black hole gains mass through accretion of matter, its event horizon will increase. Conversely, if the black hole loses mass through the emission of Hawking radiation, its event horizon will decrease.

5. Why is calculating the event horizon of a supermassive black hole important?

Calculating the event horizon of a supermassive black hole is important for understanding the properties and behavior of these extreme objects. It can also help in predicting the effects of a black hole on its surroundings, such as the influence on nearby stars and gas clouds. Additionally, knowing the size of the event horizon can provide insights into the evolution and growth of black holes over time.

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