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Did NASA Accidentally “Nuke” Jupiter? |
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On September 21, 2003 NASA deliberately directed its amazing, still-functioning Galileo spacecraft to make
one final, 108,000 mph suicidal plunge into Jupiter’s vast atmosphere.
Thus ended the incredibly successful eight-year unmanned NASA Galileo
mission … which had returned against all odds an array of phenomenal new
information on Jupiter and its “mini-solar system of moons” … in a literal,
most fitting “blaze of glory.”
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| · | September 21st: Galileo enters Jupiter’s atmosphere at over 30 miles per second. It is traveling almost in the plane of Jupiter’s equator, at an angle of about 22 degrees to the horizontal (below). |
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| · | As the more fragile parts of the spacecraft disintegrate from the enormous entry temperatures and pressures, its two 4-ft long, 124-lb RTGs – each containing 72 individual plutonium-238 capsules – separate from the main spacecraft. |
| · | Soon, the relatively fragile aluminum housing of the two RTG canisters also melts away, releasing the 144 individually sealed plutonium-238 capsules … to continue plunging deeper into Jupiter’s atmosphere on their own. |
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Because of their high-temperature, multi-layer containment – each capsule is clad in iridium (melting temperature 4435 F), encasing a floating boran-graphite membrane (melting temperature 6422° F) , in which the plutonium-238 pellets are individually sealed -- most of the plutonium capsules are NOT destroyed by Galielo’s violent entry, but in fact survive … and slow to an aerodynamic fall in the thickening Jovian atmosphere. |
The multiple layerings of iridium and graphite have acted like individual heat shields [similar to the much larger (and heavier) Galileo Probe -- which successfully entered Jupiter’s atmosphere December 7, 1995]. After slowing to sub-sonic speeds, the shielded capsules would have free-fallen through Jupiter’s increasingly dense atmosphere ... until the outside pressures inevitably caused them to implode. The key question then became: how long would it take each free-falling iridium/graphite capsule to reach “crush depth” – the depth where the outside pressures are tens of thousands of atmospheres, ~600 miles below the clouds? The depth where those pressures would cause the plutonium-238 capsules to undergo a sudden phase transition, to literally implode … initiating a violent nuclear reaction?
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The rate of a free-falling object in a planetary atmosphere is governed by an elementary equation, known as “Stokes law.”
V = (2gr²)(d1-d2)/9µ
where
V = velocity of fall (cm sec-¹),
g = acceleration of gravity (cm sec-²),
r = "equivalent" radius of particle (cm),
dl = density of particle (g cm -³),
d2 = density of medium (g cm-³), and
µ = viscosity of medium (dyne sec cm-²).
What this translates to is this:
For a given atmospheric density, an object of a given mass and surface area, under a given gravitational acceleration, will fall at a given rate. Denser objects (less surface area for their given weight) fall faster than lighter ones (this is due to simple air resistance, and NOT any non-Newtonian aspects of the laws of gravitation!). If the atmospheric density increases as an object falls to greater depths, the rate of free-fall is slowed in direct proportion to the increasing density. To a first order, increasing atmospheric pressure is approximately proportional to increasing atmospheric density, and thus a decreasing rate of free-fall.
In other words, the higher the outside gas pressure on Jupiter… the slower Galileo’s capsules would fall.
For a 6-foot, 200-lb human in Earth’s gravity, surrounded by its one bar atmospheric pressure, the final rate of fall is approximately 120 miles per hour – called its “terminal velocity.” On Jupiter, with a cloud-top gravity about 2.4 times Earth’s, and an upper atmospheric pressure less than a tenth of Earth’s, the initial rate of free-fall for an object with a similar mass-to-surface area (like Galileo’s RTGs) would be about 3000 mph. But, by the time the RTGs had disintegrated and released their 144 plutonium individual capsules, the atmospheric density/pressure would have risen to several times the Earth’s, and the surface area to weight ratio of the smaller plutonium capsules (1.5-inch by 1-inch cylinders) is MUCH greater than for the RTGs themselves. This would cut their free-fall velocity by a corresponding amount … to around 150 mph at this altitude.
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| · | As the capsules continue to fall deeper through the primarily hydrogen
atmosphere, the surrounding pressure/density continues to rise, to
thousands of times Earth’s surface density and pressure. The capsules
are now falling at a constant rate, approximately one mile per
hour …as the atmosphere transitions to an incompressible fluid,
liquid hydrogen (below). |
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| · | At this ultra-slow “terminal velocity,” it takes the
Galileo plutonium-238 capsules on the order of 700 hours – a month!
to fall to a depth inside Jupiter (~700 miles below the visible clouds)
where the outside pressure of the surrounding liquid hydrogen literally
crushes the plutonium capsules into a supercritical state— |
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At this point, one of the capsules randomly implodes … and initiates, via the resulting shockwave and intense neutron shower, a runaway nuclear chain reaction in all the other surviving capsules, now spread in a spherical falling “cloud” a few tens of miles across ~700 miles below Jupiter’s visible “surface.” The resulting cascade nuclear detonation of all the surviving capsules totals several tens of kilotons …. |
A single month ….
The simultaneous detonation of over 40 lbs of plutonium-238, over 700 miles below Jupiter’s cloud tops, instantly creates a superheated “bubble” of “million-degree plasma” deep inside Jupiter, tens miles across. Initially, this bubble has an expansion pressure of over fifty million atmospheres per square inch. Because the outside Jovian “mantle” pressure is approximately ten thousand atmospheres at this depth, the plasma sphere rapidly expands … to a diameter over fifty times as great ... until the inside and outside pressures equalize. Because of the extreme low density inside this super-heated sphere, and the higher Jovian gravity (2.4 times “Earth normal), the buoyancy forces are immense. The “bubble” immediately begins to ascend toward the visible surface, 600 miles above -- rising at an extraordinary rate of several hundred miles per hour …. [In the “Ivy Mike” 1952 nuclear test in the Pacific (above), the fireball rose to a height of 57,000 feet in only 90 seconds – which translates to a velocity of over 400 miles per hour! In the much higher pressure Jovian environment, the ascent rate of such a high-temperature, low density plasma bubble could well be ~1000 miles per hour, before slowing drastically as the “bubble” nears the top of the visible (lower density) atmosphere ….]
At this rate of ascent, the bubble (also constantly expanding, as the surrounding atmospheric pressure lessens – until it is several thousand miles across) breaks the “surface” of the Jovian atmosphere within an hour or two of detonation. The horizontal shear inside Jupiter’s atmosphere has also moved it north, away from the plane of Galileo’s entry, until it is trapped by the streaming atmospheric eddies that form the North Equatorial Belt (below) -- where it emerges as a visible phenomenon.
The intense temperatures of this nuclear plasma upwelling immediately dissociate the surrounding neutral molecular “contaminants” of Jupiter’s high altitude troposphere and stratosphere – water, ammonia and methane are instantly broken down into their component atoms. It is here that the unique “signature chemistry” which has revealed this incredible scenario takes place ….
The carbon released from the dissociation of millions of tons of CH4 (methane) and other carbon-rich molecules floating at the highest levels in the vast Jovian hydrogen/helium atmosphere as “minor” constituents, with no significant reservoir of free oxygen available to turn it into C02 (carbon dioxide), when it cools condenses into countless micron-sized pure carbon particles – “lamb black” … soot! Such particles, even though their total numbers are relatively trivial on the scale of Jupiter’s atmosphere, are extremely effective at absorbing visible wavelengths of light all across the spectrum ….
It is this unique, dark “carbon” signature – appearing as a dark black “splotch” in the highest levels of the Jovian cloud belts (below) -- which has given this entire, incredible scenario away ….
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Critics, of course, will raise all kinds of objections to this bizarre scenario. Many we have raised ourselves – like the low probability of Galileo’s plutonium even surviving entry – at 108,000 miles per hour! – to reach the necessary “crush depth” for implosion.
A far more serious objection is that the nuclear fuel Galileo carried – plutonium-238 – while ideal as a sustained heat source for making electricity via thermoelectric technology, is NOT traditionally viewed as a fissionable material appropriate for creating nuclear explosions. The plutonium isotope vastly preferred for the original “Fat Man” weapon was plutonium-239 – which, by not emitting an excess of neutrons prior to achieving supercriticality, allowed the construction of an actual implosion plutonium weapon.
However, a little-known US nuclear weapons test, carried out underground at the Atomic Energy Commission’s Nevada test site (now operated by the Department of Energy), demonstrated in 1962 that “reactor-grade” plutonium – a mix of isotopes, including plutonium-238 – could be successfully imploded. Because of the extended Galileo mission, and the pre-production of the plutonium-238 fuel capsules before its launch (coupled with their unique design – which incorporated a layering of neutron-emitting uranium-234 into their construction), long-term creation of significant quantities of highly fissionable plutonium-239 across the fifteen years since the mission was launched cannot be ruled out of the eventual Galileo plutonium ceramics … by the time they were deliberately plunged into Jupiter.
So, did any of this really happen?
The deliberate destruction of Galileo to “save” Europa, and the sudden appearance of “a mysterious dark splotch” on Jupiter just one month later -- precisely time enough to get the entering plutonium down to a depth where it could catastrophically implode – is truly a remarkable “coincidence.” Admittedly, this is strictly a case of circumstantial evidence: radioactive debris can’t be analyzed in Jupiter’s atmosphere remotely; no one has demonstrated that plutonium-238 can make a “bomb” under Jovian conditions; and there are major questions regarding the capsules even having sufficient mass for a runaway nuclear reaction, that is, if they survived entry … let alone falling intact to a depth sufficient to implode.
But, television is replete these days with highly publicized legal cases where a defendant is tried -- for murder, no less – based on strictly circumstantial evidence alone … like, a single strand of hair. The case for “something extraordinary” happening to Jupiter -- with NASA inadvertently behind it -- is based on a chain of far more solid evidence at this point.
And then, there is the troubling absence of key evidence ….
One of the lingering mysteries surrounding the sudden appearance of Meecker’s “new dark splotch” has been the seeming total non-curiosity exemplified by the professional astronomical community.
In 1994, a new “white spot” suddenly appeared in the clouds just north of Saturn’s equator. Within days, professional astronomers world wide were imaging the new disturbance with an eye toward understanding its origin and evolution – culminating in a stunning time lapse movie acquired by the Hubble Space Telescope itself (see frame, below).
Where are any of the scores of professional astronomical images – including those from HST – which should be flooding the Internet over this discovery, documenting the “enigmatic new phenomenon” that just appeared on Jupiter?!
High quality, early observations of remarkable astronomical events are standard operating procedure, especially in the case of planetary atmospheric phenomena – which can rapidly change, or even disappear entirely if early observations aren’t secured in the first few days. Yet, by all accounts, for this new phenomenon on Jupiter, all observations have been left totally to the amateur community ….
Huh?!
Is it possible that the professional “insiders,” those at the major observatories (which get most of their funding from NASA anway) -- including NASA’s own Space Telescope Institute -- know perfectly well how this atmospheric spot arrived on Jupiter … and have been quietly told not to “immortalize” another monumental miscalculation by NASA … particularly, at this politically sensitive time?
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Finally, if you discount all these ideas as simply “too far out,” there is one final scenario which neatly fits the evidence currently at hand … conceived many years ago in “2010:Odyssey Two” … from the fertile imagination of my old friend, Arthur Clarke.
For those fans of Arthur who love a good “conspiracy” -- especially if it involves our favorite space agency (anyone we know ..?) -- these observers may now discern the completion of a long-term, hidden goal in this enigmatic Jovian data … here.
In any case, stay tuned ….