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Star Trek-like shield discovered in Earth’s orbit shelters our planet from ‘killer electrons’

Dragos MitricabyDragos Mitrica
December 2, 2014
in News, Space
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Many thousands of miles above our planet’s surface, electrons whiz through close to the speed of light. These electrons can streak past Earth in under five minutes, but can  also become dangerous and have been known to destroy satellites and even injure astronauts in extreme cases. Most of the time, however, our gear and astronauts can rest safe since scientists have discovered what’s called a invisible shield or barrier lying within the rims of the Van Allen Radiation Belts that’s impenetrable to the relativistic electrons. So, despite their intense energies, the electrons can’t come close than 11,000 km from the Earth’s surface.

Shielded from harm’s way

Charged gas particles interact with Earth's radiation belts to create a barrier against relativistic electrons. Image: MIT
Charged gas particles interact with Earth’s radiation belts to create a barrier against relativistic electrons. Image: MIT

The discovery was made based on data collected by NASA’s Van Allen Probes—twin crafts that are orbiting within the harsh environments of the Van Allen radiation belts. These belts can be seen as one big torus of energetic charged particles around Earth, trapped by Earth’s magnetic field. These extend from circa 650km (inner ring) to 65,000 km (outer ring) above the Earth. The existence of two belts, sometimes considered as a single belt of varying intensity, was confirmed from information secured by launching the first U.S. earth satellite, Explorer I, sent up during the International Geophysical Year of 1957–58. The belts were named for James A. Van Allen, the American astrophysicist who first predicted the belts and then was first to interpret the findings of the Explorer satellite.

“It’s a very unusual, extraordinary, and pronounced phenomenon,” says John Foster, associate director of MIT’s Haystack Observatory. “What this tells us is if you parked a satellite or an orbiting space station with humans just inside this impenetrable barrier, you would expect them to have much longer lifetimes. That’s a good thing to know.”

Data collected over 20 months suggested there’s a “exceedingly sharp” barrier against ultra-relativistic electrons also called “killer electrons” because of their havoc wrecking potential. Oddly enough, this barrier helds steady even during times of exceeding blasts of electrons, moved forward by solar storms. Left scratching their heads, MIT researchers tried to figure out what was keeping this shield up and considered several possibilities, including effects from the Earth’s magnetic field and transmissions from ground-based radios.

A cutaway model of the radiation belts with the 2 RBSP satellites flying through them. The radiation belts are two donut-shaped regions encircling Earth, where high-energy particles, mostly electrons and ions, are trapped by Earth’s magnetic field. This radiation is a kind of “weather” in space, analogous to weather on Earth, and can affect the performance and reliability of our technologies, and pose a threat to astronauts and spacecraft. Image: NASA
A cutaway model of the radiation belts with the 2 RBSP satellites flying through them. The radiation belts are two donut-shaped regions encircling Earth, where high-energy particles, mostly electrons and ions, are trapped by Earth’s magnetic field. This radiation is a kind of “weather” in space, analogous to weather on Earth, and can affect the performance and reliability of our technologies, and pose a threat to astronauts and spacecraft. Image: NASA

 

First, the researchers looked the South Atlantic Anomaly – a patch in Earth’s magnetic field, just over South America, where the magnetic field strength is about 30% weaker than in any other region. The reasoning was that if Earth’s magnetic field was indeed responsible for the shield, then incoming electrons should fall deeper into the Earth’s atmosphere and sink into the ‘hole’. There was no such thing and the killer electrons stayed put at 11,000 km above the planet’s surface. Long-range, very-low-frequency (VLF) radio transmissions can leak into the upper atmosphere, but upon closer inspection researchers found that these could only deflect moderate energy levels, posing little shielding against the energy intensive relativistic electrons.

“It’s almost like theses electrons are running into a glass wall in space,” said Baker in a UC press release. “Somewhat like the shields created by force fields on Star Trek that were used to repel alien weapons, we are seeing an invisible shield blocking these electrons. It’s an extremely puzzling phenomenon.”

A pale Blue Dot, vulnerable, but wearing a double sweater

The Van Allen Probes (formerly known as the Radiation Belt Storm Probes (RBSP)) were designed to help us understand the sun’s influence on Earth and near-Earth space by studying the Earth’s radiation belts on various scales of space and time. Image: NASA
The Van Allen Probes (formerly known as the Radiation Belt Storm Probes (RBSP)) were designed to help us understand the sun’s influence on Earth and near-Earth space by studying the Earth’s radiation belts on various scales of space and time. Image: NASA
A geographic representation of ultra-relativistic electron fluxes, based on orbital tracks of the Van Allen Probe B spacecraft projected onto the geographical equatorial plane. As the spacecraft precesses in its elliptical orbit around the Earth, it forms a “spirograph” pattern in the Earth-centered coordinate system. Inside of this radial distance is an almost complete absence of electrons, forming the “slot” region. The superimposed circle shows a sharp, distinctive inner boundary for ultra-relativistic electrons, and how generally symmetric this boundary is around Earth. Image: Courtesy of the researchers/Haystack Observatory
A geographic representation of ultra-relativistic electron fluxes, based on orbital tracks of the Van Allen Probe B spacecraft projected onto the geographical equatorial plane. As the spacecraft precesses in its elliptical orbit around the Earth, it forms a “spirograph” pattern in the Earth-centered coordinate system. Inside of this radial distance is an almost complete absence of electrons, forming the “slot” region. The superimposed circle shows a sharp, distinctive inner boundary for ultra-relativistic electrons, and how generally symmetric this boundary is around Earth. Image: Courtesy of the researchers/Haystack Observatory

Luckily, the twin probes were equipped with instruments that could measure  electrons’ pitch angle—the degree to which an electron’s motion is parallel or perpendicular to the Earth’s magnetic field. The measurements revealed that the electrons slowly rotate their paths  causing them to fall, parallel to a magnetic field line, into Earth’s upper atmosphere, where they are likely to collide with neutral atoms and disappear. It was later found that a peculiar phenomenon called “plasmaspheric hiss” – very low-frequency electromagnetic waves in the Earth’s upper atmosphere that, when played through a speaker, resemble static, or white noise – was the actual culprit.

The hiss waves are believed to travel through a cloud of electrically charged gas that is known to surround Earth, starting at an altitude of 600 miles.  This cloud, known as the plasmasphere, interacts with the high-energy electrons, scattering from their paths.

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“It’s like looking at the phenomenon with new eyes, with a new set of instrumentation, which give us the detail to say, ‘Yes, there is this hard, fast boundary,’” Foster says.

It’s amazing how safe guarded our planet is. We have an atmosphere, a magnetic field, the radiation belts, the plasmasphere and who knows what else. If anyone had any doubt how precious and special this planet is, look no further.

Findings appeared in the journal Nature.

Tags: earthelectromagnetic waveelectronmagnetic fieldvan allen belt

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Dragos Mitrica

Dragos Mitrica

Dragos has been working in geology for six years, and loving every minute of it. Now, his more recent focus is on paleoclimate and climatic evolution, though in his spare time, he also dedicates a lot of time to chaos theory and complex systems.

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