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Spectrum of Type II/p Supernova 2012aw |
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Written by Dave Grennan
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Monday, 23 April 2012 23:35 |
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On March 16th 2012 a bright supernova was discovered by Allesandro Dimai in the nearby galaxy M95 and designated 'Supernova 2012aw'. Now of course on a cosmological scale, 'nearby' is a very relative term! M95 is approximately 38million light years away. The good news is that a supernova in such a nearby galaxy presents an ideal opportunity for amateurs with modest equipment to study the object both visually and spectroscopically. The intention of this short article is to look at the results of a spectroscopic examination and see what we can determine about this wonderful event.
There is no intention in this short article to explain supernovae and the various types. A quick google search will turn up more than enough explaination on the subject to satisfy anyone.
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Last Updated on Tuesday, 24 April 2012 09:42 |
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Quasar 2C-374 - Measuring the Redshift |
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Written by Dave Grennan
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Sunday, 15 April 2012 13:12 |
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This weekend, I acheived a long standing ambition. To measure the distance to one of the universe' most strange and distant objects. Quasars are the super-luminous cores of very distant galaxies which are thought to surround a super-massive black hole. Rather than give a dissertation on the nature of quasars, here is a link describing quasars generally and a specific link to 3C-273. If you need to go and have a read and then come back to this page.
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Last Updated on Sunday, 15 April 2012 15:58 |
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Written by Dave Grennan
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Friday, 27 January 2012 01:36 |
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(Click on the image for full sized animation)
At approximately 4pm on the afternoon of January 27th 2012. A small asteroid named 2012 BX34 will pass just 44,000miles from Earth. 2012 BX34 was only discovered on January 25th by the Catalina Sky Survey in the US. The asteroid is about 8m wide (about the size of a bus). It is rare for an asteroid to pass so close to Earth. Consider that the Moon is about 250,000 miles from us so this asteroid passes less than 1/5th of the distance to the Moon and only twice as far as geosynchronous satellites! The image sequence above was taken from Raheny Observatory, Dublin, Ireland (MPC #J41) just before midnight (going into) January 26th. Each frame is a stack of 5 x 3 second images. The images are aligned with the motion of the asteroid so the asteroid is presented as a point. This is why the stars appear to be dotted lines. The asteroid very quickly moves into the southern sky and therefore this is the only opportunity I will get to image this asteroid this year. The asteroid is approx. 24,000 times fainter than you could expect to see with the naked eye. Its travelling along close to 9km/sec. |
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Written by Dave Grennan
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Monday, 16 April 2012 22:53 |
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I began spectroscopy a couple of years ago after purchasing a wonderful spectroscope. The L200 is an IKEA type instrument (produced by Ken Harrison) which the end user assembles at home. It comes with a 600 lines/mm grating which makes it a medium resolution spectroscope. It's great for looking close up at profiles within objects. However I also wanted a '"one shot" instrument capable of capturing a full spectrum on one frame of a CCD camera. Thus after lots of thought and 'back of envelope' drawings, I came up with the idea for the "G300". I soon realised that in fact this was no new idea and that several similar instruments had been built by others. The G300 is in essence a 'Classical' spectroscope in design. The classical design consists of two lens, an entrance slit to 'sample' the light from the object and a diffraction grating which does the real work of breaking up the incoming light into its component colours (the spectrum) to be recorded on the camera.
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Last Updated on Tuesday, 17 April 2012 00:02 |
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Written by Dave Grennan
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Sunday, 24 July 2011 15:47 |
Raheny Observatory (MPC #J41)

(Click here to read the full story)
A discussion of the building, equipment and some of the techniques used at Raheny Observatory, Dublin, Ireland.
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Last Updated on Friday, 27 January 2012 01:50 |
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