Comet ISON transitioning post perihelion
Taken by Charles Coburn on November 28, 2013 @ Rescue, California USA (online SOHO)
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Date Taken: 2013:11:29 00:12:01
 
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I think comet ISON has survived it's plunge into the sun's atmosphere! NASA and other's proclaimed that the comet had disintegrated in the sun's atmosphere, but then something emerged from the other side. They said it was likely a "Ghost" or "Headless Comet" caused by the debris field following the trajectory. But I've been watching it all day and to me it looks like the tail is swinging around a nucleus that is generating more material. This is what one would expect from an intact comet, as the comet rounds the sun, it's tail gets blown ahead of it on on the way out by solar winds which are much faster than the comet. I think this sequence of four captures I made today shows that transition. This is exciting to me because since childhood I've been fascinated by this phenomenon and wondered just how the tail transitions from one side to the other. This doesn't look like the textbook illustration of the swing happening at perihelion (closest point, but rather a bit delayed because the of what I would assume is the comet's tangental speed so near the sun. But then nobody has ever seen a sun-grazing comet act like this one. Maybe this delay is due to it's extreme proximity to the surface (less than a million miles at one point). We'll have to see what the "real" astronomers say once they wake up and look at the data. I'm guessing it will survive, but will remain a challenge to see due to it's diminished size. I won't be able to try to take pictures of it until next weekend if weather permits since it will be too close to the sun until then.
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Comments
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Hi Charles... and other ISON observers
Well done. I agree
I have been working on the theory of sungrazers for several years
and have been predicting Ison would survive. It seems at least as big as Lovejoy,
and was twice as far from the solar centre - ie about 1/4 of the sunlight and
less dense hot plasma and smaller tidal forces.
I suspect the reason SDO saw nothing was that the AIA EUV lines just
were not sufficiently excited at that height - though that will need working out
in detail.
In any case this will tell us lost about ISON and comets in general.
I will be very happy to carry out a direct email discussion with interested folk
Watching excitedly to what new data come in today

Prof John C Brown
Astronomer Royal for Scotland
Glasgow
Posted by JCBrown42 2013-11-29 05:59:14
Great pictures and comments, Charles!
Thank you for remind me the helioviewer.org website, now I can follow the fate of the comet, havind updated informations.
NASA have been a shame in such case. We can get more reliable News from amateurs and independentes observers.
Also thank you, Prof. Brown.
Posted by masf494 2013-11-29 07:45:20
Charlec,
Thanks for your explanation for the direction and swing of the tail. I was already wondering why the tail was nor directed away from the sun. But the swing is a dynamic description as you descripted. Im assume, astronomers (like prof John C Brown) will analyse the swing of the tail. I hope they can give a description.
I did not look into text books, but assume the tail will be subjected to gravity and pressure from the solar wind and te outcome largely depends on the distribution of the size of the particles (molecules) in the tail.
Posted by Goejempd 2013-11-30 06:41:47
 
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