NASA Discovers Third Global Energy Field – As Fundamental as Earth’s Gravity and Magnetic Fields

Endurance Earth From Space Crop
The geographic North Pole seen from the Endurance rocket ship at 477 miles (768 kilometers) altitude above the Arctic. The faint red and green streaks at the top of the image are artifacts of lens flare. Credit: NASA

NASA’s recent mission has unveiled Earth’s ambipolar electric field, crucial for understanding atmospheric dynamics and exploring other habitable worlds.

  • A rocket team reports the first successful detection of Earth’s ambipolar electric field: a weak, planet-wide electric field as fundamental as Earth’s gravity and magnetic fields.
  • First hypothesized more than 60 years ago, the ambipolar electric field is a key driver of the “polar wind,” a steady outflow of charged particles into space that occurs above Earth’s poles.
  • This electric field lifts charged particles in our upper atmosphere to greater heights than they would otherwise reach and may have shaped our planet’s evolution in ways yet to be explored.
Earth Ambipolar Electric Field
NASA’s Endurance mission has for the first time measured the ambipolar electric field enveloping Earth, revealing its significant impact on atmospheric escape and providing key insights into the atmospheric conditions of potentially habitable planets. Credit: NASA/Conceptual Image Lab

Using observations from a NASA suborbital rocket, an international team of scientists has, for the first time, successfully measured a planet-wide electric field thought to be as fundamental to Earth as its gravity and magnetic fields. Known as the ambipolar electric field, scientists first hypothesized over 60 years ago that it drove how our planet’s atmosphere can escape above Earth’s North and South Poles. Measurements from the rocket, NASA’s Endurance mission, have confirmed the existence of the ambipolar field and quantified its strength, revealing its role in driving atmospheric escape and shaping our ionosphere — a layer of the upper atmosphere — more broadly.

Understanding the complex movements and evolution of our planet’s atmosphere provides clues not only to the history of Earth but also gives us insight into the mysteries of other planets and determining which ones might be hospitable to life. The paper was published on August 28, 2024, in the journal Nature.

An Electric Field Drawing Particles Out to Space

Since the late 1960s, spacecraft flying over Earth’s poles have detected a stream of particles flowing from our atmosphere into space. Theorists predicted this outflow, which they dubbed the “polar wind,” spurring research to understand its causes.

Some amount of outflow from our atmosphere was expected. Intense, unfiltered sunlight should cause some particles from our air to escape into space, like steam evaporating from a pot of water. But the observed polar wind was more mysterious. Many particles within it were cold, with no signs they had been heated — yet they were traveling at supersonic speeds.

“Something had to be drawing these particles out of the atmosphere,” said Glyn Collinson, principal investigator of Endurance at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and lead author of the paper. Scientists suspected a yet-to-be-discovered electric field could be at work.

The hypothesized electric field, generated at the subatomic scale, was expected to be incredibly weak, with its effects felt only over hundreds of miles. For decades, detecting it was beyond the limits of existing technology. In 2016, Collinson and his team got to work inventing a new instrument they thought was up to the task of measuring Earth’s ambipolar field.

How the Ambipolar Field Works

Scientists theorized this electric field should begin at around 150 miles (250 kilometers) altitude, where atoms in our atmosphere break apart into negatively charged electrons and positively charged ions.

Electrons are incredibly light — the slightest kick of energy could send them shooting out to space. Ions are at least 1,836 times heavier and tend to sink toward the ground. If gravity alone were in play, the two populations, once separated, would drift apart over time.

But given their opposite electric charges, an electric field forms to tether them together, preventing any separation of charges and counteracting some of the effects of gravity.


This animation starts with a close-up view of the ionosphere, represented as a blue arc over a slowly-rotating Earth (not to scale). The view then zooms in, showing nitrogen (N2) that comprises most of the atmosphere. Panning upward, the view then shows atomic oxygen, a lighter element that populates the upper portions of the ionosphere.

When photons from the Sun collide with these gases, electrons can be knocked loose. As the atoms and molecules lose electrons, they become positively charged, making them ions. This process is known as ionization.

After the oxygen atom becomes ionized, the view changes to show a collection of these ionized gases, known as plasma. When there are equal numbers of electrons and ions, the plasma, as a whole, is neither positively nor negatively charged, but neutral. However, the magnetic pull between the individual particles tethers them together by an electric field, like glue. This field is known as the ambipolar electric field.

Credit: NASA/Conceptual Image Lab

This electric field is bidirectional, or “ambipolar,” because it works in both directions. Ions pull the electrons down with them as they sink with gravity. At the same time, electrons lift ions to greater heights as they attempt to escape to space, like a tiny dog tugging on its sluggish owner’s leash.

The net effect of the ambipolar field is to extend the height of the atmosphere, lifting some ions high enough to escape with the polar wind.


This animation shows the two main effects of the ambipolar electric field: inflating the ionosphere and generating the polar wind.

The sparkling blue haze surrounding Earth represents the plasma in the ionosphere. At the beginning of the animation, the ionosphere is dense and close to Earth, but when the ambipolar electric field is applied to the plasma, the ionosphere inflates, making it taller. This happens because the tug from the energized electrons, which are connected to the heavy ions, slightly overpowers the force of gravity, creating an upward lift.

Hydrogen ions, however, are so light that the field’s upward force is ten times the downward force of gravity. This accelerates the hydrogen ions upward to supersonic speeds, enough for the ions to escape to space above Earth’s magnetic poles. This hydrogen ion outflow is known as the polar wind, shown in the animation as sparkling white lights traveling up the blue magnetic field lines and out of frame.

Credit: NASA/Conceptual Image Lab

Launching a Rocket From the Arctic

The team’s instruments and ideas were best suited for a suborbital rocket flight launched from the Arctic. In a nod to the ship that carried Ernest Shackleton on his famous 1914 voyage to Antarctica, the team named their mission Endurance. The scientists set a course for Svalbard, a Norwegian archipelago just a few hundred miles from the North Pole and home to the northernmost rocket range in the world.

“Svalbard is the only rocket range in the world where you can fly through the polar wind and make the measurements we needed,” said Suzie Imber, a space physicist at the University of Leicester, UK, and co-author of the paper.

On May 11, 2022, Endurance launched and reached an altitude of 477.23 miles (768.03 kilometers), splashing down 19 minutes later in the Greenland Sea. Across the 322-mile altitude range where it collected data, Endurance measured a change in electric potential of only 0.55 volts.

“A half a volt is almost nothing — it’s only about as strong as a watch battery,” Collinson said. “But that’s just the right amount to explain the polar wind.”

Endurance Rocket Ship Launches
The Endurance rocket ship launches from Ny-Ålesund, Svalbard. Credit: Andøya Space/Leif Jonny Eilertsen

Hydrogen ions, the most abundant type of particle in the polar wind, experience an outward force from this field 10.6 times stronger than gravity. “That’s more than enough to counter gravity — in fact, it’s enough to launch them upwards into space at supersonic speeds,” said Alex Glocer, Endurance project scientist at NASA Goddard and co-author of the paper.

Heavier particles also get a boost. Oxygen ions at that same altitude, immersed in this half-a-volt field, weigh half as much. In general, the team found that the ambipolar field increases what’s known as the “scale height” of the ionosphere by 271%, meaning the ionosphere remains denser to greater heights than it would be without it.

“It’s like this conveyor belt, lifting the atmosphere up into space,” Collinson added.

Endurance’s discovery has opened many new paths for exploration. The ambipolar field, as a fundamental energy field of our planet alongside gravity and magnetism, may have continuously shaped the evolution of our atmosphere in ways we can now begin to explore. Because it’s created by the internal dynamics of an atmosphere, similar electric fields are expected to exist on other planets, including Venus and Mars.

“Any planet with an atmosphere should have an ambipolar field,” Collinson said. “Now that we’ve finally measured it, we can begin learning how it’s shaped our planet as well as others over time.”

Reference: “Earth’s ambipolar electrostatic field and its role in ion escape to space” by Glyn A. Collinson, Alex Glocer, Robert Pfaff, Aroh Barjatya, Rachel Conway, Aaron Breneman, James Clemmons, Francis Eparvier, Robert Michell, David Mitchell, Suzie Imber, Hassanali Akbari, Lance Davis, Andrew Kavanagh, Ellen Robertson, Diana Swanson, Shaosui Xu, Jacob Miller, Timothy Cameron, Dennis Chornay, Paulo Uribe, Long Nguyen, Robert Clayton, Nathan Graves, Shantanab Debchoudhury, Henry Valentine, Ahmed Ghalib and The Endurance Mission Team, 28 August 2024, Nature.
DOI: 10.1038/s41586-024-07480-3

Endurance was a NASA-funded mission conducted through the Sounding Rocket Program at NASA’s Wallops Flight Facility in Virginia. The Svalbard Rocket Range is owned and operated by Andøya Space. The European Incoherent Scatter Scientific Association (EISCAT) Svalbard radar, located in Longyearbyen, made ground-based measurements of the ionosphere critical to interpreting the rocket data. The EISCAT radar for the Endurance mission was funded by the United Kingdom Natural Environment Research Council (NERC) and the Research Council of Norway (RCN). EISCAT is owned and operated by research institutes and research councils of Norway, Sweden, Finland, Japan, China, and the United Kingdom (the EISCAT Associates). The Endurance mission team encompasses affiliates of the Catholic University of America, Embry-Riddle Aeronautical University, the University of California, Berkeley, the University of Colorado at Boulder, the University of Leicester, U.K., the University of New Hampshire, and Penn State University.