by harry » Sat Jun 03, 2006 6:20 am
Hello Orin
What is the evidence against the Big Bang?
http://www.bigbangneverhappened.org/p27.htm
Hydrogen formation,,,,,,,,,,this is just one process.
We may have to look at first the process involved in a supernova.
http://observe.arc.nasa.gov/nasa/space/ ... th_3a.html
As the mass of the star's iron core approaches 1.4 solar masses (due to continued silicon and sulfur burning in a thin shell adjacent to the iron core), a dramatic sequence of events is being triggered:
Iron Core Collapse
Gravity, which up to now was balanced by the outward force of the pressure, decisively gains the upper hand and the iron core collapses.
In less than a second, the core collapses from a size of about 5,000 miles to one of about a dozen miles, and an enormous amount of energy is released. This collapse happens so fast that the star's outer layers have no time to react and participate in it.
The amount of energy that is released during core collapse is truly gigantic -- it is equivalent to the energy produced by 100 stars like the Sun during their entire lifetimes of more than 10 billion years!
Most of the energy released during the collapse of the iron core is carried off into space by elusive particles called neutrinos. A small fraction of the energy is deposited in the lower layers of the envelope surrounding the core and triggers the supernova explosion.
http://observe.arc.nasa.gov/nasa/space/ ... acont.html
The energy deposited in the lower layers of the envelope creates a superstrong shock wave that runs outward through the envelope toward the star's surface.
As the shock wave runs outward, it heats the envelope, induces explosive nuclear burning, and ejects the envelope at speeds of thousands of miles per second (i.e., in excess of 10 million miles/hour).
It is during this phase that elements heavier than iron are being manufactured.
When the shock wave reaches the star's surface, it very quickly heats the surface layers and brightens them. Within a day or two the exploding star becomes brighter than a billion Suns.
The result of these events is a compact stellar remnant and a rapidly expanding gaseous shell.
The stellar remnant is a neutron star or a black hole.
The expanding gaseous shell plows into the surrounding interstellar medium, and pushes, compresses, and intermingles with it. Such regions of the interstellar medium are known as supernova remnants.
Lets look at our sun as an example.
http://web.umr.edu/~om/report_to_fcr/report_to_fcr1.htm
The Sun and its planetary system formed from heterogeneous debris1-11 of a supernova (SN) that exploded 5 billion years ago12,13. Meteorites and planets recorded this as decay products of short-lived nuclides and linked variations in elemental and isotopic abundances. Cores of the inner planets grew in the central iron-rich region of the SN debris, and the Sun formed on the collapsed SN core. See Figs. 1-5.
The Sun’s radiant energy and protons in the solar wind (SW) come from the collapsed supernova core, a neutron star (NS), on which the Sun formed. The cradle (Figs. 9-12) indicates that the energy of each neutron in the Sun’s central NS exceeds that of a free neutron by @ 10-22 MeV (Figs. 13-15) Solar luminosity and the flux of solar-wind protons are generated by a series of reactions (Fig. 16): a) escape of neutrons from the central NS, b) decay of free neutrons or their capture by other nuclides, c) fusion and upward migration of H+ through material that accreted on the NS, and d) escape of H+ in the SW. An example might be:
a) The escape of neutrons from the NS, <1n> –> 1n + 10-22 MeV
b) The decay of free neutrons, 1n –> 1H+ + e- + nanti + 0.78 MeV
c) Fusion of hydrogen, 4 1H+ + 2 e- –> 4He++ + 2 n + 26.73 MeV
d) Some H+ reaches the surface and departs in the solar wind
Reactions like a) and b) produce part of the Sun’s radiant energy and perhaps the luminosity of isolated neutron stars25. Note that reaction a) alone may release more energy per nucleon than is released by the sum of reactions b) and c), the decay or capture of neutrons plus H-fusion. The well-established Solar Neutrino Puzzle26 confirms that reaction c) generates only part of the Sun’s total luminosity. Most 1H+ from b) is consumed by H-fusion, but the anomalous abundance of H (See Fig. 8) shows that 1H+ also leaks from the interior, selectively carrying lighter nuclides to the solar surface (See Fig. 6) before departing in the solar wind at an emission rate of about 2.7 x 1043 1H/yr. Homochirality in living creatures26 was likely initiated by circularly polarized light (CPL) from the Sun’s early NS. Their fate and climate changes of planets27 may depend on the half-life of this massive nucleus at the Sun’s core.
We can always workout how hydrogen was formed and if the Big Bang did occur the hydrogen production would be on similar lines.
see
http://map.gsfc.nasa.gov/m_uni/uni_101bbtest2.htmlHello Orin
What is the evidence against the Big Bang?
http://www.bigbangneverhappened.org/p27.htm
Hydrogen formation,,,,,,,,,,this is just one process.
We may have to look at first the process involved in a supernova.
http://observe.arc.nasa.gov/nasa/space/stellardeath/stellardeath_3a.html
[quote]As the mass of the star's iron core approaches 1.4 solar masses (due to continued silicon and sulfur burning in a thin shell adjacent to the iron core), a dramatic sequence of events is being triggered:
Iron Core Collapse
Gravity, which up to now was balanced by the outward force of the pressure, decisively gains the upper hand and the iron core collapses.
In less than a second, the core collapses from a size of about 5,000 miles to one of about a dozen miles, and an enormous amount of energy is released. This collapse happens so fast that the star's outer layers have no time to react and participate in it.
The amount of energy that is released during core collapse is truly gigantic -- it is equivalent to the energy produced by 100 stars like the Sun during their entire lifetimes of more than 10 billion years!
Most of the energy released during the collapse of the iron core is carried off into space by elusive particles called neutrinos. A small fraction of the energy is deposited in the lower layers of the envelope surrounding the core and triggers the supernova explosion.[/quote]
http://observe.arc.nasa.gov/nasa/space/stellardeath/stellardeath_3acont.html
[quote]The energy deposited in the lower layers of the envelope creates a superstrong shock wave that runs outward through the envelope toward the star's surface.
As the shock wave runs outward, it heats the envelope, induces explosive nuclear burning, and ejects the envelope at speeds of thousands of miles per second (i.e., in excess of 10 million miles/hour).
It is during this phase that elements heavier than iron are being manufactured.
When the shock wave reaches the star's surface, it very quickly heats the surface layers and brightens them. Within a day or two the exploding star becomes brighter than a billion Suns.[/quote]
[quote]The result of these events is a compact stellar remnant and a rapidly expanding gaseous shell.
The stellar remnant is a neutron star or a black hole.
The expanding gaseous shell plows into the surrounding interstellar medium, and pushes, compresses, and intermingles with it. Such regions of the interstellar medium are known as supernova remnants.[/quote]
Lets look at our sun as an example.
http://web.umr.edu/~om/report_to_fcr/report_to_fcr1.htm
[quote]The Sun and its planetary system formed from heterogeneous debris1-11 of a supernova (SN) that exploded 5 billion years ago12,13. Meteorites and planets recorded this as decay products of short-lived nuclides and linked variations in elemental and isotopic abundances. Cores of the inner planets grew in the central iron-rich region of the SN debris, and the Sun formed on the collapsed SN core. See Figs. 1-5.[/quote]
[quote]The Sun’s radiant energy and protons in the solar wind (SW) come from the collapsed supernova core, a neutron star (NS), on which the Sun formed. The cradle (Figs. 9-12) indicates that the energy of each neutron in the Sun’s central NS exceeds that of a free neutron by @ 10-22 MeV (Figs. 13-15) Solar luminosity and the flux of solar-wind protons are generated by a series of reactions (Fig. 16): a) escape of neutrons from the central NS, b) decay of free neutrons or their capture by other nuclides, c) fusion and upward migration of H+ through material that accreted on the NS, and d) escape of H+ in the SW. An example might be:
a) The escape of neutrons from the NS, <1n> –> 1n + 10-22 MeV
b) The decay of free neutrons, 1n –> 1H+ + e- + nanti + 0.78 MeV
c) Fusion of hydrogen, 4 1H+ + 2 e- –> 4He++ + 2 n + 26.73 MeV
d) Some H+ reaches the surface and departs in the solar wind[/quote]
[quote]Reactions like a) and b) produce part of the Sun’s radiant energy and perhaps the luminosity of isolated neutron stars25. Note that reaction a) alone may release more energy per nucleon than is released by the sum of reactions b) and c), the decay or capture of neutrons plus H-fusion. The well-established Solar Neutrino Puzzle26 confirms that reaction c) generates only part of the Sun’s total luminosity. Most 1H+ from b) is consumed by H-fusion, but the anomalous abundance of H (See Fig. 8) shows that 1H+ also leaks from the interior, selectively carrying lighter nuclides to the solar surface (See Fig. 6) before departing in the solar wind at an emission rate of about 2.7 x 1043 1H/yr. Homochirality in living creatures26 was likely initiated by circularly polarized light (CPL) from the Sun’s early NS. Their fate and climate changes of planets27 may depend on the half-life of this massive nucleus at the Sun’s core.[/quote]
We can always workout how hydrogen was formed and if the Big Bang did occur the hydrogen production would be on similar lines.
see
http://map.gsfc.nasa.gov/m_uni/uni_101bbtest2.html