logo
Why the northern lights seem more frequent than ever — from solar science to smartphone snapshots

Why the northern lights seem more frequent than ever — from solar science to smartphone snapshots

Yahoo28-02-2025

When you buy through links on our articles, Future and its syndication partners may earn a commission.
Why did the world suddenly become obsessed with the northern lights? It seems like not a week goes by without news of solar flares and, very often, a forecast for auroras in their wake. So are the northern lights being seen from farther south than usual? Or are people merely noticing them more?
Here's why the northern lights have become more visible and more talked about than ever over the past year.
Auroras happen when charged particles from the sun — the solar wind — interact with Earth's magnetic field. An auroral oval sits permanently over the Arctic and Antarctic circles at 66 degrees north and south, respectively. Locations in these regions — including Alaska, northern Canada, northern Scandinavia and northern Russia — frequently see auroras at night, between about 10 p.m. and 2 a.m. from late August and early April every year when there's enough darkness.
Related: Where and when to see the northern lights in 2025
"The fundamental processes that create them are always occurring," Tom Kerss, author of "The Northern Lights: The Definitive Guide to Auroras (Collins, 2021) and chief aurora hunter for Hurtigruten Astronomy Cruises, told Space.com. "The interaction between the Earth's magnetic field and the solar wind continuously produces auroral activity in the polar regions."
Solar maximum is one reason the northern lights are big news right now. The sun has a roughly 11-year solar cycle, during which our star's activity waxes and wanes. This activity includes solar flares, which are explosions on the sun; and coronal mass ejections (CMEs), which are clouds of charged particles that launch into space, sometimes in Earth's direction. During the lull in that cycle, called solar minimum, the sun's surface is blank and little happens.
When solar cycle activity picks up sunspots appear as black areas on the sun's surface. They can be seen through telescopes fitted with solar filters, and even through solar eclipse glasses. (Make sure to view the sun safely with the best solar viewing gear.) These sunspots are cooler areas of the sun's surface, and how many are visible correlates to how active the sun is. Solar maximum is declared when the number of sunspots peaks.
Scientists at NASA and the National Oceanic and Atmospheric Administration (NOAA) predicted that the current cycle, Solar Cycle 25 (the 25th since 1755, when regular daily records of sunspots began), would reach its maximum in July 2025. The error bars mean the actual peak — which is measured as the number of sunspots in a calendar month — could occur between November 2024 and March 2026. In October 2024, the same solar scientists announced that solar maximum had arrived. However, they also stated that this solar maximum period could continue for the following year.
Because they experience auroras frequently, regions under the auroral oval are the best places in the world to see the northern lights throughout the solar cycle. However, the intensity and visibility can still vary. Solar maximum periods will produce more spectacular and widespread displays, which can be visible at lower latitudes. In short, the intensity of the solar wind can increase — principally when a few CMEs arrive at Earth simultaneously to trigger a significant geomagnetic storm — causing the auroral oval to shift closer to the equator.
Solar Cycle 25 has outperformed predictions and explains why auroras have been seen farther from the Arctic and Antarctic circles. "With auroras being visible globally in May [2024] and then again in October [2024] and January [2025], it's been a special cycle so far," Kerss said.
There are generally more solar flares and CMEs during solar maximum, which, theoretically, occurs every 11 years. In practice, the sun is highly active on each side for a year or two.
"What's been fascinating about Solar Cycle 25 is that, so far, it's on track to exceed the expected performance of the previous Solar Cycle 24, and perhaps even Solar Cycle 23, which was a pretty good, strong cycle for auroras," Kerss said. In short, it's the best time to see auroras farther south than where the auroral oval is typically positioned for a couple of decades.
Related: What it's like to chase the northern lights along Norway's dramatic coastline
There are photos of the northern lights everywhere you look. Given that the last time the northern lights were seen far from the equator was a couple of years after the solar maximum in 2001, there's an obvious reason for this. Social media and smartphone apps didn't exist back then, and mobile phones had poor-quality cameras. Knowing about potential northern lights displays in advance was far less likely than it is today, when alerts and forecasts are posted on social media and sent out via smartphone notifications. And even if auroras did become visible back then, usually only experienced astrophotographers with expensive cameras had any success in photographing these colorful light displays.
In recent years, however, smartphones' low-light capabilities have improved dramatically; they have effectively doubled in quality with every new generation of phones. Even short exposures of the auroras are possible using a smartphone, as is real-time video. Now, anyone can take excellent images using a smartphone and share them with the world in seconds. Social media has also played a significant role in increasing awareness and interest in the northern lights, with platforms like Instagram driving trends in travel, including aurora viewing.
There is also a new generation of apps, such as the Glendale app, which eschews the often-misunderstood Kp index in favor of real-time solar wind data from satellites and ground stations to predict "substorms" — imminent aurora displays — and send alerts based on a user's location. Although experience in interpreting this real-time solar wind data is a huge help, the dissemination of this information on social media makes people more likely to be in the right place at the right time to witness sudden aurora displays.
Related stories:
—Solar Cycle 25 is still in max phase, so more aurora-boosting sun storms could be coming
—Aurora activity is just getting started. Here's why the best northern lights are yet to come.
—The sun in 2025: How the solar cycle will shape our year ahead
The ease of sharing aurora experiences on social media can sometimes lead to unrealistic expectations. "What we see with our eyes is not as vibrant as the camera sees," Kerss noted. The vibrant colors captured by cameras are often more intense than the human eye perceives, which can disappoint some viewers. Aurora hunters now use smartphones to check for suspect shapes in the sky and, in fact, auroras.
Solar maximum, smartphones and social media have fueled a growing interest in space weather, astronomy and Arctic tourism and have democratized aurora viewing and astrophotography. However, these factors have also brought new challenges in managing expectations and providing accurate information.

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

FAA requires SpaceX to investigate Starship Flight 9 mishap
FAA requires SpaceX to investigate Starship Flight 9 mishap

Yahoo

time9 hours ago

  • Yahoo

FAA requires SpaceX to investigate Starship Flight 9 mishap

When you buy through links on our articles, Future and its syndication partners may earn a commission. SpaceX needs to figure out what happened on the ninth test flight of its Starship megarocket, the U.S. Federal Aviation Administration (FAA) has decreed. Flight 9, which lifted off from SpaceX's Starbase site in South Texas on Tuesday (May 27), ended in the destruction of both of Starship's stages — its Super Heavy booster and Ship upper stage (which is also sometimes known, somewhat confusingly, as Starship). But the FAA, which grants launch licenses for U.S. operators, is only concerned about one of those explosive events. "The mishap investigation is focused only on the loss of the Starship vehicle, which did not complete its launch or reentry as planned," FAA officials wrote in an update today (May 30). "The FAA determined that the loss of the Super Heavy booster is covered by one of the approved test induced damage exceptions requested by SpaceX for certain flight events and system components," the agency explained. "The FAA evaluated each exception prior to launch approval and verified they met public safety requirements." SpaceX broke new ground on Flight 9, reusing a Super Heavy for the first time ever. This particular booster first flew on Flight 7 in January, acing its engine burn and then returning to Starbase for a successful and dramatic catch by the launch tower's "chopstick" arms. The company did not attempt another catch on Flight 9. It conducted a variety of experiments with the booster, including bringing it down to Earth on a higher "angle of attack" to increase atmospheric drag. So, for safety's sake, SpaceX steered Super Heavy toward a "hard splashdown" in the Gulf of Mexico on Tuesday. This didn't quite work out, however. "Contact with the booster was lost shortly after the start of landing burn when it experienced a rapid unscheduled disassembly approximately 6 minutes after launch, bringing an end to the first reflight of a Super Heavy booster," SpaceX wrote in a Flight 9 recap. Ship had an even harder time on Flight 9. The upper stage was supposed to make a soft splashdown in the Indian Ocean off the coast of Western Australia about 65 minutes after launch, but it suffered an "attitude control error" that prevented the vehicle from getting into the proper orientation for reentry. "Starship then went through an automated safing process to vent the remaining pressure to place the vehicle in the safest condition for reentry," SpaceX wrote in the recap. "Contact with Starship was lost approximately 46 minutes into the flight, with all debris expected to fall within the planned hazard area in the Indian Ocean." Related stories: — SpaceX reached space with Starship Flight 9 launch, then lost control of its giant spaceship (video) — Starship and Super Heavy explained — SpaceX loses Starship rocket stage again, but catches giant Super Heavy booster during Flight 8 launch (video) This was still a considerable improvement over Ship's performance on its previous two liftoffs. On both Flight 7 and Flight 8 (which launched in March), Ship was lost less than 10 minutes after liftoff, raining debris down over the Atlantic. There have been no reports of injuries or damage to public property as a result of the Flight 9 mishap, according to the FAA. There were also minimal effects on flights in U.S. airspace — an improvement over the previous two Starship launches. "The FAA activated a Debris Response Area, out of an abundance of caution, when the Super Heavy booster experienced its anomaly over the Gulf of America during its flyback toward Texas," FAA officials wrote. "The FAA subsequently determined the debris did not fall outside of the hazard area," they added. "During the event, there were zero departure delays, one flight was diverted, and one airborne flight was held for 24 minutes."

Pacific spiny lumpsucker: The adorable little fish with a weird suction cup resembling human teeth
Pacific spiny lumpsucker: The adorable little fish with a weird suction cup resembling human teeth

Yahoo

time11 hours ago

  • Yahoo

Pacific spiny lumpsucker: The adorable little fish with a weird suction cup resembling human teeth

When you buy through links on our articles, Future and its syndication partners may earn a commission. QUICK FACTS Name: Pacific spiny lumpsucker (Eumicrotremus orbis) Where it lives: Northern Pacific, from Washington to Japan and north into the Bering Sea What it eats: Small fish, jellyfish, ctenophores, crustaceans, polychaetes Pacific spiny lumpsuckers' tiny, plump bodies and adorable appearance make them essentially wild kawaii. They are awkward swimmers, so to avoid being swept off by currents in their coastal homes, their pelvic fin has evolved to act as a suction cup, enabling them to anchor themselves to a stable surface. At just 1 to 3 inches (2.5 to 7.6 centimeters) long, they are the smallest of the 27 species of lumpsuckers, also called lumpfish, some of which can grow as long as two feet (61 cm). Lumpfish are in the same order, Scorpaeniformes, as blobfish, sea robins and stonefish. Pacific spiny lumpsuckers are small, globular fish with extra-small fins which they flap wildly to get around. It makes them able-but-awkward swimmers. Living close to the coast and facing the pulls of tides and strong currents, their pelvic fins are fused to form a surprisingly strong sucker disc which lets them attach to rocks, coral or kelp, and, in aquariums, even to the side of a tank. These sucker discs are a bit fearsome to look at from the underside – like a lamprey with a circle of human teeth. That's because, like our teeth, those of the Pacific spiny lumpsucker are made from enamel. The disc also emits a green and yellow glow — though the reasons for this are not known. Males are usually red (see 'concerned strawberries') and glow red under ultraviolet light, while females are usually green to brown and don't glow under UV rays. RELATED STORIES —Pelican eel: The midnight zone 'gulper' with a giant mouth to swallow animals bigger than itself —Pearlfish: The eel-like fish that lives up a sea cucumber's butt —Pigbutt worm: The deep-sea 'mystery blob' with the rump of a pig and a ballooned belly When it's time to reproduce, only the males settle down. They stake out a territory, usually a shallow depression in warmer water where the females lay their eggs. The male fertilizes them and then she leaves and he tends to and guards the next generation from lumpsuckers don't yet have a defense the adults have — rows of enamel bumps called odontodes covering their bodies, including that toothy-looking circle on their undersides. Eventually, they will grow odontodes in spiral rows all around their bodies to protect them against predators and collisions with rough surfaces.

June's full 'Strawberry Moon' illuminates the night sky next week: Here's how to see it
June's full 'Strawberry Moon' illuminates the night sky next week: Here's how to see it

Yahoo

time13 hours ago

  • Yahoo

June's full 'Strawberry Moon' illuminates the night sky next week: Here's how to see it

When you buy through links on our articles, Future and its syndication partners may earn a commission. This month's full "Strawberry Moon" graces the night sky on June 11, putting on a spectacular show as the fully-lit disk of Earth's natural satellite rides low over the southeastern horizon. A full moon occurs each month when the moon is positioned opposite the sun in Earth's sky, which allows the lunar disk to be fully lit from our perspective. June's full moon is commonly referred to as the "Strawberry Moon" in America, but the nickname isn't a reference to its color (though there's a decent chance it will take on a yellow-orange hue when near the horizon due to our atmosphere's habit of scattering certain wavelengths of light). Rather, the evocative name is thought to have been coined by the Native American Algonquian tribes in reference to the short strawberry harvesting season that falls around this time of year, according to the Old Farmer's Almanac. Other cultures have dubbed the event the Blooming Moon, Green Corn Moon, Birth Moon and Hatching moon, to name a few. Regardless of what you call it, one thing is certain: June's full moon is sure to put on a spectacular display when it lights up the night sky next week. This month's full moon phase will occur during the early hours of June 11 for viewers in New York, at 3:44 a.m. EDT (0744 GMT). The exact timing of the event will vary depending on your location on Earth, so be sure to check a trusted website such as for specifics about your locale. The lunar disk will appear fully lit to stargazers across America when it rises above the southeastern horizon at sunset on June 10, marking the best opportunity for the astrophotography community to capture the Strawberry Moon close to the horizon. Earth's natural satellite will appear particularly large to the naked eye at moonrise thanks to the little-understood "moon illusion," a strange effect wherein the human brain convinces us that objects are larger than they actually are when in close proximity to the horizon. Each year, June's full moon treads a predictably low path across the spring sky due to its close proximity to the summer solstice — the time of the year when the sun is at its highest. This year's Strawberry Moon will ride exceptionally low — the lowest in decades according to stargazing site — thanks in part to a phenomenon that sees the moon's tilted orbit dragged around by the sun's gravitational influence. Editor's Note: If you snap a picture of the full 'Strawberry Moon' and want to share it with readers, then please send your photo along with comments about the shoot, your name and location to spacephotos@

DOWNLOAD THE APP

Get Started Now: Download the App

Ready to dive into the world of global news and events? Download our app today from your preferred app store and start exploring.
app-storeplay-store