The Astonishing Weight of a Soda Can-Sized Black Hole

The Astonishing Weight of a Soda Can-Sized Black Hole

A black hole with the throat-chopping power and gravitational pull of a can of soda might sound like a punchline, but it’s actually a fascinating topic in astrophysics. Let's delve into the calculations and explore how such a hypothetical black hole might compare to the massive cosmic beasts we know.

Dimensions of a Soda Can

The US standard can is a compact yet seemingly ordinary object. With a height of 4.83 inches, and diameters of 2.13 inches at the lid and 2.60 inches at the widest point of the body, let's convert its dimensions into metric units for easier calculation.

Volume of the can (cylinder):

(pi r^2 h pi times 0.05355^2 times 0.122682 0.001147 , text{m}^3)

However, to simplify the calculation, we will assume the can is a sphere for the purposes of the Schwarzschild Radius calculation. The formula for the volume of a sphere is:

(frac{4}{3}pi r^3 0.00042022787 , text{m}^3)

Solving for the radius:

(r left(frac{3V}{4pi}right)^{frac{1}{3}} 0.046 , text{m})

Calculating the Mass of a Soda Can-Sized Black Hole

The Schwarzschild Radius (Rs) is the radius required for a given mass to reach a surface where the escape velocity is the speed of light. The formula is:

(R_s frac{2MG}{c^2})

Where:

(R_s): Schwarzschild Radius (M): Mass in kilograms (G): Gravitational constant ((6.67408 times 10^{-11} , text{m}^3 , text{kg}^{-1} , text{s}^{-2}))) (c): Speed of light ((299792458 , text{m/s}))

To find the mass of an object with a Schwarzschild Radius of 0.046 meters:

(M frac{R_s c^2}{2G} frac{0.046 times (299792458)^2}{2 times 6.67408 times 10^{-11}} 3.097 times 10^{25} , text{kg})

Understanding the Results

This calculation shows that a black hole the size of a soda can would weigh an astonishing (3.097 times 10^{25} , text{kg}). To put this into perspective, this mass is approximately 3.29 times the mass of the Moon, which has a mass of about (7.34 times 10^{22} , text{kg}).

Black holes, contrary to their soda can counterpart, are massive cosmic phenomena. They can contain masses in the order of billions of solar masses and are characterized by their immense size and gravitational pull, often stretching entire solar systems into their grasp.

Black Holes: Not Just Soda Can-Sized

Black holes, as a rule, are not soda can-sized. They range from the extremely small Planck black holes, estimated to be around a few millimeters in diameter, to supermassive black holes found at the centers of galaxies, which can be billions of times the mass of the Sun.

However, even the theoretical concept of a tiny black hole demonstrates the unimaginable power concentrated in such a small space. For instance, a solar mass black hole, equivalent to our Sun, would have a Schwarzschild radius of approximately 3 kilometers.

The concept of a soda can-sized black hole challenges our understanding of these cosmic entities and underscores the incredible variation in black hole sizes. It also highlights the immense computational power and mathematical sophistication required to understand and predict their behavior.

Conclusion

While the idea of a soda can-sized black hole is more of a theoretical curiosity than a practical one, it provides a fascinating perspective on the scale and power of these cosmic phenomena. The calculations reveal the mind-bending density of such objects, which essentially cause time to slow down and space to curve in ways we cannot fully comprehend.

Key Takeaways

Schwarzschild Radius: The radius required for a black hole to achieve the escape velocity of light. Gravitational Constant (G): A crucial factor in determining the mass of a black hole. Mass of a Soda Can-Sized Black Hole: Approximately (3.097 times 10^{25} , text{kg}).

References

[1] Schwarzschild, K. (1916). "über das Gravitationsfeld eines Maschenk?rpers nach der Einsteinschen Theorie". Sitzungsberichte der K?niglich Preussischen Akademie der Wissenschaften. [2] Einstein, A. (1916). "Die grundlage der allgemeinen relativit?tstheorie". Annalen der Physik.