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Scientists Find That Earth and Mars are Different to the Core

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Scientists Find That Earth and Mars are Different to the Core baalke 06-28-2007
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Posted by Aidan Karley on July 17, 2007, 4:55 pm
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> The _most_ likely explanation is that he meteorites were not from mars
> in the fist place.
> We need real samples
>
While agreeing with you on the need for sample return missions,
the identification of certain meteorites as being form Mars is quite
secure. The process of impact spalling fragments off the surface also
melts small amounts of the rock on slip planes, fracture surfaces etc
(unsurprisingly), and the high pressures in the impact drives bubbles of
gas into this glass. Onec the rock fragment has wandered through space
for a few millennia it hits the Earth's atmosphere, the surface is
heated for a couple of seconds, then it crumps down into Antarctic snow
or an Egyptian dog (allegedly, for the Nakhla meteorite) and is
eventually found by a meteorite hunter. When the gas bubbles are
identified in microscope thin sections (well, "thick sections" ; about
0.1mm, polished but no cover slip) and zapped with an ion microprobe
beam, the gas composition can be measured ... and is found to have a
stable isotope composition matching that measured by the Viking landers,
not what we find on Earth.
If you're interested, I've got the papers detailing the process
somewhere.
Identification of Vesta-derived meteorites is a bit less secure,
based on the IR reflection spectrum of the fresh meteorite surfaces
matching that of Vesta. Once the plausibility of the process had been
established by the identification of the Martian meteorites, the
identification of other meteorites with Vesta had much less resistance.
Plus, there are a number of asteroids in related orbits to Vesta which
are interpreted as debris from a recent (last few million years) large
impact on Vesta.
The lunar-derived meteorites are uncommon, but securely
identified by correlation against Apollo samples.

--
Aidan Karley, FGS,
Aberdeen, Scotland
A light wave is more like a crime wave than a water wave.


Posted by Henry Spencer on July 17, 2007, 8:32 pm
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>...When the gas bubbles are identified
>in microscope thin sections ... and zapped with an ion microprobe
>beam, the gas composition can be measured ... and is found to have a
>stable isotope composition matching that measured by the Viking landers,
>not what we find on Earth.

Indeed, the match to Martian air is startlingly good. The meteorites with
the gas bubbles just have to have come from Mars; it would be much harder
to explain them originating anywhere else.

Only some of the Martian meteorites have such gas bubbles, but they are
all tied together into a family by things like odd mineralogies and
unusual oxygen-isotope ratios, so establishing that a few of them are from
Mars settles it fairly well for all of them. There is no longer any
reasonable doubt about this.

> If you're interested, I've got the papers detailing the process
>somewhere.

Try:

+ Bogard et al, "Noble gas contents of shergottites and implications
for the Martian origin of SNC meteorites", Geochim.Cosmochim.Acta
48:1723-1739, 1984.

+ Becker&Pepin, "The case for a Martian origin of the shergottites:
Nitrogen and noble gases in EETA 79001", Earth Planet Sci. Lett.
69:225-242, 1984.

+ Swindle et al, "Noble gases in SNC meteorites", Meteoritics 19:318-319,
1984.

+ Carr et al, "Martian atmospheric weathering products in SNC meteorites",
Nature 314:248-250, 1985.

> Identification of Vesta-derived meteorites is a bit less secure...
> The lunar-derived meteorites are uncommon, but securely
>identified by correlation against Apollo samples.

And there are one or two peculiar meteorites which perhaps might be from
Mercury, but we're unlikely to have confirmation of *that* for quite a
while, since we'd need (at the very least) surface analysis by a lander,
and none are planned.
--
spsystems.net is temporarily off the air; | Henry Spencer
mail to henry at zoo.utoronto.ca instead. | henry@spsystems.net

Posted by Aidan Karley on August 6, 2007, 8:27 pm
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> And there are one or two peculiar meteorites which perhaps might be from
> Mercury, but we're unlikely to have confirmation of *that* for quite a
> while, since we'd need (at the very least) surface analysis by a lander,
> and none are planned.
>
Be a bit harsher for them than for the Mars rovers. What is it -
something like 600 K towards noon? And a diurnal range of 400 K.
Severe.

--
Aidan Karley, FGS,
Aberdeen, Scotland
A light wave is more like a crime wave than a water wave.


Posted by Henry Spencer on August 8, 2007, 12:13 pm
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>> And there are one or two peculiar meteorites which perhaps might be from
>> Mercury, but we're unlikely to have confirmation of *that* for quite a
>> while, since we'd need (at the very least) surface analysis by a lander...
>>
> Be a bit harsher for them than for the Mars rovers. What is it -
>something like 600 K towards noon? And a diurnal range of 400 K.
> Severe.

Indeed, Mercury is a harsh environment even for *orbiters*, never mind
landers.

(If your orbit passes low over the sunlit side, *half the sky* is full of
oven-hot planet -- a far worse thermal problem than just having rather
brighter sunlight. This is why Mercury-orbiter designs tend to use quite
elliptical orbits: most science instruments would benefit from more time
down low, but the thermal environment is just horrible, and reasonable
spacecraft designs have to spend most of their time higher up so they can
cool off. An orbit over the terminator -- the day-night boundary -- would
be much better, although even there you'd probably want it to be somewhat
elliptical, but there's no way to *keep* an orbit over the terminator for
long without advanced propulsion. A solar sail actually would work very
nicely for this...)

On the surface, you can probably reduce both the peak temperature and the
temperature swing by landing near one of the poles... but things still get
pretty chilly at night.

ESA's BepiColombo mission originally included a small lander, but alas,
that got deleted to keep the budget under control.
--
spsystems.net is temporarily off the air; | Henry Spencer
mail to henry at zoo.utoronto.ca instead. | henry@spsystems.net

Posted by Jan Panteltje on July 18, 2007, 4:28 am
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On a sunny day (Tue, 17 Jul 2007 21:55:27 +0100) it happened Aidan Karley

>> The _most_ likely explanation is that he meteorites were not from mars
>> in the fist place.
>> We need real samples
>>
> While agreeing with you on the need for sample return missions,
>the identification of certain meteorites as being form Mars is quite
>secure. The process of impact spalling fragments off the surface also
>melts small amounts of the rock on slip planes, fracture surfaces etc
>(unsurprisingly), and the high pressures in the impact drives bubbles of
>gas into this glass. Onec the rock fragment has wandered through space
>for a few millennia it hits the Earth's atmosphere, the surface is
>heated for a couple of seconds, then it crumps down into Antarctic snow
>or an Egyptian dog (allegedly, for the Nakhla meteorite) and is
>eventually found by a meteorite hunter. When the gas bubbles are
>identified in microscope thin sections (well, "thick sections" ; about
>0.1mm, polished but no cover slip) and zapped with an ion microprobe
>beam, the gas composition can be measured ... and is found to have a
>stable isotope composition matching that measured by the Viking landers,
>not what we find on Earth.
> If you're interested, I've got the papers detailing the process
>somewhere.
> Identification of Vesta-derived meteorites is a bit less secure,
>based on the IR reflection spectrum of the fresh meteorite surfaces
>matching that of Vesta. Once the plausibility of the process had been
>established by the identification of the Martian meteorites, the
>identification of other meteorites with Vesta had much less resistance.
>Plus, there are a number of asteroids in related orbits to Vesta which
>are interpreted as debris from a recent (last few million years) large
>impact on Vesta.
> The lunar-derived meteorites are uncommon, but securely
>identified by correlation against Apollo samples.

Thank you, sounds reasonable.
I made that remark inspired by yet an other posting in the trend of:
'and now we have to rethink completely about how planets and comets...'
as seen often posted by NASA in sci.astro.
Although I agree then methods you describe are very accurate with
a low margin of error I would personally like to see some
astronauts digging on mars :-)
It seems our view of how planets are formed is still changing, and that
would have some consequences for making statements where things come from.
No mars is not geologically dead, there is a picture somewhere of a geyser
like feature.. although some claim it is a dust devil...
We really need to go there an look.

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