Although by means of spectral analysis and was recently opened in sun the atmosphere of platinum, yet it seems obvious that it is strongly dominated by metals small fractional weights. If we consider the previous conclusions are correct, then you can accept the likelihood that those initial connections through which formed elements with heavy particles, until recently, impossible large size, will occur later and as a result the density of the Sun will become extremely high compared to what it is now. I say "until now, impossible in the large size" because it is quite probably the assumption that such elements can be formed and can continue to exist in the parts of the solar mass, where the pressure is hard enough, but where the heat is not too large. And if so, hence the conclusion that the inner core of the Sun, having a higher temperature than its surface layers may be composed exclusively of metals are low atomic weight, and that this may partly be the reason of its low specific weight, furthermore, it is possible to conclude that, when over time the internal the temperature drops, can be formed elements, consisting of heavy particles, as their existence it is possible and education each object is accompanied by the development of heat {Last thoughts was added by me at the time when this book has been published I prompted by the reading of some notes Professor duara embodying outline of the lectures given them in the Royal Institute during the session of 1880 Examining the conditions under which could have formed the "our so-called elements if they consist of elementary matter", Professor Duhart, speaking on the basis of the known properties of complex substances, coming to the conclusion that in each case in education participated pressure, temperature and the nature of the surrounding gases.}. If this is true, some of it apparently it follows that the quantity of heat which must be allocated from the Sun, and the duration of the period during which it will be this selection of heat, must be much greater than if we assume that the Sun constantly will consist of prevailing in it now items and that it able to achieve just that degree of density which it permits such composition.
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Although by means of spectral analysis and was recently opened in sun
the atmosphere of platinum, yet it seems obvious that it is strongly dominated by
metals small fractional weights. If we consider the previous conclusions are correct, then
you can accept the likelihood that those initial connections through which
formed elements with heavy particles, until recently, impossible
large size, will occur later and as a result the density of the Sun
will become extremely high compared to what it is now. I say
"until now, impossible in the large size" because it is quite
probably the assumption that such elements can be formed and can
continue to exist in the parts of the solar mass, where
the pressure is hard enough, but where the heat is not too large. And if so,
hence the conclusion that the inner core of the Sun, having a higher temperature
than its surface layers may be composed exclusively of metals are low
atomic weight, and that this may partly be the reason of its low specific
weight, furthermore, it is possible to conclude that, when over time the internal
the temperature drops, can be formed elements, consisting of heavy
particles, as their existence it is possible and
education each object is accompanied by the development of heat {Last
thoughts was added by me at the time when this book has been published I
prompted by the reading of some notes Professor duara embodying
outline of the lectures given them in the Royal Institute during the session of 1880
Examining the conditions under which could have formed the "our so-called
elements if they consist of elementary matter", Professor Duhart, speaking on
the basis of the known properties of complex substances, coming to the conclusion that in
each case in education participated pressure, temperature and
the nature of the surrounding gases.}. If this is true, some of it apparently
it follows that the quantity of heat which must be allocated from the Sun, and
the duration of the period during which it will be this selection
of heat, must be much greater than if we assume that the Sun
constantly will consist of prevailing in it now items and that it
able to achieve just that degree of density which it permits such
composition.
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