Nibiru, Sirius and the Sun, are deemed to be stars. They are relatively unknown, these have a polar plane. As does Earth it has a magnetic plane rises or falls to this galactic medium and this fluctuates. One has to ponder a thought to some of these new findings. Find the ancient structures point to this, so does the importance of which the alignment of these structures thus formed for example the pyramids. This seems to have been a world wide project of such significance by there importance and being built with only one reason. As this points towards the Earths magnetic flip.
It seems to have been a project to control Earth's energetic resonance via the use of directional wavelengths. This is done true their tip to align energy. Maybe this was to stabilise the moons orbit aligning it to the Earth's Core? It was later said they were built as a high priest alter of worship for mummification. So as to get their plan correct, these were to become a world wide network of pyramids extending the globe to focal points. With Bosnian as many other locations in reach thus concluded. Some just put this age of pyramid building down, to be an enclosure for learning. Where the organisation of labour took place, like the internet today and this may make for a fantastic computer game. If this was done so the outer edge to the sun polar flip wouldn't flux, as it approached near the suns equatorial top and bottom axis. This would be a huge project that wouldn't be repeated? If it's all this is speculation, even the carvings claim that there are 10 planets with one exo planet depicted having an orbit of 39 light years, Then Earth may be the final planet in its quest for survival in our system, as it becomes the contest for zombie domination, as gravity vectors conclude and onto our reduced cranium? Here is a big forget, that some apes show more intellect, under gravitational G force than us as a species. Such is this to human civilisation, as it becomes quite a large constraint also.
MRI have shown no offence a decline in human cognitive activity due to inactivity. Earth last humanoid might not be so far into the distance future, that been said what animal will dominate the Earth. As a planet. As Venus and Mars are now out of the way this does leave the? Here is example of all the detections that have been made since the nineteenth century. Some of the earliest involve the binary star 70 Ophiuchi.
In 1855 Capt. W. S. Jacob at the East India Company's Madras Observatory reported that orbital anomalies made it "highly probable" that there was a "planetary body" in this system. In the 1890s, Thomas J. J. See of the University of Chicago and the United States Naval Observatory stated that the orbital anomalies proved the existence of a dark body in the 70 Ophiuchi system with a 36-year period around one of the stars. However, Forest Ray Moulton published a paper proving that a three-body system with those orbital parameters would be highly unstable. During the 1950s and 1960s, Peter van de Kamp of Swarthmore College made another prominent series of detection claims, this time for planets orbiting Barnard's Star. Now astronomers now generally regard all the early reports of detection as erroneous not to be considered.
It seems to have been a project to control Earth's energetic resonance via the use of directional wavelengths. This is done true their tip to align energy. Maybe this was to stabilise the moons orbit aligning it to the Earth's Core? It was later said they were built as a high priest alter of worship for mummification. So as to get their plan correct, these were to become a world wide network of pyramids extending the globe to focal points. With Bosnian as many other locations in reach thus concluded. Some just put this age of pyramid building down, to be an enclosure for learning. Where the organisation of labour took place, like the internet today and this may make for a fantastic computer game. If this was done so the outer edge to the sun polar flip wouldn't flux, as it approached near the suns equatorial top and bottom axis. This would be a huge project that wouldn't be repeated? If it's all this is speculation, even the carvings claim that there are 10 planets with one exo planet depicted having an orbit of 39 light years, Then Earth may be the final planet in its quest for survival in our system, as it becomes the contest for zombie domination, as gravity vectors conclude and onto our reduced cranium? Here is a big forget, that some apes show more intellect, under gravitational G force than us as a species. Such is this to human civilisation, as it becomes quite a large constraint also.
MRI have shown no offence a decline in human cognitive activity due to inactivity. Earth last humanoid might not be so far into the distance future, that been said what animal will dominate the Earth. As a planet. As Venus and Mars are now out of the way this does leave the? Here is example of all the detections that have been made since the nineteenth century. Some of the earliest involve the binary star 70 Ophiuchi.
In 1855 Capt. W. S. Jacob at the East India Company's Madras Observatory reported that orbital anomalies made it "highly probable" that there was a "planetary body" in this system. In the 1890s, Thomas J. J. See of the University of Chicago and the United States Naval Observatory stated that the orbital anomalies proved the existence of a dark body in the 70 Ophiuchi system with a 36-year period around one of the stars. However, Forest Ray Moulton published a paper proving that a three-body system with those orbital parameters would be highly unstable. During the 1950s and 1960s, Peter van de Kamp of Swarthmore College made another prominent series of detection claims, this time for planets orbiting Barnard's Star. Now astronomers now generally regard all the early reports of detection as erroneous not to be considered.
In 1991 Andrew Lyne, M. Bailes and S. L. Shemar claimed to
have discovered a pulsar planet in orbit around PSR 1829-10, using pulsar
timing variations.
The claim briefly received intense attention, but Lyne and
his team soon retracted it. Confirmed discoveries. These discoveries of exoplanets. See also the list of
exoplanet firsts. The three known planets of the star HR8799, as imaged by the
Hale Telescope. The light from the central star was blanked out by a vector
vortex coronagraph. 2MASS J044144 is a brown dwarf with a companion about 5–10
times the mass of Jupiter. It is not clear whether this companion object is a
sub-brown dwarf or a planet. Coronagraphic image of AB Pictoris showing a
companion (bottom left), which is either a brown dwarf or a massive planet. The
data was obtained on 16 March 2003 with NACO on the VLT, using a 1.4 arcsec
occulting mask on top of AB Pictoris.
As of 1 November 2015, a total of 1977 confirmed exoplanets
are listed in the Extrasolar Planets Encyclopaedia, including a few that were
confirmations of controversial claims from the late 1980s. The first published
discovery to receive subsequent confirmation was made in 1988 by the Canadian
astronomers Bruce Campbell, G. A. H. Walker, and Stephenson Yang of the
University of Victoria and the University of British Columbia. Although
they were cautious about claiming a planetary detection, their radial-velocity
observations suggested that a planet orbits the star Gamma Cephei. Partly
because the observations were at the very limits of instrumental capabilities
at the time, astronomers remained sceptical for several years about this and
other similar observations. It was thought some of the apparent planets might
instead have been brown dwarfs, objects intermediate in mass between planets
and stars. In 1990 additional observations were published that supported the
existence of the planet orbiting Gamma Cephei, but subsequent work in 1992
again raised serious doubts. Finally, in 2003, improved techniques allowed the
planet's existence to be confirmed. On 9 January 1992, radio astronomers
Aleksander Wolszczan and Dale Frail announced the discovery of two planets
orbiting the pulsar PSR 1257+12.
The claim briefly received intense attention, but Lyne and
his team soon retracted it. Confirmed discoveries. These discoveries of exoplanets. See also the list of
exoplanet firsts. The three known planets of the star HR8799, as imaged by the
Hale Telescope. The light from the central star was blanked out by a vector
vortex coronagraph. 2MASS J044144 is a brown dwarf with a companion about 5–10
times the mass of Jupiter. It is not clear whether this companion object is a
sub-brown dwarf or a planet. Coronagraphic image of AB Pictoris showing a
companion (bottom left), which is either a brown dwarf or a massive planet. The
data was obtained on 16 March 2003 with NACO on the VLT, using a 1.4 arcsec
occulting mask on top of AB Pictoris.
As of 1 November 2015, a total of 1977 confirmed exoplanets
are listed in the Extrasolar Planets Encyclopaedia, including a few that were
confirmations of controversial claims from the late 1980s. The first published
discovery to receive subsequent confirmation was made in 1988 by the Canadian
astronomers Bruce Campbell, G. A. H. Walker, and Stephenson Yang of the
University of Victoria and the University of British Columbia. Although
they were cautious about claiming a planetary detection, their radial-velocity
observations suggested that a planet orbits the star Gamma Cephei. Partly
because the observations were at the very limits of instrumental capabilities
at the time, astronomers remained sceptical for several years about this and
other similar observations. It was thought some of the apparent planets might
instead have been brown dwarfs, objects intermediate in mass between planets
and stars. In 1990 additional observations were published that supported the
existence of the planet orbiting Gamma Cephei, but subsequent work in 1992
again raised serious doubts. Finally, in 2003, improved techniques allowed the
planet's existence to be confirmed. On 9 January 1992, radio astronomers
Aleksander Wolszczan and Dale Frail announced the discovery of two planets
orbiting the pulsar PSR 1257+12. 
This discovery was confirmed and is generally considered to
be the first definitive detection of exoplanets.
Follow-up observations
solidified these results and confirmation of a third planet in 1994 revived
the topic in the popular press. These pulsar planets are believed to have
formed from the unusual remnants of the supernova that produced the pulsar, in
a second round of planet formation, or else to be the remaining rocky cores of
gas giants that somehow survived the supernova and then decayed into their
current orbits.On 6 October 1995, Michel Mayor and Didier Queloz of the
University of Geneva announced the first definitive detection of an exoplanet
orbiting a main-sequence star, namely the nearby G-type star 51 Pegasi.
This
discovery, made at the Observatoire de Haute-Provence, ushered in the modern
era of exoplanetary discovery. Technological advances, most notably in
high-resolution spectroscopy, led to the rapid detection of many new
exoplanets: astronomers could detect exoplanets indirectly by measuring their
gravitational influence on the motion of their host stars. More extrasolar
planets were later detected by observing the variation in a star's apparent
luminosity as an orbiting planet passed in front of it. Initially, most known exoplanets were massive planets that
orbited very close to their parent stars.
Follow-up observations
solidified these results and confirmation of a third planet in 1994 revived
the topic in the popular press. These pulsar planets are believed to have
formed from the unusual remnants of the supernova that produced the pulsar, in
a second round of planet formation, or else to be the remaining rocky cores of
gas giants that somehow survived the supernova and then decayed into their
current orbits.On 6 October 1995, Michel Mayor and Didier Queloz of the
University of Geneva announced the first definitive detection of an exoplanet
orbiting a main-sequence star, namely the nearby G-type star 51 Pegasi.
This
discovery, made at the Observatoire de Haute-Provence, ushered in the modern
era of exoplanetary discovery. Technological advances, most notably in
high-resolution spectroscopy, led to the rapid detection of many new
exoplanets: astronomers could detect exoplanets indirectly by measuring their
gravitational influence on the motion of their host stars. More extrasolar
planets were later detected by observing the variation in a star's apparent
luminosity as an orbiting planet passed in front of it. Initially, most known exoplanets were massive planets that
orbited very close to their parent stars. 
But
eventually more planets of other sorts were found, and it is now clear that hot
Jupiters are a minority of exoplanets. In 1999, Upsilon Andromedae became the
first main-sequence star known to have multiple planets. Kepler-16
contains the first discovered planet that orbits around a binary main-sequence
star system. On 26 February 2014, NASA announced the discovery of 715
newly verified exoplanets around 305 stars by the Kepler Space Telescope. These
exoplanets were checked using a statistical technique called "verification
by multiplicity".
Prior to these results, most confirmed
planets were gas giants comparable in size to Jupiter or larger as they are
more easily detected, but the Kepler planets are mostly between the size of
Neptune and the size of Earth.On 23 July 2015, NASA announced Kepler-452b, a
near-Earth-size planet orbiting the habitable zone of a G2-type star. Candidate
discoveries. As of March 2014, NASA's
Kepler mission had identified more than 2,900 planetary candidates, several of
them being nearly Earth-sized and located in the habitable zone, some around
Sun-like stars. Kepler mission – new exoplanet candidates – as the answers still remains as elusive as the Earth's core.
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