Geomagnetic Storm Unleashes Breathtaking Auroras Across US Skies

Energetic solar particles are racing toward Earth, illuminating the skies as far south as Florida in a brilliant display. Meteorologists report that the intensity was powerful enough to damage several radios.

Colors of red, purple, and green adorned the skies over Alabama, Ohio, and Texas. Forecasters from the Space Weather Prediction Center indicated that the geomagnetic storm could strengthen further as the “last and most energetic CME” – a coronal mass ejection – has not yet passed and is expected to reach Earth by Wednesday afternoon.

The aurora shines over Minneapolis, Minnesota, thanks to significant geomagnetic activity and enhanced solar forces.
Steven Garcia/Reuters

A CME represents a spectacular event where massive clouds of protons, electrons, and magnetic fields are expelled from the Sun’s outer atmosphere at immense speeds.

Upon reaching Earth’s magnetic field, known as the magnetosphere, it interacts with particles surrounding Earth, creating vibrant auroras in the northern hemisphere and auroras australis in the southern hemisphere.

The Northern Lights illuminate the night sky above Monroe, Wisconsin on Tuesday.
Ross Khalid/NurPhoto (via Getty Images)

Sean Dahl, a forecaster at the NOAA Space Weather Prediction Center located in Boulder, Colorado, noted that two CMEs have already impacted Earth, resulting in a geomagnetic storm measuring a G4 on the scale of five.

The overall magnetic field strength from these CMEs is “not only eight times stronger than usual, but also conducive for continued activity right now,” Dahl explained in a video. Posted on X.

Meteorologists cautioned that this geomagnetic storm could lead to power fluctuations, degraded GPS service, and sporadic radio disruptions.

The Northern Lights captured in Athens, Ohio on Tuesday night.
Ellie Beckaden

“Watches of this nature are exceedingly rare,” the Space Weather Prediction Center expressed in an advisory.

“We anticipate that the magnetic cloud, which is the ‘core’ of the current CME, is traversing Earth and will continue to do so throughout the night,” the agency declared early Wednesday.

A third, even more potent CME is expected to arrive on Wednesday, potentially allowing the aurora borealis to be visible further south.

Dahl mentioned that the second-highest level advisory would remain valid for several more hours, with a possibility of reaching the highest rating, G5.

Aurora over Minneapolis, Minnesota.
Steven Garcia/via Reuters

Source: www.nbcnews.com

Webb Discovers Auroras Using Free-Floating Brown Dwarfs

Astronomers utilizing the NASA/ESA/CSA James Webb Space Telescope have found evidence of energy deposition in the upper atmosphere of the nearby brown dwarf SIMP J013656.5+093347.3 caused by auroras.

Artist’s impression of aurora and brown dwarf SIMP-0136. Image credit: Evert Nasedkin.

SIMP J013656.5+093347.3 (commonly referred to as SIMP-0136) is a low-mass brown dwarf located 20 light years away in the Pisces constellation, approximately 6.12 light years from Earth.

As part of the Carina-near Stellar Association, this celestial object is estimated to be around 200 million years old.

The mass of SIMP-0136 is roughly estimated to fall between 12.7 and 17.8 times that of Jupiter.

With a spectral type of T2.5 and a temperature nearing 1,100 K, it exhibits many atmospheric properties similar to those of directly imaged exoplanets, such as HR 8799B and AF Lep b.

“Our observations have illuminated the activity of the robust aurora of SIMP-0136, which warms its atmosphere, much like the auroras on Earth and the powerful auroras found on Jupiter.”

“These measurements represent some of the most precise assessments of the atmospheres of extreme objects to this date, with direct measurements of atmospheric changes occurring for the first time.”

“Furthermore, with temperatures exceeding 1,500 degrees Celsius, SIMP-0136 will display mild heat waves this summer.”

“Our specific observations indicated that we could precisely record temperature variations of less than 5 degrees Celsius.”

“These temperature fluctuations were linked to minor alterations in the chemical makeup of this free-floating planet, hinting at storms akin to the Great Red Spot on Jupiter.

Another unexpected finding was the constancy of cloud variability in SIMP-0136.

Changes in cloud coverage might typically lead to atmospheric changes, similar to the variability observed with patches of clouds and clear skies on Earth.

However, astronomers discovered that cloud coverage remains stable across the surface of SIMP-0136.

At SIMP-0136’s temperatures, these clouds are distinct from Earth’s, primarily composed of silicate grains reminiscent of beach sand.

“Different wavelengths of light are associated with various atmospheric features,” stated Dr. Nasedkin.

“Similar to observing color changes on Earth’s surface, the color variations of SIMP-0136 are driven by alterations in atmospheric properties.”

“Utilizing advanced models enables us to deduce atmospheric temperature, chemical composition, and cloud positioning.”

“This work is thrilling as it showcases that by leveraging cutting-edge modeling techniques on Webb’s advanced datasets, we can understand the processes driving global weather throughout our solar system.”

“Understanding these meteorological processes is crucial as we continue discovering and characterizing exoplanets in the future.”

“Currently, such spectroscopic variability observations are limited to isolated brown dwarfs, but large telescopes and future studies, along with the eventual establishment of a habitable world observatory, will allow us to explore the atmospheric dynamics of exoplanets ranging from gas giants like Jupiter to rocky planets.”

The team’s survey results will be published in the journal Astronomy and Astrophysics.

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E. Nasedkin et al. 2025. JWST Weather Report: Investigating temperature variations, aurora heating, and stable cloud coverage on SIMP-0136. A&A 702, A1; doi: 10.1051/0004-6361/202555370

Source: www.sci.news

Webb Captures Dynamic Infrared Auroras on Jupiter

Jovian auroras shine hundreds of times brighter than those visible from Earth, according to a team of astronomers led by Dr. Jonathan Nichols at the University of Leicester.

These observations of Jupiter’s aurora were captured on December 25, 2023 by Webb’s near-infrared camera (NIRCAM). Image credit: NASA / ESA / CSA / STSCI / RICARDO HUESO, UPV / IMKE DE PATER, UC BERKELEY / THIERRY FOUCHET, OBSERVATORY OF PARIS / LE FLETCHER, JOSEPH DEPASQUALE, STSCI/J. NICHOLS, UNIVERSITY OF LEICESTER/M. ZAMANI, ESA & WEBB.

When high-energy particles enter the planet’s atmosphere near its magnetic poles, they collide with gas atoms, creating the auroras.

Jupiter’s auroras are not only massive in scale but also exhibit energy levels hundreds of times greater than those seen on Earth.

These auroras are primarily triggered by solar storms, where charged particles entering the atmosphere excite gas particles, resulting in vibrant red, green, and purple hues.

Additionally, Jupiter has a unique source of auroral activity—its strong magnetic field captures charged particles from its surroundings.

This includes not only those from the solar wind but also particles ejected from the volcanic moon Io.

The eruptions from Io’s volcanoes release particles that escape both the moon’s and Jupiter’s gravitational pull.

Solar storms also discharge vast amounts of charged particles towards Jupiter.

Jupiter’s immense magnetic fields accelerate these charged particles to extraordinary speeds.

When these high-velocity particles collide with the planet’s atmosphere, they excite the gas and produce radiant displays.

https://www.youtube.com/watch?v=if0vpfergju

Thanks to the advanced capabilities of the NASA/ESA/CSA James Webb Space Telescope, new insights into Jovian auroras can be gained.

The telescope’s sensitivity enables astronomers to use faster shutter speeds to capture the rapidly evolving features of the auroras.

This latest data was collected using Webb’s near-infrared camera (NIRCAM) on Christmas Day 2023.

“What a Christmas gift; it truly astonished me!” exclaimed Dr. Nichols.

“We aimed to observe how quickly the aurora transformed, hoping to see beautiful fluctuations within about an hour.”

“Instead, we witnessed the entire aurora region illuminating the sky in a spectacular display.

Astronomers noted fluctuations in the effects caused by trihydrogen ions, known as H.3+, which varied more than previously assumed.

These observations help scientists unravel how Jupiter’s upper atmosphere undergoes heating and cooling.

Additionally, several unknown phenomena were identified in the data.

“What made these observations particularly intriguing was that the NASA/ESA Hubble Space Telescope was capturing images simultaneously in ultraviolet light,” Dr. Nichols commented.

“Strangely, the brightest light observed by Webb seemed to have no corresponding feature in Hubble’s images. This left me puzzled.”

“To produce the brightness observed in both Webb and Hubble, we would require an improbable mix of a substantial quantity of very low-energy particles impacting the atmosphere.

study Published in the journal Nature Communications.

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JD Nichols et al. 2025. The dynamic infrared aurora of Jupiter. Nature Communications 16, 3907; doi:10.1038/s41467-025-58984-z

Source: www.sci.news

Solar maximum increases chances of auroras.

overview

  • A recent flurry of solar storms suggests the Sun is at its peak as part of an 11-year cycle.
  • The active period is likely to continue into next year, and more auroras may appear.
  • Next month, NASA will take an up-close look at solar activity as the Parker Solar Probe makes its closest approach to the sun ever.

The sun is awake.

Earth’s star has become more active in recent months, with giant flares erupting from the surface and streams of plasma and charged particles spewing into space. Several solar storms have been directed towards our planet, causing intense magnetic storms and the dazzling glow of the aurora borealis.

Experts say a storm of solar explosions after years of relative calm and calm is a sure sign that the star has entered a busy phase of its natural cycle, or solar maximum.

The active period is likely to continue into next year, with the potential for more solar storms and spectacular aurora borealis.

“This is definitely the season for major solar storms,” ​​said Kelly Kolek, a program scientist in NASA’s Heliophysics Division. “I think we’ll see the sky lit up again by the northern lights.”

Aurora photographed over Kiruna, Sweden on March 7th.
Leon Neal/Getty Images File

Later this month, NASA will get a close-up look at intense solar activity when the agency’s Parker Solar Probe makes its closest approach ever to the sun on December 24th.

The spacecraft is on an orbit that swoops to within 3.86 million miles of the Sun’s surface. This is closer than any other artifact in history. It is predicted that it could fly through the sun’s plasma plumes and fly into the star’s active regions.

“If you think of an American football field, if the Earth is on one side and the sun is on the other side, this is like going to the sun’s 4-yard line,” Kolek said.

Parker Solar Probe after heat shield installation in a clean room in Titusville, Florida, 2018.
Johns Hopkins APL / Ed Whitman / NASA

The Parker Solar Probe was launched in 2018 with a mission to study the sun’s atmosphere, an extremely hot region known as the corona. Last month, the car-sized spacecraft flew nearby in a maneuver that helped slingshot Venus closer to the sun.

Kolek said the spacecraft’s close encounters could provide valuable insights, especially if there are active sunspot regions (temporary features that appear as dark scratches on the sun’s surface) along its path. He said there is. Such observations could help researchers better understand how the sun’s activity rises and falls.

Solar cycles typically last about 11 years, as the Sun’s magnetic activity moves from periods of low to high magnetic activity. When a star emerges from its calm phase, or solar minimum, and reaches the peak of its solar cycle, its magnetic poles reverse and it enters solar maximum, increasing activity and erupting more frequently and violently.

The main way scientists know when the Sun has reached its maximum is by monitoring the formation of sunspots. As the sun spins, its magnetic field undulates, becoming distorted and tighter in some areas, Kolek said. This creates sunspots, which appear as dark specks in telescope images.

A huge, bright coronal loop traces magnetic field lines over the Sun’s active region in 2018.
Solar Dynamics Observatory / NASA

“The sun is a magnetic sphere, but it’s not a solid solid body, so as it rotates, its magnetic field gets twisted,” Kolek said.

the number of sunspots It increases steadily as the star moves towards its solar maximum. Once a significant decline is observed, researchers can define the beginning and end of a period of activity.

In some sunspot regions, the magnetic field can be about 2,500 times stronger than Earth’s magnetic field. According to NASA. Over time, sunspots can release vast amounts of stored magnetic energy in the form of solar storms.

This year, two major solar storms (one in May and one in early October) painted the night sky in bright pinks, greens, and purples as far south as Texas and Alabama. It surprised sky watchers. NASA said the May event was the strongest geomagnetic storm to hit Earth in the past 20 years.

On May 10th, a solar storm hit the Scottish National Monument in Edinburgh.
Jacob Anderson/AFP – Getty Images File
On October 10, the Northern Lights illuminate the desert sky of the Tonto National Forest northeast of Phoenix.
Michael Chou / USA Today Network

Auroras occur when clouds of charged particles ejected from the Sun during solar storms collide with Earth’s magnetic field and interact with atoms and molecules in Earth’s upper atmosphere. The colorful display is a beautiful byproduct of that process and is usually only seen at high latitudes. But during periods of high solar activity, the light can wander farther south than usual.

However, there may also be negative consequences. Strong magnetic storms can cause problems for astronauts in space and for GPS systems and satellites in orbit.

Source: www.nbcnews.com

Webb observes auroras on cold brown dwarf star

Using NASA/ESA/CSA’s James Webb Space Telescope, astronomers detected a brown dwarf with infrared emissions from methane, likely due to energy in the upper atmosphere. The heating of the upper atmosphere that drives this emission is associated with auroras. The brown dwarf, named W1935, is located 47 light-years away.



Artist’s impression of the brown dwarf W1935. Image credit: NASA/ESA/CSA/L. Hustak, STScI.

On Earth, auroras occur when energetic particles blasted into space from the sun are captured by Earth’s magnetic field.

They cascade into the atmosphere along magnetic field lines near the Earth’s poles, colliding with gas molecules and creating eerie, dancing curtains of light.

Jupiter and Saturn have similar auroral processes that involve interaction with the solar wind, but also receive auroral contributions from nearby active moons, such as Io (for Jupiter) and Enceladus (for Saturn). Masu.

“For an isolated brown dwarf like W1935, the absence of a stellar wind that contributes to auroral processes and accounts for the extra energy in the upper atmosphere required for methane emission is puzzling,” American Airlines astronomers said. said Dr. Jackie Faherty. Natural History Museum and colleagues.

Faherty and his colleagues used Webb to observe a sample of 12 cool brown dwarf stars.

These included object W1935, discovered by citizen scientist Dan Caselden who collaborated on the Backyard Worlds Zooniverse project, and object W2220, discovered using NASA’s Wide Field Infrared Survey Explorer.

Webb revealed in great detail that W1935 and W2220 appear to be close clones of each other in composition.

Also, the brightness, temperature, and spectral characteristics of water, ammonia, carbon monoxide, and carbon dioxide were similar.

A notable exception is that W1935 showed emission from methane, in contrast to the expected absorption feature observed for W2220. This was observed at infrared wavelengths, to which Webb is uniquely sensitive.

“We expected methane to be present because it’s everywhere in these brown dwarfs,” Faherty said.

“But instead of absorbing light, we found just the opposite. The methane was glowing. My first thought was, what the hell? Why is this object emitting methane?” Do you want it?

Astronomers used computer models to deduce what might be behind the emission.

Modeling work showed that W2220 has a predictable energy distribution in its atmosphere, becoming colder with increasing altitude.

On the other hand, W1935 produced surprising results. The best models supported a temperature inversion, where the atmosphere becomes warmer as altitude increases.

“This temperature inversion is really puzzling,” says Dr. Ben Burningham, an astronomer at the University of Hertfordshire.

“We’ve seen this kind of phenomenon on planets with nearby stars that can heat the stratosphere, but it’s outrageous to see something like this on a celestial body with no obvious external heat source. .

In search of clues, researchers looked to our backyard: the planets of our solar system.

The gas giant planet could serve as a proxy for what is seen happening 47 light-years away in the atmosphere of 1935 AD.

Scientists have noticed that planets like Jupiter and Saturn have significant temperature inversions.

Research is still ongoing to understand the causes of stratospheric heating, but leading theories about the solar system include external heating by auroras and internal energy transport from deep in the atmosphere, with the former being the leading explanation. ).

According to the research team, W1935 is the first aurora candidate outside the solar system with the signature of methane emission.

It is also the coldest aurora candidate outside the solar system, with an effective temperature of about 200 degrees Celsius (400 degrees Fahrenheit).

In our solar system, the solar wind is the main contributor to the auroral process, and active satellites like Io and Enceladus play the role of planets like Jupiter and Saturn, respectively.

W1935 does not have any companion stars, so stellar winds cannot contribute to this phenomenon. It is not yet known whether an active moon is responsible for her W1935's methane emissions.

“W1935 provides a spectacular expansion of solar system phenomena without any explanatory stellar illumination,” Faherty said.

“With Webb, we can actually ‘lift the lid’ on chemistry and figure out how auroral processes are similar or different outside of our solar system.”

The authors announced that findings this week’s AAS243243rd Meeting of the American Astronomical Society, New Orleans, USA.

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Jacqueline Faherty other. 2024. JWST exhibits the auroral features of frigid brown dwarfs. AAS243Abstract #4359

Source: www.sci.news