Close up of the supernova SN 2014J in star burst galaxy M82 in the constellation of Ursa Major.
The Type 1a supernova is the bright star like object just above the centre of the galaxy. A Type 1a supernova occurs in a binary star system when one of the stars is a white dwarf which accretes material from its companion until it exceeds a certain size and then explodes.
Type 1a supernova are used as standard candles because they all reach a certain specific peak luminosity and can therefore be used to determine the distance to remote galaxies.
It is the closest Type 1a supernova to be discovered in 42 years and was discovered by chance by students from UCL in London in mid January. Since its discovery it has been the subject of extensive follow-up observation by astronomers around the world.
Apparently the supernova is now starting to fade away.
M81 Bode’s Galaxy below, also in Ursa Major, a ‘grand design’ spiral galaxy, not far from M82. Discovered by Johann Bode in 1774.
B0th M81 and M82 are approximately 12 million light years away and are interacting with one another though their gravitational attraction. This is causing interstellar hydrogen to fall into the core of M82resulting in vigorous star formation.
Both galaxies are part of the Virgo super-cluster of galaxies.
The core of Bode’s Galaxy harbours a supermassive black hole equivalent to 70 million times the mass of our Sun.
Both images taken at home in London on 13th February using a 200mm telescope and a high sensitivity video camera.