Clarification of Answer by
livioflores-ga
on
29 Aug 2004 22:23 PDT
Hi monroe22!!
Ok, you feel that my answer is not good enough, I can accept that. But
I will use this feature to try to give you a better answer about this
topic.
First of all my apologizes forthe error that you found in the
www.gustavus reference, but I am not a chemist (only a web researcher)
so I did not noted such mistake. Note that the answer did not use this
reference, I only post it as additional for further reading.
Now the new answer:
Despite my low level knowledgement, after research for this comment I
must disagree with the opinion that the presence of oxygen and water
in the Earth and the Universe (interstellar space) cannot be explained
by today sciencist.
Here is exposed my position about this:
Shortly after the Big Bang nuclear reaction produced almost Hydrogen
and Helium of the Universe, but almost none of the heavier elements.
Some regions of the young universe would have had slightly higher
densities than others. The gravitational attraction in those regions
have promoted the formation of galaxies and stars by collapsing their
extra matter, starting from about two billion years after the Big
Bang. Some of the early stars would have been more massive than our
Sun, with enough mass to burn the original hydrogen and helium, into
heavier elements, such as carbon, oxygen, and iron. This could have
taken only a few hundred million years. After that, some of the stars
would have exploded as supernovas, and scattered the heavy elements
back into space, to form the raw material for later generations of
stars.
After hydrogen fusion, stars heavier than eight times the mass of the
Sun can go on to convert helium into carbon and oxygen, followed by
the formation of magnesium and silicon and ultimately iron.
"A star the size of the Sun will burn hydrogen into helium until the
hydrogen in the core is exhausted. At this point, the core of the star
contracts and heats up until the fusion of three He nuclei into C can
begin. Stars in this stage of evolution are known as red giants. Low
mass stars such as our Sun will then evolve into a compact object
called a white dwarf. All nuclear reactions in a white dwarf have
stopped. Higher mass stars have internal temperatures (10^8ēK) that
allow the fusion of carbon with helium to produce oxygen nuclei and
energy. For very massive stars, the exothermic fusion of low-mass
nuclei into successively more massive nuclei can proceed all the way
up to nuclei in the iron region."
From "Origin of the Elements":
http://www.lbl.gov/abc/wallchart/teachersguide/pdf/Chap10.pdf
Elements heavier than iron are formed during the explosion of a
supernova: When a large star's has consumed all its "atomic fuel"
finally collapses, then explodes and propells almost its matter into
space and also produces neutrons. This neutrons collide with the
elements from the star, building heavier elements, which are also
propelled into space by the force of the explosion.
The elements formed by nucleosynthesis in the red giant and during the
supernova become part of the interstellar dust.
Our Solar System was formed from one of this clouds of intestellar
dust about 4.6 billion years ago. This cloud had almost all the
elements that we find today in our solar system including oxygen.
"A region of the interstellar dust became progressively denser due to
gravitational attraction between the particles. Ultimately, it became
dense enough so that collisions produced larger and larger and larger
bodies (planetesimals) and ultimately, the sun and planets.
Once the formation of larger bodies commenced, the solar system formed
rapidly, probably within a few million years.
In our solar system, about 99% of the mass of the nebula went into the
sun. The sun's composition is therefore very close to that of the
original nebula, mostly hydrogen and helium.
When the sun ignited (became dense enough so that fusion of hydrogen
to helium began), it released intense radiation (solar wind) that
swept most of the volatile, or gaseous, elements out of the inner
solar system.
The "lost" elements included most of the hydrogen and helium, plus
much of the carbon and oxygen. H, He, C, O.
The elements remaining to form the Earth were mainly oxygen (bound to
metals), silicon, iron, aluminum, calcium, magnesium, sodium, and
potassium. These make up most of the rocks on the Earth today. O, Si,
Fe, Al, Ca, Mg, Na, K."
From "MSL111: Notes: The Origin of the Oceans"
http://www.sfos.uaf.edu/msl111/notes/origin.html
Note that you have interstellar clouds with hydrogen and oxygen, water
is formed in this interstellar medium.
"Cosmically, water is not uniformally abundant, its incorporation into
Earth-sized planets not necessarily constant, nor is its planetary
manifestation as aquatic habitats suitable for life a given. The
search for life in the universe must account for these variations and
the uncertainties that
accompany them. Water is formed in the interstellar medium and in the
denser molecular clouds that give rise to star-forming regions.
Differences in elemental abundance, gas-phase chemistry, and grain
chemistry will result in measurable variation in the abundance of
water in those regions. Water is a significant source of infrared
opacity in collapsing cloud cores and protostellar disks; the
efficiency at which the collapsing gas cools may control the stability
against gravitational fragmentation and the formation of binary or
multiple systems (including brown dwarf companions). The abundance of
water in protoplanetary disks is a sensitive function of the oxidation
state of the nebula and, to first order, the elemental ratio of carbon
to oxygen: the C/O ratio has been observed to vary significantly from
star to star, implying that there may be very ?wet? as well as ?dry?
planetary systems. Furthermore, the cosmochemical record in meteorites
shows that a large range in oxidation states and water abundance
existed in the early Solar System, perhaps as a result of removal of
water from the warm interior of the primordial nebula and its
condensation at greater distances. Presumably, planets formed from
different mixing ratios of this primitive material would be endowed
with different initial inventories of water. The total planetary
inventory of water may also depend on the presence of giant planets
and the efficiency of its dynamical transport as icy bodies from the
outer regions of a planetary system."
From "Water and Life in the Universe" from Institute for Astronomy at
University of Hawaii:
I suggest you to read this document.
http://www.ifa.hawaii.edu/UHNAI/Intro.pdf
Additional references:
(If one of them has a mistake, please forgive for that, thank you)
"Origin and Chemical Evolution of the Elements"
http://origins.colorado.edu/uvconf/white_final/node5.html
"Origin and Chemical Evolution of the Elements - Figure 7: Central
regions of the oxygen-rich supernova remnant"
http://origins.colorado.edu/uvconf/white_final/node5.html#N132D
"Water in the Universe"
http://www.farmweb.au.com/h2o/h2universe.html
"Water in the Solar System"
http://www.farmweb.au.com/h2o/h2solar.html
"Life in the Universe" at Professor Stephen W. Hawking's web pages:
http://www.hawking.org.uk/lectures/life.html
"The Atmosphere (& Hydrosphere)" by Dr. Rick Behl:
http://seis.natsci.csulb.edu/rbehl/300i-L06.htm
"Volcanic Gases and the Origin of the Atmosphere":
http://volcano.und.edu/vwdocs/Gases/origin.html
-------------------------------------------------------
I hope that this helps in clarify this answer.
Best regards.
livioflores-ga