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Mianeye
reply to post by Beavers
There is no debri from a star, it's not solid.
Supernova nucleosynthesis is the production of new chemical elements inside supernovae. It occurs primarily due to explosive nucleosynthesis during explosive oxygen burning and silicon burning.[1] Those fusion reactions create the elements silicon, sulfur, chlorine, argon, sodium, potassium, calcium, scandium, titanium and iron peak elements: vanadium, chromium, manganese, iron, cobalt, and nickel. As a result of their ejection from supernovae, their abundances increase within the interstellar medium. Elements heavier than nickel are created primarily by a rapid capture of neutrons in a process called the r-process. However, there are other processes thought to be responsible for some of the nucleosynthesis of heavy elements, notably a proton capture process known as the rp-process and a photodisintegration process known as the gamma (or p) process. The latter synthesizes the lightest, most neutron-poor, isotopes of the heavy elements.
Beavers
reply to post by proob4
The light took 12 million years already and has just hit us.
If the debris travelled at 10% of the speed of light, the answer would be something along the lines of 10.8 million years.
I just don't know how fast it travels..
proob4
At least 12 million years. Our own Sun will have probably all ready gone super nova by then.edit on 1/22/14 by proob4 because: (no reason given)
Beavers
reply to post by proob4
The light took 12 million years already and has just hit us.
If the debris travelled at 10% of the speed of light, the answer would be something along the lines of 10.8 million years.
I just don't know how fast it travels..
proob4
At least 12 million years. Our own Sun will have probably all ready gone super nova by then.edit on 1/22/14 by proob4 because: (no reason given)
In astronomy, the interstellar medium (or ISM) is the matter that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, dust, and cosmic rays. It fills interstellar space and blends smoothly into the surrounding intergalactic space. The energy that occupies the same volume, in the form of electromagnetic radiation, is the interstellar radiation field.
The interstellar medium is composed of multiple phases, distinguished by whether matter is ionic, atomic, or molecular, and the temperature and density of the matter. The thermal pressures of these phases are in rough equilibrium with one another. Magnetic fields and turbulent motions also provide pressure in the ISM, and are typically more important dynamically than the thermal pressure is.
Beavers
reply to post by proob4
probably yes!
and I'm not worried at all, I'll be long dead in 10.8 million years
It's not the 'doom' aspect I'm going for, I'm just interested in the maths and science behind it!
The explosion expels much or all of a star's material[2] at a velocity of up to 30000 km/s (10% of the speed of light), driving a shock wave[3] into the surrounding interstellar medium.