EARTH EXTINCTIONS
According to David Rupp
and Jack Septowski of the University of Chicago, every 27-million years Earth
has undergoes a major extinction. There have been at least six major
extinctions in the past and several minor ones in between. The Permian
extinction wiped out 98% of all life right down to most bacteria. It is my
contention that evolution cannot account for the 30-million or so plants and
animals we now have. Obviously someone is reseeding planets between extinctions
to keep life going and hopefully some more intelligent species capable of being
self-aware.
Your chances of being
killed are six times more likely in a fiery plane crash than from a falling
asteroid or meteor. We must point out that only one person has ever been hurt
by a falling meteorite. Sixty-two years ago Ann Hodge was bruised on the thigh
by a meteorite that smashed through her ceiling in Alabama.
All that changed February
15, 2013, when 1,491 people were injured by flying glass from the 400-kiloton
blast of an air-bursting meteorite over Chelyabinsk, Russia. The explosion’s
power was difficult to measure by a factor of two but it least equaled the
power of 13 Hiroshima bombs.
Its been 66-miollion
years since a global cataclysm like the famous Yucatan meteorite that killed
off the dinosaurs and paved the way for mammalian, rat-like creatures that
mainstream says evolved into mankind. Purported space threats include incoming
comets, reversals of Earth’s poles and solstice alignments with the galaxy’s
center that could supposedly beam some new king of energy toward earth. Also
don’t forget the alleged mythical planet Nibiru on a collision course toward
Earth that astronomers know about but are keeping it secret.
Then you have the
impending threat of Andromeda colliding with the Milky Way. Galaxies generally
pass one another at twenty galaxy widths. Galaxy collisions are common but rather
harmless as stars are generally separated by 1 million star widths. Stars
colliding with other stars are extremely rare even when galaxies merge.
Rearranging and disruption of life on the nearby planets may be common place.
We don’t know. The real danger would be from gravitational interference causing
coronal mass ejections that singe the surface of planets.
In 1859 British
Researcher Richard Carrington watched as enormous flares doubled the Sun’s
brightness. High speed particle matter blasts arrived one day later causing a
global aurora so brilliant that people thought dawn had arrived. The
electro-magnetic pulse cause high voltage to pass through telegraph lines
knocking some operators’ unconscious. If such an event occurred today internet
and Global position satellites would be knocked off air permanently and
electric power would be disrupted for months causing millions of people to die
of starvation and exposure. All farm machinery would be destroyed. Basically we
would be forced back into the Stone Age hunting with stick and rocks again.
My research writing
COSMOLOGICAL ICE AGES revealed there are at three other major threats to Earth.
Little Sirius B, the size of Earth is only eight light years distant and it is
very close to the critical mass of 1.47 solar masses where it could go neutron.
According to brilliant astronomer Subrahmanyan Chandrasekhar, whose
specialty was white dwarf stars, ‘when they reach 1.47 solar masses they can
turn into a neutron star wiping out solar systems within a radius of 60 light
years.’ The Chandrasekhar limit (/tʃʌndrəˈʃeɪkər/)
is the maximum mass of a stable white dwarf star.
The limit was first
indicated in papers published by Wilhelm Anderson and E. C. Stoner,
and was named after Subrahmanyan Chandrasekhar, the Indian astrophysicist who independently
discovered and improved upon the accuracy of the calculation in 1930, at the
age of 19, in India. This limit was initially ignored by
the community of scientists because such a limit would logically require the
existence of black holes, which
were considered a scientific impossibility at the time. White dwarfs resist gravitational
collapse primarily through electron
degeneracy pressure. (By comparison, main sequence stars resist collapse
through thermal pressure.) The
Chandrasekhar limit is the mass above which electron degeneracy pressure in the
star's core is insufficient to balance the star's own gravitational
self-attraction.
Consequently, white
dwarfs with masses greater than the limit would be subject to further
gravitational collapse, evolving into a different type of stellar remnant, such as a neutron star or black hole. (However, white dwarfs
generally avoid this fate by exploding before they undergo
collapse.) Those with masses under the limit remain stable as white dwarfs If
this event happened eight years ago we may be all dead in the next second.
Then you have the giant
800-solar mass Betelgeuse twelve thousand light years distant in the
constellation Orion. When it collapsed into a neutron star the radiation burst
could definitely affect life here on Earth. It may have already collapsed
twelve-thousand years ago. We have no way of knowing. One minute you would be
going about your daily life; the next everything would be a cinder.
Instead of fighting endless wars on Earth to reduce the population maybe we should be seeding life on other planets.
