logo
Here's How and When You Can See the Eta Aquariid Meteor Shower

Here's How and When You Can See the Eta Aquariid Meteor Shower

Yahoo03-05-2025

The night sky during the Eta Aquariid meteor shower in Ratnapura, Sri Lanka, on May 5, 2024. Credit - Thilina Kaluthotage—Getty Images
The weeks-long Eta Aquariid meteor shower is about to reach its peak, and people across both the Northern and Southern Hemispheres will have the opportunity to enjoy the spectacular event, which is visible to the naked eye.
Here's what people need to know in order to get the best glimpse at the Eta Aquariids.
The Eta Aquariids meteor shower peaks in May of each year, per NASA. These meteors are specifically known for their speed, and Eta Aquariid meteors can travel about 40.7 miles (65.4 kilometers) per second into Earth's atmosphere, leaving trails behind them which observers can view for several seconds to minutes.
The Eta Aquariids are created from space debris that originate from comet 1P/Halley—often considered the most famous comet. Each time Halley returns to the inner solar system, it sprays ice and rock, and though Halley only makes its way around the Sun every 76 years or so, its debris causes two different meteor showers each year: the Eta Aquariid meteor shower in May and the Orionids in October.
While expert viewpoints differ as to the exact dates and peak times, according to the American Meteor Society (AMS), the Eta Aquariids have been active since April 15, and are expected to remain so until May 27. They are set to peak on the mornings of May 4, 5, and 6. These are the ideal mornings for those in the Northern Hemisphere to view the meteor shower, and under optimal conditions—meaning without city lights—observers should be able to see about 10 to 15 Eta Aquariids per hour.Areas in the United States that boast lower instances of light pollution—such as national parks like Big Bend in Texas or Death Valley in California—will have prime viewing opportunities. Although safety precautions should be paramount for skywatchers venturing into the great outdoors.
However, those in the Southern Hemisphere will have optimal viewing opportunities, and, if lucky, could see over 50 meteors per hour.
According to NASA, the best time to watch will be at 2 a.m. local time on May 6. It's recommended that viewers give their eyes some time—around 30 minutes—to adjust to the dark. 'Avoid looking at bright lights, such as your cell phone, too, as this will take your eyes off the sky and ruin your night vision,' reads the guidance from NASA.
Viewers do not need telescopes or any special equipment to enjoy the event, but the darker the sky, the easier it will be to view the meteor shower, and the AMS states that even 'a gain of one magnitude in sky darkness can lead to a doubling of observed meteors.' So, it is suggested for those near city lights to travel away from the brightly-lit streets.
Contact us at letters@time.com.

Orange background

Try Our AI Features

Explore what Daily8 AI can do for you:

Comments

No comments yet...

Related Articles

NASA orbiter saw something astonishing peek through Martian clouds
NASA orbiter saw something astonishing peek through Martian clouds

Yahoo

time2 hours ago

  • Yahoo

NASA orbiter saw something astonishing peek through Martian clouds

NASA's longest-running Mars mission has sent back an unprecedented side view of a massive volcano rising above the Red Planet, just before dawn. On May 2, as sunlight crept over the Martian horizon, the Odyssey spacecraft captured Arsia Mons, a towering, long-extinct volcano, puncturing a glowing band of greenish haze in the planet's upper atmosphere. The 12-mile-high volcano — nearly twice the height of Mauna Loa in Hawaii — punctures a veil of fog, emerging like a monument to the planet's ancient past. The space snapshot is both visually arresting and scientifically enlightening. "We picked Arsia Mons hoping we would see the summit poke above the early morning clouds," said Jonathon Hill, who leads Odyssey's camera operations at Arizona State University, in a statement, "and it didn't disappoint." SEE ALSO: An enormous Martian cloud returns every spring. Scientists found out why. Arsia Mons sits at the southern end of a towering trio of volcanoes called the Tharsis Montes. Credit: NASA / JPL-Caltech To get this view, Odyssey had to do something it wasn't originally built for. The orbiter, which has been flying around Mars since 2001, usually points its camera straight down to map the planet's surface. But over the past two years, scientists have begun rotating the spacecraft 90 degrees to look toward the horizon. That adjustment allows NASA to study how dust and ice clouds change over the seasons. Though the image is still an aerial view, the vantage point is of the horizon, similar to how astronauts can see Earth's horizon 250 miles above the planet on the International Space Station. From that altitude, Earth doesn't fill their entire view — there's enough distance and perspective for them to see the planet's curved edge meeting the blackness of space. Odyssey flies above Mars at about the same altitude. Arsia Mons sits at the southern end of a towering trio of volcanoes called the Tharsis Montes. The Tharsis region is home to the largest volcanoes in the solar system. The lack of plate tectonics on the Red Planet allowed them to grow many times larger than those anywhere on Earth. Together, they dominate the Martian landscape and are sometimes covered in clouds, especially in the early hours. But not just any clouds — these are made of water ice, a different breed than the planet's more common carbon dioxide clouds. Arsia Mons is the cloudiest of the three. Scientists have recently studied a particular, localized cloud formation that occurs over the mountain, dubbed the Arsia Mons Elongated Cloud. The transient feature, streaking 1,100 miles over southern Mars, lasts only about three hours in the morning during spring before vanishing in the warm sunlight. It's formed by strong winds being forced up the mountainside. The cloudy canopy on display in Odyssey's new image, according to NASA, is called the aphelion cloud belt. This widespread seasonal system drapes across the planet's equator when Mars is farthest from the sun. This is Odyssey's fourth side image since 2023, and it is the first to show a volcano breaking through the clouds. "We're seeing some really significant seasonal differences in these horizon images," said Michael D. Smith, a NASA planetary scientist, in a statement. "It's giving us new clues to how Mars' atmosphere evolves over time."

NASA's Parker Solar Probe spots powerful magnetic explosion aimed at the sun's surface
NASA's Parker Solar Probe spots powerful magnetic explosion aimed at the sun's surface

Yahoo

time3 hours ago

  • Yahoo

NASA's Parker Solar Probe spots powerful magnetic explosion aimed at the sun's surface

When you buy through links on our articles, Future and its syndication partners may earn a commission. While making a death-defying dive through the sun's atmosphere, NASA's Parker Solar Probe has directly recorded a powerful plasma explosion heading toward our star's surface in unprecedented detail. Parker's new measurements found protons with about 1000 times greater energy than expected and a plasma jet shooting toward the sun, not away from it. Parker was uniquely positioned between the sun and the particles' source, allowing scientists to easily figure out where they came from. These findings indicate that the complexity and strength of tangles in the sun's magnetic field can accelerate charged particles to much greater speeds than expected from the field's strength alone. The sunward plasma jet was caused by "magnetic reconnection" in the sun's atmosphere — the explosive process in which magnetic fields fracture and reconnect. The powerful phenomenon transforms energy stored in the sun's magnetic field into energy that accelerates the solar wind — the constant stream of charged particles that the sun blasts across the solar system. Understanding magnetic reconnection is critical for making better predictions about space weather, which is driven by the solar wind and other energetic outbursts from our star. Space weather is a primary suspect for what stripped away Mars' atmosphere, turning it from a habitable planet into an icy desert wasteland. On Earth, space weather can trigger geomagnetic storms that cause blackouts, damage satellites, interfere with radio and GPS signals, and even put astronauts at risk. On the bright side, it also gives Earth its signature glorious auroras. The sun's magnetic field is extremely powerful, complex and dynamic. Space weather predictions require complicated computer simulations based on equations that describe how magnetic fields behave — but the sun is so large and convoluted that these equations will always be approximations. To improve the models' accuracy, scientists must collect extremely detailed measurements of the sun. This is where the Parker Solar Probe comes in. The Parker Solar Probe is the first mission to fly into the sun's upper atmosphere, called the corona. It has been directly measuring magnetic fields and particles in and around the corona in unprecedented detail, providing scientific insight into the heliosphere (the sun's atmosphere, which encompasses the entire solar system in a massive, elongated bubble). Related: NASA's daredevil solar spacecraft survives 2nd close flyby of our sun "These findings indicate that magnetic reconnection … is an important source of energetic particles in the near-Sun solar wind," lead study author Mihir Desai, director of the Southwest Research Institute's Department of Space Research, said in a statement. "Everywhere there are magnetic fields there will be magnetic reconnection. But the Sun's magnetic fields are much stronger near the star, so there's a lot more stored energy to be released." Understanding the workings of magnetic reconnection events could help scientists better predict harmful space weather, the researchers said. RELATED STORIES —New 8K-resolution photos of the sun show off incredible details of raging sunspots —Space photo of the week: Pink 'raindrops' on the sun captured in greatest detail ever —Powerful Mother's Day geomagnetic storm created radio-disrupting bubbles in Earth's upper atmosphere "Reports from the American Meteorological Society indicated that the powerful solar events in May 2024 wreaked havoc with farmers when extreme geomagnetic storms disrupted the precise GPS-guided navigation systems used to plant, fertilize and harvest rows of seeds, causing an estimated loss of up to $500 million in earning potential," Desai said. "Parker's access to this new data is critical, particularly as we remain in the midst of a very active solar cycle." The latest measurements of magnetic reconnection, reported in a paper published May 29 in The Astrophysical Journal Letters, are one of many new discoveries Parker has made. In 2023, over 700 peer-reviewed scientific papers were published using data collected in the probe's first four years of operation, and there are still many more discoveries to be made. The spacecraft completed its second ultra-close flyby of the sun on March 22, zooming within 3.8 million miles (6.1 million kilometers) of the sun's surface — matching its own record from December 2024.

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