Stellar Evolution Stars begin their lives as a cloud of dust, better known as a Nebula. The star begins to form as the nebula condenses through gravitational attraction. Once the attraction has made the body opaque to electromagnetic radiation, it is then classified as a Protostar. As this electromagnetic radiation is the same radiation that the star is attempting to release. Some of it stays in the Protostar and aids heating the interior. The Protostar can not produce nuclear reactions. When the core temperatures and pressures are high enough – nuclear reactions fusing Hydrogen into Helium start. The contraction then stops. Now the Protostar is classified as a Main Sequence Star Stellar Structure The gravitational attraction is balanced by the pressure from the energy released during nuclear fusion. When a star has used about 60% of the fusion is completed it will start it’s death! The temperature of the star falls and the core collapses under its gravity to stabilise. Temperature in the core rises causing more nuclear fusion – Helium to Carbon. This causes the star to expand into a Red Giant Once this relatively stable phase ends. Each star will take a different path to death depending on the mass. For this example we are going to use a star with a mass > 25 Solar Masses. In a Massive Star, the Red Giant phase is split into stages of contraction and expansion when huge quantities of different elements are fused. These form layers or shells inside the core of the star. Eventually these shells collapse into each other – causing a chain reaction. This collapse causes a shockwave that projects a large proportion of the mass of the star outwards. In a Massive star, this shock wave is classified as a Supernova. The Supernova leaves behind a body, so massive, its gravitational attraction is such that light can not escape. A Black Hole is born To form a black hole the remnant must be greater than 3 solar masses. How do we know that this happens and something that we can’t see really exists? The answer lies in binary systems where a star is seen to orbit an object that is not visible – such as Cygnus X-1