Hi Friends and Listees,

Just a few more comments on why this Schultz theory is refreshing IMO, as crazy as it initially sounded:

If this mechanism is a valid one for larger objects, it raises the following curiosities:

1. Why don't other stony meteorites with TKW's over a ton do the same thing. 2. How many fair comparisons do we have in recorded meteoritidum that are comparable, e.g. non-carbonaceous big falls which are slowed by the atmosphere. 3. If this is a valid posibility, are our thought about "destroying" killer asteroids by fragmenting them in even hotter water? e.g., what if 10% of the fragments, to pick any fraction for argument's sake, exhibit this behavior. We can't count on the atmosphere to be the guardian angel for all pieces! 4. What happens to the fragmented material at the front of the enveloped train of hurdling debris? Does it fragment and basically vaporize (get smoked) and in so doing, open up a path for what's behind? 5. And if some pieces at the front survive, the friction will slow them down - then BOOM collision with those behind - and could we have an cyclical relay team progression of renewal of momentum at the head of the train maintaining the overall velocity? 6. If this "rely team" mechanism is maintained by a long and massive particle stream behind, is this effect possible: The actual shear at the front is lowered substantially for the overall velocity, basically using a sacrificial leading edge as a re-entry heat shield.

Not agreeing with the mechanism - nor disagreeing, just brainstorming a bit. No doubt this was really smoking, does the energy disippated into making the smoke serve as a shield - amazing concept...

Best wishes and Great Health,
Doug



-----Original Message-----
From: [EMAIL PROTECTED]
To: [email protected]
Sent: Sat, 5 Apr 2008 10:26 am
Subject: Re: [meteorite-list] New, long, Carancas article II


Sterling W. wrote: 
 
"Both Schultz and I calculate that the object was still supersonic when it hit, still enclosed in a "detached" shock wave, so the sides never ablated at any point." 
 
Hi Sterling, 
 
Yes, but to Schultz's credit, he has put a novel mechanism on the table for scientific consideration of these "strange" dynamics and motivated the issue of the role of the shock wave IMO to begin with. The oriented case as presented by you and many others at that time was an extrapolation IMO. 
 
I personally like Schultz' refreshing contribution in the field. I would rather call your thoughts the natural control for Schultz' idea, and not anything particularly novel in meteoritical circles. While any idea will need to be earthshattering :-), which explanation (the basic made into a very special case or the spontaneous reorganization and its complexity - or csome combination of ideas) at this point best complies with Occam's Razor is not obvious to me. 
 
However, no matter how distorted in length vs. width, if we consider the object was over a ton, that is still a real lot of surface area to survive down to a relatively very thick atmosphere at 4 km above sea level at that speed. I don't think the shock wave could have powered any deflector shields at the front of the bus - but I'm not qualitfied at the moment to comment on that. The shear experienced by the material at the front had to be enormous in the last 5-10 kilometers. 
 
So this Schultz theory sounds good and a welcomed addition to consideration vs. the highly oriented case. 
 
Sterling - do you or does anyone know if the shock veins have been shown by the scientists to have been caused upon impact with Earth? 
 
Best wishes and Great Health, 
Doug 
 
 
-----Original Message----- 
From: Sterling K. Webb <[EMAIL PROTECTED]> 
To: [EMAIL PROTECTED]
Cc: [email protected]; [EMAIL PROTECTED]
Sent: Sat, 5 Apr 2008 1:23 am 
Subject: Re: [meteorite-list] New, long, Carancas article II 
 
 
Hi, 
 
  In this context "contained" means contained by the back 
pressure envelope of the shock wave. The meteoric material 
would be far enough away from the shock not be heated 
very much. The shock wave at the sides is the hot stuff 
from the front and it's cooling down rapidly. 
  Even in the entry of a spherical object the back side is 
not ablated. The melted rock on the back is running fluid 
from the front, not backside material that melted. And there's 
many a fine crusty meteorite whose back side is hardly touched 
by melt even though it's only a few inches away from the fire 
of re-entry. 
  The shock wave is the boundary between material moving 
faster than sound (traveling with the meteoroid) and material 
not moving faster than sound (the surrounding atmosphere). 
Check the Wikipedia entry (very good discussion): 
http://en.wikipedia.org/wiki/Shock_wave 
  "Shock waves are characterized by an abrupt, nearly 
discontinuous change in the characteristics of the medium. 
Across a shock there is always an extremely rapid rise in 
pressure, temperature and density of the flow." 
  In other words, just a little too close and you're dead 
meat! Just an inch away, you're OK. The faster an object 
goes, the more sharply bent back the shock wave is; as it 
slows, the shock wave stands out further away, until at 
the speed of sound it's at right angles to the direction of 
flight. As long as the sides of object are on the "right" side 
of the fiery shock wave, it's safe from being melted at least. 
It's like being the heat shadow. 
  Both Schultz and I calculate that the object was still 
supersonic when it hit, still enclosed in a "detached" 
shock wave, so the sides never ablated at any point. 
 
Sterling K. Webb 
------------------------------------------------------- 
----- Original Message ----- 
From: <[EMAIL PROTECTED]> 
To: "Sterling K. Webb" <[EMAIL PROTECTED]> 
Cc: <[email protected]>; <[EMAIL PROTECTED]> 
Sent: Saturday, April 05, 2008 12:44 AM 
Subject: Re: [meteorite-list] New, long, Carancas article II 
 
It would seem to me that if the stone fragmented in flight and was contained 
by the shock wave it would still be heated by the plasma and all the 
fragments would develop crusts. There appear to be some pieces with crust, 
but enought to match Schultz's theory? 
 
---- "Sterling K. Webb" <[EMAIL PROTECTED]> wrote: 
 
  Schultz and I both agree that a greater aerodynamic 
efficiency will get a chondrite to the ground faster with 
less loss of material, making an impact like Carancas 
possible. 
 
  What Schultz proposes is that the fragile material of 
Carancas fragmented early on but did not "pancake" out 
and cause an airburst, but was wrapped by the shock wave 
around the hypersonic meteoroid into a "bullet" shape 
that stayed together and kept its high speed to the ground. 
 
.... What I proposed was that the Carancas impactor was an 
elongated fragment to begin with. That is, it was a "sliver" of 
asteroid that was 4 or 5 times longer than its width when it 
entered the Earth's atmosphere. The results would be the 
same: a faster trip to the ground in (mostly) one piece. 
 
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