by kovil » Sun Jan 29, 2006 9:55 pm
I think I forgot the question. LOL
Two stars head on would be a lot of fireworks!! not to mention the attendant radiation.
In the thought experiment I see; as they are about a diameter apart they oblate into egg shaped, long ends toward each other.
As the gas atmospheres merge, high energy particle collisions and interaction begin the extra radiation effects.
Depending on their respective magnetic field alignments; a lot of varying scenarios play out, so I will basically hold that part of the vision.
Proceeding further to a 25% original diameter merger; the 'atmospheres' will give way outward as the denser material begins to impact together.
Depending on the stars absolute size, (and I'm visioning relative same size stars here), the distance to where fusion is happening will differ.
When the fusion shell is disrupted, by shock waves or actual collision, I expect that disruption will 'put the fire out' in one sense and in another sense change it to a different 'harmony' of how the particles are interacting. I would not expect a 'blow up' of fusion incident, but a kinetic reaction to density increases from the collision, throwing matter all over the local place 5-20 solar diameters rather rapidly.
Depending on the exact collision course, and if it is truly head on, the cores, depending on their real size and makeup, could do a nova style runaway reaction, or just a real messy splattering.
If the stars did not make a catastrophic explosion, nova style, then I see the fusion fires being extinguished from the massive disruption of both stars equilibriums. As the matter scatters energetically all over the place there will be lots of neutrinos etc activity, but as the double gravity potential now exists locally, in a while most of the particles will recollect and start a new star, probably 1-1/2 times the mass of the original size of the two identical size stars.. 1/2 being lost in the collision.
Mainly a big bang, splatter, and the fire goes out! It all slowly regroups and starts a new slightly larger star than was there before, with some small increase in the % of heavier elements in its makeup.
On second thought, imagining two paint balls in a head on collision, where the material splatters in a plane perpendicular to the vector of collision, a lot of material would have escape velocity energies, 50% of each star might escape. A lot of it depends on the initial gravity of each star, how fast they impact, and if the magnetic fields can help to contain anything before they are so disrupted they virtually disappear.
The stars collision velocity will be a very large factor in what happens.
===
It would almost be easier to postulate the environment on the surface of a neutron star! haha
Let's take a battleship weighing a million tons, and place it on a golf-tee shaped support that focuses all its weight onto one square centimeter.
That might not be enough pressure even ! to equal a neutron star surface gravity. But whatever it is, it's enough I would expect to make a near perfect sphere, depending on the rotation speed. And as dense and hard as any material imaginable, way beyond anything on earth.
What it's electromagnetic radiative qualities would be is an open question. But with the gravity so strong darn little can get away. It is near to black hole strength. Now some lesser neutron stars likely exist as there are probably several orders of magnitude in gravitational strength neutron stars possible. But even the least of which the surface gravity is so strong, everything is squashed flatter than anything imaginable. I would expect the local area is completely devoid of any loose particals.
On second thought, any particles found in the local area would be spirialing in at a very high velocity, so the surface atmosphere would be a whirl of particles being accumulated and absorbed at a great rate, and very energetically too; so again depending on the real gravitational forces involved, lots of things are going on; and much of it dependent on the local supply of matter which is being accumulated.
What we really need is a viewing platform!!
Where's Q when you need him !!
He sure was good as Beka's Uncle Sid on Andromeda !!
ps, Harry, I googled 'cricket rules' and got a real head full of a whole new language!!! I remember hearing cricket scores being reported on BBC one time in Scotland and it was so unintelligible as to be absolutely fascinating!!! and they went on and on about India and all sorts of places. I asked someone later what was going on, and all they could do was look confused and try to get started a couple of times, shake their head, and then just give up without even trying to explain it ! Which piqued my interest even more, that was about 20 years ago!
Thank heaven for google!
Now I can see what they were going thru! I'm just as baffeled as before because it is so darned complicated, but have an overall better conception of my ignorance! I can see why I waited 20 years!!
I think I forgot the question. LOL
Two stars head on would be a lot of fireworks!! not to mention the attendant radiation.
In the thought experiment I see; as they are about a diameter apart they oblate into egg shaped, long ends toward each other.
As the gas atmospheres merge, high energy particle collisions and interaction begin the extra radiation effects.
Depending on their respective magnetic field alignments; a lot of varying scenarios play out, so I will basically hold that part of the vision.
Proceeding further to a 25% original diameter merger; the 'atmospheres' will give way outward as the denser material begins to impact together.
Depending on the stars absolute size, (and I'm visioning relative same size stars here), the distance to where fusion is happening will differ.
When the fusion shell is disrupted, by shock waves or actual collision, I expect that disruption will 'put the fire out' in one sense and in another sense change it to a different 'harmony' of how the particles are interacting. I would not expect a 'blow up' of fusion incident, but a kinetic reaction to density increases from the collision, throwing matter all over the local place 5-20 solar diameters rather rapidly.
Depending on the exact collision course, and if it is truly head on, the cores, depending on their real size and makeup, could do a nova style runaway reaction, or just a real messy splattering.
If the stars did not make a catastrophic explosion, nova style, then I see the fusion fires being extinguished from the massive disruption of both stars equilibriums. As the matter scatters energetically all over the place there will be lots of neutrinos etc activity, but as the double gravity potential now exists locally, in a while most of the particles will recollect and start a new star, probably 1-1/2 times the mass of the original size of the two identical size stars.. 1/2 being lost in the collision.
Mainly a big bang, splatter, and the fire goes out! It all slowly regroups and starts a new slightly larger star than was there before, with some small increase in the % of heavier elements in its makeup.
On second thought, imagining two paint balls in a head on collision, where the material splatters in a plane perpendicular to the vector of collision, a lot of material would have escape velocity energies, 50% of each star might escape. A lot of it depends on the initial gravity of each star, how fast they impact, and if the magnetic fields can help to contain anything before they are so disrupted they virtually disappear.
The stars collision velocity will be a very large factor in what happens.
===
It would almost be easier to postulate the environment on the surface of a neutron star! haha
Let's take a battleship weighing a million tons, and place it on a golf-tee shaped support that focuses all its weight onto one square centimeter.
That might not be enough pressure even ! to equal a neutron star surface gravity. But whatever it is, it's enough I would expect to make a near perfect sphere, depending on the rotation speed. And as dense and hard as any material imaginable, way beyond anything on earth.
What it's electromagnetic radiative qualities would be is an open question. But with the gravity so strong darn little can get away. It is near to black hole strength. Now some lesser neutron stars likely exist as there are probably several orders of magnitude in gravitational strength neutron stars possible. But even the least of which the surface gravity is so strong, everything is squashed flatter than anything imaginable. I would expect the local area is completely devoid of any loose particals.
On second thought, any particles found in the local area would be spirialing in at a very high velocity, so the surface atmosphere would be a whirl of particles being accumulated and absorbed at a great rate, and very energetically too; so again depending on the real gravitational forces involved, lots of things are going on; and much of it dependent on the local supply of matter which is being accumulated.
What we really need is a viewing platform!!
Where's Q when you need him !!
He sure was good as Beka's Uncle Sid on Andromeda !!
ps, Harry, I googled 'cricket rules' and got a real head full of a whole new language!!! I remember hearing cricket scores being reported on BBC one time in Scotland and it was so unintelligible as to be absolutely fascinating!!! and they went on and on about India and all sorts of places. I asked someone later what was going on, and all they could do was look confused and try to get started a couple of times, shake their head, and then just give up without even trying to explain it ! Which piqued my interest even more, that was about 20 years ago!
Thank heaven for google!
Now I can see what they were going thru! I'm just as baffeled as before because it is so darned complicated, but have an overall better conception of my ignorance! I can see why I waited 20 years!!