Doom: The Dark Ages review: exciting prequel takes on too much too quickly

Doom: The Dark Ages review: exciting prequel takes on too much too quickly

      **Doom: The Dark Ages**

      **MSRP: $70.00**

      “Doom: The Dark Ages delivers plenty of excitement but may benefit from slowing down a bit.”

      **Pros:**

      - Doom Slayer gets the recognition he deserves

      - Outstanding combat

      - Complex level design

      - Stunning visuals

      **Cons:**

      

      - Complicated lore

      - Disappointing mech and dragon sequences

      - Consistently flat action

      Just a few missions into Doom: The Dark Ages, I felt as though I hit the pinnacle of action gaming. I was controlling a massive Atlan mech, dominating a battlefield that had seemed vast just moments prior. The sky was scorched above, and buildings crumbled beneath me. One by one, an army of demonic kaiju fell before my metallic fists. How could things get any more intense than this?

      They don’t, and that is both a strength and a weakness of the Doom Slayer’s latest adventure.

      In an effort to outdo the already intense shooter series that reached new heights in adrenaline with 2020's Doom: Eternal, developer Id Software cranks every aspect up to maximum from Chapter 1. The battles are quicker and more vicious, hidden lore turns into flashy cutscenes, and our hero even rides a mechadragon. Each element is an exercise in extreme escalation, attempting to push the limits of hyper-violent shooter glory. While it does reach those heights, it faces a harsh reality: there’s nowhere left to go once you reach the summit.

      Doom: The Dark Ages offers another dose of reliable thrills, building on the groundwork laid by its excellent predecessors. The power fantasy is more potent than ever, but Id Software's pursuit of excess demonstrates that there can indeed be too much when it comes to video game spectacle.

      **Year One**

      Instead of continuing from where Eternal concluded, The Dark Ages serves as a prequel to Id Software’s rebooted Doom series. It functions as an origin story for the Doom Slayer, taking inspiration from Batman: Year One, Frank Miller’s gritty portrayal of The Dark Knight’s first year. This approach establishes the narrative-focused Doom game yet, featuring significant cutscenes. It mirrors the jump from Metroid Prime to Metroid Prime 3: Corruption, where the latter expanded on a famously atmospheric adventure by deepening the lore and introducing a larger cast of characters to convey it through dialogue. The Dark Ages attempts a similar feat for Doom, albeit with mixed results.

      The story takes place during Doom’s own medieval era, where humans wage war against demons using crossbows, flails, and, of course, shotguns. This concept allows Id Software to imagine more primitive versions of classic weapons, but the narrative behind it is the most baffling chapter in Doom’s history. New characters, introduced without proper context, spend cutscenes throwing around proper nouns that ultimately lack significance. A lot of money was spent on a story that mostly amounts to “There’s a war between humans and demons.”

      However, the characterization of the Doom Slayer is more successfully handled. While earlier installments depicted him as an unstoppable killer who always maintained control, here he begins as a mere tool. His origin story portrays him as a living weapon whose personality is stripped away to create a single-minded focus on demon killing. This clever twist adds depth to his typically shallow persona, transforming it into a source of pain that drives him down a more complex path of revenge and havoc. Key moments revealing his humanity help clarify the otherwise convoluted narrative.

      **The Dark Ages goes full Hollywood**

      I understand the impulse behind this. Doom has always been a deceptively deep series. To the casual player, it might seem merely about guns and gore. Dedicated fans, however, argue that there’s much more beneath the surface, and The Dark Ages feels designed to finally appease that audience. Unfortunately, in doing so, Id sacrifices something special about the series. The old games had a mystique tied to their minimal in-game storytelling. They often felt sparse and atmospheric, allowing players’ imaginations to occupy the void. Only the most devoted fans would delve deep, uncovering secret lore concealed within books or cassette tapes. These scattered details gave games like Doom a sense of hidden history, transforming fans into archivists sharing their discoveries.

      As Doom expands, its world ironically feels smaller. Wet concrete fills every crevice, creating a uniform historical record for every player. Even minor details are documented in in-game Codex entries. The 2016 Doom reboot struck a balance, keeping the story sparse and sleek while still broadening the lore. The Dark Ages embraces a more cinematic style and loses some of its uniqueness for it.

      **Primal violence**

      The expanded scope detracts from certain aspects of The Dark Ages, yet it enhances its core action. If Eternal focused on demonstrating the Doom Slayer’s agility, this installment emphasizes raw power. The shooting mechanics remain

Doom: The Dark Ages review: exciting prequel takes on too much too quickly Doom: The Dark Ages review: exciting prequel takes on too much too quickly Doom: The Dark Ages review: exciting prequel takes on too much too quickly

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									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.
			
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					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.
			
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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? 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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. 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. 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									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. 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Doom: The Dark Ages review: exciting prequel takes on too much too quickly

Doom: The Dark Ages still offers a lot of exciting action, but its lofty ambitions render it the weakest entry in an otherwise excellent trilogy.