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By NASA
6 min read
NASA, NOAA: Sun Reaches Maximum Phase in 11-Year Solar Cycle
In a teleconference with reporters on Tuesday, representatives from NASA, the National Oceanic and Atmospheric Administration (NOAA), and the international Solar Cycle Prediction Panel announced that the Sun has reached its solar maximum period, which could continue for the next year.
The solar cycle is a natural cycle the Sun goes through as it transitions between low and high magnetic activity. Roughly every 11 years, at the height of the solar cycle, the Sun’s magnetic poles flip — on Earth, that’d be like the North and South poles swapping places every decade — and the Sun transitions from being calm to an active and stormy state.
Visible light images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, Dec. 2019) versus solar maximum (right, May 2024). During solar minimum, the Sun is often spotless. Sunspots are associated with solar activity and are used to track solar cycle progress. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
NASA/SDO Images from NASA’s Solar Dynamics Observatory highlight the appearance of the Sun at solar minimum (left, December 2019) versus solar maximum (right, May 2024). These images are in the 171-angstrom wavelength of extreme ultraviolet light, which reveals the active regions on the Sun that are more common during solar maximum. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
NASA/SDO
NASA and NOAA track sunspots to determine and predict the progress of the solar cycle — and ultimately, solar activity. Sunspots are cooler regions on the Sun caused by a concentration of magnetic field lines. Sunspots are the visible component of active regions, areas of intense and complex magnetic fields on the Sun that are the source of solar eruptions.
“During solar maximum, the number of sunspots, and therefore, the amount of solar activity, increases,” said Jamie Favors, director, Space Weather Program at NASA Headquarters in Washington. “This increase in activity provides an exciting opportunity to learn about our closest star — but also causes real effects at Earth and throughout our solar system.”
The solar cycle is the natural cycle of the Sun as it transitions between low and high activity. During the most active part of the cycle, known as solar maximum, the Sun can unleash immense explosions of light, energy, and solar radiation — all of which create conditions known as space weather. Space weather can affect satellites and astronauts in space, as well as communications systems — such as radio and GPS — and power grids on Earth.
Credits: Beth Anthony/NASA Solar activity strongly influences conditions in space known as space weather. This can affect satellites and astronauts in space, as well as communications and navigation systems — such as radio and GPS — and power grids on Earth. When the Sun is most active, space weather events become more frequent. Solar activity has led to increased aurora visibility and impacts on satellites and infrastructure in recent months.
During May 2024, a barrage of large solar flares and coronal mass ejections (CMEs) launched clouds of charged particles and magnetic fields toward Earth, creating the strongest geomagnetic storm at Earth in two decades — and possibly among the strongest displays of auroras on record in the past 500 years.
May 3–May 9, 2024, NASA’s Solar Dynamics Observatory observed 82 notable solar flares. The flares came mainly from two active regions on the Sun called AR 13663 and AR 13664. This video highlights all flares classified at M5 or higher with nine categorized as X-class solar flares.
Credit: NASA “This announcement doesn’t mean that this is the peak of solar activity we’ll see this solar cycle,” said Elsayed Talaat, director of space weather operations at NOAA. “While the Sun has reached the solar maximum period, the month that solar activity peaks on the Sun will not be identified for months or years.”
Scientists will not be able to determine the exact peak of this solar maximum period for many months because it’s only identifiable after they’ve tracked a consistent decline in solar activity after that peak. However, scientists have identified that the last two years on the Sun have been part of this active phase of the solar cycle, due to the consistently high number of sunspots during this period. Scientists anticipate that the maximum phase will last another year or so before the Sun enters the declining phase, which leads back to solar minimum. Since 1989, the Solar Cycle Prediction Panel — an international panel of experts sponsored by NASA and NOAA — has worked together to make their prediction for the next solar cycle.
Solar cycles have been tracked by astronomers since Galileo first observed sunspots in the 1600s. Each solar cycle is different — some cycles peak for larger and shorter amounts of time, and others have smaller peaks that last longer.
Sunspot number over the previous 24 solar cycles. Scientists use sunspots to track solar cycle progress; the dark spots are associated with solar activity, often as the origins for giant explosions — such as solar flares or coronal mass ejections — which can spew light, energy, and solar material out into space. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
NOAA’s Space Weather Prediction Center “Solar Cycle 25 sunspot activity has slightly exceeded expectations,” said Lisa Upton, co-chair of the Solar Cycle Prediction Panel and lead scientist at Southwest Research Institute in San Antonio, Texas. “However, despite seeing a few large storms, they aren’t larger than what we might expect during the maximum phase of the cycle.”
The most powerful flare of the solar cycle so far was an X9.0 on Oct. 3 (X-class denotes the most intense flares, while the number provides more information about its strength).
NOAA anticipates additional solar and geomagnetic storms during the current solar maximum period, leading to opportunities to spot auroras over the next several months, as well as potential technology impacts. Additionally, though less frequent, scientists often see fairly significant storms during the declining phase of the solar cycle.
The Solar Cycle 25 forecast, as produced by the Solar Cycle 25 Prediction Panel. Sunspot number is an indicator of solar cycle strength — the higher the sunspot number, the stronger the cycle. For these images and more relating to solar maximum, visit https://svs.gsfc.nasa.gov/14683.
NOAA’s Space Weather Prediction Center NASA and NOAA are preparing for the future of space weather research and prediction. In December 2024, NASA’s Parker Solar Probe mission will make its closest-ever approach to the Sun, beating its own record of closest human-made object to the Sun. This will be the first of three planned approaches for Parker at this distance, helping researchers to understand space weather right at the source.
NASA is launching several missions over the next year that will help us better understand space weather and its impacts across the solar system.
Space weather predictions are critical for supporting the spacecraft and astronauts of NASA’s Artemis campaign. Surveying this space environment is a vital part of understanding and mitigating astronaut exposure to space radiation.
NASA works as a research arm of the nation’s space weather effort. To see how space weather can affect Earth, please visit NOAA’s Space Weather Prediction Center, the U.S. government’s official source for space weather forecasts, watches, warnings, and alerts.
By Abbey Interrante
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Media Contact:
Sarah Frazier, NASA’s Goddard Space Flight Center, Greenbelt, Md.
sarah.frazier@nasa.gov
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Abbey Interrante
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Last Updated Oct 15, 2024 Related Terms
Goddard Space Flight Center Heliophysics Heliophysics Division Parker Solar Probe (PSP) Solar Science Sunspots The Sun The Sun & Solar Physics Explore More
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Solar storms and flares are eruptions from the Sun that can affect us here on Earth.
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By NASA
2 min read
Hubble Reaches a Lonely Light in the Dark
NASA, ESA, C. Gallart (Instituto de Astrofisica de Canarias), A. del Pino Molina (Centro de Estudios de Fisica del Cosmos de Aragon), and R. van der Marel (Space Telescope Science Institute); Image Processing: Gladys Kober (NASA/Catholic University of America) A splatter of stars glows faintly at almost 3 million light-years away in this new image from NASA’s Hubble Space Telescope. Known as the Tucana Dwarf for lying in the constellation Tucana, this dwarf galaxy contains a loose bundle of aging stars at the far edge of the Local Group, an aggregation of galaxies including our Milky Way, bound together by gravity. The Tucana Dwarf was discovered in 1990 by R.J. Lavery, the same year Hubble launched.
What makes the Tucana Dwarf distinct from other dwarf galaxies comes in two parts: its classification, and its isolation. As a dwarf spheroidal galaxy, it is much smaller and less luminous than most other dwarf galaxies. Dust is sparse and the stellar population skews towards the older range, giving them a dimmer look. Additionally, the Tucana Dwarf lies about 3.6 million light-years from the Local Group’s center of mass, far from the Milky Way and other galaxies. It is only one of two dwarf spheroidal galaxies in the Local Group to be this remote, making astronomers theorize that a close encounter with a larger galactic neighbor called Andromeda slingshotted it into the distance about 11 billion years ago.
Having such pristine properties enables scientists to use the Tucana Dwarf as a cosmic fossil. Dwarf galaxies could be the early ingredients for larger galaxies, and with older stars residing in such an isolated environment, analyzing them can help trace galaxy formation back to the dawn of time. For that reason, Hubble reached far across the Local Group using the capabilities of the Advanced Camera for Surveys and Wide Field and Planetary Camera 2 to meet this distant, lonely galaxy. Examining its structure, composition, and star formation history sheds light on the epoch of reionization, when the first stars and galaxies arose from the dark billions of years ago.
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Hubble’s Galaxies
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NASA’s Goddard Space Flight Center, Greenbelt, MD
claire.andreoli@nasa.gov
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Last Updated Aug 23, 2024 Editor Michelle Belleville Location NASA Goddard Space Flight Center Related Terms
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Hubble Space Telescope
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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By European Space Agency
ESA’s Earth Return Orbiter, the first spacecraft that will rendezvous and capture an object around another planet, passed a key milestone to bring the first Mars samples back to Earth.
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By European Space Agency
Image: A citizen scientist digging through data from the ESA/NASA Solar and Heliospheric Observatory has found the mission’s 5000th comet.
The tiny comet – indicated between the vertical lines in the inset – belongs to the ‘Marsden group’, named after the British astronomer Brian Marsden, who first recognised the group based on SOHO observations. Marsden group comets are thought to be pieces shed by the much bigger Comet 96P/Machholz, which SOHO observes as it passes close to the Sun every 5.3 years.
This 5000th comet was discovered by Hanjie Tan, an astronomy PhD student in Prague, Czechia. Hanjie has been comet hunting since he was just 13 years old, discovering over 200 comets since 2009.
Hanjie explains how he felt upon spotting this comet in the data: “The Marsden group comets represent only about 1.5% of all SOHO comet discoveries, so finding this one as the 5000th SOHO comet felt incredibly fortunate. It's really exciting to be the first to see comets get bright near the Sun after they've been travelling through space for thousands of years.”
Launched in 1995, SOHO studies the Sun from its interior to its outer atmosphere, providing unique views and investigating the cause of the solar wind. During the last three decades, SOHO has become the most prolific discoverer of comets in astronomical history.
The telescope’s prowess as a comet-hunter was unplanned, but turned out to be an unexpected success. With its clear view of the Sun’s surroundings, SOHO can easily spot a special kind of comet called a sungrazer – so-called because of their close approach to the Sun.
Like most who have discovered comets in SOHO’s data, Hanjie Tan is a volunteer citizen scientist, searching for comets in his free time with the Sungrazer Project. This NASA-funded citizen science project, managed by Karl Battams from the US Naval Research Lab, grew out of the huge number of comet discoveries by citizen scientists early into SOHO’s mission.
“Prior to the launch of the SOHO mission and the Sungrazer Project, there were only a couple dozen sungrazing comets on record – that’s all we knew existed,” said Karl Battams, who is the principal investigator for the Sungrazer Project. “The fact that we’ve finally reached this milestone – 5000 comets – is just unbelievable to me.”
SOHO is a cooperative effort between ESA and NASA. Mission control is based at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. SOHO’s Large Angle and Spectrometric Coronagraph Experiment, or LASCO, which is the instrument that provides most of the comet imagery, was built by an international consortium, led by the US Naval Research Lab.
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SOHO’s 4000th comet
SOHO’s 3000th comet
[Image description: A bright orange circle covers almost the whole image, with a smaller disc in the middle. Out of the smaller disc protrude wisps of the Sun's atmosphere. To the upper right of the inner circle, an inset zooms in on a small square, with vertical lines surrounding a faint smudge.]
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By NASA
On March 3, 1959, the United States launched Pioneer 4 with the goal of photographing the Moon during a close flyby. As part of the International Geophysical Year that ran from July 1, 1957, to Dec. 31, 1958, the United States planned to send five probes to study the Moon. The first three planned to orbit the Moon, while the last two simpler probes planned to photograph it during flybys. After NASA opened for business in October 1958, the new space agency inherited the Pioneer program from the Advanced Research Projects Agency, a branch of the Department of Defense established earlier in 1958 as part of America’s initiative to respond to early Soviet space accomplishments. The Jet Propulsion Laboratory in Pasadena, California, part of the U.S. Army until transferred to NASA in December 1958, built the two Pioneer lunar flyby spacecraft. While the first four missions did not succeed in reaching their target, Pioneer 4 became the first American spacecraft to flyby the Moon and enter solar orbit.
Left: A replica of the Pioneer 1 spacecraft. Image credit: courtesy National Air and Space Museum. Right: Liftoff of Pioneer 1, the first satellite launched by NASA.
The first Pioneer launch attempt on August 17, 1958, ended in failure 77 seconds after liftoff when the Thor-Able booster exploded. Engineers identified and corrected the problem with the rocket and on Oct. 11, Pioneer 1, weighing 84 pounds, thundered off from Cape Canaveral’s Launch Complex 17A. The launch took place just 10 days after NASA officially opened for business. Liftoff seemed to go well, but tracking soon showed that the spacecraft was traveling more slowly than expected and was also off course. Relatively minor errors in the first stage’s performance were compounded by other issues with the second stage, making it clear that Pioneer 1 would not achieve its primary goal of entering orbit around the Moon. The spacecraft did reach a then-record altitude of 70,770 miles about 21 hours after launch before beginning its fall back to Earth. It burned up on reentry over the Pacific Ocean 43 hours after liftoff. The probe’s instruments confirmed the existence of the Van Allen radiation belts discovered by Explorer 1 earlier in the year. The third and final lunar orbiter attempt, Pioneer 2 on November 8, met with less success. The rocket’s first and second stages performed well, but the third stage failed to ignite. Pioneer 2 could not achieve orbital velocity and only reached a peak altitude of 960 miles before falling back to Earth after a brief 42-minute flight.
Left: Juno rocket developer Wernher von Braun, left, Pioneer project engineer John R. Casani, and project scientist James A. Van Allen inspect the instruments in the Pioneer 4 spacecraft. Image credit: courtesy LIFE Magazine. Middle: Kurt H. Debus, left, and von Braun in the blockhouse for the Pioneer 4 launch. Right: Launch of Pioneer 4, the first American spacecraft to flyby the Moon and enter solar orbit.
The two lunar flyby missions came next, each carrying a radiation counter and photographic equipment. The 13-pound Pioneer 3 took off on Dec. 6. The Juno-II rocket’s first stage engine cut off early, and the probe could not reach its destination, falling back to Earth 38 hours after launch. Despite this problem, Pioneer 3 returned significant radiation data and discovered a second outer Van Allen belt encircling the Earth. The second attempt on March 3, 1959, met with more success as Pioneer 4 became the first American spacecraft to reach Earth escape velocity. The Juno-II’s second stage burned for an extra few seconds, resulting in Pioneer 4 passing at 36,650 miles of the Moon’s surface 41 hours after launch. At that distance, instead of the planned 5,000 miles, the spacecraft could not achieve its objective of photographing the Moon. Pioneer 4 then went on to become the first American spacecraft to enter solar orbit, a feat the Soviet Luna 1 accomplished two months earlier. Pioneer 4 returned radiation data for 82 hours, out to 409,000 miles, nearly twice the Earth-Moon distance, until its batteries died.
Left: Pioneer 4’s trajectory to the Moon and beyond. Right: The Deep Space Station-11, also known as Pioneer Station, in 1958.
Although these early Pioneer lunar probes met with limited mission success, the program marked the first use of the 26-meter antenna and tracking station at Goldstone, California. This antenna, completed in 1958 and known as Deep Space Station 11 (DSS-11), was the first component of what eventually became the NASA Deep Space Network. Although called Pioneer Station, DSS-11 not only followed these early spacecraft, starting with Pioneer 3, but later monitored the Ranger, Surveyor, and Lunar Orbiter robotic precursor missions and tracked the Apollo 11 Lunar Module Eagle to the Moon’s surface on July 20, 1969, and the other Apollo lunar missions as well. It also tracked Mariner, Viking, and Voyager missions to the planets before its decommissioning in 1978.
Watch a video about Pioneer 4: https://youtu.be/mM4U78sFYpQ
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