Scientists Discover New Electric Field in Earth’s Atmosphere
A faint electric field has been detected in Earth’s atmosphere, confirming a theory that scientists have held for decades. This ambipolar electric field, though weak at just 0.55 volts, could play a vital role in shaping Earth’s atmospheric evolution and its ability to support life, according to recent findings. Glyn Collinson, an atmospheric scientist at NASA’s Goddard Space Flight Center, led the Endurance rocket mission, which successfully measured this field in May 2022 above Svalbard, Norway. Collinson has described this field as a “planetary-energy field” that had eluded scientific measurement until now.
How the Ambipolar Field Affects Earth’s Atmosphere
The presence of this field is thought to explain a phenomenon observed decades ago—the polar wind. When sunlight strikes atoms in the upper atmosphere, it can cause negatively charged electrons to break free and drift into space, while the heavier, positively charged oxygen ions remain. To maintain an electrically neutral atmosphere, a faint electric field forms, tying these particles together and preventing electrons from escaping. This weak field has been shown to provide energy to lighter ions, such as hydrogen, enabling them to break free from Earth’s gravity and contribute to the polar wind.
This ambipolar electric field could have implications for planetary habitability. David Brain, a planetary scientist at the University of Colorado Boulder, noted that understanding how such fields vary across planets could shed light on why Earth has remained habitable compared to planets like Mars and Venus. Although both Mars and Venus have electric fields, the absence of a global magnetic field on those planets allowed more of their atmospheres to escape into space, potentially altering their climates significantly.
Further Research Planned
NASA has recently approved a follow-up mission with a rocket named Resolute, expected to launch soon. Collinson believes that continued investigation into planetary electric fields may help answer fundamental questions about why Earth supports life while other planets do not.
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A stunning solar eruption captured on video on the night of May 12-13 has revealed a 600,000-mile-long filament blasting away from the sun’s northern hemisphere. The outburst occurred around 8 p.m. EDT (0000 GMT) and spanned a distance more than twice that between Earth and the moon. A massive solar filament suspended above the sun’s surface became unstable and erupted, blasting a CME into space along with a cloud of plasma and magnetic energy. Preliminary models show Earth is nowhere in the firing range of this fiery ejection, but researchers are still watching the phenomenon closely.
Sun’s 600,000-Mile-Long ‘Angel-Wing’ Eruption Stuns Skywatchers, Signals Rising Solar Activity
As per the Space.com report, the eruption originated from a filament structure composed of dense, cooler solar plasma held aloft by magnetic fields. These structures often appear as dark ribbons across the sun’s disk and can become unstable without warning. Solar observers noted that this latest eruption dwarfed similar recent events, both in scale and intensity. Aurora chaser Jure Atanackov remarked that the CME from the blast was among the most spectacular seen this year, although fortunately, it is headed north and will miss Earth.
The event, dubbed the “angel-wing” or “bird-wing” eruption by observers online, was widely shared among solar watchers. Vincent Ledvina, another aurora chaser, noted its incredible visual impact, describing it as a sight worth watching on loop. The eruption is, in fact, so long, by more than a million kilometres, that it is of scientific interest and visually striking as well. Geomagnetic storms resulting from this kind of CME can affect satellites, communication systems, and even Earth.
Although it foreshadows the unpredictable nature of our host star, this particular CME does not pose a threat to Earth at the moment. Solar activity is ramping up as we approach the peak of Solar Cycle 25 in 2025. What’s more, more — and maybe more Earth-threatening — solar explosions could follow.
As a reminder of the formidable and delicate forces at play relatively close by on Earth, the sun remains a source of wonder for astronomers and skywatchers alike.
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Over 80 years, dark matter has been a great mystery for the researchers. Elusive of direct observation, it has made its existence known only by the gravitational impacts it makes on cosmic structures. Even though there is a lot of indirect evidence of its existence, the real nature of dark matter is still unknown. An important attribute of its particle is mass. While past studies have constrained the mass of fermionic dark matter using quantum principles like Pauli’s exclusion principle, bosonic dark matter remained less constrained. In a recent study, scientists have estimated a new lower bound on the mass of ultra-lightweight bosonic dark matter particles.
About the study
According to the study published in Physical Review Letters, the mass of ultralight bosonic dark matter must be more than 2 × 10-21 electron volts (eV), 100 times more than previous estimates using Heisenberg’s uncertainty principle.
The team of researchers, led by the first author of the study, Tim Zimmermann, a Ph.D. candidate at the Institute of Theoretical Astrophysics, University of Oslo, focused their method on the data of Leo II, the Milky Way’s satellite galaxy. It is a dwarf galaxy 1,000 times smaller than the Milky Way. By analyzing the internal motions of stars within Leo II—heavily influenced by dark matter—the team derived 5,000 possible dark matter density profiles using a tool called GRAVSPHERE.
They compared these with profiles generated by quantum wave functions of various dark matter particle masses. If the particle is too light, quantum fuzziness spreads it too thinly, preventing it from forming the observed structures. The study concluded that the dark matter particle must have a mass greater than 2.2 × 10⁻²¹ electron volts (eV)—over 100 times more than previous lower estimates.
Impact on dark matter studies
The findings have significant implications for popular ultralight dark matter models, particularly fuzzy dark matter, which typically proposes particles with masses around 10-22 ev.
Looking ahead, the team plans to extend their methodology to mixed dark matter scenarios, where dark matter is composed of particles with different masses.
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