A supernova was discovered in galaxy M82 during mid-January 2014.
It was discovered by Steve Fossey of University College London.
On 31st January the supernova stopped brightening at a peak magnitude of 10.5, it is the closest Type 1a supernova to be discovered in the past 40 years.
Designated as SN 2014J is a type 1a supernova which occurs in a binary system (2 stars orbiting each other) one of the stars is a white dwarf. A white dwarf is the remnant of a star that has completed its normal life cycle
and has ceased nuclear fusion. White dwarfs are however capable of further fusion reactions that release a lot of enbergy as long as their temperatures rises high enough.
This is where the companion star of the white dwarfs plays an important role.
When this white dwarf accumulates matter from its companion star it rises the temperature of the core of the star and at a specific point the white dwarf ignites and nuclear fusion (carbon fusion) starts again.
Within a few seconds of starting the nuclear fusion, a substantial fraction of the matter in the white dwarf undergoes a runaway reaction, releasing enough energy to unbind the star in a huge supernova explosion.
The typical visual absolute magnitude of a Type 1a supernova is about 5.000.000.000 times brighter than our own Sun. This also allows us to see it over a distance (in the case of M82) of over 12 million light years.
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|Maximum size:||2000 x 1500px – LRGB Color|
|Animated GIF:||1200 x 900px – Animated GIF|
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|Name||:||SN2014J (in M82)|
|Right ascension||:||09h 55m 42s|
|Declination||:||+69° 40′ 27″|
|Image date||:||Feb. 02, 2014|
|Light frames||:||5x 4 min. RGBG (each), 20x 5 min. 7nm Ha unbinned (Luminance)|
|Total integration||:||2h 40m|
|Dark frames||:||29x unbinned|
|Flat frames||:||20x p. filter unbinned
Created with an A3 size Posterpoweruk flatfield panel
|Software used||:||CCDOps, CCDSoft, Maxim DL, Photoshop CS4|
|Processing||:||CCDOPS was used for focussing. Image Acquisition was done using CCDSoft.
All separate frames were calibrated, aligned and stacked in MaxIm DL5 Pro.
Photoshop CS4 was used for further processing – curves adjustment, levels adjustment, etc.
Noel Carboni’s toolset was used as well (Local Contrast Enhancement, Deep Space Noise Reduction)
|Telescope||:||Orion Optics UK 10″ f4.8 Newton|
|Corrector||:||Televue 2″ Paracorr coma corrector with 15% increase focal length: 1380mm f/5.43|
|Mount||:||Losmandy G-11 Gemini|
|Guide camera||:||QHY5-II Mono|
|Guide scope||:||Celestron 60/700 Achromat|
|Autoguide software||:||PHD Guiding|
|Filters||:||Baader 2″ 7nm Ha, Baader 2″ RGB + IDAS LPS-P2|
|Location||:||Landgraaf, The Netherlands|
|Comment||:||All exposures were taken through IDAS LPS-2 filter which was in front of the filter wheel.
CCD Temp was set at -15.
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