Extra Solar Planets
|
The discovery of extra solar planets revolving around distant stars has been a great achievement for mankind and his quest to unlock the secrets of the universe. Their appearance has opened up the possibility of life existing outside of our own solar system among the many stars. On the other hand the extra solar planets with their documented approximations of mass, orbital speed, and distances from host stars have exposed the many flaws in present day astrophysics and how astronomers predicted the formation of planets. |
![]() |
Several
Jupiter sized planets have been found revolving in close proximity of stars at
various rates of orbital speed. One example would be the recently discovered
planet orbiting the sun-like G class star HD 38529 located approximately 138
light years from Earth. The planet’s mass orbital period and distance from the
host star respectively is a minimum of .77 of Jupiter’s mass, an orbital
period of 14.31 Earth days, and an average distance from the star is .129 AU
(Astronomical Units) or 12 million miles. But how can this planetary stellar
discovery hold up, if the foundation of planetary formation established in the
circles of elite astrophysicists dictates, that any mass similar to Jupiter has
to be a hydrogen based gas planet. Planetary formation according to present
accepted theories would have cosmic objects similar in mass and size of the gas
planets Jupiter, Saturn, Uranus, and Neptune coalescing on the outer edges of a
contracting gaseous disk of a proto solar system where solid hydrogen
precipitates around a cold rocky mass. What force would be the cause of a planet
in an outer orbit to move to an interior position? The answer would be the
strongest gravitational present in the local area or the host star. Any star
capable of changing an orbit of a planet by gravitational attraction, would also
capture it and assimilate it on impact with the solar mass. An outside
gravitational force upon a planet’s capture cannot alter motion, once directed
towards a stellar object. The result of this encounter is assimilation by the
solar mass after impact. An orbital path is maintained by other factors still
unknown to astrophysics. A repulsion force builds between the planet and the
star. The point where the repulsion force, an outward force emanating from the
star, equalizes the force of gravity, which draws the planet in that an orbit is
established. The planet’s angle of approach and velocity determines the
ellipse of the orbit. The speed of the planets’ orbit is maintained by the
angular momentum of the repulsion particles at the point of intersection of the
planet’s orbital distance from the star. Then there is the obvious, planetary
absorption of solar heat upon approach. How long would solid or liquid hydrogen
gas based planet last in an orbit that would be similar to 1/3 the distance from
our Sun to our planet Mercury? The result would be hydrogen and other light
gases boiling off the surface of the planet exposing the heavy elements of what
was the core of the planet. Many scientists will hide behind the fact that the
gravity emanating from the object would hold hydrogen even in its gaseous form.
They overlooked the obvious, a rocky core surrounded by gaseous hydrogen heated
to extremes would not be part of the planetary mass only its core would be
responsible for gravitational force, which could not provide a containment
force. A high rate of orbital speed coupled with the gravitational pull of the
solar object, would rip away the hydrogen atmosphere in a close orbit. The
pressure differentials would cause surface materials to evaporate and escape
into the low-pressure environment of outer space. There would be a steady
erosion of planetary mass. In essence, there could not be a planetary mass
fitting the parameters established by Earth’s science to explain what mankind
has discovered. Leaving a planetary mass similar to a terrestrial planet, which
according to mankind’s theory of the formation of planets does not exist in a
mass similar to a gas planet. It is time to reexamine the theory pertaining to
the formation of planetary masses within a solar system.
All Rights Reserved: © Copyright 2000