The bomb-bay doors on the B-29 Superfortress Bockscar swung open over Nagasaki, Japan, a little before noon on Aug. 9, 1945, and at 11:58 a.m. one 10,800-pound bomb fell away.
Minutes later, a 5,300-pound sphere of high explosives imploded inside the bomb casing. The blast squeezed a softball-sized, 13.6-pound plutonium core to the size of a tennis ball, a super-critical mass that started a chain reaction.
The resulting nuclear explosion killed approximately 39,000 people and injured another 25,000, according to the online Atomic Archive. It was the second use of a nuclear weapon in war and the first to employ a plutonium implosion device, still a mainstay of nuclear weapons technology.
Scientists and engineers of the Manhattan Project, the top-secret World War II nuclear weapons program, fused raw science and practical engineering to create the implosion bomb at Project Y, the Los Alamos laboratory in New Mexico. The Hanford Engineer Works along the banks of the Columbia River in central Washington produced the plutonium. The bomb was tested at an isolated desert flat near Alamogordo, N.M., known as Trinity Site.
Trinity Site today is a once-a-year tourist attraction. But 75 years later, national laboratories at Los Alamos and Hanford, part of an extensive network that is the Manhattan Project legacy, are still in business.
The two-year crash effort to build the bomb that encompassed a handful of locations nationwide has grown into 17 national laboratories and dozens of affiliated sites overseen by the Department of Energy on a budget this year of more than $34 billion.
They continue to design new weapons and maintain the nations nuclear arsenal, but most of their work is geared toward basic science that yields amazing discoveries.
Theres a lot of impressive work going on at the lab outside of the nuclear weapons programs, whether its on energy or on computing or on any number of scientific areas. They still maintain a high caliber of research in the national interest, said Steven Aftergood, a freedom-of-information advocate for the Federation of American Scientists. I wouldnt want to overlook that.
On top of its work as a weapons designer, Los Alamos National Laboratory, where the critical work of the Manhattan Project took place, today engages in basic research in myriad topics, from black holes to cloud computing and climate change. The lab is also using genomics to diagnose cases of the coronavirus.
When the Cold War ended, lab experts also turned their expertise to helping the former Soviet Union dismantle its nuclear weapons.
Los Alamos laboratory may be the most famous Manhattan Project site, but it wasnt the only one and it wasnt even the first. That distinction belongs to Argonne National Laboratory, on the outskirts of Chicago, that grew out of physicist Enrico Fermis search at the University of Chicago for the first sustained nuclear reaction.
They were trying to figure out what the critical mass is, how much uranium 235 fissile core do you actually need to start a chain reaction, said Robert Rosner, former Argonne lab director.
Argonne is one of 10 national laboratories under the Department of Energys Office of Science. While some, like Argonne, Hanford (today the Pacific Northwest National Laboratory) and Oak Ridge, have roots in the Manhattan Project, they no longer work primarily on weapons development. The Pacific Northwest lab, for example, played a part in the detection of gravity waves in 2015.
Argonne, originally known by its code name, the Metallurgical Lab, became the home of the civilian nuclear power program, Rosner said. It created the worlds very first power reactor, the Experimental Breeder Reactor, at Argonne West, now the Idaho National Laboratory.
Three national laboratories are still primarily devoted to the work of nuclear weapons, including their non-nuclear components. Los Alamos, Lawrence Livermore National Laboratory in Livermore, Calif., and Sandia National Laboratory in Albuquerque, N.M., fall under the authority of the National Nuclear Security Administration.
The Manhattan Project employed as many as 130,000 people and cost nearly $2 billion, about $28.6 billion today. Work at Los Alamos alone cost taxpayers about $74 million, or $1.06 billion today, according to the Brookings Institution.
The Energy Department in fiscal year 2019 budgeted $2.9 billion for Los Alamos National Laboratory, of which 66%, or $1.9 billion, was intended for weapons programs.
At its height during World War II, Los Alamos employed about 5,000 people. Today there are over 12,000 people in the lab, just the lab, Rosner said during a phone interview July 15.
In addition to the raw and applied sciences the labs produce, they preserve a model for integrating scientists, engineers and other experts across a variety of fields that is not widely practiced in the commercial world, Rosner said.
Integrated teams are the secret behind national laboratories, he said. Universities traditionally cannot do this, and the reason is that were a silo. We have a physics department, a chemistry department theres a math department.
Academics find rewards in their own disciplines, said Rosner, who is now a professor of astronomy and astrophysics at the University of Chicago. Most physicists working at Los Alamos are astrophysicists, he said.
Astrophysicists are a good example of that. Astronomers, Rosner said. Theyre not thinking about money; theyre thinking about the universe, right? The Big Bang.
Few commercial enterprises can afford research and development the way the labs do it, he said. The old Bell Laboratories, before its break-up in 1982, produced significant advances, such as the silicon chip.
Ask yourself, does AT&T or Verizon or all of the other what used to be called Baby Bells, do they have big, basic research labs? he said.
The uglier legacy left by the Manhattan Project and the weapons labs is written in starker terms, including cleanup decrees, damage awards and the burden of nuclear weapons themselves.
As the Cold War ended, public attention came to bear on health risks to workers at Los Alamos and other sites; the accumulation of toxic waste, documented or not; poor management; and a culture of secrecy.
The worst example, the Hanford Nuclear Reservation, is what remains of the dirty work of bombmaking: 586 square miles that include nine decommissioned reactors that produced weapons-grade plutonium and a staggering amount of radioactive waste, according to the Northwest Power and Conservation Council.
About 53 million gallons of chemicals used to separate plutonium from uranium remains stored in 177 underground tanks, of which 70 are leaking and sending a radioactive plume toward the nearby Columbia River, according to the council. The site, one of the most dangerous and polluted in the U.S., includes 1,700 individual waste sites and about 500 contaminated buildings.
At Los Alamos, self-appointed watchdog Greg Mello, founder of the Los Alamos Study Group, has documented decades of worker health problems, industrial accidents and toxic waste. He also campaigns against a program underway to expand the lab to make plutonium pits for a new generation of nuclear warheads.
Theres been a pretty high cost across the warhead complex for pursuing the nuclear arms race, Mello said by phone July 28.
Drawing on reports from the Department of Labor and by investigative journalists, he estimates the federal government has paid out billions for 1,599 death claims at Los Alamos alone from its beginnings through June 2016.
This is a technology that has had horrible effects, Mello said. Direct health effects, as well as, I would say, effects on world politics and on the shape of American democracy have been even worse.
Although a government program enacted in 2000 has paid thousands of claims by workers across the nuclear weapons complex for work-related illnesses, the link to some of those illnesses with weapons work is disputed by some as tenuous, at best.
However, some problems with the labs are indisputable. An era of mismanagement at Los Alamos gave rise in 2000 to the National Nuclear Security Administration, the new overseer within the Energy Department. The state of New Mexico has issued Los Alamos lab several cleanup decrees and federal audits have found mishandled or missing materials.
A 2018 report by the Energy Department inspector general, for example, found discrepancies in the way the Los Alamos lab handled beryllium, a toxic metallic element used in nuclear reactors.
Los Alamos sometimes has problems accounting for nuclear materials, Aftergood said. He directs the Federation of American Scientists Project on Government Secrecy. Every now and then theres either an espionage case or an episode of misplaced classified records.
The worldwide nuclear stockpile peaked at more than 70,000 warheads around 1987, most of them held by the former Soviet Union, according to the federation. Today that arsenal is less than 20,000 warheads, including those held by China, Pakistan, India, North Korea, the U.K., France and Israel.
Part of the mission at weapons labs is stockpile stewardship, ensuring in an age of nuclear and thermonuclear test bans that aging weapons will work if deployed.
Tests above ground, underwater and in space were outlawed in 1963. The last U.S. nuclear test took place underground on Sept. 23, 1992. The Comprehensive Nuclear Test Ban Treaty has been awaiting Senate ratification since 1997.
The U.S. instead tests its weapons using supercomputer simulations fed by data collected from the real things.
I understand fully why we have atomic weapons, nuclear weapons. This is not a mystery to me, said Rosner, who is also a member of The Bulletin of Atomic Scientists, another group that sprang from the original Manhattan Project scientists, and chairs its Science and Security Board. And if youd asked me was it a good idea that we had the Manhattan Project my answer is: Hell, yes.
Discoveries in nuclear physics made the bomb inevitable, he said. Its one of those things; the genies out of the bottle and here we are.
Unlike anti-weapons advocates, Rosner said he believes the U.S. will always have atomic weapons if potential adversaries have them, too. However, hes against actual atomic testing, a move that would permit China, Russia and other nuclear powers to catch up with the U.S. hedge in testing data.
He also believes in adhering to and renewing existing nuclear nonproliferation treaties.
What has happened over the last five years? Were at the point of almost undoing everything that was done, something that took decades, you know, to put in place is basically now almost completely gone, he said.
Mello, an advocate for nuclear disarmament, agrees the U.S. seeking advantage by abrogating longstanding treaties is a terrible idea, is stupid.
He said nuclear weapons are a national burden, and not just in terms of the health effects, toxic waste and expense surrounding them, he said.
We never became the kind of country that we might have become, given since we devoted and still devote a majority of our discretionary income to military affairs, Mello said, and the acme of violence of this is nuclear weapons.
ditzler.joseph@stripes.comTwitter: @JosephDitzler
Read more from the original source:
From the Manhattan Project, a legacy of discovery and a national burden - Stars and Stripes
- Rotational spectra of isotopic species of methyl cyanide, CH_3CN, in their ground vibrational states up to terahertz frequencies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmological parameter extraction and biases from type Ia supernova magnitude evolution [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Continuous monitoring of pulse period variations in Hercules X-1 using Swift/BAT [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Constraining the ortho-to-para ratio of H{_2} with anomalous H{_2}CO absorption [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- A photometric and spectroscopic study of the new dwarf spheroidal galaxy in Hercules - Metallicity, velocities, and a clean list of RGB members [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Electron beam – plasma system with the return current and directivity of its X-ray emission [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The propagation of the shock wave from a strong explosion in a plane-parallel stratified medium: the Kompaneets approximation [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Analysis of hydrogen-rich magnetic white dwarfs detected in the Sloan Digital Sky Survey [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Letter: Centaurus A as TeV \gamma-ray and possible UHE cosmic-ray source [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Young pre-low-mass X-ray binaries in the propeller phase - Nature of the 6.7-h periodic X-ray source 1E 161348-5055 in RCW 103 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative rates and electron impact excitation rates for transitions in Cr VIII [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Solar granulation from photosphere to low chromosphere observed in Ba II 4554 Å line [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Does the HD 209458 planetary system pose a challenge to the stellar atmosphere models? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Effect of asymmetry of the radio source distribution on the apparent proper motion kinematic analysis [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Destriping CMB temperature and polarization maps [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Search for cold debris disks around M-dwarfs. II [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Precise data on Leonid fireballs from all-sky photographic records [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An X-ray view of 82 LINERs with Chandra and XMM-Newton data [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radio observations of ZwCl 2341.1+0000: a double radio relic cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Candidate free-floating super-Jupiters in the young \sigma Orionis open cluster [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The metallicity gradient as a tracer of history and structure: the Magellanic Clouds and M33 galaxies [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- XMMSL1 J060636.2-694933: an XMM-Newton slew discovery and Swift/Magellan follow up of a new classical nova in the LMC [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The inner rim structures of protoplanetary discs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The solar Ba{\sf II} 4554 Å line as a Doppler diagnostic: NLTE analysis in 3D hydrodynamical model [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnetic evolution of superactive regions - Complexity and potentially unstable magnetic discontinuities [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Low-mass protostars and dense cores in different evolutionary stages in IRAS 00213+6530 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- PMAS optical integral field spectroscopy of luminous infrared galaxies - I. The atlas [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- First AGILE catalog of high-confidence gamma-ray sources [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Radiative hydrodynamics simulations of red supergiant stars - I. interpretation of interferometric observations [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Extrasolar planets and brown dwarfs around A–F type stars - VII. \theta Cygni radial velocity variations: planets or stellar phenomenon? [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Cosmic rays and the magnetic field in the nearby starburst galaxy NGC 253 - II. The magnetic field structure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Physical structure and water line spectrum predictions of the intermediate mass protostar OMC2-FIR4 [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The bright galaxy population of five medium redshift clusters - II. Quantitative galaxy morphology [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Dust in brown dwarfs and extra-solar planets - II. Cloud formation for cosmologically evolving abundances [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The quiet Sun magnetic field observed with ZIMPOL on THEMIS - I. The probability density function [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Complexity in the sunspot cycle [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Properties and nature of Be stars - 26. Long-term and orbital changes of \zeta Tauri [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The massive Wolf-Rayet binary LSS 1964 (=WR 29) - II. The V light curve [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Supernova progenitor stars in the initial range of 23 to 33 solar masses and their relation with the SNR Cassiopeia A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of Star Clusters [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Table of the 10 Brightest stars within 10 Parsecs of the Sun [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Hertzsprung-Russell Diagram of the Nearest Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Magnitude and Color in Astronomy [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Stellar Types [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Spotting the Minimum [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Structure and Evolution of Brown Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- No Bang from the Big Bang Machine [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Sizes of the Stars and the Planets [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- An Implausible Light Thrust [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- the Masses of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Degeneracy Pressure [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Introduction to Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Radii of Degenerate Objects [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Inevitability of Black Holes [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Scientific Pig-Out [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Degenerate Dwarfs [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- The Neutrino Cooling of Neutron Stars [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Overview of Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Energetics of Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Nuclear Reactions in Thermonuclear Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Core-Collapse Supernovae [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Neutrinos and SN 1987A [Last Updated On: November 8th, 2009] [Originally Added On: November 8th, 2009]
- Revealing the sub-AU asymmetries of the inner dust rim in the disk around the Herbig Ae star R Coronae Austrinae [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Probing the dust properties of galaxies up to submillimetre wavelengths - I. The spectral energy distribution of dwarf galaxies using LABOCA [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On the physical origin of the second solar spectrum of the Sc II line at 4247 Å [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- On detecting the large separation in the autocorrelation of stellar oscillation times series [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Imaging the spotty surface of Betelgeuse in the H band [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Chandra observation of Cepheus A: the diffuse emission of HH 168 resolved [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- A planetary eclipse map of CoRoT-2a - Comprehensive lightcurve modeling combining rotational-modulation and transits [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The chemical composition of carbon stars. The R-type stars [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Flow instabilities of magnetic flux tubes - IV. Flux storage in the solar overshoot region [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Fragmentation of a dynamically condensing radiative layer [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Temporal variations of the CaXIX spectra in solar flares [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Deuterium chemistry in the Orion Bar PDR - “Warm” chemistry starring CH_{2}D^+ [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Metal abundances in the cool cores of galaxy clusters [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- The nature of the X-ray binary IGR J19294+1816 from INTEGRAL, RXTE, and Swift observations [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]
- Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902 [Last Updated On: December 13th, 2009] [Originally Added On: December 13th, 2009]