From a 17-mile-long particle accelerator to a football-field–sized space observatory, here are seven massive machines that have made an equally huge impact on how we build, how we observe our universe, and how we lift rockets into space. We’ve also included a bonus machine: a technological marvel-to-be that may be just as influential once it’s completed.



The Large Hadron Collider, a particle accelerator located at CERN outside of Geneva, Switzerland, is the largest machine in the world: It has a circumference of almost 17 miles and took around a decade to build. The tubes of the LHC are a vacuum; superconducting magnets guide and accelerate two high-energy particle beams, which are moving in opposite directions, to near-light-speed. When the beams collide, scientists use the data to find the answers to some of the most basic questions of physics and the laws that govern the universe we live in.

Since the LHC started up in 2008, scientists have made numerous groundbreaking discoveries, including finding the once-theoretical Higgs boson particle—a.k.a. the “God” particle—which helps give other particles mass. Scientists had been chasing the Higgs boson for five decades. The discovery illuminates the early development of the universe, including how particles gained mass after the Big Bang. Scientists are already working on the LHC’s successor, which will be three times its size and seven times more powerful.


Built in 1965, NASA’s crawler-transporters are two of the largest vehicles ever constructed: They weigh 2400 tons each and burn 150 gallons of diesel per mile. In contrast, the average semi truck gets roughly 6.5 miles per gallon. The vehicles’ first job was to move Saturn V rockets—which took us to the moon and measured 35 stories tall when fully constructed—from the massive Vehicle Assembly Building (the largest single-room building in the world) to the launch pad at Cape Canaveral. The 4.2-mile trip was a slow one; the transporters traveled at a rate of 1 mph to ensure the massive rockets didn’t topple over. Without a vehicle to move rockets from the spot they were stacked to the launch pad, we never could have gotten off the ground, much less to the moon.

After our moon missions, the crawler-transporters were adapted to service the Space Shuttle program, and moved the shuttles from 1981 to 2003. Since the retirement of the orbiters, these long-serving machines are once again being repurposed to transport NASA’s new Space Launch System (SLS), which, at 38 stories tall, will be the biggest rocket ever constructed when it’s ready, hopefully in a few years (the timeline is in flux due to budgetary issues).



Three football fields could fit inside the National Ignition Facility, which holds the largest, most energetic, and most precise laser in the world (it also has the distinction of being the world’s largest optical instrument). NIF—which took about a decade to build and opened in 2009—is located at the Lawrence Livermore National Laboratory in Livermore, California. Its lasers are used to create conditions not unlike those within the cores of stars and giant planets, which helps scientists to gain understanding about these areas of the universe. The NIF is also being used to pursue the goal of nuclear fusion. If we can crack the code for this reaction that powers stars, we’ll achieve unlimited clean energy for our planet.

“Laser” is an acronym for light amplification by stimulated emission of radiation. A laser is created when the electrons in atoms in special glasses, crystals, or gases absorb energy from an electrical current or another laser and become “excited.” The excited electrons move from a lower-energy orbit to a higher-energy orbit around the atom’s nucleus. When they return to their normal or “ground” state, the electrons emit photons (particles of light).

These photons are all at the same wavelength and are “coherent,” meaning the crests and troughs of the light waves are all in lockstep. In contrast, ordinary visible light comprises multiple wavelengths and is not coherent.

Laser light is different from normal light in other ways as well. First, its light contains only one wavelength (one specific color). The particular wavelength of light is determined by the amount of energy released when the excited electron drops to a lower orbit. Second, laser light is directional. Whereas a laser generates a very tight beam, a flashlight produces light that is diffuse. Because laser light is coherent, it stays focused for vast distances, even to the moon and back.

The National Ignition Facility has now been in operation for 10 years, but how did such an extraordinary facility come to be built? The journey to NIF was an epic one, resulting in a facility that has changed the face of science forever.

Stay Tuned

In NIF, as in most large lasers, intense flashes of white light from giant flashlamps “pump” electrons in large slabs of laser glass to a higher-energy state that lasts only about one-millionth of a second. A small pulse of laser light “tuned” to the excited electrons’ energy is directed through the glass slabs. This laser pulse stimulates the electrons to drop to their lower, or ground, energy states and emit a laser photon of exactly the same wavelength.

An optical switch traps the low-energy laser pulse in the main amplifier for four passes through the laser glass slabs. Mirrors at both ends of the glass amplifier cause the photons to travel back and forth through the glass, stimulating more electrons to drop to their lower energy states and emit photons. This process produces huge numbers of photons of the same wavelength and direction—an extremely bright and straight beam of light. In this way the initial low-energy pulse is amplified by more than a quadrillion times to create 192 highly energetic, tightly focused laser beams that converge in the center of the Target Chamber.

Lasers Are Everywhere

Lasers can be tiny constituents of microchips or as immense as NIF, which is ten stories high and as wide as three football fields. Lasers are found in a dazzling range of products and technologies, including CD and DVD players, metal-cutting machines, measuring systems, and eye and cosmetic surgery. Early lasers could produce peak powers of some 10,000 watts. Modern lasers can produce pulses that are billions of times more powerful. Scientists have demonstrated NIF’s ability to generate more than 500 trillion watts of power.

Some lasers, such as ruby lasers, emit short pulses of light. Others, like helium–neon gas lasers or liquid dye lasers, emit light that is continuous. NIF, like the ruby laser, emits pulses of light lasting only billionths of a second.

Laser light does not need to be visible. NIF beams start out as invisible infrared light and then pass through special optics that convert them to visible green light and then to invisible, high-energy ultraviolet light for optimum interaction with the target.


When Seattle decided it needed a giant tunnel to replace an aging highway through the middle of the city, the city contracted with Hitachi Zosen Corporation to build the biggest tunnel boring machine in the world to do the job. The scope of Bertha’s work had no precedent in modern-day digging, given the dense, abrasive glacial soil and bedrock it had to chew through.

In 2013, Bertha—named after Bertha Knight Landes, Seattle’s first female mayor—was tasked with building a tunnel that would be big enough to carry four lanes of traffic (a two-lane, double-decker road). Bertha needed to carve through 1.7 miles of rock, and just 1000 feet in, the 57-foot, 6559-ton machine ran into a steel pipe casing that damaged it. Many predicted that Bertha was doomed, but after a massive, on-the-spot repair operation by Hitachi Zosen that took a year-and-a-half, the borer was up and running again.

In April 2017, Bertha completed its work, and engineers started the process of dismantling it; its parts will be used in future tunnel boring machines. Bertha set an example for what is possible in future urban tunnel work—but it’s unlikely that tunnel boring machines will get much bigger than Bertha because of the sheer weight of the machine and the amount of soil it can move at once. Bertha’s tunnel is scheduled to open in 2019.

DARPA Looks for Tunneling Breakthroughs

DARPA is funding breakthroughs in tunneling. The Underminer project aims to demonstrate the feasibility of rapidly constructing tactical tunnel networks to provide secure logistics infrastructure to pre-position supplies or resupply troops as they move through an area.

General Electric Research Center and Colorado School of Mines will focus on development of an integrated solution for Underminer technology and operational needs.

Colorado School of Mines has a web page dedicated to their new tunneling project.

Mike Mooney and his Colorado School of Mines team are using AI to characterize ground conditions, learn how to tunnel really fast, and minimize tunneling-induced building deformation.

Tunnel boring machines (TBMs) excavate through highly uncertain and poorly characterized heterogeneous soil and rock. TBM interaction with the ground is very complex, with dozens of integrated processes governing the efficiency and effectiveness of tunnel construction. Such complex processes in highly unknown environments are ideal for AI intelligent learning, a process whereby the TBM learns-while-doing, continuously improving its performance to best achieve the tunneling objectives. In this research we are using artificial intelligence techniques and constrained optimization to learn and implement the best tunneling strategy for the encountered ground.

There will be the development of rapid tunneling.

Boring Company Tunnel Machines
Elon Musks Boring Company is not directly involved in the DARPA project. They are leaders in developing faster tunneling.

The first three boring machines used by The Boring Company are:

Godot, a conventional tunnel boring machine made by Canadian company Lovat, which is used for research purposes.
Line-storm, a highly modified conventional boring machine. In February 2019, Elon Musk estimated in a tweet that Line-storm would be active “in a month or so”.
Prufrock is a BoringCompany designed machine. It is slated to support a 15x improvement in tunneling speed over the existing state of the art in 2017. It has the same diameter as a Dragon spacecraft (3.7 metres (12 ft)). In February 2020, Prufrock was shown assembled in a Twitter post.

Colorado School of Mines is also looking at Large-Diameter Tunnel Lining Design, Dynamic Risk Mapping and Midtown Immersed Tube Tunnel Analysis.

Sandia National Laboratories will conduct technology exploration and integration to address current process and system limitations.

The performers will focus on tunneling approaches, downhole sensing, and operations concepts. Underminer seeks to merge breakthroughs in horizontal drilling, trenchless boring technologies, and robotics to create a set of systems allowing consistent underground access.

Fast creation of tactical tunnels could benefit contingency operations such as rapid ammunition resupply, rescue missions and other functions.

Tunneling Industry

Recent years have seen significant advances in tunneling equipment and materials. TBM (Tunnel Boring Machines) and microtunneling equipment with enhanced data acquisitions, cutter/tool wear monitoring and replacement capabilities. All forms of tunnel lining — precast segmental, cast-in-place, and shotcrete — have benefited from advances in steel and synthetic fiber.

SOURCES- DARPA, Colorado School of Mines, Tunneling Online, Boring Company
Written By Brian Wang,

Tunnel Boring Machine   a shitload of information on this site




The international space station is a highly efficient machine, equipped with instrumentation and life support equipment, that has kept humans alive in the inhospitable environment of low-Earth orbit since November 2, 2000. It’s the biggest satellite orbiting the Earth made by humans. The major components were sent into space over a two-year period, but construction has slowly continued over the last decade, with astronauts adding the Columbus science laboratory and Japanese science module. The first module, Zarya, was just 41.2 feet by 13.5 feet; now, the ISS is 356 feet by 240 feet, which is slightly larger than a football field. The station currently has about 32,333 cubic feet of pressurized volume the crew can move about in. That’s about the same area as a Boeing 747 (though much of the ISS’s space is taken up by equipment). The U.S.’s solar panels are as large as eight basketball courts.

From the space station, scientists have made such important discoveries as what extended zero-G does to the human body, where cosmic rays come from, and how protein crystals can be used to treat cancer. Though NASA expects the most modern modules of the ISS to be usable well into the 2030s, by 2025 the agency may begin “transitioning” much of its ISS operations—and costs—to the private sector [PDF] with an eye on expanding the commercial potential of space.


That looks exactly like the spiral in the sky over Norway… 

What Is This Mysterious Spiral Anomaly in the Norwegian Sky?December 9, 2009 Norway awaiting the arrival of Barack Obama see a strange phenomenon arriving out of the eastern sky.   You know the “spiral” is another symbol that is very significant to the  Satanists/Kabbalists/Illuminati/Magicians.

Jun 3, 2015

The Laser Inferometer Gravitational-Wave Observatory (LIGO) is actually made up of four different facilities—two laboratories and two detectors located 2000 miles apart, in Hanford, Washington, and Livingston, Louisiana. The detectors, which took about five years to build and were inaugurated in 1999, are identical L-shaped vacuum chambers that are about 2.5 miles long and operate in unison. The mission of these machines is to detect ripples in the fabric of spacetime known as gravitational waves. Predicted in 1915 by Einstein’s theory of general relativity, gravitational waves were entirely theoretical until September 2015, when LIGO detected them for the first time. Not only did this provide further confirmation of general relativity, it opened up entirely new areas of research such as gravitational wave astronomy. The reason the two detectors are so far from each other is to reduce the possibility of false positives; both facilities must detect a potential gravitational wave before it is investigated.


Image credit: The SXS (Simulating eXtreme Spacetimes) Project


Gravitational Waves Detected 100 Years After Einstein’s Prediction

News Release • February 11, 2016

Visit The Detection Portal

See also: LIGO Hanford Press Release

LIGO Opens New Window on the Universe with Observation of Gravitational Waves from Colliding Black Holes

WASHINGTON, DC/Cascina, Italy

For the first time, scientists have observed ripples in the fabric of spacetime called gravitational waves, arriving at the earth from a cataclysmic event in the distant universe. This confirms a major prediction of Albert Einstein’s 1915 general theory of relativity and opens an unprecedented new window onto the cosmos.

Gravitational waves carry information about their dramatic origins and about the nature of gravity that cannot otherwise be obtained. Physicists have concluded that the detected gravitational waves were produced during the final fraction of a second of the merger of two black holes to produce a single, more massive spinning black hole. This collision of two black holes had been predicted but never observed.


The gravitational waves were detected on September 14, 2015 at 5:51 a.m. Eastern Daylight Time (09:51 UTC) by both of the twin Laser Interferometer Gravitational-wave Observatory (LIGO) detectors, located in Livingston, Louisiana, and Hanford, Washington, USA. The LIGO Observatories are funded by the National Science Foundation (NSF), and were conceived, built, and are operated by Caltech and MIT. The discovery, accepted for publication in the journal Physical Review Letters, was made by the LIGO Scientific Collaboration (which includes the GEO Collaboration and the Australian Consortium for Interferometric Gravitational Astronomy) and the Virgo Collaboration using data from the two LIGO detectors.

Based on the observed signals, LIGO scientists estimate that the black holes for this event were about 29 and 36 times the mass of the sun, and the event took place 1.3 billion years ago. About 3 times the mass of the sun was converted into gravitational waves in a fraction of a second—with a peak power output about 50 times that of the whole visible universe. By looking at the time of arrival of the signals—the detector in Livingston recorded the event 7 milliseconds before the detector in Hanford—scientists can say that the source was located in the Southern Hemisphere.

According to general relativity, a pair of black holes orbiting around each other lose energy through the emission of gravitational waves, causing them to gradually approach each other over billions of years, and then much more quickly in the final minutes. During the final fraction of a second, the two black holes collide into each other at nearly one-half the speed of light and form a single more massive black hole, converting a portion of the combined black holes’ mass to energy, according to Einstein’s formula E=mc2. This energy is emitted as a final strong burst of gravitational waves. It is these gravitational waves that LIGO has observed.

The existence of gravitational waves was first demonstrated in the 1970s and 80s by Joseph Taylor, Jr., and colleagues. Taylor and Russell Hulse discovered in 1974 a binary system composed of a pulsar in orbit around a neutron star. Taylor and Joel M. Weisberg in 1982 found that the orbit of the pulsar was slowly shrinking over time because of the release of energy in the form of gravitational waves. For discovering the pulsar and showing that it would make possible this particular gravitational wave measurement, Hulse and Taylor were awarded the Nobel Prize in Physics in 1993.

The new LIGO discovery is the first observation of gravitational waves themselves, made by measuring the tiny disturbances the waves make to space and time as they pass through the earth.

“Our observation of gravitational waves accomplishes an ambitious goal set out over 5 decades ago to directly detect this elusive phenomenon and better understand the universe, and, fittingly, fulfills Einstein’s legacy on the 100th anniversary of his general theory of relativity,” says Caltech’s David H. Reitze, executive director of the LIGO Laboratory.

The discovery was made possible by the enhanced capabilities of Advanced LIGO, a major upgrade that increases the sensitivity of the instruments compared to the first generation LIGO detectors, enabling a large increase in the volume of the universe probed—and the discovery of gravitational waves during its first observation run. The US National Science Foundation leads in financial support for Advanced LIGO. Funding organizations in Germany (Max Planck Society), the U.K. (Science and Technology Facilities Council, STFC) and Australia (Australian Research Council) also have made significant commitments to the project. Several of the key technologies that made Advanced LIGO so much more sensitive have been developed and tested by the German UK GEO collaboration. Significant computer resources have been contributed by the AEI Hannover Atlas Cluster, the LIGO Laboratory, Syracuse University, and the University of Wisconsin- Milwaukee. Several universities designed, built, and tested key components for Advanced LIGO: The Australian National University, the University of Adelaide, the University of Florida, Stanford University, Columbia University of the City of New York, and Louisiana State University.

“In 1992, when LIGO’s initial funding was approved, it represented the biggest investment the NSF had ever made,” says France Córdova, NSF director. “It was a big risk. But the National Science Foundation is the agency that takes these kinds of risks. We support fundamental science and engineering at a point in the road to discovery where that path is anything but clear. We fund trailblazers. It’s why the U.S. continues to be a global leader in advancing knowledge.”

LIGO research is carried out by the LIGO Scientific Collaboration (LSC), a group of more than 1000 scientists from universities around the United States and in 14 other countries. More than 90 universities and research institutes in the LSC develop detector technology and analyze data; approximately 250 students are strong contributing members of the collaboration. The LSC detector network includes the LIGO interferometers and the GEO600 detector. The GEO team includes scientists at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute, AEI), Leibniz Universität Hannover, along with partners at the University of Glasgow, Cardiff University, the University of Birmingham, other universities in the United Kingdom, and the University of the Balearic Islands in Spain.

“This detection is the beginning of a new era: The field of gravitational wave astronomy is now a reality,” says Gabriela González, LSC spokesperson and professor of physics and astronomy at Louisiana State University.

LIGO was originally proposed as a means of detecting these gravitational waves in the 1980s by Rainer Weiss, professor of physics, emeritus, from MIT; Kip Thorne, Caltech’s Richard P. Feynman Professor of Theoretical Physics, emeritus; and Ronald Drever, professor of physics, emeritus, also from Caltech.

“The description of this observation is beautifully described in the Einstein theory of general relativity formulated 100 years ago and comprises the first test of the theory in strong gravitation. It would have been wonderful to watch Einstein’s face had we been able to tell him,” says Weiss.

“With this discovery, we humans are embarking on a marvelous new quest: the quest to explore the warped side of the universe—objects and phenomena that are made from warped spacetime. Colliding black holes and gravitational waves are our first beautiful examples,” says Thorne.

Virgo research is carried out by the Virgo Collaboration, consisting of more than 250 physicists and engineers belonging to 19 different European research groups: 6 from Centre National de la Recherche Scientifique (CNRS) in France; 8 from the Istituto Nazionale di Fisica Nucleare (INFN) in Italy; 2 in The Netherlands with Nikhef; the Wigner RCP in Hungary; the POLGRAW group in Poland; and the European Gravitational Observatory (EGO), the laboratory hosting the Virgo detector near Pisa in Italy.  WOW, WHERE DOES ALL THIS MONEY COME FROM TO PAY ALL THESE GUYS AND MAINTAIN ALL THIS EQUIPMENT?

Fulvio Ricci, Virgo Spokesperson, notes that, “This is a significant milestone for physics, but more importantly merely the start of many new and exciting astrophysical discoveries to come with LIGO and Virgo.”

Bruce Allen, managing director of the Max Planck Institute for Gravitational Physics (Albert Einstein Institute), adds, “Einstein thought gravitational waves were too weak to detect, and didn’t believe in black holes. But I don’t think he’d have minded being wrong!”

“The Advanced LIGO detectors are a tour de force of science and technology, made possible by a truly exceptional international team of technicians, engineers, and scientists,” says David Shoemaker of MIT, the project leader for Advanced LIGO. “We are very proud that we finished this NSF-funded project on time and on budget.”

At each observatory, the two-and-a-half-mile (4-km) long L-shaped LIGO interferometer uses laser light split into two beams that travel back and forth down the arms (four-foot diameter tubes kept under a near-perfect vacuum). The beams are used to monitor the distance between mirrors precisely positioned at the ends of the arms. According to Einstein’s theory, the distance between the mirrors will change by an infinitesimal amount when a gravitational wave passes by the detector. A change in the lengths of the arms smaller than one-ten-thousandth the diameter of a proton (10-19 meter) can be detected.

“To make this fantastic milestone possible took a global collaboration of scientists—laser and suspension technology developed for our GEO600 detector was used to help make Advanced LIGO the most sophisticated gravitational wave detector ever created,” says Sheila Rowan, professor of physics and astronomy at the University of Glasgow.

Independent and widely separated observatories are necessary to determine the direction of the event causing the gravitational waves, and also to verify that the signals come from space and are not from some other local phenomenon.

Toward this end, the LIGO Laboratory is working closely with scientists in India at the Inter-University Centre for Astronomy and Astrophysics, the Raja Ramanna Centre for Advanced Technology, and the Institute for Plasma to establish a third Advanced LIGO detector on the Indian subcontinent. Awaiting approval by the government of India, it could be operational early in the next decade. The additional detector will greatly improve the ability of the global detector network to localize gravitational-wave sources.

“Hopefully this first observation will accelerate the construction of a global network of detectors to enable accurate source location in the era of multi-messenger astronomy,” says David McClelland, professor of physics and director of the Centre for Gravitational Physics at the Australian National University.   ARE THEY KIDDING???

Additional video and image assets can be found here:



The Russians originally had a rival to the U.S. Space Shuttle program: a reusable winged spacecraft of their own called the Buran—and in the 1980s, they developed the AN-225 Mriya in order to transport it. With a wingspan the size of the Statue of Liberty, a 640-ton weight, six engines, and the ability to lift into the air nearly a half-million pounds, it’s the longest and heaviest plane ever built. Mriya first flew in 1988, and since the Buran was mothballed in 1990 after just one flight (due to the breakup of the Soviet Union rather than the plane’s capabilities), the AN-225 has only been used sparingly.

The monster plane has inspired new ideas. In 2017, Airspace Industry Corporation of China signed an agreement with Antonov, the AN-225’s manufacturer, to built a fleet of aircraft based on the AN-225’s design that would carry commercial satellites on their backs and launch them into space. Currently, virtually all satellites are launched from rockets. Meanwhile, Stratolaunch, a company overseen by Microsoft co-founder Paul Allen, is building a plane that will be wider (but not longer) than Mriya. The giant plane will carry a launch vehicle headed for low-Earth orbit.


This forward-thinking project, funded by Amazon and Blue Origin founder Jeff Bezos, focuses on reminding people about their long-term impact on the world. Instead of a traditional clock measuring hours, minutes, and seconds, the Clock of the Long Now measures times in years and centuries. The clock, which will be built inside a mountain on a plot of land in western Texas owned by Bezos, will tick once per year, with a century hand that advances just once every 100 years. The cuckoo on the clock will emerge just once per millennium. Construction began on the clock in early 2018. When this massive clock is completed—timeline unknown—it will be 500 feet high. What will be the impact of this one? Only the people of the 120th century will be able to answer that question.