Toggle light / dark theme

This essay was posted previously last year and removed and has appeared in abridged form in the European Space Safety online Magazine and can also be found on Yahoo voices.

Several dates are cited as marking the beginning of the space age. Sputnik, October 4th, 1957, Yuri’s day April 12th, 1961, and the first successful V-2 launch by the Nazis on October 3rd, 1942, to name a few. Some prefer December 21st, 1968, when human beings first escaped the Earth’s gravitational field on Apollo 8. When studying the events that allowed man to leave Earth, future historians may agree on a date not generally associated with space flight. July 16th, 1945 was Trinity, the first nuclear weapon test. Stanislaw Ulam, a 36-year-old Polish mathematician who helped build “the gadget”, visited ground zero after the test. Ulam later conceived the idea of propelling a spaceship with atomic bombs. Near the end of his life the eccentric genius stated the idea was his greatest work.

When considering nuclear propulsion, it must be understood that space is not an ocean, though often characterized as one. The distances and conditions are not comparable. While chemical energy has allowed humankind to travel across and above the surface of Earth, the energy required to travel in space is of a different order. Water, in the form of steam, was the agent of change that brought about the industrial revolution. Fossil fuel, burned and transformed by steam into mechanical work, would radically change the world in the span of a century. What is difficult for moderns to understand is not only how limited human capabilities were before steam, but how limited they are in the present in terms of space travel. The psychological limits of human beings limit space journeys to a few years. Chemical propulsion is not capable of taking human beings to the outer solar system and back within those crew limits. The solution is a reaction one million times more powerful. Nuclear energy is to the space age as steam was to the industrial age.

Space is not an ocean and this was the correct lesson drawn by Stanislaw Ulam after that suddenly bright morning in 1945. While metal can barely contain and harness chemical energy, Ulam thought outside that box and accepted nuclear energy could never be contained efficiently by any material. However, nuclear energy could be harnessed to push a spaceship in separate events to the fantastic velocities required for interplanetary travel without any containment problems at all- by using bombs. An uncontained burst of nuclear generated plasma could be withstood by a surface momentarily before the physical matter had time to melt.

Sixty years after Ulam’s stroke of genius, atomic bomb propulsion still has no competition as the only available propulsion system for practical interplanetary travel. This fact is almost completely unknown to the public. The term “ISP”, expressed in seconds, is used in measuring the efficiency of a rocket engine and chemical rockets have low ISP numbers but high thrust. The most efficient rocket engines, such as the space shuttle main engines, with a listed ISP of 453 seconds are also among the most powerful. Atomic bomb propulsion, thanks to the billions of dollars poured into star wars weapons research, would have an ISP exceeding 100,000 seconds. While other propulsion systems that use electricity have similar or higher numbers, the amount of thrust is trivial and requires months or years of continuous operation to develop any significant velocity. Considering space travel as not only a speed and distance problem, but also a time and distance problem, low thrust lengthens any missions to the outer solar system beyond crew limits. The thrust imparted by atomic bombs can in a short period easily accelerate thousands of tons to the comparatively extreme speeds necessary and then coast. Unlike an electric propulsion failure, a few dud bombs need not doom a mission or crew.

Though an incredible use of awesome power, the obstacles to employing bomb propulsion are not technical as some of the best engineers and physicists on the planet evaluated and validated the concept. A cadre of celebrity scientists also endorsed atomic bomb propulsion, including Werner Von Braun, who was present as a Nazi SS officer at the first successful V-2 launch, and as an American citizen at the launch of Apollo 8. Arthur C. Clarke and Carl Sagan were also supporters. The first serious work on bomb propulsion was done by physicist Freeman Dyson and weapon designer Ted Taylor on the top secret project Orion. Dyson’s son, in his book Project Orion, refers to the classified star wars project Casaba Howitzer. This device focused most of the energy of a nuclear explosion in one direction. Ted Taylor’s specialty was small warheads and he designed the Orion bombs, aka “pulse units.” The “unclassified” state of the art in nuclear weapons can direct 80 percent of bomb energy into a slab of propellant, converting this mass into a jet of superheated plasma. A pusher plate would absorb the blast without melting for the fraction of a second it lasts and accelerate the spaceship in steps with each bomb. Perhaps the closest experience to riding in an atomic bomb propelled spaceship would be repeated aircraft carrier catapult launches. Instead of the ocean- space, instead of supersonic fighters- a thousand ton spaceship.

Project Orion was canceled due to nuclear weapon treaties requiring international consent for using any such devices in space. A parallel to the failure of atomic bomb propulsion may be found in an examination of the industrial age. In The Most Powerful Idea in the World: A Story of Steam, Industry, and Invention, author William Rosen theorizes English patent law was the key enabler of the industrial age by allowing inventors to retain and profit from their intellectual property. The atomic bomb originated with a letter to President Roosevelt in 1939 from pacifist Albert Einstein- who was afraid the Nazi’s might build one first. With the human race living at the bottom of a deep, damp, and easily contaminated gravity well, atom bombs have never been applied successfully to a peaceful purpose. Stan Ulam, who lost most of his family in the holocaust, held the patent on atomic bomb propulsion. In the space age, nuclear weapon treaties and anti-nuclear activism have had the opposite effect of patent law and prevented atomic bomb propulsion from opening up the solar system to human exploration and colonization. Ironically, the nuclear industry is not safe on Earth- but deep space seems designed for it. There are no contamination or waste hazards, no long-term storage problems.

The problems with space travel are more than just the political barriers to detonating nuclear devices. The space industry is ipso facto a nuclear industry. Not only is nuclear energy the only practical source of propulsion in deep space, nuclear radiation generated by supernova and other celestial sources permeate space outside the protection of the earth’s atmosphere. All astronauts are radiation workers. Most, but sadly not all, space radiation is relatively easy to shield against. Many will argue using atomic bombs for propulsion is unnecessary. The presence of a small percentage of highly damaging and deeply penetrating particles- the heavy nuclei component of galactic cosmic rays makes a super powerful propulsion system mandatory. The tremendous power of atomic bomb propulsion is certainly able to propel the heavily shielded capsules required to protect space travelers. The great mass of shielding makes chemical engines, inefficient nuclear thermal rockets, the low thrust forms of electrical propulsion, and solar sails essentially worthless for human deep space flight. Which is why atomic bomb propulsion is left as the only “off the shelf” viable means of propulsion. For the foreseeable future, high thrust and high ISP to propel heavy shielding to the required velocities is only possible using bombs. The most useful and available form of radiation shielding is water. While space may not be an ocean, it appears human beings will have to take some of the ocean with them to survive.

The water comes before the bombs in human space flight because of the humans. The radiation hazards of long duration human space flight beyond earth orbit are only recently being addressed after decades of space station experience. The reason for this neglect is low earth orbit space stations are shielded from much of the radiation found outside the Earth’s Van Allen belts and magnetic field. An appreciation of the heavy nuclei component of galactic cosmic radiation, as well as solar events, will put multi-year human missions beyond earth orbit on hold indefinitely until a practical shield is available. While vested interests continue to promote inferior or non-existent technology, dismissing the radiation hazards and making promises they cannot keep, radiation scientists studying deep space conditions are skeptical- to say the least.

In the March 2006 issue of Scientific American magazine, Dr. Eugene Parker explained in simple terms survivable deep space travel. In “Shielding Space Travelers”, Parker states, “cosmic rays pose irreducible risks.” The premise of this statement is revealed when the only guaranteed solution to reducing the risk- a shield massing hundreds of tons- is deemed impractical. Active magnetic shields and other schemes are likewise of no use because while they may stop most radiation, the only effective barrier to heavy nuclei is mass and distance. The impracticality of a massive shield is due to first the expense of lifting hundreds of tons of shielding into space from Earth, and secondly propelling this mass around the solar system. Propelling this mass is not a problem if using atomic bombs, however, another problem arises. Even if the bombs could be politically managed, there is still the need to escape Earth’s gravitational field with all that shielding. Bomb propulsion is ideal for deep space but cannot be used in Earth orbit due to the Earth’s magnetic field trapping radioactive fallout that eventually enters the atmosphere. Not only lifting the shielding into orbit but chemically boosting it to a higher escape velocity away from the Earth is thus doubly problematic. Earth is a deep gravity well to climb out of.

The situation changed in March 2010 when NASA reported Mini-SAR radar aboard the Chandrayaan-1 lunar space probe had detected what appeared to be ice deposits at the lunar North Pole. An estimated 600 million tons of ice in sheets a couple meters thick. Moon water would allow a spaceship in lunar orbit to fill an outer hull with the 500+ tons of water required to effectively shield a capsule from heavy nuclei. This would enable an empty spaceship to “travel light” to the Moon and then boost out of lunar orbit using atomic bomb propulsion with a full radiation shield. Parker’s guaranteed but impractical solution had suddenly become practical. Fourteen feet of water equals the protection of the Earth’s air column at an altitude of 18,000 feet above sea level. This would protect astronauts not only from all forms of cosmic radiation but the most intense solar storms and the radiation belts found near the moons of Jupiter. With water and bombs, epic missions of exploration to the asteroid belt and outer planets are entirely possible. The main obstacles are again political, not technical. Bombs work, water works, and the Moon is in range of chemically propelled spacecraft launched from Earth.

There are other challenges to long duration beyond earth orbit human space flight but the solutions have been known for many decades. Zero gravity debilitation causes astronauts to weaken and permanently lose bone and bone marrow mass. The most practical solution, theorized since the early 1930′s, was investigated in 1966 during the Gemini 11 mission. A 100-foot tether experiment with the capsule attached to an Agena booster was successful in generating a small amount of artificial gravity by spinning the two vehicles. Equal masses on the ends of a tether can efficiently generate centrifugal force equal to one gravity. The concept is to “split the ship” when not maneuvering under power so the 500+ tons of shielded capsule is on one end and the rest of the craft of equal mass is reeled out on the other end of a thousand foot or more tether. Looking out through 14 feet of water, the crew of such a spaceship would view a slowly rotating star field. Long duration missions may last close to half a decade and the only option for providing air and water is to use a miniature version of Earth’s ecosystem. Equipment to enable a closed cycle life support system providing years of air and water is now available in the form of plasma reformers and facilitated by tons of water in which to grow algae or genetically modified organisms. With Earth radiation, Earth gravity, and air and water endlessly purified on board, crews can push their psychological limits as many years and as far out into the solar system as the speed of their atomic spaceships allow.

At the time of this writing, in early 2011, the outlook for human space flight is not encouraging. There are zero prospects for funding a long duration beyond earth orbit mission. Using atomic bombs to push minimum spaceship masses of over one thousand tons around the solar system for years at a time would cost as much as several major U.S. department of defense projects combined. Space flight is inherently expensive; there is no cheap. However, there is a completely valid military mission for atomic bomb propelled spaceships. Planetary protection became an issue in 1980 after the Chicxulub impact crater in Mexico was assigned blame for the mass extinction of the dinosaurs. Though overshadowed by the cold war, the impact threat remains. Comet and asteroid impacts are also the stuff of Hollywood movies and this is unfortunate in that a grave threat to the survival of life on earth is viewed as fictional entertainment. The impact threat is not science fiction; it is quite real, as the frequent near misses and geologic evidence of repeated extinction events show. Optimized directional bombs used in bomb propulsion could also be employed to deflect comets and asteroids long before they approach Earth.

While the consequences of ignoring the threat of an inevitable tsunami, earthquake, or hurricane are bad, the consequences of ignoring the inevitable comet or asteroid impact are apocalyptic. It is not only random impacts that could strike at any time the human race need guard against. In April of 2010 renowned physicist Stephen Hawking warned of alien civilizations posing a possible threat to humanity. Several large comets purposely crashed into a planet to wipe out the majority of indigenous life and prepare for the introduction of invasive alien species may be a common occurrence in the galaxy. Before readers scoff, they might consider towers brought down by jetliners, the discovery of millions of planets, and other recent unlikely events. It is within our power to defend Earth from the very real threat of an impact, and at this time self-defense is the only valid reason to go into space instead of spending the resources on Earth improving the human condition. Protecting our species from extinction is the penultimate moral high ground above all other calls on public funds. The vast treasure expended by nations threatening each other is not protecting the human race at all. Earth is defenseless. President Ronald Reagan in his 1983 Star Wars speech said, “I call upon the scientific community who gave us nuclear weapons to turn their great talents to the cause of mankind and world peace.” President Barack Obama has expressed a desire to reduce the world nuclear arsenal and converting these weapons to propulsion devices would do so. A powerful force of nuclear powered, propelled, and armed spaceships cannot guarantee Earth will not suffer a catastrophe. The best insurance for our species is to establish, in concert with a spaceship fleet, several independent self-supporting off world colonies in the outer solar system. The first such colony would mark the beginning of a new age.

Time line

1939 (August) Einstein sends letter recommending atomic bomb.

1939 (September) Germany invades Poland, World War 2 begins.

1942 First successful V-2 rocket launch by the Nazis.

1945 Trinity, the first atomic bomb is detonated.

1957 Sputnik achieves orbit using a rocket designed to carry an atomic bomb.

1961 Yuri Gagarin orbits Earth.

1966 Gemini 11 mission demonstrates artificial gravity.

1967 Outer Space Treaty restricts nuclear weapons in space.

1968 Apollo 8 crew escapes Earth’s gravitational field.

1980 Chicxulub impact crater revealed as dinosaur killer.

1983 Ronald Reagan gives Star Wars speech.

2006 Eugene Parker explains survivable deep space travel.

2010 (March) Millions of tons of ice are discovered on the Moon.

2010 (April) Stephen Hawking warns of alien civilization threat.

References

George Dyson, 2002, Project Orion: The True story of the Atomic Spaceship, Henry Holt and Company, LLC

Eugene Parker, March 2006, Shielding Space Travelers, Scientific American Magazine

William Rosen, 2010, The Most Powerful Idea in the World: A Story of Steam, Industry, and Invention, Random House

It’s the centennial year of the Titanic disaster, and that tragedy remains a touchstone.

The lifeboat angle is obvious. So is the ice hazard: then it was icebergs, now it’s comets.

But 100 years of expanding awareness has revealed the other threats we’re now aware of. We have to think about asteroids, nano- and genotech accidents, ill-considered high-energy experiments, economic and social collapse into oligarchy and debt peonage, and all the many others.

What a great subject for a Movie Night! Here are some great old movies about lifeboats and their discontents.

Lifeboat Triple Feature: https://lifeboat.com/blog/?p=3764

They’re full of situations about existential risks, risk assessment, prudential behavior, and getting along in lifeboats if we absolutely have to. The lesson is: make sure there are enough lifeboats and make darn sure you never need to use them.

Anyway, I finally got my review of the show done, and I hope it’s enjoyable and maybe teachable. I’d welcome additional movie candidates.

Creative Commons License
Party LIke It’s 1912… by Clark Matthews is licensed under a Creative Commons Attribution-NonCommercial-NoDerivs 3.0 Unported License.
Based on a work at https://lifeboat.com/blog/?p=3764.
Permissions beyond the scope of this license may be available at https://lifeboat.com.

Here are links to NASA live broadcast of Curiosity’s landing on Mars. Curiosity is the one ton car-sized rover that NASA is landing on Mars today.

This is another step in Man’s great adventure into interstellar space. Well Done, NASA.

NASA TV: http://www.nasa.gov/multimedia/nasatv/index.html

NASA Ustream: http://www.ustream.tv/nasajpl

NASA TV Schedule: http://www.nasa.gov/multimedia/nasatv/MM_NTV_Breaking.html

Today’s (August 5, Sunday 2012) Schedule (All Programs Eastern Time Zone):

6 a.m. – Replay of NASA Science News Conference – Mars Science Laboratory/Curiosity Rover Mission Status and Entry, Descent and Landing Overview (8÷4) – HQ (All Channels)

7 a.m. – Replay of NASA Science News Conference – MSL Mission Science Overview (8÷2) – HQ (All Channels)

8 a.m. – Replay of NASA Science News Conference – Mission Engineering Overview (8÷2) – HQ (All Channels)

9 a.m. – NASA Television Video File – HQ (All Channels)

10 a.m. – 12 p.m. — Replay of NASA Social for the Mars Science Laboratory/Curiosity Rover Landing – HQ (All Channels)

12 p.m. – NASA Television Video File – HQ(All Channels)

12:30–1:30 p.m. — NASA Science News Conference Mars Science Laboratory/Curiosity Rover Pre-Landing News Conference — Rover Communication overview — JPL (All Channels)

1:30 p.m. – Replay of NASA News Conference to Announce New Agreements for Next Phase of Commercial Crew Development – HQ (All Channels)

2 p.m. – Replay of ISS Update (8÷3) – HQ (All Channels)

3 p.m. — NASA Science News Conference Mars Science Laboratory/Curiosity Rover Pre-Landing News Conference — Rover Communication overview – JPL (All Channels)

4–6 p.m. – Replay of NASA Social for the Mars Science Laboratory/Curiosity Rover Landing – HQ (All Channels)

6–7 p.m. — NASA Science News Conference — NASA Science Mission Directorate — JPL (All Channels)

11 p.m. — Mars Science Laboratory/Curiosity Rover Landing Coverage of Entry Decent and Landing (Commentary #1 Begins 11:30 p.m.) — JPL (Public and Education Channels)

11 p.m. — Mars Science Laboratory/Curiosity Rover Landing Coverage of Entry Decent and Landing (Clean Feed with Mission Audio Only) — JPL (Media Channel)

—————————————————————————————————

Benjamin T Solomon is the author & principal investigator of the 12-year study into the theoretical & technological feasibility of gravitation modification, titled An Introduction to Gravity Modification, to achieve interstellar travel in our lifetimes. For more information visit iSETI LLC, Interstellar Space Exploration Technology Initiative

Tom Kerwick challenged my warnings by claiming that the observed longevity of white dwarfs, in spite of the constant bombardment by cosmic rays, provides a convincing safety argument regarding the currently running nuclear collisions experiment at CERN. This claim is important but, unfortunately, inconclusive as I shall try to demonstrate.

It is true that the collisions performed at CERN are relatively meager compared to cosmic-ray energies. The current, approximately 10 TeV collisions between equal-momentum particles at CERN correspond to 10.000 TeV cosmic ray protons hitting a stationary proton on earth or a white dwarf. The thousand-fold increase is a consequence of the relativistic energy-momentum law being applicable.

If 10.000 TeV (= 10 to the 16 electron volt) look like much, cosmic ray energies up to 10 to the 22 electron volt (a million times more) have been measured. However, if the latter are translated back into symmetric collisions of the CERN type, they are “only” a thousand times more energetic than CERN’s (owing to the square-root rule implicit in the mentioned law).

The fact that white dwarfs appear to be resilient to this bombardment is living proof that the cross section of CERN-generated miniature black holes (as well as their up to a thousand times more massive cosmic-ray generated analogs) must be minuscule. Specifically, their diameter must lie below that of a lepton (electron or quark). While an electron’s diameter is often supposed to be zero, neutrino absorption in solid matter yields a finite value (about ten to the negative 24 meter). In addition, the Telemach theorem guarantees a non-zero electron diameter.

So far, the cosmic rays cannot be shown not to be generating ultra-fast miniature black holes. When generated, the latter need to be rare enough not to leave a black hole get stuck inside the white dwarf in question. Otherwise white dwarf stars would no longer exist, as Tom stresses. The difference between earth and a white dwarf lies in the latter’s by 5 orders of magnitude higher density. It renders the white dwarf by so many orders of magnitude more vulnerable to ultra-fast natural black holes. Hence we have 3 numbers which jointly limit the lifespan of white dwarfs: The collision rate of CERN-like (or stronger) cosmic rays impinging on their surface; the fraction of these events leading to the formation of a black hole; and the free path length of an ultrafast miniature black hole inside white-dwarf matter.

None of these three parameters is currently known. Nevertheless as long as the black hole is markedly smaller than a lepton, it is the latter’s diameter alone that determines the cross section. Therefore, it is possible to draw a conclusion: White-dwarf longevity is limited by cosmic rays if the energy of the latter (CERN size or larger) suffices to generate black holes. In this case, “very old” white dwarfs cannot exist. This is a testable prediction.

The cooling rate of white dwarfs happens to be very low owing to their minuscule surface-to-mass ratio. Our cosmos is currently assumed to be only 14 billion years old (about the age of globular star cluster in our galaxy). Ultra-old white dwarfs should not be observable for that reason alone. As it happens, the new prediction is theory-independent, however. Ultra-old cold white dwarfs are therefore worth looking for empirically. If they are found, two important implications follow: (i) our universe is older than generally anticipated; (ii) the LHC experiment is safe. If, on the other hand, ultra-old white dwarfs prove empirically absent, this fact confirms the big bang theory at face value. However, if the recent theory of cryodynamics holds true (which implies a very much larger age of the universe), a measured absence of ultra-old white dwarfs implies that cosmic rays produce white-dwarf eating black holes. In that case, there is a high probability that the LHC is currently producing earth-eating black holes.

Therefore an astronomical test of the safety of the LHC experiment, based on white dwarf longevity, exists. The same claim was made by Tom. The difference lies alone in the fact that he assumes that the collision rate of micro black holes with leptons is much higher (due to a higher lepton diameter being apparently assumed). This difference led him to predict a very much shorter lifespan for white dwarfs. Since that prediction is defied by observation, his conclusion was that CERN is safe.

It will be important for everyone to learn if Tom Kerwick (perhaps in conjunction with Giddings and Mangano whom he quotes) can defend his prediction of a much higher collision rate with leptons for ultrafast natural mini-black holes inside white dwarfs. If so, CERN can perhaps be exculpated for its public refusal to update its 4-year-old safety report while continuing at a nonlinearly increased collision rate.

I thank Henry Gebhardt, Boris Hagel and Tobias Muller for discussions. For J.O.R.

While emailing back and forth with Ron Kita, I realized that it would be useful to compile a list of researchers who have published serious papers, past & present, in the new field of propulsion physics (gravity modification is an example) at least for the purpose of finding out how many countries are at some stage in this field.

This is important to do if we are to hasten the theoretical & technological development to leave Earth on a commercially feasible scale. I was surprised by what I found.

Below is the list. I’m sure it is not complete but it is a start. If you know of anyone who should be on this list, please let me know, and I will update this post.

Here are the ground rules for including a name.

1) They must have published their research in a journal accessible to the public (preferably in English as I’m monolingual and cannot verify the validity if it is not). This excludes anyone in secret projects or black projects (therefore Greenglow, Phantom & Skunk), or could not reach the level of research where peer review would consider the paper acceptable.

2) Excludes papers related to conventional technologies. This excludes sails, tethers, conventional fuels, ion propulsion and nuclear detonations.

3) Excludes the extension of conventional physics. For example, it is estimated that doing interstellar travel to Alpha Centauri, with conventional fuels would require a fuel cost of approximately 3.4x 2011 World GDP.

4) Exclude papers requiring ‘Millennium Theories’. Millennium Theories are theories that will require more than a 100 years to falsify. This eliminates research using exotic matter. For example, it is estimated that doing interstellar travel to Alpha Centauri, with antimatter would cost of approximately 43,000x 2011 World GDP.

5) Includes researchers attempting to solve anomalies or unexplained observations, today, but exclude those whose focus is not propulsion.

6) Includes researches in established organizations but excludes researchers involved in the test methodologies or the management of such programs.

7) It would be desirable if the publishing journal/conference was associated with a national organization such as AIP, AIAA, Elsevier or other similar organizations.

Country Count People Count Country Last Name First Name
1 1 Austria Hense Klause
1 2 Austria Marhold Klause
1 3 Austria Tajmar Martin
2 4 Brazil De Aquino Fran
2 5 Brazil Alcubierre Miguel
3 6 Canada Hathaway George
4 7 China Li Ning
4 8 China Wu Ning
5 9 Finland Nieminen R.
6 10 France de Matos Clovis
7 11 Greece Provatidis Christopher
8 12 India Gupta R.C.
9 13 Italy Modanese Giovanni
9 14 Italy Ummarino G.A.
10 15 Japan Hayasaka Hideo
10 16 Japan Musha Takaaki
10 17 Japan Nishino Kimio
10 18 Japan Takeuchi Sakae
11 19 Romania Agop M.
11 20 Romania Buzea C. Gh.
11 21 Romania Ciobanu B.
12 22 Russia Podkletnov Eugene
13 23 Slovakia Sima Jozef
13 24 Slovakia Sukenık Miroslav
14 25 South Korea Tajmar Martin
15 26 UK Laithwaite Eric
16 27 USA Brandenburg John
16 28 USA Brantley Whitt
16 29 USA Chiao Raymond Y.
16 30 USA Clark Rod
16 31 USA Cramer John
16 32 USA Forward Robert
16 33 USA Fralick Gustave
16 34 USA Gaines J
16 35 USA Haisch Bernard
16 36 USA Hammer Jay
16 37 USA Kir Asit
16 38 USA Koczor Ron
16 39 USA Maclay Jordan
16 40 USA March Paul
16 41 USA Michael George
16 42 USA Milonni Peter
16 43 USA Murad Paul
16 44 USA Niedra Janis
16 45 USA Noever David
16 46 USA Puthoff Hal
16 47 USA Reuda Alfonso
16 48 USA Richland Center
16 49 USA Robertson Glen (Tony)
16 50 USA Rounds Frederic
16 51 USA Sanderson L
16 52 USA Serry Michael
16 53 USA Solomon B.T.
16 54 USA Torr D.G.
16 55 USA Villareal Carlos
16 56 USA Woods Clive
16 57 USA Woodward James

There are 16 countries! and 57 researchers. In a 2011 email to us, James Woodward had suggest that there are only about 35 of us seriously researching propulsion physics, on this planet. He came close, or I’m being generous. OK you can exclude Finland and India because I do not think these two countries have a concerted effort to develop a new propulsion technology.

Thanks to Ron Kita for pointing me to Takaaki Musha (Honda), Kimio Nishino (Toyota) and RC Gupta. I was surprised that Honda and Toyota, the car companies were interested in gravity modification.

Ron had also suggested Mike Gamble (supposedly of Boeing, and I did not attempt to either confirm or disprove his employement), and Brice Cassenti. I did not include Cassenti because his work was on Biefield Brown, which is an electric field effect.

Propulsion physics is about anything that is not related to gliding, rocketry, jets, electric motors, and internal combustion engines. I included South Korea because Tajmar is there now.

I excluded Mike Gamble, and here’s why. At SPESIF 2012 (which I had not attended) he announced that ‘Boeing has been using a “scissoring gyroscope” style of inertial propulsion for satellite maneuvering for years!’ and showed a picture (see http://www.integrityresearchinstitute.org/Enews/EnewsMar2012.htm).

I am very skeptical. I could not make out what the picture shows, and in my opinion a “scissoring gyroscope” type technology is too jerky to be used as a means of satellite propulsion.

Kumaran Sanmugathasan had suggested Mehran Keshe of Belgium, he does not satisfy the rules. Thanks Kumaran.

Gary Stephenson had suggested many, many names. Thanks Gary. Gary had also suggested S.M. Godwin & V.V. Roschin of Russia, but I could not find enough information about them with respect to the rules, above, and have to exclude them.

Hope this blog posting will increase the number of serious researchers in the new field of propulsion physics, increase the funding, and raise the awareness of propulsion physics as opposed to astronomy or cosmology.

—————————————————————————————————

Benjamin T Solomon is the author & principal investigator of the 12-year study into the theoretical & technological feasibility of gravitation modification, titled An Introduction to Gravity Modification, to achieve interstellar travel in our lifetimes. For more information visit iSETI LLC, Interstellar Space Exploration Technology Initiative

- From Integrationalism

In April of 2010 the Library of Congress announced that it will acquire all of the public tweets for future generations to review. It’s quite the ambitious effort from a technological standpoint, considering all of the data migration and storage as the micro-blogging social network grows. The initiative also has some uncovered ethical and democratic potential that are currently being overlooked.

Twitter as a platform is empowering the creators of the world to understand how their co-conspirers and consumers are affecting the discovery, development, and delivery of new goods & services to be brought to market. For instance, Marketing and other R&D departments across the globe at the enterprise scale are using social networks like Twitter to monitor and improve their CRM (Customer Relationship Management) processes. These aren’t rigid customer service initiatives, but also customer discovery initiatives. Social networking is giving new meaning to the idea that supply & demand are never ending sphere of interaction; further, confusing the philosophical ideal of who might our creators and consumers be.

This is important because ownership is allocated to creators of sorts, regardless of initial or latter impact.

At current, the world is enduring a series of spiking economic crisis, and as the engineers and economists try and root-cause to remedy our problems, the political conservatism that we all possess at some extent is making it difficult to justify spreading the wealth. Moral and Political arguments haven’t been working over the millennia or most recently. The books/rants/calls for gifting larger amounts to working-poor, nor distributing wealth at high rates to compensate the lesser valued have yielded a change in the gap between those with an immense value and those without. This crisis is not one of lost value, or population growth, or technological change. It is (and has always been) one of poorly allocated ownership. Those causes can be debated separately.

Ownership is paramount in distributing value to individuals and institutions, outside of charity. I don’t think it necessary to elaborate on how miniscule charity is in the known world. It’s legally defensible and mathematically quantifiable. One of the missions of the Library of Congress is to log intellectual property; further, so that it may (if necessary) be defended on the behalf of stakeholders. The initiative to capture tweets for the future generations should not only be technologically charged, but it should be economically charged to assign ownership to authors. This effort would assist greatly in identifying the degrees of separation between the various stakeholders in the discovery, development, and delivery of things.

Recently Seth Shostak of the SETI Institute, wrote an article in the Huffington Post How to Find Extraterrestrial Life. He had proposed that the search for extraterrestrial life was a three-way horse race. According to Shostak:

(1) Discover Life Nearby: This is the search for life in our solar system.

(2) Sniff It Out: Do the sort of spectral analysis that might detect atmospheric gases caused by biology.

(3) Eavesdrop On ET: Otherwise known as SETI, is the effort to detect radio signals or laser flashes from technically savvy extraterrestrials.

Neat, Shostak has set the frame work for further dscussions. Note that the (1) is the search for the existance of life based molecules. That (2) is the search for life forms, whether past or present. And (3) is the search for extraterrestrial intelligence.

He says that a priori all are equally likely to be successful. Lets think again.

With respect to (1) Discover Life Nearby, lets look at the record. Using the Mars Exploration Rovers, Spirit & Opportunity, as examples, Spirit which was 2.3m wide, covered 8.81 km over 581 sols (a Martian day that is approximately an Earth day), that is approximately 19 m2 per day. Given that the surface of Mars is 144,798,500 km2 it will take Spirit about 7.6 × 1012 days or 208,340,844 centuries, to examine the total surface of Mars. That is, assuming randomness, and that life did exist on Mars in the past, the quick & dirty probability of finding life on Mars on any day with current technology is 1.3 × 10-13. We have a better idea of Mars. It is mostly barren. However, not a clue about the Europa the moon of Jupiter, that is believed to have oceans beneath its ice.

With current projections it likely that NASA will have a satellite at Europa in the 2020–2030 time frame.

So, we can make 2 types of guesses. Assuming that life started on Europa some millions ago, then the probability (from a detection perspective) of finding life on Europa is good, close to 1. However, if Europa is a liquid version of Mars, then the probability is on the order of 1 × 10-13.

Therefore, the time frame for discovery of extraterrestrial life by (1) Discover Life Nearby, is about 2025 assuming no budgets cuts or other re-prioritizations.

With respect to (2) Sniff It Out, scientists estimate that there are about 1 x 1010 Earth like planets in our Milky Way. Lets assume that the Goldilocks Zone is a necessity. Using Pluto as the outer extreme of planets in a Star Local system, and Mars and Venus as boundaries of our Goldilocks Zone, then the approximate probability of finding one of these Earth-like planets in the Goldilocks Zone is 2.89 × 10-2. This reduces the number of Earth-like planets capable of supporting life to 289,340,102. Or the probability of finding life on at least one of these planets (assuming life is present) is at least 3.45 × 10-9.

I would estimate that the time frame for detecting extraterrestrial life is between today, and 35 years from now to 2047.

It could be any day now as the Dutch using the Very Large Telescope in the Chilean Andes have detected carbon monoxide on a planet hugging the star Tau Bootis that is 51 light-years away. The other end of my estimate is 2047. This is because developing a technology like the James Webb telescope was 30 years in the making.

So (2) Sniff It Out, has a better chance of finding evidence of life than (1) Discover Life Nearby.

Now how about (3) Eavesdrop On ET? As the author of the 12-year study An Introduction to Gravity Modification, it is slim. Sorry, Tarter, Shostak and all of you at the SETI Institute. But wait, I haven’t finished.

Look at our civilization. In 1895 Guglielmo Marconi proved that long distance radio transmission was possible. In 117 years we have exponentially evolved our technological sophistication to what it is today, 2012.

As the author of the 12-year study An Introduction to Gravity Modification I have proposed (see page 195) the existence of subspace, where everything is probabilistic, and light speed is not a restriction. Therefore, if confirmed, there is the strong possibility that by 2025/2035 this planet will go radio silent, because all our transmissions will be through subspace.

That is, the window to observe a radio intelligent extraterrestrial civilization is about 100 to 150 years, then they go silent. 100–150 years is an immensely thin slice or duration compared to the distances of stars even within our own galaxy, the Milky Way. Or the probability of detecting extraterrestrial radio transmissions within our own galaxy is approximately 1.25 × 10-6. It is actually a little better than this but I am using quick & dirty for this blog posting, and this will do. This is much better than a posteriori 1 × 10-13 for (1) Discover Life Nearby and 3.45 x 10-9 for (2) Sniff It Out.

So SETI, keep eavesdropping, and we can expect confirmation of Extraterrestrial Life by 2047 latest.

—————————————————————————————————

Benjamin T Solomon is the author & principal investigator of the 12-year study into the theoretical & technological feasibility of gravitation modification, titled An Introduction to Gravity Modification, to achieve interstellar travel in our lifetimes. For more information visit iSETI LLC, Interstellar Space Exploration Technology Initiative

In it he reports on a gorilla in a cage who could be brought to phrenetic laughter by his human friend’s pretending to bite him into his toe. Quote: “If you have never seen a gorilla in a fit of laughter, I recommend searching out such a sight before you pass from this world.”

This is absolutely human behavior. If you know about the cross-caring theory, which explains how a young child interacting with his bonding partner is getting “moved” into suspecting benevolence shown towards him, then you realize that the same thing can be accomplished with a caged or non-caged gorilla.

I recently mentioned Margaret Howe, a pupil of my late friend Gregory Bateson’s. There are important insights about the mission of humankind on our planet and beyond (“galactic export”) that would make it a great pity if this “second level of human social evolution on earth and in the solar system” was going to be clipped.

I know I am being impossible, but finding outrageous things that tickle everyone in her or his heart so as to be moved is the real mission of science. I fantasize talking with a gorilla – or orangutan – about the long-stretched “toe” of the visualized Schwarzschild metric of a black hole, both of us laughing.

If you think dolphins are preferable, I shall not object. I found a proof recently, though, that orangutans have the most highly developed brain identified so far. The fact that the latter is lightweight owing to its carrier’s arboreal existence, does not detract from its functional superiority. The proof is based on the mathematics of the traveling salesman problem (second version).

Ray Kurzweil hopes we can build artificial brains of matching caliber soon – via the brain equation, I would add. But it would be fun to first make friends with our hardware-wise stronger natural relatives. Including – perhaps – giant octopuses and mantis shrimps ( https://www.youtube.com/watch?feature=endscreen&NR=1&v=nKgStQ8Scs0 ).

Could CERN not make a tiny little break to admit a “safety-regained discussion” as it could be called in anticipation?

http://www.aljazeera.com/programmes/insidestory/2012/07/2012759585764599.html (at minutes 09:00–10:10, 11:00–12:03, 12:35–13:25, 16:08–17:13) gave me a world-wide forum again. The rest of the media and all colleagues of mine keep their mouths shut.

There is logic behind this schizophrenic world-wide attitude: In case the outlaw is right, one can later always claim that not the whole planet was part of the conspiracy of silence since one high-ranking international outlet reported. However, this strategy is not logical. For if I am right and the worst case materializes, the fig leaf will go under as well.

My class yesterday in which this riddle was touched upon in passing helped me see the mechanism: My results on black holes are too much advanced from the planet-wide accepted lore to be understandable to any colleague.

Imagine the “generic 3-pseudosphere.” Its lower-dimensional analog in ordinary 3-space, the 2-pseudosphere (the so-called Newton pseudosphere) looks like two trumpets with infinitely long, infinitely thinned-out mouth pieces, glued together head-on with their bells ( http://en.wikipedia.org/wiki/File:The_Pseudosphere.jpg ). This smooth monster has the same volume as a sphere of the same (maximal) diameter, and also the same surface area and the same (if negative) curvature: a kind of miracle. Hence the name “pseudo-sphere.”

By cutting it in the middle to take only one half of it, and then making the trumpet generic by giving it a non-zero asymptotic radius – the Schwarzschild radius – at its infinitely far-away tip (and adding one dimension), you get the correct reality of the space surrounding a black hole. Although there is beautiful related work by Yu Tian at al. ( http://arxiv.org/pdf/hep-th/0411004.pdf ), this is beyond the heads of the whole community. They simply cannot follow.

My late friend Benoit Mandelbrot created a storm with the opposite insight – that there are compact finite volumes with an infinite surface area. In the present dual case, the little ant on the flat outer rim of the trumpet, headed for the middle, cannot believe that the way towards the latter (the so-called “horizon”) is infinitely long. No one saw this before.

But this is “art for art’s sake,” is it not? No: this is physics. And, strangely, the survival of the planet hinges on a single person of public clout believing me.

Thank you, everyone, for kindly having bent your mind.

“If the rate of change on the outside
exceeds the rate of change on the inside, the end is near”
- Jack Welch

Complex societies are heavily addicted to expensive, vulnerable and potentially hazardous infrastructure. We rely on a healthy environment for production of food and access to clean water. We depend on technological infrastructure for energy supplies and communications. We are deeply addicted to economic growth to support growing populations and consumption. If one of these pillars of modern society crumbles our existence will collapse like a house of cards.

The interdependencies and complexities of the system we call modern society has become so intertangled that finding a robust and simple solution to our problems has become close to impossible. Historically the cold war gave us the logic of a “balance of terror”. This logic, originally concerned with a balance of U.S. vs. Soviet military capacities, has lead to an increasingly expensive way of reducing risk and ever expanding bureaucracies to keep us “virtually safe”.

With the onset of a global economic recession, drastic climate change, deadly natural disasters, raging civil wars and diminishing natural resources we need a new logic. A set of moral laws for reducing risk and mitigating consequences applicable at a low cost from the bottom up of entire societies.

The concept of resilience is based on the idea that disasters are inevitable and a natural part of existence. Our best defense is preparedness and engineering systems that not only can withstand heavy strains but also absorb damage. The Institute for Resilient Infrastructure at the University of Leeds gives this definition of “Resilience”;

Resilience can also be explained in terms of durability. A durable material, component or system is one which can cope with all the known, predictable loads to which it will be subjected throughout its life. As well as physical loads – stresses and strains – we include environmental loads (e.g. temperature, weather), economic loads (e.g. the scarcity of resources or financial turmoil) and social loads (e.g. changes in legislation or of use, terrorist attack, changes in demography or society’s expectations and demands).

In the 1970s about 100 disasters were recorded worldwide every year. According to the International Disaster Database an average of 392 disasters were reported per year in the last decade. In 2011 we saw record greenhouse gas emissions, melting Arctic sea ice, extreme weather and the earthquake in Japan resulting in the world’s second worst nuclear disaster. Current systems for mitigation of risk are obviously not capable of handling the overwhelming challenges confronting us.

The price tag for disasters in 2011 reached a record high of $265 billion. Most of that cost ($210 billion) came from the tsunami in Japan, but flooding in Australia, tornadoes in the United States and earthquakes in New Zealand contributed substantially. The increasingly turbulent weather patterns wreaking havoc across the planet may only be the beginning of a period of drastic climate change.

In addition to climate change industrial society faces depleted natural resources, degradation of infrastructure and systemic limits to growth. The ongoing economic crisis is a symptom of a deeper structural failure. Governments are running out of options when solving a debt crisis with more debt is the last resort. We rely on short term solutions for long term problems.

We are facing a different type of threat originating from within the system itself, an endogenous and internal failure of our civilizational paradigm. Growing populations stress our dependency on non-renewable resources supported by potentially hazardous nuclear power. The case of the Fukushima nuclear accident illustrates that large population located on limited land is extremely vulnerable to unpredictable events like earthquakes or other catastrophic “wild cards”. From the perspective of risk analysis the state of Japan is a model of the entire planet.

To make the situation even more acute the horizon of Homo Sapiens is full of threats like global pandemics and emerging technologies that could permanently wipe us off the face of the earth. Nanotechnology, synthetic biology and geoengineering hold the promise of a quick fix but also have the potential to cause irreversible harm to the biosphere and human life.

Technology is without a doubt a part of a permanent solution for sustainable life on the planet. The bottom up approach to resilience is about awakening a culture that rewards autonomy and self-sufficiency. Resilience is more than durable engineering. Resilience has to become an obligatory way of thinking and eventually a way of life.

10 robust resilient strategies:
1. Sustain a culture that rewards autonomy and self-sufficiency.
2. Share practical solutions and stockpile resilient ideas instead of canned food.
3. Support intra-generational sharing of knowledge on how to live in accord with nature.
4. Develop alternative economic systems; use Bitcoins and barter when possible.
5. Refine high-tech solutions but favor low tech; HAM radios beat cell phones in emergencies.
6. Grow your own food; become an urban gardener or start a farm revival project.
7. Reduce energy consumption with geothermal energy, local water mills, wind mills and solar panels.
8. Use a condom; think eugenically — act passionately.
9. Keep a gun; if you are forced to pull it – know how to use it.
10. Stay alive for the sake of the next generation.

This article is co-published on Interesting Times Magazine.