On Jan 30, 4:15 pm, Chris L Peterson <
c...@alumni.caltech.edu> wrote:
> On Mon, 30 Jan 2012 15:42:29 -0800 (PST), Brad Guth
>
One more time: (not that you'll ever change your closed mindset)
There you go again, being so perfectly negative and unable to prove
that anyone else is even half as smart as yourself, in that you might
as well stop pretending and just be the intellectual black hole (aka
Sheldon Cooper) that you are.
Obviously you still can't do the volumetric displacement math on
behalf of that 2500 km crater, much less adding up all those other
sufficiently big ones that should almost double that volume of lose
material. So, where the hell did all that enormous volume of lose
basalt shards go, if not extensively towards Earth?
Remember, that within just a few cm depth, those NASA/Apollo guys
struck fused bedrock, as in they couldn't seem to force those probes
deeper for any further penetration (nothing the least bit lose under
their magic clumping moon dirt that was so nicely monochromatic,
highly reflective and not hardly the least bit paramagnetic or much
less anticathode or otherwise metallicity worthy). It’s almost as
though they’d mistakenly landed on a certain isolated private guano
island, that badly needed a spendy UN ticket to fly (that’s an inside
little sarcastic joke that’s actually not meant to be funny).
So, do tell us what sort of inert fluff-ball smacked into our moon and
made that 2500 km crater, which apparently gave off or ejected hardly
any shards (at least most of which didn't seem to stick with the
moon).
-
Each month the atmosphere of Earth deflects and/or vaporizes a fairly
large number of meteors and smallish asteroids (roughly 100 per day),
not to mention fending off the hundred tonnes of smaller stuff per
day, that which our naked moon doesn’t have the same built-in or
automatic defensive option. There’s well over a hundred fireballs
spotted per day, and that obviously doesn’t include the other
thousands per day that go unnoticed.
http://www.astronomycafe.net/qadir/q896.html
“In a recent article in the journal Nature, March 28, 1996 vol. 380,
page 323, Dr.s A.D. Taylor, W. J. Baggaley and D. I. Street at the
University of Adelaide in Australia discuss the results of their 1
year radar monitoring of incoming meteors. When meteorites slam into
the atmosphere, they produce ionization in the atmosphere. Radar echos
from this momentary ionization allow the velocity, altitude and
distance to be determined if you have two or more such installations
for triangulation. The AMOR radar in New Zealand was used for a year
in this fashion to detect 350,000 faint echos from very small
meteorites with sizes between 10 - 100 microns. This works out to
nearly 1000 every day, just from this site alone! Over 1508 of these
meteorites ( 0.9 percent) were found to be traveling at speeds up to
several hundred kilometers per second!”
“On any given day, the estimates are than the Earth intercepts about
19,000 meteorites weighing over 3.5 ounces, every year of which fewer
than 10 are ever recovered. About 2800 meteorites are in museums from
previous 'falls' and are chemically found to represent about 20 or so
distinct parent-bodies. The Earth acquires about 100 tons per day of
dust-sized micro-meteoroids.”
So, it's quite a wonder how all of these billions of years that our
physically naked and dark moon has been missing out on collecting its
fair share of dust, as well as having been avoiding its share of all
those further significant impacts.
Let us suggest that the moon only attracts or runs itself into a
highly conservative 10 tonnes per day as of the last billion years.
That’s only 3.65e12 tonnes of dust, not to mention averaging another
ten fold that much for each billion years before that, nor having
mentioned those bigger than dust meteorites of 0.1+ kg, plus that
otherwise absolutely monstrous 2500 km crater plus having to account
for roughly that much lose crater debris again from all those other
big craters combined, is hardly suggesting our moon isn’t pulverized
with many meters depth of dust and lose shards.
My crude conservative math has 4.055e15 tonnes of that 10~100 micron
dust accumulated within 4 billion years, and that’s not even including
those 0.1+ kg meteors as impactors, or much less worthy of whatever
generated those enormous craters. That’s a lot of lose influx when
there’s only 3.8e13 m2 of surface area to work with (roughly 106.7
tonnes/m2), most of which seems to be missing in action, because it
sure as hell didn’t get washed down into muds that compacted into
rock.
The notion that Earth doesn’t have those trillions of tonnes worth of
lunar basalt is kind of silly, that is unless you and your friends can
manage to tell us where else it went (because the vast bulk of it is
apparently not found on the moon). How about you do your own math
without being artificially conservative like myself, telling us how
many 10~100 micron plus larger hits per m2 does our naked moon get to
deal with per day.
Also while you’re at it. We’d like to know how that naked moon
manages to avoid being just as nasty as those Van Allen belts, and why
has it been such a good source of gamma if it supposedly doesn’t have
hardly any surface metallicity to work with.
The average solar wind as is, blows a 900,000 km trail of heated and
ionized sodium away from our moon. But how much nearby solar wind
density and velocity does it take in order to blow or extract those
typically heavier particles of dust off the naked surface of our moon?
(perhaps a recently nearby planet creation did the trick, unless that
moon had otherwise bounced off Earth).