Super Nova Remnant ED102 From Hubble (APOD 29 Aug 2006)
- orin stepanek
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Super Nova Remnant ED102 From Hubble (APOD 29 Aug 2006)
http://antwrp.gsfc.nasa.gov/apod/ap060829.html
the view of this nova with the SMC almost overshadows the fact that Hubble is studying the remnants of Ed102.
With all the knowledge we gain from Hubble like this view of the super nova in the SMC; I think it is important to keep Hubble upgraded. For all the cost of building this wonderful space telescope; it is worth keeping it going because it has opened the windows to valuable information. At least until a bigger better one is put into service.
Orin
the view of this nova with the SMC almost overshadows the fact that Hubble is studying the remnants of Ed102.
With all the knowledge we gain from Hubble like this view of the super nova in the SMC; I think it is important to keep Hubble upgraded. For all the cost of building this wonderful space telescope; it is worth keeping it going because it has opened the windows to valuable information. At least until a bigger better one is put into service.
Orin
Star twinkle effect in hubble pictures (APOD 29 Aug 2006)
This might be a faq, but I could not easily find the answer. I apologize if this has already been discussed many times before.
I noticed that on the APOD of august 28, 2006 ( http://antwrp.gsfc.nasa.gov/apod/ap060829.html ) the bigger stars show 'twinkles' in the exact vertical and horizontal directions. Does anyone know what causes these lines of light? Are they an undesired artefact that cannot be removed easily?
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Matthijs Sypkens Smit
I noticed that on the APOD of august 28, 2006 ( http://antwrp.gsfc.nasa.gov/apod/ap060829.html ) the bigger stars show 'twinkles' in the exact vertical and horizontal directions. Does anyone know what causes these lines of light? Are they an undesired artefact that cannot be removed easily?
--
Matthijs Sypkens Smit
Hi matthijs
The effect is called bleeding, its when charge in the CCD bleeds up and down columns and across rows when the target saturates the detector. In other words the brightest pixel in the centre of the star image cannot hold any more electrons (which are released by the light impinging on the chip) so the charge tends to fall down the rows and columns. They can generally be removed by taking more shorter exposures so that the central pixel does not saturate. However if pretty pictures are not the main driver (and generally they arent) then they dont tend to cause too many problems so its easier not to break up the exposures.
The effect is called bleeding, its when charge in the CCD bleeds up and down columns and across rows when the target saturates the detector. In other words the brightest pixel in the centre of the star image cannot hold any more electrons (which are released by the light impinging on the chip) so the charge tends to fall down the rows and columns. They can generally be removed by taking more shorter exposures so that the central pixel does not saturate. However if pretty pictures are not the main driver (and generally they arent) then they dont tend to cause too many problems so its easier not to break up the exposures.
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http://www.ocastronomers.org/gallery/artifact.asp
A good explination is found here
http://www.astronomy-images.com/Equipme ... -vanes.htm
A good explination is found here
http://www.astronomy-images.com/Equipme ... -vanes.htm
- orin stepanek
- Plutopian
- Posts: 8200
- Joined: Wed Jul 27, 2005 3:41 pm
- Location: Nebraska
Here's more information found because of Hubble!
http://hubblesite.org/newscenter/newsde ... s/2006/42/
Let shuttle service to Hubble be restored.
Orin
http://hubblesite.org/newscenter/newsde ... s/2006/42/
Let shuttle service to Hubble be restored.
Orin
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