The Kármán Line: The Theoretical Boundary Between Earth and Space

Do you ever wonder where Earth's atmosphere ends and outer space begins? One of the concepts that sought to answer this question is the Kármán Line, often referenced as the boundary between our planet's atmosphere and the dark void of space.

The Kármán Line lives 100 kilometers (62 miles) above the Earth's surface, a whopping 330,000 feet. But why is it termed a 'theoretical' boundary? What thought process derives its particular height above the surface?

Earth from space. The sun shines on the planetary horizon.
 

Newton's Thought Experiment

In the 17th century, long before the Kármán Line was ever conceived, Sir Isaac Newton presented a fascinating thought experiment. He imagined a mountain reaching high above the Earth's atmosphere with a cannon resting at its peak.

Newton declared that if you fired the cannon, the cannonball would travel some distance before being pulled back to Earth by gravity. With every consecutive cannon ball fired, the cannon shoots faster and farther than before. As the cannonball's speed increases, a point is reached where the cannonball never lands.

A surreal world inside of Newton's mind. A world with three cannonballs, each faster than the last. The final cannonball reaches orbital velocity.

Instead, it perpetually descends towards Earth, but Earth's curvature pulls away just as fast. This doesn't mean the cannonball is beyond Earth's gravity; it's continually in freefall, maintaining a circular path around the Earth due to its momentum.

This conceptual scenario illustrates the concept of an object in orbit, precisely how today's satellites maintain their positions in space.

Enter Theodore von Kármán

Fast forward to the 20th century. In 1956, a Hungarian-American aerospace engineer named Theodore von Kármán, entertained by Newton's thought experiment, looked closer into the concept.

Scientists study the world as it is, engineers create the world that never has been.
— Theodore von Kármán

Von Kármán started to calculate at what altitude the atmosphere becomes too thin to support aeronautical flight because there wouldn't be enough air molecules to generate lift on a traditional aircraft's wings.

He determined that by around 100 kilometers (or roughly 62 miles) above Earth, the required velocity to achieve aerodynamic lift would equal the velocity needed for a theoretical orbital motion around the Earth without any lift. At this height, aerodynamics becomes irrelevant, and the realm of spaceflight and astrodynamics begins.

Given his significant contributions, the boundary line at 100 kilometers was named in his honor.

Why 'Theoretical'?

It's termed 'theoretical' because the Kármán Line isn't a sharp, clear-cut boundary: The atmosphere doesn't abruptly end at this altitude. Instead, it gradually tapers off into space.

The choice of 100 kilometers is somewhat arbitrary. Still, it provides a valuable standard, especially for distinguishing between aeronautics (the study of flight or travel through the air) and astronautics (the science of space travel).

The distinction between 'flight' in the atmosphere and 'flight' in space is necessary, particularly when considering the vastly different dynamics, engineering, and principles that apply to each domain.

The Fédération Aéronautique Internationale (FAI)

Established in 1905, the FAI promotes the safe and sustainable advancement of aerospace activities by establishing standards, certifications, and the recognition of remarkable achievements in the field.

The FAI is the world's primary authority for aeronautics and astronautics record-keeping. This organization is responsible for adopting the Kármán Line as the international standard, demarcating the boundary between Earth's atmosphere and outer space.

The USA's Different Take on the Boundary of Space

While the Kármán Line is internationally recognized, some U.S. entities see it differently. NASA and the U.S. Air Force place the boundary of space at 50 miles (about 80 kilometers) above Earth's surface.

This definition has its roots in empirical observations from the earliest days of space exploration. They argue that above this altitude, the atmosphere's effects on spacecraft become negligible, and the conditions are much more 'space-like.'

Additionally, multiple pilots who flew on the X-15 program were awarded astronaut wings by the U.S. Air Force. While two flights exceeded the Kármán Line, many reached altitudes above 50 miles but below 62 miles. Yet, those pilots are still considered astronauts by the U.S. standard.

It's worth noting that the distinction between the two definitions goes beyond academics. It has implications for the burgeoning commercial space industry, determining, for instance, when space tourists can officially be called 'astronauts.' Both definitions, while differing, provide essential perspectives on where our home planet's atmosphere wavers and the cosmos beyond begins.

A space rocket departing a launch pad.
 

Final Thoughts

While Newton's cannonball gave us insight into orbital dynamics, Theodore von Kármán provided the initial calculations to understand where our atmosphere's influence diminishes and space takes over.

While Theodore didn't set out to establish an international standard, the Kármán Line, albeit theoretical, offers a tangible point of reference in the seamless gradient from the blue of our skies to the blackness of space. It reminds us of the ever-blurring line between the sky we can touch and the stars we yearn to reach.


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Matthew Scott

Once a computer game programmer, now a CFII/MEI who's passionate about learning and teaching aviation. My first computer game was Microsoft Flight Simulator 98. Swapped the virtual skies for the real deal and never looked back. I still love simulators, though!

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