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Message Subject You know all those strange rumblings and booms people are hearing all over the world? It is coming from space!
Poster Handle xen
Post Content
Could you elaborate some? I am intrigued!
 Quoting: Mojofabulous


earth's shields are temporarily down to allow these (and those from aquila, sirius, arcturus) energies to incorporate into her main operating system ;)

the below links don't tell the entire story but give you a good idea of what we're dealing with!

[link to hyperphysics.phy-astr.gsu.edu]

Cygnus X-3 has an orbital period about its companion of only 4.79 hours. Intriquing underground events in the Soudron iron mines in October 1985 included 60 anomalous muon events in a 3¡ cone around Cygnus X-3 with a precise period of 4.79 hours, so they clearly came from that source. But that requires a neutral particle traveling at almost precisely the speed of light, and there are no reasonable candidates for such a particle.

[link to www.marciabartusiak.com]

The traditional' interpretation of the star's composition is being challenged by a group of audacious physicists who offer as evidence some curious subatomic particles picked up by their protondecay detectors. The evidence now suggests that the star is a compact globe of more basic subatomic particlesquarks. (Quarks are the building blocks of protons and neutrons.) If this is so, astronomers could be forced to revise their theories of astrophysics.

[link to www.sciencedaily.com]

Cygnus X-3 is a strange case indeed, being one of the brightest radio source in the Galaxy except when it descends into a radio quenched state.
distant quasars, powered by supermassive black holes, pump even greater amounts of energy into space.
The gamma rays observed by AGILE were in the form of flares at energies of about 100 million electron volts. the flares preceded radio jets and occurred during a decline in high-energy X-rays from Cygnus X-3

The very complex behaviour of Cygnus X-3 requires monitoring throughout the electromagnetic spectrum from radio through X-rays and now including also gamma-ray emission. Not until we have gathered data from all possible wavelengths we can start to form a unified picture of this enigmatic object. Microquasars have strong magnetic fields which can store enormous amount of energy. During these gamma-ray flares this stored energy can accelerate charged particles to observed high energies which prompts them to emit gamma rays. Then the magnetic gate opens, and radio-emitting blobs are pushed out of the system producing the major radio flares


[link to www.mythicalireland.com]

This means Sirius, like the midwinter Sun, would have been visible from inside the chamber of Newgrange. In addition, Deneb, the bright star of the swan constellation Cygnus, was setting momentarily due north - something it only does for a couple of centuries in the whole 25,800-year cycle, and curiously, something which it only does at Newgrange's latitude. If you extend an imaginary line out from the chamber of Newgrange into the distance, it intersects another neolithic passage-tomb, the one at Fourknocks. Fourknocks has a passage which is orientated towards the north-north-east, where neither Sun nor Moon can rise. This, we think, is the rising place of Deneb at the critical precessional moment.

[link to 2011energy.alternate-healing-science-christian.ca]

More recently scientists are beginning to consider that high-energy cosmic rays might have played such a role, causing alterations in DNA sequences that become are carried forwards through subsequent generations. Evidence also suggests that human cognitive ability is much more directly affected by cosmic-ray effects as many of the great geniuses in modern history emerged in times of increased cosmic-ray density

A different concept for pulsars and quasars comes to light in the electric cosmology where the powering force of the Universe is recognized to be nearly entirely electric energy flowing in plasma. In this context the pulsating energy patterns are recognized as the result of repetitive electric discharge events between two closely related stellar bodies

Our sun emits all of these in a modest fashion, being powered by continuous electric discharges. Cygnus x3 stands out in that its radiated energy burst are more energetic. Since Cygnus x3 is not optically visible and is 'seen' only in x-ray light, retails are sparse, but it appears that we may be looking down the barrel of a stellar equivalent of a super-energetic plasma focus device
When cosmic rays reach the Earth they typically do so in a scattered fashion and with just enough energy that few hundred feet of concrete is sufficient to dissipate their energy and stop them. Being electrically charged, they typically pass clear through the atomic structures in their path, according to the electric repulsion principles. (High-energy neutrons in comparison are immensely destructive, by not having an electric charge that assures collision avoidance.) Cosmic-ray particles from Cygnus x3 are evidently electrically charged, but differ in that their greater energy content enables them to penetrate (at least) 2000 feet of rock


[link to atlantisrisingmagazine.com]

Cygnus X-3’s production of high energy gamma rays is merely one facet of its extraordinary influence on the solar system, for it is known to spew out electromagnetic radiation across a broad spectrum of frequencies, from radio waves and infrared radiation to higher frequency X-rays and cosmic radia­tion. This is because Cygnus X-3 has additionally been proposed as the galaxy’s first “microblazar,” a galactic form of a so-called “blazar.”
So what exactly is a blazar? Electromagnetic radiation and cosmic particles across a whole range of frequencies are produced by black holes and neutron stars as they “accrete” gaseous matter, generally from close proximity stars, which they then use to create a highly energized ring of ionized gas that encircles the star around its equator and is thought to be the source of the high energy gamma rays now being monitored from Earth. This so-called accretion disk feeds the star, which every so often “powers up” by emitting unimaginable jets of plasma (ionized gas) that ex­tend in opposite directions along the star’s axis of rotation


[link to blogs.physicstoday.org]

Now, two teams of researchers have made the first definitive detection of high-energy gamma rays, the most powerful type of electromagnetic radiation, from this small but nearby stellar system.

[link to www.nasa.gov]

Every 4.8 hours, a compact companion embedded in a disk of hot gas wheels around the star. "This object is most likely a black hole, but we can't yet rule out a neutron star," Corbet noted.

[link to ttt.astro.su.se]

Cygnus X-3 is one of the brightest X-ray binaries, discovered already 40 years ago [1],

extensively studied, but still poorly understood and usually referred to as a ‘peculiar source’. The identification of the donor as a Wolf-Rayet star [2] classifies it as a high mass X-ray binary (HMXB), despite its typical low mass binary period of 4.8 hours [3].

The system is located at a distance of 9 kpc ([4], assuming 8 kpc for the distance to the galactic centre; [5]), close to the Galactic plane. It shows signs of unusually strong and complex absorption, a consequence of the whole system being enshrouded in the wind of its companion Wolf-Rayet star. The problem in separating wind features from those arising in the photosphere of the companion makes determinations of radial velocity difficult, hence the masses of the components remain uncertain and the nature of the compact object unknown.

Despite its classification as a HMXB, the binary period in Cyg X-3 is thus extremely short, implying a very small orbital separation ( 5R ). The period has been found to increase on a timescale of 850 000 yr [15], with mass loss from a massive companion as the most favoured explanation [16]. The 4.8 hour modulation was first observed in soft X-rays [3] where the pulse shape is quasi-sinusoidal [17] and asymmetric with a slow rise and a faster decline. In hard X-rays [18], the modulation is present with a comparable strength but with a more symmetric pulse shape.


[link to news.discovery.com]

[link to images.nrao.edu]

[link to astrons.sabanciuniv.edu]

[link to www.dailygalaxy.com]

[link to www.andrewcollins.com]
 
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