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By NASA
Explore This Section Science Uncategorized Helio Highlights: July… Home Framework for Heliophysics Education About Helio Big Idea 1.1 Helio Big Idea 1.2 Helio Big Idea 1.3 Helio Big Idea 2.1 Helio Big Idea 2.2 Helio Big Idea 2.3 Helio Big Idea 3.1 Helio Big Idea 3.2 Helio Big Idea 3.3 Helio Missions Helio Topics Resource Database About NASA HEAT More Highlights Space Math 5 min read
Helio Highlights: July 2025
5 Min Read Helio Highlights: July 2025
When astronauts return to the Moon, they will need to know what the Sun is doing in order to keep themselves safe and healthy. Credits:
NASA A Trip to the Moon
In July 1969, astronauts Neil Armstrong and Buzz Aldrin became the first humans to walk on the Moon. Now, NASA and its international partners in the Artemis accords are working to send humans back there, this time to stay. The trip will be challenging, especially since space is a very uninviting place for humans! One unexpected source of danger will be the Sun.
The Sun: Friend and Foe
The energy the Sun provides allows life on Earth to thrive. But this energy can also be dangerous to us. This danger can be as simple as getting a sunburn if you are out in the sunlight for too long, or as complex as a geomagnetic storm causing chaos in our satellite network.
This animation demonstrates a simulation by the MAGE model of Earth’s magnetosphere being hit by a geospace storm in May 2024, the strongest in nearly 20 years. Storms like this are caused by solar weather that could endanger astronauts en route to the Moon or active on its surface during future missions. NASA’s Scientific Visualization Studio and CGS Team Things get more complicated in space. On Earth, the atmosphere and magnetosphere protect us from most solar energy. But spacecraft and astronauts in space don’t have this protection. For astronauts on upcoming Artemis missions to the Moon, the Sun’s radiation could cause anything from ruined electronics to a greater long-term risk of cancer.
The Real Risks
On August 2, 1972, a massive solar storm began with the eruption of sunspot MR11976. One of the Coronal Mass Ejections (CMEs) it produced raced from the Sun to Earth in less than 15 hours. That’s a record that still stands today! This led to power grid fluctuations and caused havoc with spacecraft in flight. Recently declassified U.S. military records show that the storm caused sea mines off the Vietnamese coast to explode, as well.
Importantly, the August 1972 solar storm happened in between the Apollo 16 and 17 missions to the Moon. Studies show that astronauts en route to the Moon, and especially astronauts on the surface, could have been badly sickened by the radiation that came with it. This threat remains real if a solar storm of similar severity were to occur during future Lunar missions.
Watchful Protectors
Organizations like NASA and NOAA keep an eye on the Sun, to forecast potential sources of danger. If a solar flare or Coronal Mass Ejection (CME) is on the way, scientists should be able to spot the danger ahead of time so that steps can be taken to reduce the damage. For astronauts going to the Moon, this may be as simple as taking shelter in a special part of their spacecraft.
An animated gif of a Coronal Mass Ejection (CME) erupting from the surface of the Sun in September 2024. If a CME like this was aimed at the Moon, the intense energy it carried could damage spacecraft electronics and even cause severe radiation sickness in astronauts. NOAA/NASA NOAA’s Space Weather Follow-On (SWFO) program sustains their space weather observations and measurements. NOAA’s CCOR-1 flew on the GOES-19 spacecraft and provides crucial near-real-time CME data. The CCOR-2 instrument will fly on SWFO-L1. Other missions include SOHO, a long-running collaboration between NASA and the European Space Agency, and HERMES, a NASA heliophysics instrument intended for the Lunar Gateway that will orbit the Moon.
NASA’s Moon to Mars Space Weather Analysis Office (M2M SWAO) also conducts real-time space weather assessments. These support new capabilities for understanding space weather impacts on NASA exploration activities, including on the Moon.
The Moon as a Laboratory
A big part of the reason we want to go back to the Moon is the amazing level of information we can learn about the history of the Solar System. “Any object in our solar system doesn’t just exist in isolation,” explains Prabal Saxena, a Research Space Scientist in the Planetary Geology, Geophysics & Geochemistry Lab at NASA’s Goddard Space Flight Center. “It is constantly interacting with meteorites and meteors. That’s why you see a lot of the impact creators on the Moon. But it is also constantly interacting with the Sun.” This can come from the solar wind, CMEs, and other forms of solar energy hitting the Moon’s barren surface.
Pictured is the Lunar Swirl Reiner Gamma, a geological feature on the surface of the moon. In areas that are magnetically protected, the ground stays relatively bright. Just outside of the shielded regions, radiation-induced chemical reactions darken the landscape, effectively “sunburning” the lunar surface. NASA/GSFC/Arizona State University Saxena points out that the Moon’s relative lack of a magnetosphere means that Lunar surface material effectively traps evidence of the past habits of the Sun. “A lot of the energetic particles that we would otherwise see deflected by Earth’s magnetosphere and atmosphere are impacting the surface of the Moon. So you can actually trace back what the history of the Sun might be.”
He compares this to scientists taking ice cores to get a glimpse into Earth’s atmospheric history. With everything from evidence of the prehistoric solar atmosphere to information on how the Sun affects water on the lunar surface locked in rocks left largely untouched for millions of years, it is clear why NASA wants to go back and have another look around.
Going Back
But it is still important to keep an eye on the potential dangers to explorers both metallic and organic. In an interview, Lennard Fisk, former NASA Associate Administrator for Space Science and Applications, described a conversation he had with Neil Armstrong. More than anything else during Apollo 11, Armstrong was afraid of a solar flare. He knew he could depend on his spacecraft and crewmates. But space weather was an uncontrollable variable.
We had a different understanding of space weather in 1969. Space radiation, including the solar wind, was a new discovery back then. But research done in those early days helped make breakthroughs still paying off today, and we are building upon these discoveries with new missions that continue to advance our knowledge of the Sun and the rest of our solar system.
Additional Resources
Lesson Plans & Educator Guides
NASA Helio Club
Study Unit
Six lessons created for a middle-school audience to introduce basic heliophysics concepts to learners.
Space Weather Math
Hands-on activities with embedded math problems that explore the causes and effects of space weather.
“Solar Storms and You” Educator Guide
A downloadable educator guide with a variety of activities on the science of solar storms for learners grades 5-8.
Interactive Resources
Magnetic Earth
Interactive Resource
An animation with information on Earth’s magnetic field and its role in creating northern lights, and an interactive activity allowing students to experiment with magnetism.
Student HelioViewer:
Solar Data Interactive
A student-friendly interactive with accessible NASA data about the Sun and its features, including solar flares, magnetic fields, sunspots, and Coronal Mass Ejections (CMEs).
Webinars & Slide Decks
What is Space
Weather Video
This approximately 3-minute video summarizes space weather and explains its effects on the rest of the Solar System.
Science Update: Space Weather on Our
Approach to Solar Max
A webinar about the solar storm on May 10th, 2024, which led to auroras being visible across North America.
Astronaut Dr. John
Phillips Discusses
Space Radiation
Dr. John Phillips, NASA astronaut and space plasma physicist, talks about his work and personal experience with space radiation on the Space Weather Living History podcast.
Dr. Lennard Fisk
Discusses Heliophysics History at NASA
Former Associate Administrator Dr. Lennard Fisk recounts the evolution of the Heliophysics Division at NASA.
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By NASA
Skywatching Skywatching Home What’s Up Meteor Showers Eclipses Daily Moon Guide More Tips & Guides Skywatching FAQ Night Sky Network Venus-Jupiter Conjunction and Meteor Mojo
Jupiter and Venus shine brightly in the mornings as they appear to graze each other in the sky on the 11th and 12th. The Perseids are washed out by the Moon.
Skywatching Highlights
All Month – Planet Visibility:
Mercury: Pops up above the horizon during the second half of August. Appears very low, below 10 degrees altitude. Venus: Shines very brightly in the east each morning before sunrise, about 20 to 30 degrees above the horizon. Mars: Can be observed low in the west during the hour after sunset, appearing about as bright as the brightest stars in the Big Dipper. Jupiter: Appears in the east each morning, together with Venus, but much less bright. Saturn: Observable late night to dawn. Rises around 10:30 p.m. early in the month, and around 8:30 p.m. by the end of the month. Find it high in the south as sunrise approaches. Skywatching Highlights:
August 11 & 12 – Venus-Jupiter Conjunction – The two brightest planets have a close meetup over several days, appearing closest over two days on the 11th and 12th, at just a degree apart.
August 19 & 20 – Moon with Jupiter & Venus – A slim lunar crescent joins Jupiter and Venus — still relatively close in the sky after their conjunction. They appear in the east in the several hours preceding sunrise.
August 12th-13th – Perseids Peak – The celebrated annual meteor shower will be hampered by an 84%-full Moon on the peak night. A few bright meteors may still be seen in the pre-dawn hours, but viewing conditions are not ideal this year.
All month – The Dumbbell Nebula (M27) – One of the easiest planetary nebulas to observe, M27 appears within the Summer Triangle star pattern, high overhead in the first half of the night.
Transcript
What’s Up for August? Jupiter and Venus have a morning meetup, we check out this year’s Perseid meteor shower, and peek into the future of our own Sun.
Mars is the lone planet in the early evening sky this month, visible low in the west for about an hour after the sky starts to darken. It’s now only about 60% as bright as it appeared back in May.
Saturn is rising by about 10 pm, and you’ll see it showing up a bit earlier each evening as the month goes on. You’ll find it in the east after dark with the constellations Cassiopeia and Andromeda. The Ringed Planet makes its way over to the western part of the sky by dawn, where early risers will find it on August mornings.
The real highlight of August is the close approach of Jupiter and Venus. They shine brightly in the east before sunrise throughout the month. The pair begin the month farther apart, but quickly approach each other in the sky. They appear at their closest on the 11th and 12th — only about a degree apart. Their rendezvous happens against a backdrop of bright stars including Orion, Taurus, Gemini, and Sirius. A slim crescent Moon joins the pair of planets after they separate again, on the mornings of the 19th and 20th.
Sky chart showing the eastern sky before sunrise on August 11th, with Venus and Jupiter only a degree apart. NASA/JPL-Caltech One of the best annual meteor showers, the Perseids, peaks overnight on August 12th and into the 13th. Unfortunately, this year the Moon is nearly full on the peak night, and its glare will wash out all but the brightest meteors. While that’s not so great for Perseid watchers, the good news is that another favorite annual meteor shower, the Geminids, is poised for Moon-free viewing in December.
August is a great time to see one of the easiest-to-observe nebulas in the sky.
The Dumbbell Nebula, also known as M27, is high overhead on August nights. It’s a type of nebula called a “planetary nebula.”
A nebula is a giant cloud of gas and dust in space, and planetary nebulas are produced by stars like our Sun when they become old and nuclear fusion ceases inside them. They blow off their outer layers, leaving behind a small, hot remnant called a white dwarf. The white dwarf produces lots of bright ultraviolet light that illuminates the nebula from the inside, as the expanding shell of gas absorbs the UV light and re-radiates it as visible light.
The Dumbbell Nebula, nicknamed for its dumbbell-like shape, appears as a small, faint patch of light about a quarter of the width of the full moon in binoculars or a small telescope. It lies within the Summer Triangle, a pattern of stars that’s easy to find overhead in the August sky. You’ll find the nebula about a third of the way between its bright stars Altair and Deneb.
Sky chart showing the Summer Triangle asterism, with the location of the Dumbbell Nebula (M27) indicated. NASA/JPL-Caltech Here’s hoping you get a chance to observe this glimpse into the future that awaits our Sun about 5 billion years from now. It’s part of a cycle that seeds the galaxy with the ingredients for new generations of stars and planets — perhaps even some not too different from our own.
Here are the phases of the Moon for August.
The phases of the Moon for August 2025. NASA/JPL-Caltech You can stay up to date on all of NASA’s missions exploring the solar system and beyond at science.nasa.gov. I’m Chelsea Gohd from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.
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By European Space Agency
Week in images: 28 July - 1 August 2025
Discover our week through the lens
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By NASA
View of the NASA Glenn Research Center hangar from the Cleveland Hopkins International Airport runway during a testing flight on Thursday, June 13, 2024. The Operations and Integration Building sits to the hangar’s right.Credit: NASA/Sara Lowthian Hanna NASA’s Glenn Research Center in Cleveland is seeking proposals for the use of its historic aircraft hangar, along with a parking lot, tarmac, and a small neighboring office building. Proposals are due by 1 p.m. EDT on Nov. 28.
The hangar, formally known as the Flight Research Building, is available for lease by signing a National Historic Preservation Act agreement for a 10-year base period and two optional five-year extensions.
NASA first announced plans to lease the Flight Research Building and other facilities in May 2024 under the government’s Enhanced Use Lease authority. These lease agreements allow space, aeronautics, and other related industries to use agency land and facilities, reducing NASA’s maintenance costs while fostering strategic partnerships that spur innovation.
“Glenn is making great progress as we modernize our Cleveland and Sandusky campuses to support NASA’s future missions,” said Dr. Jimmy Kenyon, Glenn’s center director. “Through Enhanced Use Leases, we’re ensuring full use of land and facilities while preserving an iconic, historic building and creating regional economic opportunities.”
The property available for lease includes up to 6.7 acres of land, which contains the heated aircraft hangar, Operations and Integration Building, parking lot, and tarmac. The hangar is 160 feet by 280 feet, and the Operations and Integration Building is 5,947 square feet. Proceeds from this lease will be used to maintain Glenn facilities and infrastructure.
Visible from Brookpark Road and Cleveland Hopkins International Airport, Glenn’s hangar was the first building completed after the center was established in 1941. It has sheltered many unique aircraft used to perform vital research. From studying ice accumulation on aircraft wings to the first use of laser communications to stream 4K video from an aircraft to the International Space Station, Glenn flight research has contributed to aviation safety, atmospheric studies, and cutting-edge technology development.
Interested parties should contact both Carlos Flores at carlos.a.flores-1@nasa.gov and Diana Munro at diana.c.munro@nasa.gov to sign up for a walk-through from Monday, Sept. 8, to Friday, Sept. 12, or the week of Oct. 6.
For a 360-degree virtual tour of the Flight Research Building, visit:
https://www3.nasa.gov/specials/hangar360/
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Jan Wittry
Glenn Research Center, Cleveland
216-433-5466
jan.m.wittry-1@nasa.gov
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