We're looking for bright, young, ambitious people who are ready to join Canada's premier new media and music marketing company!
Supernova is proud to offer students and young professionals the opportunity to gain hands-on experience in the music industry through our internship program. We are always seeking ambitious individuals who are ready to learn first hand what a position in the modern music industry entails.
Successful applicants will be involved with every aspect of our concerts, sales, customer relations, market research, client support and social media operations under the supervision of an experienced team of elite managers.
Find out what really happens backstage by being a part of it. Send your cover letter, stating why you want to work in the music and new media industry, and a
resume to corina@supernova.com
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Stars are sustained by the nuclear fusion reactions taking place in their cores. For stars on the main sequence, such as our own Sun, this mostly involves combing hydrogen to form helium. The energy that these reactions produce is enough to support their mass against its own gravity.
As a star runs out of fuel it can expand and will begin to form heavier elements such as carbon and iron (most of the matter in our solar system comes from extra-solar sources). Once it finally exhausts all of its fuel it will begin to collapse. It is here that the stars begin to undergo different fates.
Our own sun will collapse until it becomes a white dwarf, at this point the Pauli exclusion principle keeps the electrons in the star far enough apart to resist further collapse - this energy is called 'electron degeneracy'.
Stars greater than 1.4 times the mass of the Sun (called the Chandrasekhar limit after the Indian physicist who discovered it on his way to England) will tend to explode in a supernova casting off much of their mass. A small central core will remain and like smaller stars this will collapse only this time electron degeneracy will not be enough to support the star's mass against its gravitational collapse and it will continue to shrink until it becomes a tiny, but hugely massive, neutron star held together by neutron degeneracy.
If neutron degeneracy is not enough to resist the star's collapse it will continue to shrink until the matter is all compressed into an infinitely small, infinitely dense point called a singularity. This is the centre of a black hole.