Skip to main content

Scientists Discover Way to Send Information into Black Holes Without Using Energy

Scientists Measure Rocket Re-Entry Pollution for the First Time

For the first time in history, scientists have directly measured pollution caused by a rocket burning up in Earth’s upper atmosphere. The breakthrough happened after part of a Falcon 9 rocket re-entered Earth’s atmosphere on February 19, 2025, creating a dramatic fireball visible across Europe.

While many people admired the glowing streak across the sky, a team of German scientists quickly turned their attention to something far more serious: pollution left behind in one of the least understood parts of our atmosphere.

Their findings, published in the journal Communications Earth & Environment, may change how the world thinks about the environmental impact of the rapidly growing space industry.


A Spectacular Re-Entry Sparks Scientific Opportunity

In the early hours of February 19, 2025, the upper stage of a Falcon 9 rocket re-entered Earth’s atmosphere in an uncontrolled descent. As it tumbled through the sky, it exploded into a brilliant fireball visible from the United Kingdom to Poland.

Behind the beauty, however, was a rare scientific opportunity.

A research team led by Robin Wing and Gerd Baumgarten from the Leibniz Institute of Atmospheric Physics in Germany had been preparing for such an event. They rushed to activate their specialized instruments to capture data from the rocket’s debris trail.

Their goal was ambitious: measure pollution in a region of the atmosphere that scientists often call the “ignorosphere.”


What Is the “Ignorosphere”?

The “ignorosphere” is a nickname scientists use for the region between 50 and 100 kilometers above Earth. It includes the mesosphere and the lower thermosphere.

This area is extremely difficult to study. It is too high for weather balloons and too low for satellites to orbit easily. As a result, very little is known about pollution in this zone.

Yet this region plays an important role in Earth’s climate system and in protecting life from harmful solar radiation. Any pollutants released here could behave very differently compared to pollution near the ground.

That’s why understanding what rockets leave behind during re-entry is so important.


How Scientists Measured the Pollution

To detect pollution, the German team used a technology called LIDAR (Light Detection and Ranging). LIDAR works by sending out powerful laser pulses into the sky and analyzing the light that bounces back.

If particles such as dust, smoke, or metal atoms are present, they reflect the laser light differently. By studying these reflections, scientists can identify the type and concentration of materials in the atmosphere.

During the Falcon 9 re-entry, the researchers detected something unusual: a sudden spike in lithium nearly 100 kilometers above Earth.


A Lithium Plume in the Upper Atmosphere

The LIDAR instruments revealed a plume containing lithium at levels 10 times higher than normal for that part of the atmosphere.

Lithium is commonly used in rocket batteries and other onboard systems. When the rocket burned up during re-entry, components containing lithium vaporized and spread into the surrounding air.

By tracking the plume’s movement, the scientists traced it back to the location west of Ireland where the rocket re-entered.

This was the first time researchers successfully measured pollution from a rocket re-entry at such high altitudes before it dispersed.

The achievement proves that it is possible to monitor this type of pollution in real time — a major step forward for atmospheric science.


Why High-Altitude Pollution Matters

Pollution released at 75 kilometers above Earth does not behave the same way as pollution at ground level.

According to the researchers, one ton of emissions released at this altitude could have an impact equivalent to 100,000 tons released at the surface. That is because the upper atmosphere is thinner and more sensitive to chemical changes.

Pollutants in this region can:

  • Influence climate processes

  • Interfere with atmospheric chemistry

  • Contribute to ozone depletion

  • Affect how solar radiation interacts with Earth

Even though the upper atmosphere feels distant from daily life, changes there can eventually impact weather patterns and the protective ozone layer that shields us from harmful ultraviolet (UV) radiation.


A Warning for the Future

The study describes this event as a “harbinger” — a warning sign of what may come.

The number of satellites orbiting Earth is increasing rapidly. Currently, there are around 14,000 active satellites in space.

But that number could grow dramatically.

China has applied for permission to launch approximately 200,000 satellites in the coming years. Meanwhile, Elon Musk’s company SpaceX has applied to launch up to one million additional satellites.

Each satellite must eventually re-enter Earth’s atmosphere, either in a controlled or uncontrolled manner. That means more rocket launches — and more debris burning up overhead.

If every re-entry releases metals and other pollutants into the upper atmosphere, the cumulative impact could be significant.


Lack of Regulation

One of the most concerning aspects highlighted by experts is the absence of clear regulations.

Eloise Marais, a professor of atmospheric chemistry at University College London who was not involved in the study, emphasized that there are currently no specific rules targeting pollution in the upper atmosphere.

While governments regulate emissions at ground level, pollution in higher atmospheric layers remains largely unmonitored and unregulated.

As space activity increases, policymakers may need to develop international standards to manage emissions from rocket launches and satellite re-entries.


A New Era of Atmospheric Monitoring

This groundbreaking measurement opens the door to future research.

Now that scientists have proven it is possible to detect and analyze rocket re-entry pollution in the upper atmosphere, more monitoring systems could be developed worldwide.

Future studies may examine:

  • Other metals released during re-entry

  • Long-term accumulation of pollutants

  • Effects on ozone chemistry

  • Impact on climate systems

Understanding these effects will be crucial as humanity enters a new era of intense space activity.


Balancing Progress and Responsibility

The space industry is expanding rapidly. Satellites power modern life — enabling GPS navigation, global communication, weather forecasting, and internet access in remote areas.

But progress comes with responsibility.

Just as industrial pollution on Earth required scientific study and environmental regulations, space-related pollution must now receive similar attention.

The fiery Falcon 9 re-entry over Europe was more than a spectacular light show. It marked the beginning of a new field of environmental research — one focused not on what happens at ground level, but on what happens high above our heads.

For the first time, scientists have captured clear evidence of rocket pollution in the upper atmosphere.

As humanity sends more machines into space, the question is no longer whether this pollution exists — but how much of it we are willing to allow.

The sky may look clean and endless, but even there, our footprint is beginning to show.

Reference: Measurement of a lithium plume from the uncontrolled re-entry of a Falcon 9 rocket, Communications Earth & Environment (2026). DOI: 10.1038/s43247-025-03154-8

Comments

Popular

Scientists Discover Way to Send Information into Black Holes Without Using Energy

For years, scientists believed that adding even one qubit (a unit of quantum information) to a black hole needed energy. This was based on the idea that a black hole’s entropy must increase with more information, which means it must gain energy. But a new study by Jonah Kudler-Flam and Geoff Penington changes that thinking. They found that quantum information can be teleported into a black hole without adding energy or increasing entropy . This works through a process called black hole decoherence , where “soft” radiation — very low-energy signals — carry information into the black hole. In their method, the qubit enters the black hole while a new pair of entangled particles (like Hawking radiation) is created. This keeps the total information balanced, so there's no violation of the laws of physics. The energy cost only shows up when information is erased from the outside — these are called zerobits . According to Landauer’s principle, erasing information always needs energy. But ...

Black Holes That Never Dies

Black holes are powerful objects in space with gravity so strong that nothing can escape them. In the 1970s, Stephen Hawking showed that black holes can slowly lose energy by giving off tiny particles. This process is called Hawking radiation . Over time, the black hole gets smaller and hotter, and in the end, it disappears completely. But new research by Menezes and his team shows something different. Using a theory called Loop Quantum Gravity (LQG) , they studied black holes with quantum corrections. In their model, the black hole does not vanish completely. Instead, it stops shrinking when it reaches a very small size. This leftover is called a black hole remnant . They also studied something called grey-body factors , which affect how much energy escapes from a black hole. Their findings show that the black hole cools down and stops losing mass once it reaches a minimum mass . This new model removes the idea of a “singularity” at the center of the black hole and gives us a better ...

How Planetary Movements Might Explain Sunspot Cycles and Solar Phenomena

Sunspots, dark patches on the Sun's surface, follow a cycle of increasing and decreasing activity every 11 years. For years, scientists have relied on the dynamo model to explain this cycle. According to this model, the Sun's magnetic field is generated by the movement of plasma and the Sun's rotation. However, this model does not fully explain why the sunspot cycle is sometimes unpredictable. Lauri Jetsu, a researcher, has proposed a new approach. Jetsu’s analysis, using a method called the Discrete Chi-square Method (DCM), suggests that planetary movements, especially those of Earth, Jupiter, and Mercury, play a key role in driving the sunspot cycle. His theory focuses on Flux Transfer Events (FTEs), where the magnetic fields of these planets interact with the Sun’s magnetic field. These interactions could create the sunspots and explain other solar phenomena like the Sun’s magnetic polarity reversing every 11 years. The Sun, our closest star, has been a subject of scient...