WUBBA LUBBA DUB DUB Part 2 Aliens, Energy & Time Travel

https://steemit.com/arg/@j1337/wubba-lubba-dub-dub-part-2-common-era-kepler-supernovas-star-of-bethlehem-aliens-unlimited-energy-flux-capacitor

Back To The Future!
Alternative names for the Anno Domini era include vulgaris aerae

In the AD year numbering system, whether applied to the Julian or Gregorian calendars, AD 1 is preceded by 1 BC. There is no year "0" between them, so a new century begins in a year which has "01" as the final digits (e.g., 1801, 1901, 2001). New millennia likewise are considered to have begun in 1001 and 2001. This is at odds with the much more common conception that centuries and millennia begin when the trailing digits are zeroes (1800, 1900, 2000, etc.); for example, the worldwide celebration of the new millennium took place on New Year's Eve 1999, when the year number ticked over to 2000.

For computational reasons, astronomical year numbering and the ISO 8601 standard designate years so that AD 1 = year 1, 1 BC = year 0, 2 BC = year −1, etc. In common usage, ancient dates are expressed in the Julian calendar, but ISO 8601 uses the Gregorian calendar and astronomers may use a variety of time scales depending on the application. Thus dates using the year 0 or negative years may require further investigation before being converted to BC or AD.

Common Era = Vulgar Era

Johannes Kepler first used "Vulgar Era" to distinguish dates on the Christian calendar from the regnal year typically used in national law. He was a German mathematician, astronomer, and astrologer.

Kepler is a key figure in the 17th-century scientific revolution. He is best known for his laws of planetary motion, based on his works Astronomia nova, Harmonices Mundi, and Epitome of Copernican Astronomy. These works also provided one of the foundations for Isaac Newton's theory of universal gravitation.

He did fundamental work in the field of optics, invented an improved version of the refracting telescope (the Keplerian telescope), and was mentioned in the telescopic discoveries of his contemporary Galileo Galilei. He was a corresponding member of the Accademia dei Lincei in Rome.

Kepler lived in an era when there was no clear distinction between astronomy and astrology, but there was a strong division between astronomy (a branch of mathematics within the liberal arts) and physics (a branch of natural philosophy). Kepler also incorporated religious arguments and reasoning into his work, motivated by the religious conviction and belief that God had created the world according to an intelligible plan that is accessible through the natural light of reason. Kepler described his new astronomy as "celestial physics", as "an excursion into Aristotle's Metaphysics", and as "a supplement to Aristotle's On the Heavens", transforming the ancient tradition of physical cosmology by treating astronomy as part of a universal mathematical physics

The Supernova of 1604
In October 1604, a bright new evening star (SN 1604) appeared, but Kepler did not believe the rumors until he saw it himself. Kepler began systematically observing the nova. Astrologically, the end of 1603 marked the beginning of a fiery trigon, the start of the about 800-year cycle of great conjunctions; astrologers associated the two previous such periods with the rise of Charlemagne (c. 800 years earlier) and the birth of Christ (c. 1600 years earlier)
SN 1604, also known as Kepler's Supernova, Kepler's Nova or Kepler's Star, was a supernova of Type Ia that occurred in the Milky Way, in the constellation Ophiuchus. Appearing in 1604, it is the most recent supernova in our own galaxy to have been unquestionably observed by the naked eye, occurring no farther than 6 kiloparsecs or about 20,000 light-years from Earth.

The Star of Bethlehem—analogous to the present new star—would have coincided with the first great conjunction of the earlier 800-year cycle.

1611 he published the first description of the hexagonal symmetry of snowflakes and, extending the discussion into a hypothetical atomistic physical basis for the symmetry, posed what later became known as the Kepler conjecture, a statement about the most efficient arrangement for packing spheres.

Kepler is a space observatory launched by NASA to discover Earth-size planets orbiting other stars.Named after astronomer Johannes Kepler, the spacecraft was launched on March 7, 2009, into an Earth-trailing heliocentric orbit. The principal investigator was William J. Borucki.

Designed to survey a portion of our region of the Milky Way to discover Earth-size exoplanets in or near habitable zones and estimate how many of the billions of stars in the Milky Way have such planets,Kepler's sole scientific instrument is a photometer that continually monitors the brightness of approx 150,000 main sequence stars in a fixed field of view.These data are transmitted to Earth, then analyzed to detect periodic dimming caused by exoplanets that cross in front of their host star.

Since 1988, over 3,000 exoplanets have been confirmed by all detection methods, including the Kepler mission. As of 1 July 2018, there are 3,797 confirmed planets in 2,841 systems, with 632 systems having more than one planet. Kepler's field of view covers 115 square degrees, around 0.25 percent of the sky, or "about two scoops of the Big Dipper". Thus, it would require around 400 Kepler-like telescopes to cover the whole sky. The Kepler field contains portions of the constellations Cygnus, Lyra, and Draco. The scientific objective of Kepler is to explore the structure and diversity of planetary systems. This spacecraft observes a large sample of stars to achieve several key goals:

To determine how many Earth-size and larger planets there are in or near the habitable zone (often called "Goldilocks planets") of a wide variety of spectral types of stars.
To determine the range of size and shape of the orbits of these planets.
To estimate how many planets there are in multiple-star systems.
To determine the range of orbit size, brightness, size, mass and density of short-period giant planets.
To identify additional members of each discovered planetary system using other techniques.
Determine the properties of those stars that harbor planetary systems.(edited)
On May 10, 2016, NASA announced that the Kepler mission had verified 1,284 new planets.Based on their size, about 550 could be rocky planets. Nine of these orbit in their stars' habitable zone:
Kepler-1638b
Kepler-1606b
Kepler-1544b
Kepler-1410b
Kepler-1455b
Kepler-560b
Kepler-705b
Kepler-1593b
Kepler-1229b

The Kepler Input Catalog is a publicly searchable database of roughly 13.2 million targets used for the Kepler Spectral Classification Program and the Kepler mission. The catalog alone is not used for finding Kepler targets, because only a portion of the listed stars (about one-third of the catalog) can be observed by the spacecraft.
NASA Exoplanet Archive, online exoplanet catalog
Other space-based exoplanet search projects
CHEOPS (2019)
CoRoT (2006–2012)
Gaia (since 2013)
PlanetQuest (since 2002)
PLATO (2026)
TESS (since 2018)
Other ground-based exoplanet search projects
APF (since 2013)
HATNet (since 2001)
HARPS (since 2003)
NGTS (since 2015)
PlanetQuest (since 2002)
SuperWASP (since 2002)


The SuperNova Early Warning System (SNEWS) is a network of neutrino detectors designed to give early warning to astronomers in the event of a supernova in the Milky Way, our home galaxy, or in a nearby galaxy such as the Large Magellanic Cloud or the Canis Major Dwarf Galaxy. As of May 2018, SNEWS has not issued any supernova alerts, as the most recent known supernova remnant in the Milky Way was around the turn of the 20th century, and the most recent supernova confirmed to have been observed was Kepler's Supernova in 1604.

Powerful bursts of electron neutrinos (νe) with typical energies of the order of 10 MeV and duration of the order of 10 seconds are produced in the core of a red giant star as it collapses on itself via the "neutronization" reaction, i.e. fusion of protons and electrons into neutrons: pe−→nνe. It is expected that the neutrinos are emitted well before the light from the supernova peaks, so in principle neutrino detectors could give advance warning to astronomers that a supernova has occurred and may soon be visible. The neutrino pulse from supernova 1987A arrived 3 hours before the associated photons – but SNEWS was not yet active and it was not recognised as a supernova event until after the photons arrived. However, SNEWS is not able to give advance warning of a type Ia supernova, as they are not expected to produce significant numbers of neutrinos. Type Ia supernovae, caused by a runaway nuclear fusion reaction in a white dwarf star, are thought to account for roughly one-third of all supernovae.

Supernova nucleosynthesis is a theory of the nucleosynthesis of the natural abundances of the chemical elements in supernova explosions, advanced as the nucleosynthesis of elements from carbon to nickel in massive stars by Fred Hoyle in 1954. In massive stars, the nucleosynthesis by fusion of lighter elements into heavier ones occurs during sequential hydrostatic burning processes called helium burning, carbon burning, oxygen burning, and silicon burning, in which the ashes of one nuclear fuel become, after compressional heating, the fuel for the subsequent burning stage. During hydrostatic burning these fuels synthesize overwhelmingly the alpha-nucleus (A = 2Z) products. A rapid final explosive burning is caused by the sudden temperature spike owing to passage of the radially moving shock wave that was launched by the gravitational collapse of the core. W. D. Arnett and his Rice University colleagues demonstrated that the final shock burning would synthesize the non-alpha-nucleus isotopes more effectively than hydrostatic burning was able to do, suggesting that the expected shock-wave nucleosynthesis is an essential component of supernova nucleosynthesis. Together, shock-wave nucleosynthesis and hydrostatic-burning processes create most of the isotopes of the elements carbon (Z = 6), oxygen (Z = 8), and elements with Z = 10–28 (from neon to nickel).

As a result of the ejection of the newly synthesized isotopes of the chemical elements by supernova explosions their abundances steadily increased within interstellar gas. That increase became evident to astronomers from the initial abundances in newly born stars exceeding those in earlier-born stars. To explain that temporal increase of the natural abundances of the elements was the main goal of stellar nucleosynthesis. Hoyle's paper was the founding paper of that theory; however, ideas about nuclear reactions in stars providing power for the stars is often confused with stellar nucleosynthesis. Realize that nuclear fusion in stars can occur with negligible impact on the abundances of the chemical elements.

T2K (Tokai to Kamioka, Japan) is a particle physics experiment that is a collaboration between several countries, including Japan, Canada, France, Germany, Italy, South Korea, Poland, Russia, Spain, Switzerland, the United States, and the United Kingdom. It is the second generation follow up to the K2K experiment, a similar long baseline neutrino oscillation experiment. The J-PARC facility produces an intense off-axis beam of muon neutrinos. The beam is directed towards the Super-Kamiokande detector, which is 295 km away. The main goal of T2K is to measure the oscillation of ν μ to ν e and to measure the value of θ13, one of the parameters of the Pontecorvo–Maki–Nakagawa–Sakata matrix.

On June 15, 2011, the T2K collaboration announcedthe observation of six electron neutrino-like events compared to an expected background of 1.5, a significance of 2.5 standard deviations.

On July 19, 2013, at the European Physical Society meeting in Stockholm, the international T2K collaboration announced a definitive observation of muon neutrino to electron neutrino transformation.
Neutrino oscillation is a quantum mechanical phenomenon whereby a neutrino created with a specific lepton flavor (electron, muon, or tau) can later be measured to have a different flavor. The probability of measuring a particular flavor for a neutrino varies between 3 known states as it propagates through space.

First predicted by Bruno Pontecorvo in 1957, neutrino oscillation has since been observed by a multitude of experiments in several different contexts. Notably, the existence of neutrino oscillation resolved the long-standing solar neutrino problem.

Neutrino oscillation is of great theoretical and experimental interest, as the precise properties of the process can shed light on several properties of the neutrino. In particular, it implies that the neutrino has a non-zero mass, which requires a modification to the Standard Model of particle physics
Stellar nucleosynthesis is the theory explaining the creation (nucleosynthesis) of chemical elements by nuclear fusion reactions between atoms within the stars. Stellar nucleosynthesis has occurred continuously since the original creation of hydrogen, helium and lithium during the Big Bang. It is a highly predictive theory that today yields excellent agreement between calculations based upon it and the observed abundances of the elements. It explains why the observed abundances of elements in the universe grow over time and why some elements and their isotopes are much more abundant than others. The theory was initially proposed by Fred Hoyle in 1946,who later refined it in 1954. Further advances were made, especially to nucleosynthesis by neutron capture of the elements heavier than iron, by Margaret Burbidge, Geoffrey Burbidge, William Alfred Fowler and Hoyle in their famous 1957 B2FH paper, which became one of the most heavily cited papers in astrophysics history.
The most important reactions in stellar nucleosynthesis:

Hydrogen fusion:
Deuterium fusion
The proton–proton chain
The carbon–nitrogen–oxygen cycle
Helium fusion:
The triple-alpha process
The alpha process
Fusion of heavier elements:
Lithium burning: a process found most commonly in brown dwarfs
Carbon-burning process
Neon-burning process
Oxygen-burning process
Silicon-burning process
Production of elements heavier than iron:
Neutron capture:
The R-process
The S-process
Proton capture:
The Rp-process
The P-process
Photodisintegration

Hydrogen fusion (nuclear fusion of four protons to form a helium-4 nucleus) is the dominant process that generates energy in the cores of main-sequence stars. It is also called "hydrogen burning", which should not be confused with the chemical combustion of hydrogen in an oxidizing atmosphere. There are two predominant processes by which stellar hydrogen fusion occurs: proton-proton chain and the carbon-nitrogen-oxygen (CNO) cycle. Ninety percent of all stars, with the exception of white dwarfs, are fusing hydrogen by these two processes. Every second, the Sun fuses 500 million tons of hydrogen into helium, releasing about 5 million tons of gamma rays that eventually heat and illuminate Earth. For a long time (Project Matterhorn started in 1951), nuclear fusion has been considered a very desirable power source because the fuel is virtually free, and the process releases vast amounts of energy and no pollutants.

There are two competing approaches for the artificial creation of nuclear fusion: Magnetic confinement, which uses massive magnetic force to contain the fusing plasma within a tokamak (doughnut) device, and inertial confinement, which uses lasers to create enough heat and pressure to trigger nuclear fusion. Magnetic confinement is usually considered a better prospect for the limitless production of clean energy and indeed, magnetic confinement will be used by the 500-megawatt ITER fusion reactor in France but a lot of work is still being done on inertial confinement by the likes of California’s National Ignition Facility (NIF), which uses 500 trillion watts of laser light to kick-start fusion reactions.

Right now at ITER, a vast fusion chamber that’s three stories high is due to begin fusing deuterium-tritium fuel in 2026. ITER is hoping to produce 500 megawatts over 1,000 seconds from just 50 megawatts of input power and 0.5 grams of hydrogen fuel. If it’s a success, an actual fusion power plant, called DEMO, will be built. NIF, the 500-trillion-watt “star power” laser fusion center, hopes that 2012 will see the first experiment that produces more power than it consumes and pending successful ignition, the Lawrence Livermore National Laboratory will begin full scale planning on the LIFE power plant. 50 Megawatts + .5 gram Hydrogen= 500 Megawatts in 1,000 seconds.

We could assume 500 trillion watts turns into 5 Quadrillion Watts.

In order to travel through time, the vehicle integrated with the flux capacitor needed to be traveling at 88 mph (140.8 km/h), and required 1.21 gigawatts of power (1,210,000,000 watts), originally supplied by a plutonium-powered nuclear reactor.

The flux capacitor consisted of a box with three small, flashing incandescent lamps arranged as a "Y", located above and behind the passenger seat of the time machine. Accessing the flux capacitor safely required disconnection of the capacitor drive, as the Dymo warning label at the top of the unit — DISCONNECT CAPACITOR DRIVE BEFORE OPENING — pointed out. The coils that can be seen across the front and along the rear sides can be referenced as the temporal demodulation coils as used in the original blueprints of the vehicle. These play a key part to open a hole in the time barrier.

The time machine's return trip (from 1955 back to 1985), plutonium was not available, so a lightning rod was connected directly into the flux capacitor and was used while the vehicle sustained 88 m.p.h. Plutonium was used once again for a trip forward in time at least 30 years, and at some point thereafter the plutonium reactor was replaced by a Mr. Fusion home energy generator from the future that was fueled by extracting hydrogen atoms from garbage.

The DeLorean once again came back to 1985 and proceeded to travel to 2015, where it was stolen by Biff Tannen, taken back to 1955 and returned to 2015 without Doc's knowledge. When they returned in 1985, they found it was a different present, so they traveled back to 1955 to fix the space-time continuum. The DeLorean was again struck by lightning in the year 1955, this time by accident. The lightning created an overload and caused a malfunction in the time circuits sending the vehicle back to January 1, 1885. Earlier, the 1885 date was already displayed before the lightning hit, after the LED read-outs flashed.

The DeLorean was then hidden in the Delgado Mine by Doc for 70 years because suitable replacement parts were not invented until 1947. It was recovered from the mine in 1955 and repaired by Doc's 1955 counterpart, thus restoring it to working order. Since both gasoline and garbage were available, the next trip back to 1885 was performed under the car's own power.

Due to a broken fuel line, the DeLorean's final trip from 1885 to 1985 was partially powered by a steam locomotive pushing the vehicle up to 88 mph while using Mr. Fusion to generate the 1.21 gigawatts required to activate the flux capacitor and break the time barrier. Doc returns to 1985 in a time machine made from a locomotive. This used a flux capacitor that Doc was able to power using steam (at least with the propulsion requirement for time travel), located on the front of the train, in place of the lamp.

AND thats how we get back to WUBBA LUBBA DUB DUB!!!

It also puts us to 1985, when a part of Caimeo happened!!!

Information overloaded.
MIND BLOWN>>>Marianas web =Caimeo=Flux Capacitor = Hydrogen fusion = Time Travel = Unlimited Energy = ALIEN & HOW TO FIND THEM AND HOW THEY WOULD FIND US.

That's how you properly do a #QuantumTimeHack