I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages.

I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages.

      The competition for Ultra phones has intensified this year, with every brand striving to release a model that can rival the camera capabilities of the Samsung Galaxy S25 Ultra.

      Samsung's newest camera powerhouse boasts four cameras: a 200MP primary sensor, a 50MP ultrawide lens, and two telephoto lenses. One telephoto lens includes a 10MP sensor with 3x optical zoom, while the other features a 50MP sensor equipped with 5x optical zoom.

      Since its debut in January, I have captured thousands of images with the Galaxy S25 Ultra across various countries. Although devices like the Oppo Find X8 Ultra and Xiaomi 15 Ultra outshine it in certain situations, the Galaxy S25 Ultra still produces outstanding photographs.

      Here are some of my favorite shots and the reasons behind them.

      The top phone for portrait mode variety

      Andy Boxall / Digital Trends

      I have always appreciated Samsung’s portrait mode for many reasons, with the most significant being the variety of options available. While other manufacturers offer different portrait modes, Samsung phones uniquely include my favorite feature: color point.

      Color Point is designed to create artistic and distinctive portrait photos by separating the subject from the background, keeping the foreground in color while rendering the background in grayscale. The outcome can be visually stunning; I have been using this feature for my social media avatars for years.

      Beyond Color Point, Samsung’s portrait mode provides other enjoyable features. A standard blur option softens the background, while three additional modes emulate various lighting effects: Studio, High-key Mono, and Low-key Mono. There's also a backdrop mode that allows users to create a colored background behind the subject.

      Notably, you can adjust both the effect and its intensity both before and after capturing the photo, and all the same features are compatible with the front-facing camera. In terms of versatility, no other phone offers the extensive range of portrait mode features that the Galaxy S25 Ultra does.

      High quality and vibrant colors in many pictures

      Oppo Find X8 Ultra (left) vs Galaxy S25 Ultra (right)

      The post-processing on images taken with Samsung devices typically results in a consistent look, creating instantly recognizable visuals. The Galaxy S25 Ultra is no exception; while Samsung has dialed down some of the color saturation for a more natural appearance, the camera still produces high-quality, vibrant images.

      This phone excels at capturing high-saturation ultra-wide photos. Some devices, like the Pixel 9 Pro, focus on natural colors at the cost of vibrancy, leading users to apply filters before sharing on social media.

      The Galaxy S25 Ultra generates excellent, Instagram-ready photos that often require minimal editing. Many users will find these images more visually appealing than those from competitors, despite being less accurate or natural. Pictures that are visually striking tend to receive a better reception on social media, which is how most individuals share their experiences.

      What about the telephoto cameras?

      Andy Boxall / Digital Trends

      One of the primary reasons to invest in the Galaxy S25 Ultra is its dual telephoto cameras. Samsung has been enhancing its telephoto capabilities for years, enabling the Galaxy S25 Ultra to capture stunning images at various focal lengths.

      While the Galaxy S25 Ultra may no longer dominate as it once did—particularly with rivals like the Oppo Find X8 Ultra and OnePlus 13 demonstrating better zoom capabilities—it can still produce remarkable photos.

      Within the viewfinder, there are several options corresponding to different focal lengths. The 2x zoom is a crop of the main 200MP sensor, while the 3x and 5x options utilize dedicated telephoto lenses. There are also 10x and greater zoom options that combine AI and data from the various sensors for hybrid zoom capabilities.

      Nonetheless, while the Galaxy S25 Ultra excels at lower focal lengths, Samsung's Space Zoom feature has not held up as well over time. Previously, Space Zoom was revolutionary and outperformed the competition, but now rivals have caught up and even surpassed the Galaxy S25 Ultra.

      For instance, the OnePlus 13, which has only one telephoto lens, is more proficient at 30x and even its maximum 120x zoom compared to the Galaxy S25 Ultra.

      In addition, the Oppo Find X8 Ultra, which features two telephoto lenses, similarly shows that even the Oppo Find X, which has just one telephoto lens like the OnePlus 13, can capture better 30x images than Samsung’s flagship.

      However, despite some competitors excelling in certain areas, the Galaxy S25 Ultra still offers an impressive zoom camera that will satisfy most users.

      The Galaxy S25 Ultra camera is adaptable yet has its limitations

      Nirave Gondhia / Digital Trends

      For many years, the Galaxy S25 Ultra was considered the gold standard for photography, especially when excluding devices from Huawei.

      Even as its stature fades amid strong competition, it remains one of the most versatile cameras available. The only drawback is that it has transitioned from being the

I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages. I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages.

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Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. 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This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? 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Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. This new image utilizes a property of light known as polarization to unveil the powerful magnetic fields surrounding the massive black hole. Read more Hubble captures the striking jets of a newborn star A recent image from the Hubble Space Telescope showcases the incredible events occurring as a new star comes into existence. Within a swirling cloud of dust and gas, a newly formed star is emitting powerful jets, ejecting material and cutting through the dust of the surrounding nebula to create this breathtaking scene. The image depicts a system referred to as FS Tau, situated 450 light-years away within a region known as Taurus-Auriga. This area hosts many stellar nurseries where new stars are forming, making it a popular target for astronomers examining star formation. However, this particular system is distinguished by the dramatic characteristics of its newborn star, which has developed an impressive structure known as a Herbig-Haro object. Read more Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. "That's where scientists usually look for tidal disruption events. However, this one is not at the center; it’s approximately 2,600 light years away. It is the first optically discovered off-nuclear TDE." A six-panel illustration showcases a tidal disruption event around a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) In addition to Hubble, researchers utilized other instruments like NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope to study the TDE — as depicted above. The black hole starts as a dark and elusive object, but when a star approaches too closely, it is gravitationally captured and elongated, or more technically, “spaghettified” into an extreme form. This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? We anticipate that they will eventually coalesce, but theorists have predicted a population of black holes that roam within galaxies.” The researchers suggest that the two supermassive black holes in this galaxy could potentially merge in the future, a monumental event that would generate gravitational waves capable of being detected from Earth. This research is set to be published in The Astrophysical Journal Letters. Georgina has been writing about space for Digital Trends for six years, covering topics related to human space exploration and planetary… Amazing image reveals the magnetic fields of our galaxy’s supermassive black hole The Event Horizon Telescope collaboration, known for capturing the historic first image of a black hole, has produced another stunning black hole image. This one illustrates the magnetic fields swirling around the supermassive black hole located at the center of our galaxy, Sagittarius A*. Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. 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Read more Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. "That's where scientists usually look for tidal disruption events. However, this one is not at the center; it’s approximately 2,600 light years away. It is the first optically discovered off-nuclear TDE." A six-panel illustration showcases a tidal disruption event around a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) In addition to Hubble, researchers utilized other instruments like NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope to study the TDE — as depicted above. The black hole starts as a dark and elusive object, but when a star approaches too closely, it is gravitationally captured and elongated, or more technically, “spaghettified” into an extreme form. This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? 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Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. This new image utilizes a property of light known as polarization to unveil the powerful magnetic fields surrounding the massive black hole. Read more Hubble captures the striking jets of a newborn star A recent image from the Hubble Space Telescope showcases the incredible events occurring as a new star comes into existence. Within a swirling cloud of dust and gas, a newly formed star is emitting powerful jets, ejecting material and cutting through the dust of the surrounding nebula to create this breathtaking scene. 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Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. "That's where scientists usually look for tidal disruption events. However, this one is not at the center; it’s approximately 2,600 light years away. It is the first optically discovered off-nuclear TDE." A six-panel illustration showcases a tidal disruption event around a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) In addition to Hubble, researchers utilized other instruments like NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope to study the TDE — as depicted above. The black hole starts as a dark and elusive object, but when a star approaches too closely, it is gravitationally captured and elongated, or more technically, “spaghettified” into an extreme form. This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? We anticipate that they will eventually coalesce, but theorists have predicted a population of black holes that roam within galaxies.” The researchers suggest that the two supermassive black holes in this galaxy could potentially merge in the future, a monumental event that would generate gravitational waves capable of being detected from Earth. This research is set to be published in The Astrophysical Journal Letters. Georgina has been writing about space for Digital Trends for six years, covering topics related to human space exploration and planetary… Amazing image reveals the magnetic fields of our galaxy’s supermassive black hole The Event Horizon Telescope collaboration, known for capturing the historic first image of a black hole, has produced another stunning black hole image. This one illustrates the magnetic fields swirling around the supermassive black hole located at the center of our galaxy, Sagittarius A*. Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. This new image utilizes a property of light known as polarization to unveil the powerful magnetic fields surrounding the massive black hole. Read more Hubble captures the striking jets of a newborn star A recent image from the Hubble Space Telescope showcases the incredible events occurring as a new star comes into existence. Within a swirling cloud of dust and gas, a newly formed star is emitting powerful jets, ejecting material and cutting through the dust of the surrounding nebula to create this breathtaking scene. The image depicts a system referred to as FS Tau, situated 450 light-years away within a region known as Taurus-Auriga. This area hosts many stellar nurseries where new stars are forming, making it a popular target for astronomers examining star formation. However, this particular system is distinguished by the dramatic characteristics of its newborn star, which has developed an impressive structure known as a Herbig-Haro object. Read more Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. "That's where scientists usually look for tidal disruption events. However, this one is not at the center; it’s approximately 2,600 light years away. It is the first optically discovered off-nuclear TDE." A six-panel illustration showcases a tidal disruption event around a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) In addition to Hubble, researchers utilized other instruments like NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope to study the TDE — as depicted above. The black hole starts as a dark and elusive object, but when a star approaches too closely, it is gravitationally captured and elongated, or more technically, “spaghettified” into an extreme form. This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? We anticipate that they will eventually coalesce, but theorists have predicted a population of black holes that roam within galaxies.” The researchers suggest that the two supermassive black holes in this galaxy could potentially merge in the future, a monumental event that would generate gravitational waves capable of being detected from Earth. This research is set to be published in The Astrophysical Journal Letters. Georgina has been writing about space for Digital Trends for six years, covering topics related to human space exploration and planetary… Amazing image reveals the magnetic fields of our galaxy’s supermassive black hole The Event Horizon Telescope collaboration, known for capturing the historic first image of a black hole, has produced another stunning black hole image. This one illustrates the magnetic fields swirling around the supermassive black hole located at the center of our galaxy, Sagittarius A*. Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. This new image utilizes a property of light known as polarization to unveil the powerful magnetic fields surrounding the massive black hole. Read more Hubble captures the striking jets of a newborn star A recent image from the Hubble Space Telescope showcases the incredible events occurring as a new star comes into existence. Within a swirling cloud of dust and gas, a newly formed star is emitting powerful jets, ejecting material and cutting through the dust of the surrounding nebula to create this breathtaking scene. The image depicts a system referred to as FS Tau, situated 450 light-years away within a region known as Taurus-Auriga. This area hosts many stellar nurseries where new stars are forming, making it a popular target for astronomers examining star formation. However, this particular system is distinguished by the dramatic characteristics of its newborn star, which has developed an impressive structure known as a Herbig-Haro object. Read more Illustration depicting a tidal disruption event surrounding a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) Black holes are the ravenous giants of the universe: extremely dense entities capable of consuming any material that ventures too close and then obliterating it. Recent observations from astronomers using the Hubble Space Telescope have captured a black hole actively consuming a star, tearing it apart and producing a significant burst of radiation. This radiation burst, known as a tidal disruption event (TDE), enabled researchers to locate the black hole. The TDE identified as AT2024tvd was remarkable for a particularly uncommon reason: while most supermassive black holes are usually found at the very center of a galaxy, this one is a nomadic rogue. "The typical location for massive black holes within a galaxy is at the center, similar to our Sag A* at the heart of the Milky Way,” said lead researcher Yuhan Yao from UC Berkeley. "That's where scientists usually look for tidal disruption events. However, this one is not at the center; it’s approximately 2,600 light years away. It is the first optically discovered off-nuclear TDE." A six-panel illustration showcases a tidal disruption event around a supermassive black hole. NASA, ESA, STScI, Ralf Crawford (STScI) In addition to Hubble, researchers utilized other instruments like NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope to study the TDE — as depicted above. The black hole starts as a dark and elusive object, but when a star approaches too closely, it is gravitationally captured and elongated, or more technically, “spaghettified” into an extreme form. This process results in a disk-shaped cloud of material encircling the black hole, and this material rapidly spirals into the black hole, generating a flash of radiation across X-ray to radio wavelengths that can be detected from Earth, revealing that the black hole is not centrally located in the galaxy as anticipated. In fact, this galaxy contains not just one supermassive black hole, but two: one at the galactic center and the other as a wandering entity. It is believed that this situation arises when two smaller galaxies collide and merge to create a larger galaxy. “Massive black holes typically reside at the centers of galaxies, but we know that galaxies undergo mergers — that is how they grow. When two galaxies combine to become one, multiple black holes emerge,” explained co-author Ryan Chornock, also from UC Berkeley. “What happens next? We anticipate that they will eventually coalesce, but theorists have predicted a population of black holes that roam within galaxies.” The researchers suggest that the two supermassive black holes in this galaxy could potentially merge in the future, a monumental event that would generate gravitational waves capable of being detected from Earth. This research is set to be published in The Astrophysical Journal Letters. Georgina has been writing about space for Digital Trends for six years, covering topics related to human space exploration and planetary… Amazing image reveals the magnetic fields of our galaxy’s supermassive black hole The Event Horizon Telescope collaboration, known for capturing the historic first image of a black hole, has produced another stunning black hole image. This one illustrates the magnetic fields swirling around the supermassive black hole located at the center of our galaxy, Sagittarius A*. Black holes are difficult to photograph because they engulf anything that strays too close, including light, due to their immensely strong gravitational pull. However, this does not render them invisible. While the black hole itself cannot be seen, the material circling around the edges of the event horizon glows brightly enough to be captured on camera. This new image utilizes a property of light known as polarization to unveil the powerful magnetic fields surrounding the massive black hole. Read more Hubble captures the striking jets of a newborn star A recent image from the Hubble Space Telescope showcases the incredible events occurring as a new star comes into existence. Within a swirling cloud of dust and gas, a newly formed star is emitting powerful jets, ejecting material and cutting through the dust of the surrounding nebula to create this breathtaking scene. The image depicts a system referred to as FS Tau, situated 450 light-years away within a region known as Taurus-Auriga. This area hosts many stellar nurseries where new stars are forming, making it a popular target for astronomers examining star formation. However, this particular system is distinguished by the dramatic characteristics of its newborn star, which has developed an impressive structure known as a Herbig-Haro object. Read more The Samsung Galaxy S25 FE may prioritize performance over cost. The Samsung Galaxy S25 FE may prioritize performance over cost. If Samsung Foundry cannot produce sufficient Exynos chips on schedule, the alternative plan involves MediaTek. Nonnas: How Stephen Chbosky and Liz Maccie crafted an ode to food and family. Nonnas: How Stephen Chbosky and Liz Maccie crafted an ode to food and family. In a conversation with Digital Trends, Stephen Chbosky and Liz Maccie talk about their touching family comedy, Nonnas.

I captured 4000 images with the Galaxy S25 Ultra; here’s an overview of its advantages and disadvantages.

Having taken over 4,000 pictures with the Galaxy S25 Ultra in the last four months, here are the strengths and weaknesses of Samsung's camera powerhouse.