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.
Results of a very brief observing session this evening between tea and the clouds rolling in here in London.
More magnification than last week with a larger telescope and also using a UHC filter to improve contrast.
First up is M42 The Great Orion Nebula, the nearest star forming region with reflection, emission and dark nebula all evident.
Next up is M82 in Ursa Major with supernova 2014. M82 is a starburst galaxy 12 million light years away in Ursa Major (The Plough). The 2014 type 1a supernova can be clearly seen in the upper side of the galaxy. M82 is apparently 5 times more luminous than the Milky Way.
Next is an edge on spiral galaxy in the Lynx constellation called NGC 2683. Just visible as a slender fuzzy strip but with a particularly bright core. Discovered by William Herschel in 1788, and often referred to as the UFO galaxy it is located about 20million light years away and receding from us at about 400km/second.
Lastly but not particularly visually impressive but rewarding to find none the less is the globular cluster called NGC 2419, the ‘Intergalactic Wanderer’, again in the Lynx constellation (the fuzzy grey blob in the centre of the image below). This object is a gravitationally bound group of up to 1 million stars that orbits the Milky way at a great distance of some 300,000 light years and is one of the most distant globular clusters in our galaxy. It orbits the centre of the galaxy only once every 3 billion years or so. It was also discovered by William Herschel in 1788.
Image Credit: X-ray: NASA/CXC/SAO; Infrared: NASA/JPL-Caltech; Optical: MPIA, Calar Alto, O. Krause et al.
A multi-wavelength image using data combined from 3 seperate telescopes, namely the Chandra x-ray observatory, the infra-red Spitzer space telescope and the optical earth based Calar Alto telescope in Spain.
The Tycho supernova remnant is located about 13,000 light years away in the constellation of Cassiopeia and is the aftermath of a violent explosion of a white dwarf star that was first spotted as a new star shining brilliantly by the famous Danish astronomer Tycho Brahe in 1572, see below. The remnant is currently approximately 55 light years in diameter.
Following his observation of this new star which shone as brightly as Venus and could be seen in the day for 2 weeks, Tycho Brahe was so excited that he devoted the rest of his life to astronomy.
Brahe was a particularly colourful character known for his silver nose as well as mystery surrounding his death. Note his enlarged ‘observing’ eye.