The Real History Behind Christopher Nolan’s ‘Oppenheimer’


The “father of the atomic bomb” has long been misunderstood. Will the new film finally get J. Robert Oppenheimer right?

Cillian Murphy as J. Robert Oppenheimer in Christopher Nolan's new film

Cillian Murphy as J. Robert Oppenheimer in Christopher Nolan’s newest film Universal Pictures

Andy Kifer

Since the end of World War II, historians and artists alike have been fascinated by the brilliant, enigmatic J. Robert Oppenheimer, the theoretical physicist who led the Manhattan Project laboratory that developed the atomic bomb. Beginning as early as 1946, documentariestelevision miniseriesplaysbooksgraphic novelsfeature films and even an opera have explored the scientist’s life, work and legacy. In recent years, however, much of that complexity has been reduced to a single popular image: the broken genius, haunted by his own invention, reciting a line from the Bhagavad Gita in a 1965 NBC News documentary. “Now I am become death, the destroyer of worlds,” Oppenheimer intones.

But Oppenheimer’s life was about far more than regret. “[He] was interesting as the father of the bomb,” says Kai Bird, co-author of the 2005 Pulitzer Prize-winning biography American Prometheus: The Triumph and Tragedy of J. Robert Oppenheimer. “But the real arc in the story is the tragedy.”

YouTube Logo

Christopher Nolan’s Oppenheimer,which opens in theaters on July 21, will be the first feature-length film to tackle the scientist’s life in its entirety, and it promises to be spectacular. Starring Cillian Murphy of “Peaky Blinders” fame in the title role alongside an ensemble A-list cast, the film (which uses American Prometheus as its main source material) will reintroduce the scientist and the top-secret bomb project he helmed to a new generation of Americans. Oppenheimer provides an opportunity to revisit this charismatic, contradictory man and reconsider how previous attempts to tell his story have succeeded—and failed—at fathoming one of the 20th century’s most fascinating public figures.

Oppenheimer and the Manhattan Project

Born into a secular Jewish family in New York City in 1904 and educated at Manhattan’s Ethical Culture School, Oppenheimer graduated summa cum laude from Harvard University in just three years. If Harvard was easy, growing out of his awkward adolescence was harder. He struggled with mental health issues while pursuing a graduate degreeat the University of Cambridge—“I was on the point of bumping myself off,” he later recalled—and ended up on probation after lacing an apple with chemicals and leaving it on his tutor’s desk. But by the time World War II broke out in 1939, Oppenheimer had transformed himself into a respected physicist at the University of California, Berkeley. “He was sort of a caricature of the eccentric professor,” Bird says, an intellectual omnivore who read Sanskrit, loved Elizabethan poetryrode horses and made a great martini.

He had also fallen in love with Jean Tatlock (played by Florence Pugh in Nolan’s film), a dues-paying member of the Communist Party who awakened his interest in politics. Oppenheimer was “likely sympathetic to … communist goals,” according to the nonprofit Atomic Heritage Foundation, but he never officially joined the party. (“Any attempt to label Robert Oppenheimer a party member is a futile exercise—as the FBI learned to its frustration over many years,” wrote Bird and co-author Martin J. Sherwin, who died in October 2021 at age 84, in American Prometheus.) But many of his closest friends and family were party members at one point or another: his brother, Frank Oppenheimer; his friend Haakon Chevalier; and his future wife, Kitty Oppenheimer. These associations would cast suspicion on the physicist himself later in his life.

A circa 1950 photograph of Albert Einstein (left) and Oppenheimer (right)
A circa 1950 photograph of Albert Einstein (left) and Oppenheimer (right) Public domain via Wikimedia Commons

Oppenheimer’s political leanings didn’t prevent him from being recruited, in early 1942, for a secret project authorized by President Franklin D. Roosevelt that was drawing scientists from all over the country. Three years earlier, Albert Einstein had written a letter to Roosevelt warning that breakthroughs in nuclear fission promised “extremely powerful bombs of a new type.” Now, the race was on to figure out how to build one of these bombs before Germany did.

In the summer of 1942, Oppenheimer organized a series of secret seminars at Berkeley, where the United States’ top physicists roughed out the outlines of a possible bomb. As it turned out, Oppenheimer was a natural manager. “I don’t know how he had acquired this facility for handling people,” said Edward Teller, a colleague who would later testify against him. “Those who knew him well were really surprised.”

That September, General Leslie Groves (played by Matt Damon in the new film), an Army engineer who’d previously overseen construction of the Pentagon, took over as head of what was by then called the Manhattan Project, after its inaugural offices in lower Manhattan. Groves knew construction but not physics, so the charming Berkeley physicist caught his eye. “Oppenheimer was the first scientist Groves had met on his tour who grasped that building an atomic bomb required finding practical solutions to a variety of cross-disciplinary problems,” wrote Bird and Sherwin. He wasn’t an obvious choice—“He couldn’t run a hamburger stand,” said a Berkeley colleague—but in October 1942, Groves named Oppenheimer the project’s scientific director.

Oppenheimer (left) and General Leslie Groves (right) at ground zero of the nuclear bomb test site
Oppenheimer (left) and General Leslie Groves (right) at ground zero of the nuclear bomb test site Public domain via Wikimedia Commons

The government operation brought hundreds, and eventually thousands, of scientists, civilians and Army personnel to a mesa in Los Alamos, New Mexico. Their ranks eventually included Teller, Hans BetheRichard FeynmanSeth NeddermeyerRobert SerberKenneth BainbridgeEnrico Fermi and many others. (Nolan’s film portrays each of these figures and, judging by the full cast list, more or less recreates the entire field of theoretical physics in the 1930s and ’40s, including Kenneth Branagh as Nobel Prize winner Niels Bohr.) The scientists reported directly to Oppenheimer, who, at 38, was learning on the job how to run a lab.

Oppenheimer’s lab was only one part of the Manhattan Project. Built on the site of a former boys’ school, Los Alamos was one of three “secret cities” seized and transformed by the U.S. government in late 1942 and early 1943. The other two—Oak Ridge, Tennessee, and Hanford, Washington—accounted for the vast majority of the manpower, expense and industrial scale of the project, which employed an estimated half a million people between 1942 and 1945. At Oak Ridge, uranium was refined at the largest factory in the world, newly built for that purpose. In Hanford, an area half the size of Rhode Island was cleared of residents, their houses bulldozed to make way for reactors to produce plutonium. “I told you it couldn’t be done without turning the whole country into a factory,” Bohr said to Teller in 1944. “You have done just that.”

At Los Alamos, Oppenheimer came into his own as a gifted leader. “[He] had a very distinctive voice that was very soft,” says Bird. “You had to listen very carefully, but he was magnetic.” That magnetism kept the lab productive even after an initial design for the bomb, known as Thin Man, had to be scrapped in July 1944. Ultimately, the scientists settled on two workable designs for a bomb, which they called Fat Man and Little Boy. At 5:29 a.m. on July 16, 1945, almost three years of work culminated in the first nuclear detonation in history. Known as the Trinity test, it lit the hills of the New Mexico desert.

A group of physicists at a 1946 Los Alamos colloquium
A group of physicists at a 1946 Los Alamos colloquium. Oppenheimer is third from left in the second row, wearing a black jacket and tie. Other scientists featured in the image include Enrico Fermi, Edward Teller and Richard Feynman. Los Alamos National Laboratory via Wikimedia Commons

Oppenheimer, already famously thin, had lost weight during the project, and during the countdown, he reportedly barely breathed. Later dramatizations had the scientist reciting the line from the Bhagavad Gita during the moment of detonation (Oppenheimer himself later claimed the line had come to him then), but he reportedly said something closer to “It worked.”

After the test, Oppenheimer was transformed by relief. “I’ll never forget the way he stepped out of the car,” fellow Manhattan Project scientist Isidor Isaac Rabi later said. “His walk was like High Noon … this kind of strut. He had done it.”

On August 6, 1945, the Enola Gay dropped Little Boy on the Japanese city of Hiroshima. Three days later, Bockscardropped Fat Man on Nagasaki. Estimates of deaths from the two bombings vary widely, from a contemporary figure of around 110,000 to a later estimate of closer to 210,000. On August 15, Emperor Hirohito announced Japan’s surrender.

The battle over the bomb

In the years immediately following the war, public opinion about the use of the atomic bomb hadn’t yet solidified. The first time Oppenheimer appeared on the big screen was in August 1946, when he starred in the 18-minute documentary “Atomic Power,” which was part of Time’s “The March of Time” series. Onscreen, Oppenheimer (one of several figures who participated in the film, including Einstein, Groves and Rabi) re-enacts waiting anxiously for the detonation at Trinity with Rabi, who gives a stilted performance as he reassures his boss, “It’s going to work all right, Robert. And I’m sure we’ll never be sorry for it.”

YouTube Logo

In fact, Oppenheimer was already sorry. In October 1945, he told President Harry S. Truman (played by Gary Oldman in Nolan’s film), “Mr. President, I feel I have blood on my hands.” The tide of public opinion was also beginning to turn. Three weeks after “Atomic Power” was released, John Hersey’s searing, book-length article “Hiroshima” appeared in the New Yorker, awakening many Americans for the first time to the horrors of the bomb.

Fearing they were losing the battle for the history books, Truman and other officials sprang into action, compelling former Secretary of War Henry Stimson to defend the use of the bomb in a Harper’s magazinearticle published in February 1947. The story, which reads as a simple recitation of the facts, portrays the decision to use the bomb as one made with sagacious care. It introduced the argument—repeated often since—that the bomb prevented an Allied land invasion of Japan that would have cost “over a million casualties, to American forces alone.”

“That article really set the history for most Americans for the next generation,” Bird says. “And the narrative was, ‘Oh, it was a difficult decision. It was terrible. But it was necessary, and it saved perhaps a million American lives.’”

The first major Hollywood film about the bomb, The Beginning or the End, debuted the month after Stimson’s article. Initially conceived by atomic scientists as a way to educate the public about the dangers of nuclear warfare, the movie went through script approvals and retakes ordered by Groves and Truman that turned it into a “pro-bomb celebration—dictated by the Pentagon and White House,” wrote Greg Mitchell in his 2020 book, The Beginning or the EndHow Hollywood—and America—Learned to Stop Worrying and Love the Bomb.

Poster for the 1947 film The Beginning or the End
Poster for the 1947 film The Beginning or the End Metro-Goldwyn-Mayer
The Hiroshima atom bomb cloud two to five minutes after detonation
The Hiroshima atom bomb cloud two to five minutes after detonation Public domain via Wikimedia Commons

Directed by Norman Taurog, the film “is so instructive because it is the earliest, and one of the most complete, reassertions of the pro-bomb narrative just when doubts were being raised,” Mitchell tells Smithsonian magazine. “Even Truman got involved, to the extent of ordering a costly retake and getting the actor playing him fired. The studio voluntarily handed over control of the film to the Pentagon, via Groves, and the White House. Oppenheimer himself caved to pressure.”

The Beginning or the End claimed the American military dropped warning leaflets about the atomic bomb on Hiroshima and that the Enola Gay came under attack from Japanese antiaircraft missile fire on its bombing run. Like Stimson’s article, it depicted Truman carefully working through the decision to drop the bomb before arriving at a pivotal moment.

In fact, the U.S. did not drop leaflets warning of the atomic bomb specifically, though pilots may have dropped more general notices of impending attacks on Hiroshima, and the Enola Gay did not come under antiaircraft fire. Many historians disagree that there was a single moment of “decision” on Truman’s part. In an essay included in the 2020 anthology The Age of HiroshimaAlex Wellerstein, a nuclear historian at the Stevens Institute of Technology in New Jersey, wrote that Truman “was actually quite peripheral to most of the decisions that led to the use of the weapons.” Wellerstein argued that Truman may have even mistakenly believed that Hiroshima was a military target rather than a city made up largely of civilians. As for that figure of one million projected American casualties, Bird later asked Stimson’s ghostwriter, Mac Bundy, where he got it. “He looked at me,” Bird recalls, “and he says, ‘Oh, we pulled it out of thin air.’”

Oppenheimer described the script of The Beginning or the End as “without purpose or insight.” Another physicist, Leo Szilardput it even more bluntly: “If our sin as scientists was to make and use the atomic bomb, then our punishment was to watch The Beginning or the End.”

Cillian Murphy, as J. Robert Oppenheimer, walks through a crowd of photographers
Murphy, as Oppenheimer, walks through a crowd of photographers. The real Oppenheimer started speaking out publicly about the dangers of atomic warfare soon after the war’s end. Universal Pictures

The Oppenheimer security hearing

Almost immediately, Oppenheimer began speaking out publicly about the dangers of atomic warfare, even as he continued to act as a nuclear weapons consultant for the U.S. government. In November 1945, he told an audience in Philadelphia that the bomb was “by all the standards of the world we grew up in … an evil thing.” He gave television interviews starkly elucidating the risk of nuclear war. In 1949, as the head of an advisory committee for the newly formed Atomic Energy Commission (AEC), he delivered a report warning against developing a hydrogen bomb—a fusion weapon more powerful than the Trinity, Hiroshima or Nagasaki bombs—that had been conceived by fellow Manhattan Project scientist Teller. “A super bomb might become a weapon of genocide,” Oppenheimer wrote. “A super bomb should never be produced.” In 1953, he gave a speech likening the nuclear-capable United States and Soviet Union to “two scorpions in a bottle, each capable of killing the other, but only at the risk of his own life.”

Oppenheimer’s outspoken warnings made him a target, and in December 1953, amid McCarthy-era paranoia about Soviet spies in the highest levels of government, AEC Chairman Lewis Strauss (played by Robert Downey Jr. in Nolan’s film), who harbored a dislike for Oppenheimer, called the scientist into his office and told him his top-secret security clearance had been revoked. Oppenheimer insisted on defending himself, leading the AEC to call what became a highly publicized security hearing to resolve the matter.

The monthlong hearing, which began on April 12, 1954, amounted to an X-ray of Oppenheimer’s adult life. Transgressions large and small were dragged into the open and held up to exacting scrutiny. Key pieces of the case against Oppenheimer included his close friendship with Chevalier, a scholar of French literature at Berkeley and a card-carrying Communist whom the physicist had once protected from incrimination, as well as Oppenheimer’s opposition to Teller’s hydrogen bomb. The usually persuasive scientist panicked under questioning by AEC lawyer Roger Robb; at one point, caught in a contradiction, Oppenheimer accounted for his defense of Chevalier by admitting bluntly, “I was an idiot.” But he also had to defend personal matters, such as his decision to spend a night with his communist ex-fiancée, Tatlock, in the summer of 1943, while he was working at Los Alamos, six months before she died by suicide in 1944. Why did he have to see her? The committee asked. “Because she was still in love with me,” Oppenheimer responded.

A 1946 photo of Oppenheimer
A 1946 photo of Oppenheimer Public domain via Wikimedia Commons
Edward Teller
Edward Teller, the former Manhattan Project scientist who later testified against Oppenheimer at his security hearing Public domain via Wikimedia Commons

On May 27, the board overseeing the hearings voted 2 to 1 not to reinstate Oppenheimer’s security clearance. “I personally think that our failure to clear Dr. Oppenheimer will be a black mark on the escutcheon of our country,” wrote lone dissenter Ward V. Evans. Either way, Oppenheimer’s relationship with the U.S. government was now officially over. He returned to Princeton, New Jersey, where he’d been the director of the Institute for Advanced Study since 1947. The hearings “destroyed him,” Rabi later said. Another friend, diplomat George Kennan, remembered trying to comfort Oppenheimer by telling him he’d surely be welcome abroad. “His answer, given to me with tears in his eyes: ‘Damn it, I happen to love this country.’”

Oppenheimer tried to minimize the importance of the hearings. “I think of this as a major accident, much like a train wreck or the collapse of a building,” he told a reporter. “It has no relation or connection to my life. I just happened to be there.” As much as he might have wished that to be true, Oppenheimer’s downfall during the hearings came to define him in the public eye. In 1964, the German playwright Heinar Kipphardt drew directly on the published transcripts of the security hearings for his In the Matter of J. Robert Oppenheimer. Discussing the play with the Washington Post,perhaps still trying to prevent his downfall from defining him, Oppenheimer said, “The whole damn thing was a farce, and these people are trying to make a tragedy out of it.”

In an attempt at public rehabilitation, President Lyndon B. Johnson presented Oppenheimer with the Enrico Fermi Award, the AEC’s highest honor, in 1963. Nonetheless, the physicist never fully recovered from the blow to his reputation. He lived out the rest of his days in Princeton, where he kept his job at the Institute for Advanced Study until 1966, and died of cancer there in February 1967. As the New York Times wrote in his obituary, “This bafflingly complex man nonetheless never fully succeeded in dispelling doubts about his conduct.”

Florence Pugh (left) as Jean Tatlock and Cillian Murphy (right) as J. Robert Oppenheimer
Florence Pugh (left) as Jean Tatlock and Murphy (right) as Oppenheimer Universal Pictures

Oppenheimer’s security clearance remained revoked until December 2022, when the Department of Energy vacated the commission’s 1954 decision. “Oppenheimer occupies a central role in our history for leading the nation’s atomic efforts during World War II and planting the seeds for the Department of Energy’s national laboratories,” said Secretary of Energy Jennifer Granholm in a statement. “As time has passed, more evidence has come to light of the bias and unfairness of the process that Dr. Oppenheimer was subjected to, while the evidence of his loyalty and love of country [has] only been further affirmed.”

The myth of Oppenheimer

In the more than 50 years since Oppenheimer’s death, popular culture has taken varied approaches to exploring his life. The Peabody Award-winning 1981 documentary The Day After Trinityfocused on his regret over his role in building the bomb. The 1980 BBC TV miniseries “Oppenheimer,” by contrast, starred a thin, quietly charismatic Sam Waterston and was more interested in the question of Oppenheimer’s communist ties and his downfall.

Later fictional depictions of Oppenheimer grew less interested in complex readings of his psychology and often flattened him into a character who sometimes bordered on the ridiculous. In 1989, director Roland Joffé made a big-budget bet on the story of the Manhattan Project in Fat Man and Little Boy. Despite an A-list cast—Paul Newman as Groves, John Cusack as a fictional Manhattan Project scientist, Laura Dern as that scientist’s girlfriend—the film flopped. The script was simplistic, the dialogue groan-inducing (“Naked. Isn’t that a beautiful word?” Dern says to Cusack when propositioning him) and veracity an afterthought. But the film suffered most from the performance of Dwight Schultz, best known to viewers from “The A-Team” and “Star Trek: The Next Generation,” as Oppenheimer. Schultz brought a blankness to his portrayal of a man who famously had charisma to spare. “Schultz is stiff and actorly,” wrote the Washington Post. “Like an irredeemably tone-deaf singer, he hits only false notes.”

YouTube Logo

In the otherwise excellent TV show “Manhattan,” which ran for two seasons in 2014 and 2015, Daniel London played Oppenheimer as an already broken man, as though the actor’s only reference for the character was the famous “I am become death” interview. His Oppenheimer was more interested in self-preservation than the success of the project, whereas the real Oppenheimer of the Los Alamos years was a nimble ball of energy, guiding the complex endeavor toward completion thanks to his keen feeling for the challenges his fellow scientists faced.

No list would be complete without one other fictional depiction of Oppenheimer: Pulitzer Prize-winning composer John Adams’ 2005 opera, Doctor Atomic. If Oppenheimer objected to Kipphardt’s play, he surely would have found Doctor Atomic’s elevation of his life into an operatic Faustian tragedy ridiculous. But the opera, which centers around the days leading up to the Trinity test and culminates in the detonation of the first atomic bomb, was rapturously received by critics and has been restaged several times since its debut. In the New York Times, science writer Dennis Overbye wrote that the opera had disabused him of his preconceptions about the bomb: “I long ago concluded that there was not much new to say about the atomic bomb. But I was wrong. As I was watching … I began to wonder if anything had yet been said that counted.”

President Lyndon B. Johnson presents Oppenheimer (left) with the Enrico Fermi Award in 1963.
President Lyndon B. Johnson presents Oppenheimer (left) with the Enrico Fermi Award in 1963. Public domain via Wikimedia Commons

Nolan’s Oppenheimer

Before Sherwin’s death in 2021, he and Bird read several scripts based on American Prometheus. One, Bird says, was boring. Another was just weird: “It had dream sequences, a ghost speaking Oppenheimer’s poetry. It had a scene in which [Oppenheimer] is at a cocktail party in Berkeley and imagines himself dropping a cyanide pill into Edward Teller’s drink and watching him collapse on the floor and die in agony.” Bird and Sherwin sent back a long memo detailing the script’s many historical errors.

So Bird was relieved when, in fall 2021, he became one of a handful of people outside the film’s production to read Nolan’s take on Oppenheimer. “I think it’s a fabulous script,” Bird says. Unlike other recent depictions, it covers scenes from Oppenheimer’s entire life and doesn’t shy away from the moral questions of the bomb. “Nolan covers in a very deft way the argument among the physicists over whether the bomb was necessary or not and has Oppenheimer after Hiroshima saying the bomb was used on a virtually already defeated enemy,” Bird adds. “People who know nothing about Oppenheimer will go thinking they’re going to see a movie about the father of the atomic bomb.” Instead, “they’re going to see this mysterious figure and a deeply mysterious biographical story.”

Regardless of whether subject matter experts believe there is nothing new to say, the general public’s understanding of Oppenheimer and the Manhattan Project hasn’t changed significantly since Stimson’s 1947 Harper’s article. After all, most people’s sense of history doesn’t come by way of the academy or densely researched biographies. Visiting Los Alamos myself a few years ago, I asked a docent what they thought might renew public interest in the history of the Manhattan Project.

The answer? “A movie.”

Cillian Murphy as Oppenheimer
Murphy as Oppenheimer (center, speaking into microphone) Universal Pictures

“Oppenheimer himself couldn’t make up his mind how he felt about making and helping to use the bomb, right to the end of his life,” says Mitchell. Until now, “filmmakers also couldn’t seem to get a handle on his conflicting emotions and statements. In that sense, he is a valuable audience surrogate, severely divided or conflicted on these questions.”

Nolan’s film arrives at a precarious moment in which optimism about nuclear disarmament is giving way to talk of a new nuclear ageFew world leaders today have direct experience with the horrors of nuclear bombs, and some younger people are ignorant of even basic facts about World War II. But perhaps our distance from Oppenheimer’s era also presents an opportunity.

“Today, almost 80 years have passed since the end of World War II,” says Cynthia C. Kelly, president of the Atomic Heritage Foundation. Now, she adds, “the public can more openly consider different interpretations of atomic history.”

Why did it take so long for a director of Nolan’s caliber to take on Oppenheimer’s story? Perhaps it’s because we’re only now far enough away from those world-changing events to be open to seeing them—and him—with fresh eyes.

That’s no easy task. As Oppenheimer himself told an interviewer in 1948, “If you’ve lived a life that isn’t free and open with people, it’s almost impossible to unsnarl it, to unravel the ball of twine.”

YouTube Logo

The mind of Oppenheimer, inventor of nuclear bomb who turned pacifist


main img

Cillian Murphy essays the role of J Robert Oppenheimer in Christopher Nolan’s Oppenheimer.

STORY HIGHLIGHTS

J Robert Oppenheimer was a physicist and director of the Manhattan Project, which developed the world’s first nuclear bomb. He witnessed the destructive power of the bomb in Hiroshima and Nagasaki. Despite his role in the creation of the most destructive force the world has ever seen, he became an outspoken advocate for nuclear disarmament. Christopher Nolan’s upcoming biopic, Oppenheimer, promises to explore the scientist’s complicated life and legacy.

In the early morning of July 16, 1945, J Robert Oppenheimer, a physicist, and director of the Manhattan Project, watched as the world’s first nuclear bomb exploded in the New Mexico desert. The blast was so powerful that it lit up the sky like a second sun, and Oppenheimer later recalled that he thought of a verse from the Hindu scripture the Bhagavad Gita just then: “If the radiance of a thousand suns were to burst at once into the sky, that would be like the splendor of the mighty one.” It was one other verse from the scripture that he spoke of and has come to be deeply associated with him. Lord Krishna, an incarnation of Vishnu, is in his universal form, and proclaims to Arjun: “Now I am become Death, the destroyer of worlds.” 

The technology that Oppenheimer helped develop served as the basis of Little Boy and Fat Man, two atomic bombs that laid waste to the Japanese cities of Hiroshima and Nagasaki in August 1945. The bombings effectively ended World War II, as Imperial Japan surrendered.

Oppenheimer had been instrumental in the development of nuclear weapons, but witnessing the destructive power of the bomb he helped invent made him question the morality of what he had done. In the years that followed, he became an outspoken advocate for nuclear disarmament, a stunning transformation that actually came very quickly after the destruction in Japan.

Who was J Robert Oppenheimer?

Born in New York City in 1904, Oppenheimer was a child prodigy with a passion for science. He studied at Harvard University and the Christ’s College, Cambridge, and in the 1930s, he became involved in the study of atomic physics. In 1942, he was recruited by the US government to work on the Manhattan Project, a top-secret program to develop the world’s first nuclear bomb.

Oppenheimer was appointed as the director of the Los Alamos laboratory in New Mexico, where the bomb was designed and built. He oversaw a team of thousands of scientists, engineers, and support staff, and he worked tirelessly to ensure that the bomb was ready for use as soon as possible. Despite his efforts, the bomb was not completed in time to be used in the European theatre of World War II, but it was ultimately, as describe above, used to devastating effect against Japan.

Oppenheimer, the unlikely apostle of peace

Only 11 days after the bombings in Japan, Oppenheimer urged then-US president Harry S. Truman to ban nuclear weapons. But the president was by now worried about Soviet Union’s aggression and paid him no heed. Oppenheimer also told Truman that he (Oppenheimer) had blood on his hands. 

It is believed by scholars that Oppenheimer’s request to Truman was not actually driven by the death and destruction in Japan, but by the possibility of further devastation that atomic weapons in the future could bring.

Oppenheimer had become disillusioned with the technology he had helped create. He began to publicly speak out against the proliferation of nuclear weapons, and he became an advocate for arms control and disarmament.

He strongly opposed the development and test of the H-bomb, a weapon with far greater destructive power than the original atomic bomb, in 1952. But his opposition to the bomb did not go down well with the government. It was the time of McCarthyism, after all — a time of intense anti-communist suspicion and persecution of dissenting voices. He was removed from the Atomic Energy Commission.

In 1954, Oppenheimer’s political views came under scrutiny when he was accused of being a security risk by the US government. During the height of the Cold War, Oppenheimer’s past associations with left-wing political groups and his vocal opposition to nuclear testing made him a target of suspicion for many in the government.

Despite his contributions to the Manhattan Project, Oppenheimer was ultimately stripped of his security clearance and barred from further government work. In the years that followed, Oppenheimer continued to speak out against nuclear weapons, and became a prominent voice in the anti-nuclear movement. 

The threat of nuclear weapons in the present time

The devastating impact of nuclear weapons is something that cannot be understated, with the potential to annihilate entire cities and leave a lasting impact on the environment for years to come. A full-fledged nuclear war would obliterate all life from earth. Moreover, the rise of non-state actors and terrorist groups has added a new dimension to the threat of nuclear weapons. The possibility of nuclear weapons falling into the wrong hands and being used for malicious purposes is hard to ignore. In the decades following Oppenheimer’s death in 1967, there have been several scares, but until now, his fears have blessedly not come to pass.

Christopher Nolan’s Oppenheimer

Oppenheimer’s story will be explored on the big screen with Christopher Nolan’s upcoming biopic of the scientist, titled simply Oppenheimer. The film, which is set to star Cillian Murphy in the role, promises to be a thought-provoking and insightful exploration of Oppenheimer’s life and legacy. The film also features Emily Blunt, Robert Downey Jr., Matt Damon, Rami Malek, Florence Pugh, Benny Safdie, Michael Angarano, Josh Hartnett, and Kenneth Branagh in the cast.

Edge of darkness: looking into the black hole at the heart of the Milky Way


A black hole as depicted in the 2014 film Interstellar. Director Christopher Nolan consulted astrophysicists to get a ‘realistic’ image.
A black hole as depicted in the 2014 film Interstellar. Director Christopher Nolan consulted astrophysicists to get a ‘realistic’ image.

At the heart of our galaxy, a vast black hole is devouring matter from the dust clouds that surround it. Little by little, expanses of interstellar material are being swallowed up by this voracious galactic carnivore that, in the process, has reached a mass that is 4m times that of our sun.

The Milky Way’s great black hole is 25,000 light years distant, surrounded by dense clusters of stars, shrouded by interstellar dust and, like all other black holes, incapable of emitting light.

Yet scientists believe they will soon be able to take a photograph of this interstellar behemoth – an extraordinarily ambitious feat that will involve the creation of a radio telescope that has the effective size of our entire planet and whose operation will involve scientists from four continents.

“It is going to be very, very hard to take this photograph but we think we now have the technological capability to do it,” says Manchester University astronomer Tom Muxlow, based at the Jodrell Bank observatory in Cheshire.

“To be precise, we are not going to take a direct photograph of the black hole at our galaxy’s heart. We are actually going to take a picture of its shadow. It will be an image of its silhouette sliding against the background glow of radiation of the heart of the Milky Way. That photograph will reveal the contours of a black hole for the first time.”

Our galaxy’s great black hole is also known as Sagittarius A*, because it lies in the constellation Sagittarius and the data collection that will be used to create its image is set to take place in April. However, it will probably require a further six months of work to put together the observations made by all of the Event Horizon Telescope project’s component telescopes, which include instruments at the south pole and in the Andes, Hawaii and Europe.

The resulting image, say scientists, could look very much like the one created by director Christopher Nolan for the film Interstellar. Working with US astrophysicist Kip Thorne, Nolan went to considerable pains to develop something that looked like a “realistic” black hole. Gargantua, as it is named in the film, is depicted as a round black patch that hangs menacingly in the sky with swirling, luminous strands of matter pouring into it.

These strands of matter are known as an accretion disc. “In fact, the accretion disc around the black hole in our galaxy’s core is likely to be much thicker, geometrically, than the one in Interstellar, and so look somewhat different,” says Thorne. Nevertheless, most astronomers believe the film’s black hole is a good representation of what might be seen when the Event Horizon Telescope does its work.

A black hole is a region of space where matter has collapsed in on itself and become compressed into an incredibly small region. Its gravitational pull is so great nothing can escape from it – not even light. The point of no return, the boundary at which a black hole’s gravitational pull becomes so great nothing can emerge, is known as an event horizon.

“The event horizon is a surface in space-time, and if you go beyond that then you cannot get out again,” says Robert Laing, of the European Southern Observatory, a partner in the project. “Not even light can get out.”

The fact that light cannot escape black holes makes them tricky to observe, to say the least. However, we know they exist because they affect nearby dust clouds, stars and galaxies. As discs of material swirl around black holes they become extremely hot and give off electromagnetic radiaiton that can be detected in telescopes. “That radiation will provide the background against which we hope to see the shadow of the black hole at our galaxy’s heart,” adds Muxlow.

US astrophysicist Kip Thorne helped design the black hole for the film Interstellar.
US astrophysicist Kip Thorne helped design the black hole for the film Interstellar.

Astronomers study black holes for several reasons. They are crucial to our attempts to understand the formation of galaxies, for example, and the EHT should provide vital observations for this work. However, its main purpose is simply to test general relativity. Einstein’s great theory has stood up well to scientific scrutiny over the last century – the recent discovery of gravitational waves, predicted by general relativity, being a good example. Black holes are also predicted by Einstein’s work and although astronomers have gleaned enough information to be sure they exist, their exact structures and shapes are unclear. The Event Horizon Telescope should put that right.

“We want to see whether the idea of a black hole having an event horizon is actually right and whether the quantitative predictions of what its shadow should look like are correct,” says Laing. “If general relativity is wrong in some way, you should eventually be able to see deviations from its predictions in the shape of the shadow and behaviour of our galaxy’s great black hole.”

In other words, if Einstein’s equations break down anywhere, they are most likely to do so at the edge of a black hole, where the fabric of space-time is being stretched more severely than any other place in the cosmos. As Laing says: “It’s the ultimate test.”

For example, if the shadow is precisely circular, this would indicate our galaxy’s black hole is not rotating. However, most predictions suggest that it should be spinning – which would produce a disc that has a dent.

The production of this evidence will strain the ingenuity and technological expertise of astronomers to their limits. Vast amounts of data, collected from observatories across the planet, will have to be combined to create a single image, an international collaboration that is being led by Shep Doeleman at the Harvard Smithsonian Center for Astrophysics.

“We are going to take advantage of the fact that all the gas and dust that is trying madly to fall into the black hole heats up to billions of degrees and the black hole casts a shadow against that intense light,” Doeleman said in a recent interview. “With the Event Horizon Telescope we capture light at different points on the Earth’s surface because our telescopes will be watching the same black hole at the same time. We freeze that light. We record it on hard-disk drives and then fly them back to a central computing cluster.” The computer will then create the image of the black hole.

In the UK, our astronomers’ main involvement in the project is channelled through our membership of the European Southern Observatory, which runs an array of 66 radio telescopes in the Andes called Alma (the Atacama Large Millimeter/submillimeter Array). This is one of the main instruments involved in the Event Horizon Telescope.

“To see through the dust and other material that lies between us and the centre of our galaxy, we have to use radiation that is about a millimetre in wavelength,” says Professor Tim O’Brien, another Jodrell Bank astronomer. “That compares with the wavelength of the light that we detect in our eyes, which is hundreds of times shorter in wavelength.”

The Milky Way, at whose centre lies the supermassive black hole Sagittarius A*.
The Milky Way, at whose centre lies the supermassive black hole Sagittarius A*.

This difference has a crucial consequence. Studying radiation with longer wavelengths makes it easier to peer through the dusty hearts of galaxies, including our Milky Way. However, to detect and study such radiation, astronomers need instruments that have far bigger collecting dishes than optical telescopes require. For an instrument designed to study millimetre-length radiation, you will need a telescope that is hundreds of times larger than a normal optical telescope, which gathers radiation of a much shorter wavelength. “In fact, if you want to observe, in detail, an object that is so distant and so obscured by dust as the black hole at the galaxy’s centre, you will have to design one that is as big as an entire planet,” says O’Brien.

Building a planet-sized telescope suggests all sorts of practical difficulties. Fortunately, there are ways round the problem. By combining the observations of a number of telescopes from different parts of the world, it is possible to create a machine that has equivalent gathering power to an Earth-sized device. The technique is known as very long baseline interferometry or VLBI and, in this case, it will create an instrument of unprecedented observing power. “The Event Horizon Telescope is the equivalent of a telescope that would allow you to read a newspaper headline on the moon while standing on the Earth,” says Muxlow.

The Event Horizon Telescope has not been designed solely to study our Milky Way’s black hole, however. Astronomers have other targets for it to observe. In particular, they plan to use it to try to take images of an even more remote object: a super-giant, elliptical galaxy in the constellation Virgo known as the M87 galaxy. It is 53m light years from the Earth and it also has a black hole at its heart.

“M87’s black hole is much larger than our galaxy’s but it is much further away, so it is going to be just as hard to study as the one that is inside the Milky Way,” said Laing. “However, the M87 black hole is much more active than our black hole. It is sucking in matter from surrounding space and ejecting it again in a spectacular jet, while our black hole is fairly quiescent at present. It will be very useful to compare the two black holes. black holes.”

Some of the antennas of the Atacama Large Millimeter/submillimeter Array (Alma) in the Atacama desert, Chile.
Pinterest
Some of the antennas of the Atacama Large Millimeter/submillimeter Array (Alma) in the Atacama desert, Chile. Photograph: Alamy

Just when we will get a chance to see these shadowy images of black holes is a different matter. Data from the different observatories that make up the Event Horizon Telescope will fill dozens of hard drives, the equivalent of 10,000 laptops’ worth of information. Shipping these from the South Pole Telescope, the project’s remotest instrument, is likely to take weeks, if not months. Then the data has to be combined on computers. “I think it will take at least nine months after we take our observations before we compile our first images,” says Muxlow.

Other problems that could affect the telescope’s cross-galactic photo bid in April include the weather, or to be more precise the levels of water vapour in the atmosphere. Water vapour plays havoc with observations made at millimetre wavelengths. Hence the placing of the Alma observatory high in the Andes – Atacama is one of the world’s driest places. Similarly, the south pole has a desert climate, almost never receiving any precipitation. These aid the EHT’s observing prowess but can occasionally be disrupted by weather that brings in unexpected clouds of water vapour. “We remain hopeful we will get our image in the next year, nevertheless,” says Laing.

Inception ending: Christopher Nolan finally discusses the meaning behind that spinning top


 

inception.jpg

Christopher Nolan has discussed the controversial and ambiguous ending to his film Inception, which saw a spinning top rotating and wobbling a little before cutting to black.

Unsurprisingly, he didn’t just say “it was all a dream” and then drop the mic, but gave a more nuanced explanation of what it was intended to symbolise, during a speech made to a graduating Princeton University class.

He started off with a pre-amble about pragmatism:

“In the great tradition of these speeches, generally someone says something along the lines of ‘Chase your dreams,’ but I don’t want to tell you that because I don’t believe that. I want you to chase your reality.

“I feel that over time, we started to view reality as the poor cousin to our dreams, in a sense….I want to make the case to you that our dreams, our virtual realities, these abstractions that we enjoy and surround ourselves with – they are subsets of reality.”

According to The Hollywood Reporter, he then went on to link this idea to the conclusion of Inception:

“The way the end of that film worked, Leonardo DiCaprio’s character Cobb — he was off with his kids, he was in his own subjective reality. He didn’t really care anymore, and that makes a statement: perhaps, all levels of reality are valid. The camera moves over the spinning top just before it appears to be wobbling, it was cut to black.

“I skip out of the back of the theater before people catch me, and there’s a very, very strong reaction from the audience: usually a bit of a groan. The point is, objectively, it matters to the audience in absolute terms: even though when I’m watching, it’s fiction, a sort of virtual reality. But the question of whether that’s a  dream or whether it’s real is the question I’ve been asked most about any of the films I’ve made. It matters to people because that’s the point about reality. Reality matters.”

It’s an elegant and thought-provoking explanation, though perhaps not as clear cut as some would like.

Then again, they never are. Sopranos creator David Chase has been asked to explain his big cut-to-black ending repeatedly for a decade now, and rightly insists that its beauty lies in its ambiguity and lack of closure.

Astronomers discovered an ‘Interstellar’ black hole


Fans of “Interstellar” take note: Astronomers might have just discovered a black hole similar to the one in Christopher Nolan’s film. And the discovery coincides with a mysterious flash, observed in 2015, thought to be the brightest supernova on record. Turns out, it probably wasn’t a supernova at all.

http://www.businessinsider.com/astronomer-discovered-interstellar-black-hole-2016-12?IR=T