Category: Oort cloud

Solar System Status Update

May 23, 2016 / / 0 Comments

The Oort cloud, which extends a few light years beyond the outer Solar System, is full of motherships of the Galactic Confederation, a large gathering of representatives of hundreds of thousands of positive races from throughout the Galaxy:https://en.w...

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The Ganymede Portal

April 19, 2015 / / 0 Comments


The Ganymede Portal on the largest moon of Jupiter is the most important location in our Solar System.

It is the strongest energetic pathway in our Solar system which leads to the Galactic Central Sun. Sirius is a midway station between the Galactic Center and the Ganymede Portal, stepping down the vibrational frequency of the Central Sun energy to the degree that our Sol system can absorb.
There is a huge Galactic Confederation underground base on Ganymede which is a central hub for all intelligent positive races working upon the liberation of our Solar system and planet Earth especially.
That base is the main stronghold of the Jupiter Command and they are operating the portal towards the Galactic Center.
The base is located near the center of the Gallileo Regio:
The Ganymede Portal is the main beacon of Light for this Solar System including our planet. Without that portal being open, humanity would not survive the Archon invasion in 1996 and would be now extinct. Exopolitical events have much more influence on geopolitical situation than most people realize. The Archons have cleverly labeled everyone with more that a passing interest in cosmos as a »lunatic« to ensure that people would not detect the real source of the problems we have on Earth.
You can read two excellent summaries of the exopolitical background of the planetary situation here:

You can also connect energetically in your meditations with the Ganymede Portal, as it is the strongest source of spiritual Light in our Solar System:



As the next phase of MOSS will be activated in May, the activity of the Ganymede Portal will increase dramatically. This portal will also be the main transmitter of energies from the Galactic Central Sun at the Event.
After the Event, members of the Cabal who do not choose or are not able to accept the Light, will be processed through a sorting facility, which is located in one section of the Ganymede underground base. Many of those Cabal members will be then taken to the Galactic Central Sun for restructuring. 
The Ganymede portal is purifying the plasma accretion vortex strings (tunnels of Set) that extend from planet Earth beyond our Solar System into the Local Bubble:
While at the same time our Solar System is entering a sector of the Galaxy that will trigger more drastic changes and much sooner than scientists are willing to admit:
Scientific evidence is mounting about unusual activity in the Oort cloud. Astronomers are detecting radio signals which are coming from the Spheres since their arrival in 2001:
Powerful people with much potential positive influence upon the exopolitical and geopolitical situation are reading this blog. For this and also for other reasons I would ask people with deep intel about secret space programs to contact me at cobraresistance@gmail.com for possible future cooperation. 

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Birth of the Nibiru Legend? Astronomers Say Alien Star System Buzzed Our Sun

February 19, 2015 / / 0 Comments

Scholz's star - shown in this artist's impression - is currently 20 light-years away. But it once came much closerExcerpt from bbc.comAn alien star passed through our Solar System just 70,000 years ago, astronomers have discovered.  No othe...

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Was this Star Nibiru? Scientists Discover Star Made Closest Approach to Our Solar System 70,000 Years Ago

February 17, 2015 / / 0 Comments


Astronomers identify the closest known flyby of a star to our solar system Photo Credit: Flickr


Excerpt from americanlivewire.com

A low-mass red dwarf star passed through the outer Oort Cloud 70,000 years back in the closest approach made by any star into our system, discovers a team of researchers from various countries.

Lying in the constellation Monoceros and known as Scholtz’s star, it is a part of a binary system and has 8% the mass of the sun. Its companion, a brown dwarf, is said to have 6%.
The lowest end of the stellar spectrum, brown dwarfs are larger than gas giants but not as much so as to sustain hydrogen fusion for a larger period of time.

Due to its faint appearance, Scholtz’s star was discovered only a year ago by astronomer Ralf Dieter-Scholz in Potsdam, Germany, through the use of NASA’s WISE (Wide Field Infrared Survey Explorer), which mapped the entire sky in infrared during the years 2010 and 2011.

At the same time, the radial velocity of the star depicted that it was moving away from the solar system much faster than expected.
These motions led the researchers to conclude that either the star is headed toward our system, or moving away from it.

After analyzing the data, Mamajek concluded, “…The radial velocity measurements were consistent with it running away from the Sun’s vicinity–and we realized it must have had a close flyby in the past.”

Through the use of computer models, it was seen that the star passed about 5 trillion miles from our solar system around 70,000 years ago.

Mamajek and his team are 98 percent certain Scholtz’s star traveled through the outer Oort Cloud.

Although Scholtz’s star is 10th magnitude, too dim to be seen with the naked eye, it is magnetically active, which can cause it to flare at times and become significantly brighter. If this happened during its close approach to our solar system, prehistoric humans might have actually seen it.

The researchers published their findings in Astrophysical Journal Letters.

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Rosetta readies for its close rendezvous with a comet ~ Video

October 27, 2014 / / 0 Comments






sciencenews.org

Very soon, on November 12, a spacecraft called Rosetta will sidle up to a comet, steady itself and drop a 100-kilogram robotic lander toward the hunk of rock, dust and ice. The lander, named Philae, will drift through space, tugged only slightly by the gravity of the comet, commonly called 67P. Mission scientists will be holding their breath for what could be several anxiety-filled hours to see if Philae lands where and how it’s supposed to.

The exercise — the first attempt to set a lander on a comet — is as nerve-racking as landing on Mars or the moon, with some added challenges. Comets and other small space rocks have much less gravity than planets or moons, which is why it will take Philae close to seven hours to float to comet 67P’s surface. Then there’s the comet’s speed: Rosetta will drop the lander toward 67P as the comet shoots through the solar system at 55,000 kilometers per hour.

Add to that a comet's unpredictable nature: At any moment and without warning, 67P might spew out jets of gas and dust. Such eruptions could blow the spacecraft off course or skew the lander’s trajectory so it hits a boulder or misses its mark.

Early in the mission, scientists estimated that Philae had a 70 to 75 percent chance of successfully touching down on the comet, officially known as 67P/Churyumov-Gerasimenko. They made that prediction when they thought the comet was shaped like a potato. In July, Rosetta began sending pictures of 67P, indicating it looks more like a rubber duck — two masses connected by a thin neck. The new shape adds a bit more uncertainty to Philae sticking its landing.


The potential payoff of this mission is worth the hazards and the nail-biting, says Matt Taylor, Rosetta’s project scientist at the European Space Agency’s Science and Technology Center in Noordwijk, the Netherlands. Comets, along with asteroids, are thought to be the oldest, most pristine relics of the early solar system. We can’t go back billions of years to the birth of the sun, Taylor says, so exploring comets and asteroids may be the best option for learning how the solar system evolved. Studying their geology and chemistry could give clues to how the planets became what they are today and whether comets brought water and other ingredients for life to Earth.

Cometary close-up

Rosetta’s rendezvous with the comet, which is currently traveling between the orbits of Mars and Jupiter, has been a long time coming. The mission was first conceived in the late 1970s. By late 2002, when ESA was preparing to finally launch Rosetta, disaster struck. As part of a separate mission, the same type of rocket that was set to carry Rosetta exploded three minutes after liftoff. That rocket failure delayed Rosetta’s launch, closing the window to the original target of the mission, 46P/Wirtanen. Over the next few months, scientists scrambled to find another comet that would be at the right place in the solar system at the right time. 67P fit the bill.

Rosetta finally launched in 2004. Ten years later, on August 6, the spacecraft began orbiting 67P, and its 11 instruments started scrutinizing myriad characteristics of the comet (SN: 9/6/14, p. 8). Those instruments, plus the cameras and sensors on the Philae lander, are designed to map 67P, determine what it’s made of and observe how its chemistry might change as it swings around the sun.
As 67P approaches the sun, its ice transforms directly to water vapor and other gases, which, along with dust, shoot outward. These jets collide with other particles from the sun to form two tails. Unlike Halley’s comet and its showy run in 1986, 67P’s tails won’t be visible to the naked eye. But Rosetta will have a front-row seat on the action. As the comet’s tails grow, Rosetta will give scientists their most detailed look at a comet and the changes it goes through.

Already, Rosetta’s high-resolution photos have shown scientists that 67P looks different than other comets explored with spacecraft. It may even be two comets merged together with a surface that’s a mountain climber’s dream.

“The team really hit the jackpot with this comet,” says Donald Brownlee, a planetary scientist at the University of Washington in Seattle. Seeing a duck-shaped comet with house-sized boulders, craggy craters and 150-meter-high cliffs “really knocks your socks off,” he says. The bath-toy shape and rugged surface indicate that the comet has had an interesting life history, one scientists are eager to learn about. But first, they’ve got to get their instruments down to the comet’s surface.

“This very particular shape of the comet doesn’t make it easy to land,” Philae project manager Stephan Ulamec of the German Aerospace Center in Cologne said at a September 15 news conference. But the team has confirmed that it will attempt to set the lander down in November on a sliver of flat land on 67P’s small lobe, or head. The spot is flanked by cliffs, crevices and a few boulders.

It is also covered in carbon-rich dust, according to Rosetta’s measurements, which makes mission scientists extremely happy with the site, says lead lander scientist Jean-Pierre Bibring of the Université Paris-Sud in Orsay, France. The lander, he explains, can immediately start testing the comet’s surface and drill deeper to look for traces of ice and complex carbon-based compounds, which are among the major requirements for life.

Ice and certain complex carbon compounds are also some of the characteristics thought to distinguish comets from asteroids, the other early inhabitants of the solar system.

Rethinking space rocks


Distinctions blur Comets and asteroids seem to be different at first glance. But more detailed descriptions from space missions such as Rosetta suggest that the two types of space rocks may have more in common than scientists initially thought.
Source: NASA

“At first glance, comets are fundamentally different from asteroids, the way ice cream is different from a cookie,” says NASA scientist Claudia Alexander, based at the Jet Propulsion Laboratory in Pasadena, Calif. Most asteroids appear to be made of rocky materials and no water. Comets, however, seem to be icier. These distinctions are thought to explain where comets and asteroids originated as the solar system formed.Scientists think that around 4.6 billion years ago, the solar system started to form as a giant cloud of gas and dust collapsed inward and coalesced. Most of the material got pulled into the center of the cloud to form the sun. The rest condensed into a handful of huge rocks that became planets plus smaller bodies that became comets and asteroids.

In that scenario, asteroids probably formed between Mars and Jupiter, where it was too hot for water and other ices to survive. Comets, on the other hand, probably condensed farther out in this embryonic cloud where it was considerably cooler and ice could persist and start to attach to clumps of gas and dust.

If comets formed far out in the Kuiper belt or Oort cloud, where there was a lot more ice, they could have ferried a lot more water to Earth than did asteroids from the inner solar system.

“That’s the conventional wisdom,” says Alexander, a leader of the U.S. arm of Rosetta. NASA contributed electronics and three instruments to the mission; at least one of these instruments will look at 67P’s water.

Rosetta and Philae will give scientists a chance to virtually “get their hands on” the comet’s ice, says Alexander. That could help them figure out pretty quickly whether comets like 67P brought water to Earth billions of years ago.

The first question: What type of water is on 67P? If it is the same H2O that makes up Earth’s oceans, then perhaps 67P and similar comets brought that water to Earth. But if 67P, like most comets studied so far, contains a larger amount of the heavy hydrogen isotope called deuterium than does water found on Earth, then the idea that comets brought most of the water here is less likely.

That opens the door for the paradoxical idea that asteroids were the main source of our planet’s water. Scientists have recently found at least one asteroid with water. For example, the asteroid Ceres (actually large enough to be considered a dwarf planet) orbits the sun on a path between Mars and Jupiter, but it spouts off water vapor, sort of like a comet.

To confuse matters further, Rosetta’s observations indicate that 67P has characteristics of an asteroid. The comet, for example, isn’t covered in surface ice. Instead, its water appears to be stored deeper within its core.

These observations hint that comets and asteroids aren’t as radically different as scientists had thought. Instead, they may fall on a continuum with rocky, dry asteroids on one end, really icy comets on the other and everything else in between, Alexander says.

Getting warmer

When a comet gets close to the sun, a lot of its ice turns to vapor, and dust comes shooting out of its core. The comets with shorter orbits around the sun — 67P takes a brief 6.5 years — could eventually lose all of their ice and vapor leaving only rock and dust. Of course, scientists can’t really understand the long-term fate of 67P and other comets until they figure out the chemistry of what happens as a comet swings close to the sun on its elliptical orbit.
“We have theories about what happens to a comet as it gets closer and then moves away from the sun, but we do not understand how a comet really works,” says retired ESA scientist Gerhard Schwehm, one of the original leaders of the Rosetta mission.

That’s because scientists have never been able to stay with one for very long. All the previous comet missions have been flybys, lasting a few hours. If Philae sticks its November landing, it could work on the surface of 67P until March 2015, when the sun’s heat will become too hot for the lander to function. Rosetta will stay with 67P through August, when the comet reaches its closest point to the sun at a distance of 185 million kilometers. But Rosetta won’t give up there. It will continue orbiting the comet until at least December 2015.

A MOUNTAIN OF A COMET 67P is average in size when it comes to icy space rocks. Compared with human-made structures, however, it’s a behemoth, miniaturizing several iconic world wonders and rivaling the height of many of Earth’s famous mountains.
Source: ESA Credit: NAVCAM/Rosetta/ESA, adapted by M. Atarod

Spending a year or more with 67P will give scientists a chance to track how the sun’s heat changes the comet’s composition over time. To do this, Philae will first identify the elements and compounds that make up the comet’s surface. These materials may have survived unchanged for billions of years and could give scientists clues to what materials were available when the solar system started to form.Scientists are most interested in molecules containing carbon and hydrogen (SN: 11/1/14, p. 7), which could have existed even before the birth of the solar system. Investigators are also looking for amino acids and other building blocks of life that may have been brought to Earth by comets. Past missions have found both kinds of materials on comets before (see sidebar above, “Comets visited by spacecraft”). If they exist on 67P, they could add more evidence for scientists’ ideas that comets delivered the ingredients for life to Earth.

However, because scientists have never studied a comet while it faces the sun’s intense heat, they cannot be sure if these molecules are primordial or if they formed later, after being cooked by the sun. There are hints to support both origin stories. Rosetta’s observations could tell scientists if some of the molecules they see on the comet predate the solar system, or if they are created in reactions from the sun’s heat.

The comet’s chemistry could also have implications for places far beyond Earth, says Edward Young, a geochemist at the University of California, Los Angeles. “Establishing the link between these primitive building blocks of planets and our own planet will go a long way toward helping us understand whether rocky planets with at least as much water as Earth are the norm, or not,” he says.
That’s a lofty goal, one that hinges on a spectacular landing and the final 14 months of Rosetta’s 10-year voyage.




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NASA captures high-resolution images of comet Sliding Spring

October 23, 2014 / / 0 Comments


 Diagrams show how comet will approach Mars.


The Mars Reconnaissance Orbiter captures images of Comet C/2013 A1, also known as Sliding Spring after the observatory which discovered it, as it flies past Mars on October 19th. The comet originated in the Oort Cloud, which is located in the distant reaches of our solar system.

These images were taken by the Orbiter’s High Resolution Imaging Science Experiment (HiRISE) camera while the comet flew approximately 86,000 miles from Mars at a speed of 35,700 miles per hour (57,400 km/h) relative to the planet.
Greg Giles



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Comet Siding Spring Soars Past Mars

October 19, 2014 / / 0 Comments

Astrophotographer Damian Peach captures Siding Spring (green smudge at lower-centre) on approach to Mars (saturated star-like object)bbc.comA recently discovered comet has whizzed past Mars, giving scientists a unique chance to study an object from...

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NASA prepares its science fleet for Mars comet encounter ~ Video

October 10, 2014 / / 0 Comments


NASA assets to observe Comet Siding Spring


Excerpt from
astronomy.com

Comet Siding Spring will pass within about 87,000 miles (139,500 kilometers) of the Red Planet on October 19.


NASA’s extensive fleet of science assets, particularly those orbiting and roving Mars, have front-row seats to image and study a once-in-a-lifetime comet flyby Sunday, October 19.

Comet C/2013 A1, also known as Comet Siding Spring, will pass within about 87,000 miles (139,500 kilometers) of the Red Planet — less than half the distance between Earth and our Moon and less than one-tenth the distance of any known comet flyby of Earth.

Siding Spring’s nucleus will come closest to Mars around 2:27 p.m. EDT, hurtling at about 126,000 mph (56 kilometers per second). This proximity will provide an unprecedented opportunity for researchers to gather data on both the comet and its effect on the martian atmosphere.

Siding Spring came from the Oort Cloud, a spherical region of space surrounding our Sun and occupying space at a distance between 5,000 and 100,000 astronomical units (1 AU is the average Earth-Sun distance). It is a giant swarm of icy objects believed to be material left over from the formation of the solar system.

Siding Spring will be the first comet from the Oort Cloud to be studied up close by spacecraft, giving scientists an invaluable opportunity to learn more about the materials, including water and carbon compounds, that existed during the formation of the solar system 4.6 billion years ago.

Some of the best and most revealing images and science data will come from assets orbiting and roving the surface of Mars. In preparation for the comet flyby, NASA maneuvered its Mars Odyssey orbiter, Mars Reconnaissance Orbiter, and the newest member of the Mars fleet, Mars Atmosphere and Volatile EvolutioN (MAVEN), in order to reduce the risk of impact with high-velocity dust particles coming off the comet.

In addition, Earth-based and space telescopes, including NASA’s iconic Hubble Space Telescope, will be in position to observe the unique celestial object. The agency’s astrophysics space observatories — Kepler, Swift, Spitzer, Chandra — and the ground-based Infrared Telescope Facility on Mauna Kea, Hawaii —will be tracking the event.

NASA’s asteroid hunter, the Near-Earth Object Wide-field Infrared Survey Explorer, has been imaging and will continue to image the comet as part of its operations. And the agency’s two Heliophysics spacecraft, Solar Terrestrial Relations Observatory and Solar and Heliophysics Observatory, will image the comet. The agency’s Balloon Observation Platform for Planetary Science, a suborbital balloon-carried telescope, already has provided observations of the comet in the lead-up to the close encounter with Mars.



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Pleiadian Portal Activation Report

May 21, 2014 / / 0 Comments


Pleiadian Portal activation was successful. Confederation motherships have positioned themselves inside the Oort cloud. Many of them (mostly from the Pleiadian fleet) are now already within our solar system to prepare for the final liberation of the planet.
The Resistance is now assuming a more active role inside the solar system. Beyond their main stronghold on planet X, they are building many active bases in outer solar system.
Pluto's moon Charon, which was once a military warehouse for the dark forces, is now one of the main military command centers of the Resistance for the final defeat of the Chimera group.
Many female members of the Resistance are living on some objects in outer solar system and using them as relay stations of the Goddess energy from the Galactic Central Sun towards planet Earth. 
The main relay station inside our solar system for the Goddess energy from the Galactic center is a centaur asteroid Chariklo. Many female members of the Pleiadian fleet and the Resistance Movement are located there, meditating and channeling Goddess energy from the Galactic center and sending it towards Earth to assist in harmonizing humanity. Rings have been discovered around Chariklo just a few months ago:



Those rings serve as a stargate which relays Goddess energy into our solar system.
The main stronghold of female Lightwarriors of the Resistance Movement under wise leadership of a woman with a codename Ariel is on Eris, a small planetary body on the edge of the Solar system:
Ganymede, the largest of Jupiter's moons, is the location of the main communications hub for this solar system which includes teams from the Galactic Confederation, the Ashtar Command, Pleiadian, Sirian and Andromedan fleet and also the Resistance Movement. 
Many new bases of the Light forces will be established in the inner solar system in the very near future, especially on asteroids, Mars and the Moon. 
On the surface of our planet, the energy of the Pleiadian portal was relayed through many individuals and groups that were meditating. The main anchor was our group in Switzerland, which was very dedicated and strong. The Light was bright and the skies were clear. One participant of the conference has shared this photo of Confederation extraterrestrial craft that was taken in Mount Shasta some time ago:






Around the time of the Pleiadian Portal activation, the QEG group in Morocco has achieved overunity in their free energy prototype development, according to some sources:
The energies of the Pleiadian Portal activation have irritated the Archons to organize a new wave of attacks on my work through misinformed and manipulated »truthers« on the surface of this planet. To get a better perspective on my work, you can read this excellent article:
I have suggestion for all the Lightworkers and Lightwarriors. Instead of attacking each other, you can direct your energy into something like this:
Victory of the Light!

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