HOW DID THE PLANETS FORM?
By Edward Hujsak
( What follows seems obvious, but there
are theories and theories, all supported by their own sets of
conjectures.)
A common theory about the moon,
generally accepted, is that it was scarfed out of Earth when a huge
asteroid passed close by. Another theory is that it was somehow
handed off from Venus. But evidence to the contrary is in plain
sight. Mars, Jupiter, Saturn, Uranus, Neptune.....all have multiple
moons....as many as sixty-seven in orbits around Jupiter.
What is uncontested is that the
planets' beginnings were in the form of gas blobs. Uncontested
because the outer planets, Jupiter, Saturn, Uranus and Neptune still
exist in that state. It is likely, from observation of other planets,
that surrounding the gas blobs were lots of rocks which were
gradually drawn into the gaseous spheres through loss of momentum
caused by collisions, and gravity, ending up as solid planets with a
surrounding atmosphere.Some of the rocks were too big to be drawn in.
Our moon is one of them.
How the planets evolved after that is
apparently dependent on the strength of their gravitational fields.
Mercury, for example was too small to hold on to its atmosphere.
Closest to the sun, it was simply blown away by solar pressure.
Venus, next closest to the sun, with a gravity like Earth's, has an
atmosphere rich in carbon dioxide, a greenhouse gas, and its nearness
to the sun resulted in runaway global warming.... a window into a
possible fate for Earth if carbon dioxide concentration reaches a
tipping point. We do not have any idea what that tipping point is.
Earth, occupying an orbit averaging
about ninety-four million miles from the sun, had a strong carbon
dioxide component component. When it cooled, plant life became
possible, out of which the atmosphere acquired a strong oxygen
component. That, in turn, made animal life possible.
Mars, unfortunately, with a gravity
only thirty-eight percent that of Earth, suffered the same fate as
Mercury. Its atmosphere was blown away. Some life may have formed
there, and possibly still exists in underground caverns but so far no
evidence has been uncovered. A visitor to Mars might survive in a
deep cavern. But had better like to eat mushrooms, as they would
likely thrive in a damp. warm enclosure.
The outer gas planets will
probably never reach a state like Earth- a large body of merged rock
with a surrounding thin atmosphere, though they have all accumulated
some rocks, as shown by evidence of solid cores. Also, the gas blobs
are just too big. There simply aren't enough rocks. Saturn, maybe,
if collisions cause enough loss of momentum to cause the ring
matter to be drawn in. But Saturn is pretty far out. Solar pressure,
the only known significant disturbing influence is small at Saturn's
distance from the sun.
In any case, none of the giant gas
planets could support life as we know it.
Planet forming – a big show- and
right before our eyes! Slow, though. A lifetime is too short to see
any action.
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