Helio Highlights: May 2025

Helio Highlights: May 2025

3 min read

Helio Highlights: May 2025

3 Min Read

Helio Highlights: May 2025

A grayscale top-down image of the North Pole showing the glowing band of the Northern Lights circling the Earth
A satellite image showing the extent of the Northern Lights during part of the Mother’s Day 2024 solar storms.
Credits:
NOAA

One year ago, solar storms lit up the night sky. Why?

The Sun is 93 million miles away from Earth, on average. Even though it’s far away, we can still see and feel its effects here. One of the most beautiful effects are the auroras – colorful lights that dance across the sky near the North and South Poles. These are also called the Northern and Southern Lights. They happen when tiny particles from the Sun hit gas molecules in our atmosphere and give off energy.

Sometimes the Sun becomes very active and sends out a lot more energy than normal. When this happens, we can see auroras in places much farther from the poles than normal. In May 2024, around Mother’s Day, the Sun sent powerful solar storms in the direction of Earth. These storms were also called the Gannon Storms, named after Jennifer Gannon, a scientist who studied space weather. The Northern Lights could be seen as far south as Puerto Rico, Hawaii, Mexico, Jamaica, and the Bahamas. The Southern Lights were also visible as far north as South Africa and New Zealand.

Red and green streaks of an aurora radiate out from the center of the photo. Black silhouettes of trees line the edge.
Aurora Borealis seen from British Columbia, Canada on May 10, 2024.
NASA/Mara Johnson-Groh

Scientists who study the Sun and its effects on our solar system work in a field called heliophysics. Their studies of the Sun have shown that it goes through cycles of being more active and less active. Each one of these cycles lasts about 11 years, but can be anywhere from 8 to 14 years long. This is called the Solar Cycle.

The middle of each cycle is called Solar Maximum. During this time, the Sun has more dark spots (called sunspots) and creates more space weather events. The big storms in May 2024 happened during the Solar Maximum for Solar Cycle 25.

On May 8 and 9, 2024, an active area on the Sun called AR3664 shot out powerful solar flares and several huge bursts of energy called coronal mass ejections (CMEs). These CMEs headed straight for Earth. The first CME pushed aside the normal solar wind, making a clear path for the others to reach us faster. When all this energy hit our atmosphere, it created auroras much farther from the poles than usual. It was like the Sun gave the auroras a huge power boost!

A grayscale top-down image of the North Pole showing the glowing band of the Northern Lights circling the Earth
Eruptions of Solar material into space as seen on May 7 (right) and May 8 (left), 2024. These types of eruptions often come just before a larger Coronal Mass Ejection (CME), including the ones which caused the Mother’s Day solar storms.
NASA/SDO

Auroras are beautiful to watch, but the space weather that creates them can also cause problems. Space weather can mess up radio signals, power grids, GPS systems, and satellites. During the May 2024 storms, GPS systems used by farmers were disrupted. Many farmers use GPS to guide their self-driving tractors. Since this happened during peak planting season, it may have cost billions of dollars in lost profit.

Because space weather can cause so many problems, scientists at NASA and around the world watch the Sun closely to predict when these events will happen. You can help too! Join local science projects at schools, teach others about the Sun, and help make observations in your area. All of this helps us to learn more about the Sun and how it affects our planet.

Here are some resources to connect you to the Sun and auroras

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Stellar Duo

Stellar Duo

Two stars with diffraction spikes shine brightly in the image. The larger star, at lower right, is in a bright blue cloud of gas and dust, while the smaller star at upper left is in a red haze. The clouds are somewhat patchy. Smaller red stars are scattered around them.
ESA/Hubble & NASA, J. Bally, M. Robberto

NASA’s Hubble Space Telescope captured a bright variable star, V 372 Orionis, and its companion in this festive image in this image released on Jan. 27, 2023. The pair lie in the Orion Nebula, a colossal region of star formation roughly 1,450 light-years from Earth.

V 372 Orionis is a particular type of variable star known as an Orion Variable. These young stars experience some tempestuous moods and growing pains, which are visible to astronomers as irregular variations in luminosity. Orion Variables are often associated with diffuse nebulae, and V 372 Orionis is no exception; the patchy gas and dust of the Orion Nebula pervade this scene.

Text credit: European Space Agency (ESA)

Image credit: ESA/Hubble & NASA, J. Bally, M. Robberto

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Monika Luabeya

Curiosity Blog, Sols 4589 – 4592: Setting up to explore Volcán Peña Blanca

Curiosity Blog, Sols 4589 – 4592: Setting up to explore Volcán Peña Blanca

A grayscale photo of a Martian landscape shows very rough, rocky, and cracked terrain
Navcam view of the ~3 ft high ridge that marks the eastern side of Volcán Peña Blanca.  The ridge is currently about 35 ft away from the rover, and the team used images like this during today’s planning to decide the exact location for Curiosity’s approach.
NASA/JPL-Caltech

Written by Abigail Fraeman, Deputy Project Scientist at NASA’s Jet Propulsion Laboratory

Earth planning date: Thursday, July 3, 2025

The team was delighted this morning to learn that Wednesday’s drive had completed flawlessly, placing us in a stable position facing a ~3 foot high ridge located ~35 feet away.  This ridge is the eastern edge of a feature the team has informally named “Volcán Peña Blanca.” This feature certainly looked intriguing in orbital images, but once we saw Curiosity’s pictures of it from the ground, we decided it was cool enough to spend the time to investigate it closer.  The images from the ground show a lot more detail than is visible in orbit, including clear sedimentary structures exposed along the ridge face which could provide important clues about how the rocks in the boxwork-bearing terrain were initially deposited – dunes? Rivers? Lakes? The team picked their favorite spot to approach the ridge and take a closer look during Wednesday’s planning, so Curiosity made a sharp right turn to take us in that direction.  Using today’s images, we refined our plan for the exact location to approach and planned a drive to take us there, setting us up for contact science on Monday.

We had the opportunity to plan four sols today, to cover the U.S. 4th of July holiday weekend, so there was lots of time for activities besides the drive.  Curiosity is currently sitting right in front of some light toned rocks, including one we gave the evocative name “Huellas de Dinosaurios.” It’s extremely unlikely we’ll see dinosaur footprints in the rock, but we will get the chance to investigate it with APXS, MAHLI, and ChemCam.  We also have a pair of ChemCam only targets on a more typical bedrock target named “Amboro” and some pebbles named “Tunari.”  Mastcam will take a high resolution of mosaic covering Volcán Peña Blanca, some nearby rocks named “Laguna Verde,” a small light colored rock named “Suruto,” and various patterns in the ground. Two ChemCam RMI mosaics of features in the distant Mishe Mokwa face and environment monitoring activities round out the plan.

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Curiosity Blog, Sol 4588: Ridges and troughs

Curiosity Blog, Sol 4588: Ridges and troughs

A grayscale photo of a Martian landscape shows very rough, rocky, and cracked terrain extending from the foreground to a horizon line in the distance, across the middle of the frame.
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4,587 (2025-07-02 07:33:39 UTC).
NASA/JPL-Caltech

Written by Lucy Thompson, APXS Collaborator and Senior Research Scientist at the University of New Brunswick, Canada

Earth planning date: Wednesday, July 2, 2025

As we traverse the boxwork terrain, we are encountering a series of more resistant ridges/bedrock patches, and areas that are more rubbly and tend to form lower relief polygonal or trough-like features. We came into planning this morning in one of the trough-like features after another successful drive. The science team is interested in determining why we see these different geomorphological and erosional expressions. Is the rock that comprises the more resistant ridges and patches a different composition to the rock in the troughs and low relief areas? How do the rocks vary texturally? Might the resistant bedrock be an indicator of what we will encounter when we reach the large boxworks that we are driving towards?

We managed to find a large enough area of rock to safely brush (target – “Guapay”), after which we will place APXS and MAHLI to determine the composition and texture. ChemCam will also analyze a different rock target, “Taltal” for chemistry and texture, and we will also acquire an accompanying Mastcam documentation image. The resistant ridge that we are planning to drive towards (“Volcan Pena Blanca”) and eventually investigate will be captured in a Mastcam mosaic. ChemCam will utilize their long-distance imaging capabilities to image the “Mishe Mokwa” butte off to the southeast of our current location, which likely contains bedrock layers that we will eventually pass through as we continue our climb up Mount Sharp.

After a planned drive, taking us closer to the “Volcan Pena Blanca” ridge, MARDI will image the new terrain beneath the wheels, before we execute some atmospheric observations. Mastcam will make a tau observation to monitor dust in the atmosphere and Navcam will acquire a zenith movie. Standard DAN, RAD and REMS activities round out the plan.

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Week Starts with Muscle Stimulation and Cellular Research During Cargo Transfers

Week Starts with Muscle Stimulation and Cellular Research During Cargo Transfers

This long-duration photograph was taken from the International Space Station orbiting 260 miles above the Indian Ocean off the coast of the Indonesian island of Java. City lights and lightning storms streak below star trails above Earth's atmopsheric glow.
This long-duration photograph was taken from the International Space Station orbiting above the Indian Ocean off the coast of the Indonesian island of Java. City lights and lightning storms streak below stars trailing above Earth’s atmopsheric glow.
NASA

The Expedition 73 crew kicked off the week studying electrical muscle stimulation and cellular immunity to protect crew health in microgravity. The orbital residents are also unpacking a new cargo craft and continuing to support the Axiom Mission 4 (Ax-4) crew aboard the International Space Station.

NASA Flight Engineers Nichole Ayers and Anne McClain joined each other in the Columbus laboratory module on Monday and explored stimulating muscles with small electrical signals to help prevent space-caused muscle atrophy. Ayers wore electrodes as McClain operated biomedical gear sending electrical impulses to her legs simulating load forces on the ground. Researchers are exploring electrical muscle stimulation to supplement daily space workouts and keep astronauts fit in weightlessness.

Ayers then partnered with NASA Flight Engineer Jonny Kim assisting him as he inspected hatches in the Quest airlock and the Harmony module and downlinked photographs for further analysis by engineers on the ground. Kim began his day in the Tranquility module replacing orbital plumbing components then switched over to the Destiny laboratory module and swapped out research hardware.

Station Commander Takuya Onishi from JAXA (Japan Aerospace Exploration) began his shift with a standard cognition test then documented his meals and medication for the day. Afterward, Onishi set up computer hardware that supports the advanced resistive exercise device then collected his saliva samples for stowage in the Kubik incubator and later analysis to study cellular changes in microgravity.

Before she assisted Ayers, McClain serviced spacesuit life support gear then checked cable connections on a computer that supports the MUSES commercial Earth observation hardware. McClain also worked throughout the day supporting the Ax-4 crew members as they conducted their private research.

Veteran astronaut and Ax-4 Commander Peggy Whitson spent Monday assisting her Ax-4 crewmates Shubhanshu Shukla, Sławosz Uznański-Wiśniewski, and Tibor Kapu during their busy day of space experiments. The quartet explored a wide array of subjects including space agriculture to provide fresh food for crews, how blood circulates in space, a human-computer interface, and more on Monday.

The new Progress 92 cargo craft is being unloaded today after its docking to the Poisk module on Saturday, July 5. Roscosmos Flight Engineers Sergey Ryzhikov and Alexey Zubritskiy opened Progress’ hatch on Sunday and continued working into Monday transferring some of its three tons of food, fuel, and supplies into the orbital outpost. Ryzhikov later activated a camera pointed at Earth that students will remotely control for a weeklong observation session. Flight Engineer Kirill Peskov assisted his cosmonaut crewmates with the cargo work, worked on computer electronics gear, and photographed the external condition of Poisk with the Progress 92 docked to it.

Learn more about station activities by following the space station blog, @space_station on X, as well as the ISS Facebook and ISS Instagram accounts.

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Mark A. Garcia