June's Strawberry Moon treats skywatchers to a rare low-riding show (photos)
June's full 'Strawberry Moon' lit up the night sky last night, treating skywatchers to a rare once-in-a-18-year display as it rode low across the southern horizon.
Skywatchers were served the lowest full moon in almost two decades, thanks in part to a quirk of orbital mechanics known to astronomers as a "major lunar standstill". This phenomenon occurs over a two-year period when the moon's tilted orbit is at its greatest inclination relative to our planet's celestial equator (which is essentially Earth's normal equator projected out into space).
During a major lunar standstill, the moon can be seen rising and setting at more extreme positions on the horizon, while tracking a very high — or low — path through the night sky depending on the time of year. June's Strawberry Moon occurs close to the southern solstice for those in the southern hemisphere, which means that it's never particularly high in the sky to begin with. The major lunar standstill exacerbated this effect, making the June full moon the lowest full moon in almost two decades.
This month's full Strawberry Moon was named for the brief fruit picking season that occurs around this time each year by Algonquian, according to the Old Farmer's Almanac.
Read on to see the best pictures of the 2025 Strawberry Moon as captured by the global astrophotography community. As always, if you missed last night's full moon don't worry. The lunar disk will continue to appear (almost) fully lit for the next few nights, so be sure to read up on the best practices for observing and photographing the lunar surface as it transitions to a waning gibbous moon in the coming days.
Space enthusiast Marwella Zhang was able to capture this detailed portrait of the Flower Moon around midnight from Bangka Island in Indonesia, while grappling with the haze caused by tropical storm Wutip.
"After sunset, the sky was starting to get clear," Zhang told Space.com in an email. "I took my first shot, but the sky was still hazy. By midnight, as it had been predicted, the sky got clear, and I took the opportunity to get a better shot of the moon."
New York's photography contingent also showed up in force to capture stunning compositions of the full moon framed by the iconic city skyline. Photographer Gary Hershorn was able to position himself to capture the orange orb of the Strawberry Moon hanging above the spire of the Empire State Building on the night of June 10.
Hershorn also used a powerful lens to snap the moment Earth's natural satellite appeared to brush up against the famous landmark, creating a colorful scene that blends the warm reflected sunlight bouncing off the lunar surface with the glow of the city beneath.
Kristin Louise Raught caught a striking view of the Strawberry Moon hanging over the ghostly form of Mt. Rainier in Washington State on June 10. "I went out to get a photo of the moon directly over Tahoma (Mt. Rainier) but I saw the ferry coming and wanted to include it in the photo," Raught told Space.com in an email.
"Rather than wait for the moon to align with the mountain, I decided to instead catch the ferry at the last possible moment before it disappeared behind the building on the pier," explained Raught. "I wanted to preserve the detail in the moon, so I opted for less light in the photo overall. I was happy that the sailboat was positioned so perfectly at this moment, it adds a wonderful detail to the photo."
Andrew von Rathonyi took a different approach when eyeing the moon from the town of Irondequoit, New York, choosing to frame the celestial body as it appeared to graze the top of a low-hanging cloud, illuminating its fringes with reflected sunlight.
One particularly striking shot was captured by Ahsan Mohammed Ahmed Ahmed in the city of Halabja, Iraq, which featured the silhouette of a man playing the violin on a hillside, framed by the rising form of the full moon.
Ismael Adnan Yaqoob was able to snap the Strawberry Moon as it rose above a ferris wheel in the Iraqi city of Duhok on the night of June 10, at which point it had moved further from the horizon, losing the orange glow of moonrise.
Photographer Isla Terli was able to snap the silhouette of a passenger airliner from Turkey as it passed across the face of the full Strawberry Moon, along with the prominent craters, ejecta rays and lunar seas that mark its surface.
Twitter/X user @VeronicaJoPo caught the Strawberry Moon traveling low over Ely Cathedral in the town of Little Downham, Cambridgeshire, in the UK around the full moon phase.
Finally, photographer Isla Terli was able to capture this atmospheric shot of the Strawberry Moon rising over the Selimiye Mosque in the Turkish city of Edirne, soon after it had emerged from below the southeastern horizon.
Remember, the Strawberry Moon will appear almost completely lit in the nights following its full moon phase, which occurred at 3:44 a.m. EDT (0744 GMT) in the early hours of June 11 for viewers in New York.
Editor's Note: If you capture a picture of the Strawberry Moon and want to share your astrophotography with Space.com's readers, then please send your photo(s), comments, name and location to spacephotos@space.com.
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles
Yahoo
33 minutes ago
- Yahoo
Astronomers discover strange new type of supernova: 'This is the first time we have seen a star that was essentially stripped to the bone'
When you buy through links on our articles, Future and its syndication partners may earn a commission. Astronomers have used a new type of extreme supernova in which a massive star was stripped right "down to the bone" to better understand the process of stellar life and death. When other massive stars die in supernova explosions, astronomers detect strong signals of light elements like hydrogen and helium that existed at the surface of the star. However, in this supernova, designated SN2021yfj and located 2.2 billion light-years from Earth, this team found a different chemical signature. This contained traces of heavier elements like silicon, sulfur, and argon that originate from deeper within the progenitor star. If dying stars have onion-like structures with lighter elements at their surfaces and heavier elements toward their iron cores as astrophysicists currently theorize, then this star must have somehow lost its outer layers, thus exposing inner silicon and sulfur-rich layers before it "went nova." This would not only confirm the layered structure of massive stars, but it also give stellar scientists a rare glimpse at the interior of a star prior to it exploding in a supernova. "This is the first time we have seen a star that was essentially stripped to the bone," team leader and Northwestern University scientist Steve Schulze said in a statement. "It shows us how stars are structured and proves that stars can lose a lot of material before they explode. Not only can they lose their outermost layers, but they can be completely stripped all the way down and still produce a brilliant explosion that we can observe from very, very far distances." SN2021yfj, first spotted in September 2021 by the Zwicky Transient Facility (ZTF), suggests that while our models of stellar life and death and star structure may be correct, they may not fully describe the explosive death throes of all stars. "This event quite literally looks like nothing anyone has ever seen before," Northwestern University researcher and team member Adam Miller said. "It was almost so weird that we thought maybe we didn't observe the correct object. This star is telling us that our ideas and theories for how stars evolve are too narrow. It's not that our textbooks are incorrect, but they clearly do not fully capture everything produced in nature. "There must be more exotic pathways for a massive star to end its life that we hadn't considered." The team's research was published on Wednesday (Aug. 20) in the journal Nature. A burning onion in space The progenitor stars of supernovas are between 10 and 100 times as massive as the sun, but still generate their energy via the nuclear fusion of lighter elements to heavier elements at their cores. Whereas the sun will die when it has finished fusing its core hydrogen to helium in around 5 billion years, more massive stars have the pressures and temperatures at their cores to fuse progressively heavier and heavier elements right up to iron. As this process unfolds, lighter elements continue to undergo nuclear burning in the outer shells of massive stars. When the cores of massive stars are hearts of pure iron, they collapse, and a supernova is triggered, ripping away the outer layers. The collapsing iron core eventually becomes a neutron star, or in the case of the most massive stars, a black hole. To obtain information about supernovas, astronomers look for the signatures of chemical elements using a process called spectroscopy. The team was able to gain a spectroscopic picture of SN2021yfj using the W.M. Keck Observatory in Hawaii. "We thought we had fully lost our opportunity to obtain these observations," said Miller. "So, we went to bed disappointed. But the next morning, a colleague at UC Berkeley unexpectedly provided a spectrum. Without that spectrum, we may have never realized that this was a strange and unusual explosion." This revealed that SN2021yfj stands apart from other supernovas because the layers that were ripped away during its explosive end went deeper than what has been seen in the deaths of other massive stars. Astronomers have seen elements as heavy as carbon or oxygen during other supernovas due to the prior loss of stars' outer hydrogen layers. However, no elements heavier than this, and thus from deeper within the progenitor stars, have been seen before. "We saw an interesting explosion, but we had no idea what it was," Schulze said. "Almost instantly, we realized it was something we had never seen before, so we needed to study it with all available resources." The spectrum of SN2021yfj didn't just contain traces of heavy elements; it was dominated by strong signals of heavy elements like silicon, sulfur and argon. Thus, it became evident very early in this investigation that there was something particularly extreme and violent about SN2021yfj. "This star lost most of the material that it produced throughout its lifetime," Schulze explained. "So, we could only see the material formed during the months right before its explosion. Something very violent must have happened to cause that." Related Stories: — 'This is the holy grail of theoretical physics.' Is the key to quantum gravity hiding in this new way to make black holes? — Astronomers trace mysterious blast of X-rays to 'Die Hard' star that refuses to perish (video) — Is our universe trapped inside a black hole? This James Webb Space Telescope discovery might blow your mind What caused this particular supernova to be violent is still somewhat mysterious, with several possible scenarios including a massive pre-supernova eruption, unusually strong stellar winds, or even a companion star stripping outer material away from this dying star prior to its explosive death. However, the team thinks the most likely explanation is multiple episodes of so-called "pair instability" during which nuclear fusion is reignited, causing powerful bursts of energy that blow away the outer shells of the star. This is akin to the massive star effectively ripping itself apart before its supernova death. The bright emission that allowed SN2021yfj to be spotted by the ZTF would have been caused by shells of ejected material catching up with and slamming into previously ejected shells. "While we have a theory for how nature created this particular explosion," Miller concluded. "I wouldn't bet my life that it's correct, because we still only have one discovered example. "This star really underscores the need to uncover more of these rare supernovae to better understand their nature and how they form."
Yahoo
38 minutes ago
- Yahoo
Astronomers trace massive cosmic explosion back 12 billion years. 'This is the most distant event where we can directly see light escaping from around stars'
When you buy through links on our articles, Future and its syndication partners may earn a commission. Astronomers have used a newly discovered and still mysterious class of cosmic explosions to better understand the process of stellar life and death in the distant universe. The blasts in question are Fast X-ray Transients (FXTs), recently discovered outbursts of X-rays that last for just a few minutes. The source of FXTs has been shrouded in mystery. Now, with the aid of the Einstein Probe X-ray space telescope, astronomers have tracked one FXT, designated EP240315A, back to its source after travelling towards Earth for 12 billion years. "We've known that these unique explosions exist for some time, but it is only now, thanks to the new Einstein Probe mission, that we can pinpoint them in near real time," team member Peter Jonker, of Radboud University, said in a statement. Occurring in galaxies located billions of light-years away and lasting anywhere from seconds to hours, FXTs have proved difficult to trace back to their sources. Despite this, astronomers have theorized that FXTs may occur when massive stars go supernova, collapsing and leaving behind black holes. "This event is novel and interesting because only a handful of FXTs had been discovered until very recently, and their origin was a mystery, primarily because they had been found in archival observations," team member and University of Lancaster researcher Samantha Oates said in the statement. "By the time they were discovered, it was too late to perform follow-up of these transient X-ray objects at other wavelengths to get other information about what might be causing them." The team thus perfected their mapping of EP240315A using the ATLAS optical telescope system, the Very Large Telescope (VLT) in northern Chile, and the Gran Telescopio Canarias, located in Spain. "These observations show that this explosion happened when the universe was less than 10% of its current age - the light has been travelling to us for 12 billion years," team member Andrew Levan, of Radboud University, said. "The combination of the distance and the brightness means this explosion gave off more energy in a few seconds than the sun will over its entire life." Are Fast X-ray Transients and Gamma-ray Bursts cousin cosmic explosions? The extreme energy of the FXTs and data regarding blasts of energy called gamma-rays suggest that FXTs and gamma-ray bursts (GRBs) are, at least sometimes, related. GRBs are the most powerful and violent explosions in the known universe, brief flashes of high-energy radiation that result from some of the universe's most explosive events, including the death of massive stars and the subsequent birth of black holes. Unlike FXTs, GRBs have been studied by humanity for around half a century. "A real question is whether all of the FXTs come from GRB-like systems, or if there is much more diversity," Jonker added. "Our paper shows that many of them might be gamma-ray bursts, but there are good reasons to think there is much more still to discover." When the team looked at observations of EP240315A, collected by the VLT, they found that its source was surrounded by very little material. In particular, they noted a dearth of hydrogen in this region. Hydrogen filters ultraviolet light, preventing it from effectively traversing the cosmos. When this FXT was launched, around 1.8 billion years after the Big Bang, hydrogen was bombarded by ultraviolet light, causing it to be ionized. "Our observations show that perhaps 10% of the ultraviolet light created in the host galaxy of the FXT is escaping to ionize the universe," said team member Andrea Saccardi, the French Alternative Energies and Atomic Energy Commission (CEA) Saclay. "This is the most distant event where we can directly see light escaping from around stars. "Galaxies like this are probably really important for reionization." The FXT EP240315A was one of the first events detected by the Einstein Probe, which launched on Jan. 9, 2024. "In the year since this first object, we have found and studied another 20 of these outbursts," Levan added. "They [FXTs] are living up to their promise as an exciting new way to explore both how stars end their lives, and also what the universe was like in the distant past." Related Stories: — 'This is the holy grail of theoretical physics.' Is the key to quantum gravity hiding in this new way to make black holes? — Astronomers trace mysterious blast of X-rays to 'Die Hard' star that refuses to perish (video) — Is our universe trapped inside a black hole? This James Webb Space Telescope discovery might blow your mind Oates explained that this research exemplifies how the Einstien Probe is revolutionizing the detection of FXTs and their further study. "The Einstein Probe has opened up a new window on the universe, allowing us to probe the origin of these transient X-ray phenomena and widen our knowledge of the behavior associated with the deaths of massive stars," she concluded. The team's research was published on Tuesday (Aug. 19) in the journal Nature Astronomy.
Yahoo
4 hours ago
- Yahoo
Astronomers trace massive cosmic explosion back 12 billion years. 'This is the most distant event where we can directly see light escaping from around stars'
When you buy through links on our articles, Future and its syndication partners may earn a commission. Astronomers have used a newly discovered and still mysterious class of cosmic explosions to better understand the process of stellar life and death in the distant universe. The blasts in question are Fast X-ray Transients (FXTs), recently discovered outbursts of X-rays that last for just a few minutes. The source of FXTs has been shrouded in mystery. Now, with the aid of the Einstein Probe X-ray space telescope, astronomers have tracked one FXT, designated EP240315A, back to its source after travelling towards Earth for 12 billion years. "We've known that these unique explosions exist for some time, but it is only now, thanks to the new Einstein Probe mission, that we can pinpoint them in near real time," team member Peter Jonker, of Radboud University, said in a statement. Occurring in galaxies located billions of light-years away and lasting anywhere from seconds to hours, FXTs have proved difficult to trace back to their sources. Despite this, astronomers have theorized that FXTs may occur when massive stars go supernova, collapsing and leaving behind black holes. "This event is novel and interesting because only a handful of FXTs had been discovered until very recently, and their origin was a mystery, primarily because they had been found in archival observations," team member and University of Lancaster researcher Samantha Oates said in the statement. "By the time they were discovered, it was too late to perform follow-up of these transient X-ray objects at other wavelengths to get other information about what might be causing them." The team thus perfected their mapping of EP240315A using the ATLAS optical telescope system, the Very Large Telescope (VLT) in northern Chile, and the Gran Telescopio Canarias, located in Spain. "These observations show that this explosion happened when the universe was less than 10% of its current age - the light has been travelling to us for 12 billion years," team member Andrew Levan, of Radboud University, said. "The combination of the distance and the brightness means this explosion gave off more energy in a few seconds than the sun will over its entire life." Are Fast X-ray Transients and Gamma-ray Bursts cousin cosmic explosions? The extreme energy of the FXTs and data regarding blasts of energy called gamma-rays suggest that FXTs and gamma-ray bursts (GRBs) are, at least sometimes, related. GRBs are the most powerful and violent explosions in the known universe, brief flashes of high-energy radiation that result from some of the universe's most explosive events, including the death of massive stars and the subsequent birth of black holes. Unlike FXTs, GRBs have been studied by humanity for around half a century. "A real question is whether all of the FXTs come from GRB-like systems, or if there is much more diversity," Jonker added. "Our paper shows that many of them might be gamma-ray bursts, but there are good reasons to think there is much more still to discover." When the team looked at observations of EP240315A, collected by the VLT, they found that its source was surrounded by very little material. In particular, they noted a dearth of hydrogen in this region. Hydrogen filters ultraviolet light, preventing it from effectively traversing the cosmos. When this FXT was launched, around 1.8 billion years after the Big Bang, hydrogen was bombarded by ultraviolet light, causing it to be ionized. "Our observations show that perhaps 10% of the ultraviolet light created in the host galaxy of the FXT is escaping to ionize the universe," said team member Andrea Saccardi, the French Alternative Energies and Atomic Energy Commission (CEA) Saclay. "This is the most distant event where we can directly see light escaping from around stars. "Galaxies like this are probably really important for reionization." The FXT EP240315A was one of the first events detected by the Einstein Probe, which launched on Jan. 9, 2024. "In the year since this first object, we have found and studied another 20 of these outbursts," Levan added. "They [FXTs] are living up to their promise as an exciting new way to explore both how stars end their lives, and also what the universe was like in the distant past." Related Stories: — 'This is the holy grail of theoretical physics.' Is the key to quantum gravity hiding in this new way to make black holes? — Astronomers trace mysterious blast of X-rays to 'Die Hard' star that refuses to perish (video) — Is our universe trapped inside a black hole? This James Webb Space Telescope discovery might blow your mind Oates explained that this research exemplifies how the Einstien Probe is revolutionizing the detection of FXTs and their further study. "The Einstein Probe has opened up a new window on the universe, allowing us to probe the origin of these transient X-ray phenomena and widen our knowledge of the behavior associated with the deaths of massive stars," she concluded. The team's research was published on Tuesday (Aug. 19) in the journal Nature Astronomy.