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What We Know About the Biggest Unseen War of ‘Star Trek’

What We Know About the Biggest Unseen War of ‘Star Trek’

For as much as it presents itself as a vision of a utopian, idealistic society, much of Star Trek remains defined by its relation to conflict. There’s the lingering question over Starfleet’s values as a military organization or a scientific exploratory force, or defining conflicts like those against the Klingons, the Borg, and the Dominion that form major pillars of Star Trek lore. But that’s always been the case, and for nearly 60 years, Star Trek‘s early days have been defined by one conflict above all: one that continues to shape and fascinate the series to this day, even though it’s never actually been portrayed on screen.

The Earth-Romulan War has become one of Star Trek‘s most enduring mysteries largely for one reason alone: that its very existence was introduced in what would go on to become one of the most revered episodes of Star Trek ever made, “Balance of Terror.” The 14th episode of original Trek‘s first season, “Balance” introduced both the audience and its heroes alike to the Romulan people, as well as teased the details of the deadly conflict between them and Earth. But it also laid the groundwork for just why the conflict has spent nearly six decades off-screen in Star Trek with the revelation that the Romulans were so secretive, no human ever actually made visual contact with a member of the species until the events of the episode, itself set over a century after the conclusion of the war.

That singular choice has defined the conflict’s place in Star Trek storytelling ever since. The franchise has come close—apocryphal books have filled in their own versions of the war in broad strokes, and both cancelled projects, such as the initial plans for Star Trek: The Beginning or even, as we learned last week, Scott Bakula and Michael Sussman’s plans for a potential post-Enterprise spinoff, Star Trek: United, have wanted to lift the lid on it. But even now, part of what makes it so alluring to fans is that we know so little about it.

That doesn’t mean we know nothing, however.

Prelude to Conflict

© Paramount

Romulan frustration with United Earth began to reach a fever pitch in the early 2150s, as the exploratory and diplomatic mission of the NX-01 Enterprise effectively turned humanity into a diplomatic superpower. By the middle of the decade, a war-torn Alpha Quadrant had largely resolved into a tense but peaceful field of diplomacy between the most prominent species in interstellar society (the Vulcans, the Andorians, and the Tellarites) in large part due to the negotiation efforts of Captain Archer and his crew.

This greatly displeased the Star Empire, which relied on a volatile galaxy to keep its own operations covert. The Romulans increased attempts to reopen wedges between the major powers of the quadrant but also faced an internal reckoning within its own borders: an increasing desire to see the Romulans and Vulcans reunited as a singular society. While we know that the Romulan and Vulcan peoples eventually achieved reunification at some point before the 32nd century, the version being looked to in the 2150s was very different: Romulan agents working with the head of the Vulcan High Command, V’Las, attempted to surreptitiously support the administrator’s plans for a Vulcan invasion of Andoria, which in turn would lead to Vulcan submitting to reunification under the behest of Romulus. But again, V’Las’ attempts to bring Vulcan and Andoria into conflict were exposed by the efforts of Archer and the Enterprise, setting back the Romulans’ influence on their ancestral homeworld.

The Star Empire escalated plans with the Babel Crisis in 2155, launching drone ships piloted remotely by telepaths. Targeting Tellarite and Andorian vessels on the borders of the two powers at the height of trade negotiations between the two worlds on the planet Babel, the Romulan drone ships were capable of using multispectral emitters to visually mask their appearance, allowing Romulan agents to sow discord among the Tellarites and Andorians by posing as each other to attack trade routes.

The Romulans’ plans backfired, however: the Babel Crisis was thwarted by the combined efforts of United Earth, Tellar, Andoria, and Vulcan, who formed a joint operation to combine a fleet of ships from all four species to track and locate the drone warships, ultimately defeating them. Instead of inciting renewed conflict throughout the Alpha and Beta Quadrants, the Romulan effort ultimately stabilized the region altogether. Shortly after the crisis came to an end, representatives from humanity, the Tellarites, the Andorians, and the Vulcans convened a conference that would eventually lay the groundwork for the Coalition of Planets, an unprecedented interstellar alliance, later that same year.

The Four-Year War

Star Trek Enterprise Romulan Bird Of Prey 22nd Century
© Paramount

The emergence of the Coalition of Planets was what ultimately pushed the Romulan Star Empire into open conflict, with the Earth-Romulan War beginning in earnest in 2156. Little remains known about the exact nature of the war, other than that it was seemingly largely waged between the Romulans and United Earth forces. Just over a century after its conclusion, when tensions between Starfleet and Romulus arose, Spock described the conflict as primitive by contemporary standards: ships on both sides of the war were vastly inferior to the standards and size of those used by galactic powers in the 22nd century and incapable of holding prisoners of war, and the majority of the weaponry used was still atomic in nature.

This totality of destruction also meant that both the Romulans and the Coalition powers never actually made visual communication with either side over the four years the conflict dragged on, keeping the Romulans’ general identity—and their ancestral connections to the Vulcans—a secret throughout the war.

What is known about the Earth-Romulan War is that it concludes four years later in 2160 after the Battle of Cheron. Again, the circumstances of that battle are largely unknown outside of two factors: that it was fought between the Romulans and a Human/Vulcan/Andorian/Tellarite alliance (presumably under the banner of the Coalition of Planets), and that the battle was an absolute disaster for Romulan forces. Defeat was near total, and memory of how poorly the battle for the Star Empire went would continue to have military and political ramifications for centuries.

Centuries of Aftermath

Star Trek Strange New Worlds Neutral Zone Map 2259
© Paramount

The end of the war would have huge ramifications for the Alpha and Beta Quadrants for generations to come. A peace treaty, agreed to over subspace radio between Starfleet and the Romulans, led to the establishment of a Neutral Zone between the borders of allied space and the Star Empire, an area of space neither side could move ships into or through without it being seen as an act of war. Little is known as to how the Romulans monitored their side of the Zone, as the Star Empire retreated from astropolitics for the best part of a century in the wake of the war’s conclusion. However, Starfleet monitored its side of the zone with the establishment of outpost monitoring stations housed on asteroids.

A year after the conflict concluded, the Coalition of Planets was dissolved to make way for the formal founding of the United Federation of Planets in 2161. Now led by President Jonathan Archer, the Federation ushered in a new age of galactic politics, as more and more member worlds joined the four founding planets of Earth, Tellar, Andoria, and Vulcan, and Starfleet became its primary interstellar task force.

It wouldn’t be for another 100 years that the Romulans would test the constraints of their peace treaty with the now-Federation, when an unnamed Romulan commander attacked and destroyed four of Starfleet’s monitoring stations along the edge of the neutral zone. Ultimately destroyed in turn by the U.S.S. Enterprise, the Federation’s flagship, the incident marked the first known visual communication between humanity and the Star Empire, exposing the Romulans’ visual similarity to the Vulcans.

This waxing and waning of Romulan involvement beyond the borders of the Star Empire would persist until the Empire’s collapse in 2387 after the star of the Romulus system went supernova, destroying both Romulus and its sister world, Remus. For a brief time in the 22nd century, the Romulans formed diplomatic relations and trade deals with their Beta Quadrant counterparts in the Klingon Empire, and in 2311, conflict between the Federation and the Star Empire briefly erupted in the Tomed Incident, which concluded with a new treaty that reinforced the Neutral Zone’s borders and prohibited the Federation from researching ship-based cloaking technology, a key technological advantage long held by the Romulans, as well as the Star Empire’s return to isolation.

Only one major incident reflected an act of diplomatic alliance between the Federation and the Romulans across those centuries of general distrust: in 2374, at the height of the Federation’s war against the Gamma-Quadrant-based Dominion, the Romulans were pushed to enter the conflict alongside the Federation after years of neutrality when a high-ranking member of the Romulan Senate, Vreenak, was seemingly assassinated by Dominion forces in an attempt to cover up evidence of Dominion and Cardassian plans to invade the Star Empire. The Romulans would go on to play a pivotal role in alliance with the Federation and Klingon Empire for the remainder of the war, even providing cloaking devices to Starfleet vessels like the U.S.S. Defiant in a limited capacity.

Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.

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With all the excitement of movies to come this week thanks to CinemaCon, it was almost easy to forget that MGM provided an interesting update on one of our favorite movies of the year that’s already out: Project Hail Mary will head back to IMAX theaters this weekend for an extended theatrical run. But that extension also means one thing: you’ll have to wait to stream it at home for a good while longer.

During its presentation at CinemaCon this week MGM confirmed that Phil Lord and Chris Miller’s sci-fi hit would make its return to IMAX screens for a limited-time, one-week run starting this weekend, a move that will likely inch Project Hail Mary ever closer to crossing the $600 million box office mark. But to put a finer point on the news, Miller took to Twitter yesterday to confirm specifically that the extension means you won’t be able to watch the film at home for the forseeable future.

“It won’t be on streaming any time soon,” Miller’s tweet reads in part. “This is a movie that needs to be seen on a big screen […] Bring friends and loved ones. It’s an experience to share with others.”

Project Hail Mary launched on March 20, so it’s not too surprising that it’s not headed home just yet—it’s just shy of a month into its theatrical window, which has now been extended by at least another week with the return to IMAX. But as studios begin to try realigning towards more theatrical releases with longer exclusivity windows again (one of the lingering aftereffects of covid’s impact on movie theaters), we should probably expect some of the biggest films of the year and beyond to try and hold off of hitting streaming for as long as they can.

At least in Project Hail Mary‘s case, you can still go and see it somewhere, even if it’s not at home. Good things come to those who wait, but for now, you can head to a movie theater to get your fix again.

Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.

#Project #Hail #Mary #Wont #Coming #Streaming #TimeAmazon MGM,Project Hail Mary,Streaming">‘Project Hail Mary’ Won’t Be Coming to Streaming Any Time Soon
                With all the excitement of movies to come this week thanks to CinemaCon, it was almost easy to forget that MGM provided an interesting update on one of our favorite movies of the year that’s already out: Project Hail Mary will head back to IMAX theaters this weekend for an extended theatrical run. But that extension also means one thing: you’ll have to wait to stream it at home for a good while longer. During its presentation at CinemaCon this week MGM confirmed that Phil Lord and Chris Miller’s sci-fi hit would make its return to IMAX screens for a limited-time, one-week run starting this weekend, a move that will likely inch Project Hail Mary ever closer to crossing the 0 million box office mark. But to put a finer point on the news, Miller took to Twitter yesterday to confirm specifically that the extension means you won’t be able to watch the film at home for the forseeable future.

  We announced yesterday that MGM is extending the exclusive theatrical window for PROJECT HAIL MARY so it won’t be on streaming anytime soon. This is a movie that needs to be seen on a big screen – and w a full return to IMAX screens for 1 week only starting this weekend, make… https://t.co/suK8NYpgWM — Christopher Miller (@chrizmillr) April 16, 2026  “It won’t be on streaming any time soon,” Miller’s tweet reads in part. “This is a movie that needs to be seen on a big screen […] Bring friends and loved ones. It’s an experience to share with others.” Project Hail Mary launched on March 20, so it’s not too surprising that it’s not headed home just yet—it’s just shy of a month into its theatrical window, which has now been extended by at least another week with the return to IMAX. But as studios begin to try realigning towards more theatrical releases with longer exclusivity windows again (one of the lingering aftereffects of covid’s impact on movie theaters), we should probably expect some of the biggest films of the year and beyond to try and hold off of hitting streaming for as long as they can.

 At least in Project Hail Mary‘s case, you can still go and see it somewhere, even if it’s not at home. Good things come to those who wait, but for now, you can head to a movie theater to get your fix again.  Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.      #Project #Hail #Mary #Wont #Coming #Streaming #TimeAmazon MGM,Project Hail Mary,Streaming

thanks to CinemaCon, it was almost easy to forget that MGM provided an interesting update on one of our favorite movies of the year that’s already out: Project Hail Mary will head back to IMAX theaters this weekend for an extended theatrical run. But that extension also means one thing: you’ll have to wait to stream it at home for a good while longer.

During its presentation at CinemaCon this week MGM confirmed that Phil Lord and Chris Miller’s sci-fi hit would make its return to IMAX screens for a limited-time, one-week run starting this weekend, a move that will likely inch Project Hail Mary ever closer to crossing the $600 million box office mark. But to put a finer point on the news, Miller took to Twitter yesterday to confirm specifically that the extension means you won’t be able to watch the film at home for the forseeable future.

“It won’t be on streaming any time soon,” Miller’s tweet reads in part. “This is a movie that needs to be seen on a big screen […] Bring friends and loved ones. It’s an experience to share with others.”

Project Hail Mary launched on March 20, so it’s not too surprising that it’s not headed home just yet—it’s just shy of a month into its theatrical window, which has now been extended by at least another week with the return to IMAX. But as studios begin to try realigning towards more theatrical releases with longer exclusivity windows again (one of the lingering aftereffects of covid’s impact on movie theaters), we should probably expect some of the biggest films of the year and beyond to try and hold off of hitting streaming for as long as they can.

At least in Project Hail Mary‘s case, you can still go and see it somewhere, even if it’s not at home. Good things come to those who wait, but for now, you can head to a movie theater to get your fix again.

Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.

#Project #Hail #Mary #Wont #Coming #Streaming #TimeAmazon MGM,Project Hail Mary,Streaming">‘Project Hail Mary’ Won’t Be Coming to Streaming Any Time Soon‘Project Hail Mary’ Won’t Be Coming to Streaming Any Time Soon
                With all the excitement of movies to come this week thanks to CinemaCon, it was almost easy to forget that MGM provided an interesting update on one of our favorite movies of the year that’s already out: Project Hail Mary will head back to IMAX theaters this weekend for an extended theatrical run. But that extension also means one thing: you’ll have to wait to stream it at home for a good while longer. During its presentation at CinemaCon this week MGM confirmed that Phil Lord and Chris Miller’s sci-fi hit would make its return to IMAX screens for a limited-time, one-week run starting this weekend, a move that will likely inch Project Hail Mary ever closer to crossing the $600 million box office mark. But to put a finer point on the news, Miller took to Twitter yesterday to confirm specifically that the extension means you won’t be able to watch the film at home for the forseeable future.

  We announced yesterday that MGM is extending the exclusive theatrical window for PROJECT HAIL MARY so it won’t be on streaming anytime soon. This is a movie that needs to be seen on a big screen – and w a full return to IMAX screens for 1 week only starting this weekend, make… https://t.co/suK8NYpgWM — Christopher Miller (@chrizmillr) April 16, 2026  “It won’t be on streaming any time soon,” Miller’s tweet reads in part. “This is a movie that needs to be seen on a big screen […] Bring friends and loved ones. It’s an experience to share with others.” Project Hail Mary launched on March 20, so it’s not too surprising that it’s not headed home just yet—it’s just shy of a month into its theatrical window, which has now been extended by at least another week with the return to IMAX. But as studios begin to try realigning towards more theatrical releases with longer exclusivity windows again (one of the lingering aftereffects of covid’s impact on movie theaters), we should probably expect some of the biggest films of the year and beyond to try and hold off of hitting streaming for as long as they can.

 At least in Project Hail Mary‘s case, you can still go and see it somewhere, even if it’s not at home. Good things come to those who wait, but for now, you can head to a movie theater to get your fix again.  Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.      #Project #Hail #Mary #Wont #Coming #Streaming #TimeAmazon MGM,Project Hail Mary,Streaming

With all the excitement of movies to come this week thanks to CinemaCon, it was almost easy to forget that MGM provided an interesting update on one of our favorite movies of the year that’s already out: Project Hail Mary will head back to IMAX theaters this weekend for an extended theatrical run. But that extension also means one thing: you’ll have to wait to stream it at home for a good while longer.

During its presentation at CinemaCon this week MGM confirmed that Phil Lord and Chris Miller’s sci-fi hit would make its return to IMAX screens for a limited-time, one-week run starting this weekend, a move that will likely inch Project Hail Mary ever closer to crossing the $600 million box office mark. But to put a finer point on the news, Miller took to Twitter yesterday to confirm specifically that the extension means you won’t be able to watch the film at home for the forseeable future.

“It won’t be on streaming any time soon,” Miller’s tweet reads in part. “This is a movie that needs to be seen on a big screen […] Bring friends and loved ones. It’s an experience to share with others.”

Project Hail Mary launched on March 20, so it’s not too surprising that it’s not headed home just yet—it’s just shy of a month into its theatrical window, which has now been extended by at least another week with the return to IMAX. But as studios begin to try realigning towards more theatrical releases with longer exclusivity windows again (one of the lingering aftereffects of covid’s impact on movie theaters), we should probably expect some of the biggest films of the year and beyond to try and hold off of hitting streaming for as long as they can.

At least in Project Hail Mary‘s case, you can still go and see it somewhere, even if it’s not at home. Good things come to those who wait, but for now, you can head to a movie theater to get your fix again.

Want more io9 news? Check out when to expect the latest Marvel, Star Wars, and Star Trek releases, what’s next for the DC Universe on film and TV, and everything you need to know about the future of Doctor Who.

#Project #Hail #Mary #Wont #Coming #Streaming #TimeAmazon MGM,Project Hail Mary,Streaming

Let’s use our car again, but this time we’ll get real numbers from the accelerometer in our smartphone. Say we start at a red light and then accelerate at 2 m/s2 (meters per second squared) for five seconds. From the equation above, Δv1 would be 2 x 5 = 10 m/s, so that’s our velocity. Now, after cruising for a while, we accelerate again at 1 m/s2 for five more seconds. Δv2 is then 1 x 5 = 5 m/s. Adding these two changes, our velocity is now 15 m/s. And so on.

The only problem is that inertial measurement isn’t as accurate as the Doppler method over long periods, because small errors will keep accumulating. That means you need to recalibrate your system periodically using some other method.

Optical Navigation

On Earth, people have long navigated by the stars. In the northern hemisphere, just find Polaris. It’s called the North Star because Earth’s axis of rotation points right at it. That’s why it appears stationary, while the other stars seem to revolve around it. If you point a finger at Polaris you’ll be pointing north, and you can use that orientation to go in whatever direction you want.

Now, if you can measure the angle of Polaris above the horizon, you’ll also know your latitude. If the angle is 30 degrees, you’re at latitude 30 degrees. See, it’s easy. And once you can measure position, you just need to do it twice and record the time interval to find your velocity.

But celestial navigation works because we know how the Earth rotates, and that doesn’t help in a spacecraft. Oh well, can we just use the stars like you would use the cows on the side of the road? Nope. The stars are so far away, astronauts would need to travel for many, many generations to detect any shift in their position. Like the airplane flying over the sea, you’d seem to be stationary, even while traveling 25,000 mph.

But we can still use the basic idea. For optical navigation in space, a spacecraft can locate other objects in the solar system. By knowing the precise location of these objects (which change over time) and where they appear relative to the viewer, it’s possible to triangulate a position. And again, by taking multiple position measurements over time, you can calculate a velocity.

In the end, even though spaceships lack speedometers, it’s possible to track their speed indirectly with a little physics. But it’s just another example of how flying in space is really, totally different—and way more complicated—than driving or flying on Earth.

#Astronauts #Fast #Theyredot physics,physics,astronomy,space,spacecraft,moon landing,navigation,acceleration">How Can Astronauts Tell How Fast They’re Going?Let’s use our car again, but this time we’ll get real numbers from the accelerometer in our smartphone. Say we start at a red light and then accelerate at 2 m/s2 (meters per second squared) for five seconds. From the equation above, Δv1 would be 2 x 5 = 10 m/s, so that’s our velocity. Now, after cruising for a while, we accelerate again at 1 m/s2 for five more seconds. Δv2 is then 1 x 5 = 5 m/s. Adding these two changes, our velocity is now 15 m/s. And so on.The only problem is that inertial measurement isn’t as accurate as the Doppler method over long periods, because small errors will keep accumulating. That means you need to recalibrate your system periodically using some other method.Optical NavigationOn Earth, people have long navigated by the stars. In the northern hemisphere, just find Polaris. It’s called the North Star because Earth’s axis of rotation points right at it. That’s why it appears stationary, while the other stars seem to revolve around it. If you point a finger at Polaris you’ll be pointing north, and you can use that orientation to go in whatever direction you want.Now, if you can measure the angle of Polaris above the horizon, you’ll also know your latitude. If the angle is 30 degrees, you’re at latitude 30 degrees. See, it’s easy. And once you can measure position, you just need to do it twice and record the time interval to find your velocity.But celestial navigation works because we know how the Earth rotates, and that doesn’t help in a spacecraft. Oh well, can we just use the stars like you would use the cows on the side of the road? Nope. The stars are so far away, astronauts would need to travel for many, many generations to detect any shift in their position. Like the airplane flying over the sea, you’d seem to be stationary, even while traveling 25,000 mph.But we can still use the basic idea. For optical navigation in space, a spacecraft can locate other objects in the solar system. By knowing the precise location of these objects (which change over time) and where they appear relative to the viewer, it’s possible to triangulate a position. And again, by taking multiple position measurements over time, you can calculate a velocity.In the end, even though spaceships lack speedometers, it’s possible to track their speed indirectly with a little physics. But it’s just another example of how flying in space is really, totally different—and way more complicated—than driving or flying on Earth.#Astronauts #Fast #Theyredot physics,physics,astronomy,space,spacecraft,moon landing,navigation,acceleration

flying in space is really, totally different—and way more complicated—than driving or flying on Earth.

#Astronauts #Fast #Theyredot physics,physics,astronomy,space,spacecraft,moon landing,navigation,acceleration">How Can Astronauts Tell How Fast They’re Going?

Let’s use our car again, but this time we’ll get real numbers from the accelerometer in our smartphone. Say we start at a red light and then accelerate at 2 m/s2 (meters per second squared) for five seconds. From the equation above, Δv1 would be 2 x 5 = 10 m/s, so that’s our velocity. Now, after cruising for a while, we accelerate again at 1 m/s2 for five more seconds. Δv2 is then 1 x 5 = 5 m/s. Adding these two changes, our velocity is now 15 m/s. And so on.

The only problem is that inertial measurement isn’t as accurate as the Doppler method over long periods, because small errors will keep accumulating. That means you need to recalibrate your system periodically using some other method.

Optical Navigation

On Earth, people have long navigated by the stars. In the northern hemisphere, just find Polaris. It’s called the North Star because Earth’s axis of rotation points right at it. That’s why it appears stationary, while the other stars seem to revolve around it. If you point a finger at Polaris you’ll be pointing north, and you can use that orientation to go in whatever direction you want.

Now, if you can measure the angle of Polaris above the horizon, you’ll also know your latitude. If the angle is 30 degrees, you’re at latitude 30 degrees. See, it’s easy. And once you can measure position, you just need to do it twice and record the time interval to find your velocity.

But celestial navigation works because we know how the Earth rotates, and that doesn’t help in a spacecraft. Oh well, can we just use the stars like you would use the cows on the side of the road? Nope. The stars are so far away, astronauts would need to travel for many, many generations to detect any shift in their position. Like the airplane flying over the sea, you’d seem to be stationary, even while traveling 25,000 mph.

But we can still use the basic idea. For optical navigation in space, a spacecraft can locate other objects in the solar system. By knowing the precise location of these objects (which change over time) and where they appear relative to the viewer, it’s possible to triangulate a position. And again, by taking multiple position measurements over time, you can calculate a velocity.

In the end, even though spaceships lack speedometers, it’s possible to track their speed indirectly with a little physics. But it’s just another example of how flying in space is really, totally different—and way more complicated—than driving or flying on Earth.

#Astronauts #Fast #Theyredot physics,physics,astronomy,space,spacecraft,moon landing,navigation,acceleration

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