<p><BR/>Replying to:<BR/><DIV CLASS='Discussion_PostQuote'>Thanks you all for the posts, I know indeed there is no possible candidate to become a SN within 50 Ly from the Earth, but the question is merly hypotetichal, <span style="font-weight:bold" class="Apple-style-span">only to know how fast the shock wave could reach the earth estimating the 15 Ly distance the light will take 15 years to reach the planet but, what about the rest of it </span>and I m not talking about only the gamma rays brust, but aso the energy released form such explosion<br /> Posted by Zhelom1973</DIV></p><p>In the initial explosion, stellar material can be ejected at velocities up to 10% of the speed of light, but the actual rate of expansion over time can be highly variable, depending on the density of the surrounding interstellar medium. So to answer your question, the soonest the electromagnetic radiation can reach us is 15 years, as was already stated, and the very soonest the expanding debris shell can reach us is 150 years, but it would probably take much longer. Here's some excerpts from an interesting website:</p><p><span style="font-family:Arial;font-size:12px;-webkit-border-horizontal-spacing:2px;-webkit-border-vertical-spacing:2px" class="Apple-style-span"><a style="font-family:Arial,'SansSerif'" name="evolve"></a><span style="font-style:italic" class="Apple-style-span">As the ejecta expand out from the star, it passes through the surrounding interstellar medium, heating it from 10</span><sup style="font-family:Arial,'SansSerif'"><span style="font-style:italic" class="Apple-style-span">7</span></sup><span style="font-style:italic" class="Apple-style-span"> to 10</span><sup style="font-family:Arial,'SansSerif'"><span style="font-style:italic" class="Apple-style-span">8</span></sup><span style="font-style:italic" class="Apple-style-span"> K, sufficient to separate electrons from their atoms and to generate thermal X-rays. The interstellar material is accelerated by the shock wave and will be propelled away from the supernova site at somewhat less than the shock wave's initial velocity. This makes for a thin expanding shell around the supernova site encasing a relatively low density interior.</span></span></p><span style="font-family:Arial;font-size:12px;-webkit-border-horizontal-spacing:2px;-webkit-border-vertical-spacing:2px" class="Apple-style-span"><a style="font-family:Arial,'SansSerif'" name="evolve"></a><p style="font-family:Arial,'SansSerif'"> </p><table border="0" style="font-family:Arial,'SansSerif'"><tbody><tr style="font-family:Arial,'SansSerif'"><td style="font-size:12px;font-family:Arial,'SansSerif'"><span style="font-style:italic" class="Apple-style-span">While the material swept up by the shock is much less than the mass of the stellar ejecta, the expansion of the stellar ejecta proceeds at essentially a constant velocity equal to the initial shock wave speed, typically of the order of 10,000 km/s. This is known as the "free expansion" phase and may last for approximately 200 years, at which point the shock wave has swept up as much interstellar material as the initial stellar ejecta. The supernova remnant at this time will be about 10 light years in radius. Although the remnant is radiating thermal X-ray and synchrotron radiation across a broad range of the electromagnetic spectrum (from radio to X-rays), the initial energy of the shock wave will have diminished very little. Line emission from the radioactive isotopes generated in the supernovae contribute significantly to the total apparent brightness of the remnant in the early years, but do not significantly effect the shock wave.</span>