About observational astronomy: Difference between revisions
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=== Creating color images === | === Creating color images === | ||
=== Supernova === | === Supernova === | ||
Revision as of 13:30, 8 February 2008

Astronomers can gain an understanding of objects in the universe by studying them with a telescope. Observational astronomy is the process of collecting and analyzing data to learn about these objects. In this learning project a computer program will be used to view and study images taken with a telescope to learn basic concepts in astronomy.
Activities
A CCD (Charge-coupled device) imaging system is a type of digital camera that is very sensitive to the dim light from distant objects. The CCD camera is attached to a telescope and the images are stored on a computer where they can later be analyzed. Astronomical images are stored in a computer file format called FITS. These images can be opened and viewed by using computer software that understands this file format.
Creating color images
Supernova
The Observational astronomy/Supernova page has images of galaxies where a supernova has been observed recently. In this activity we will retrieve images taken before the supernova occured, and compare them to the new images.
- Start Aladin and click on the Load... button. In the Server selector window click on DSS and select an image server. In the Target box enter the name of the galaxy which is UGC14 and then choose POSS1_Red for the Survey. Click Submit.
- In the Aladin multiview window click on the icon labeled pixel. In the Pixel mapping popup window click on the Reverse button to change the image from a negative to a positive.
- To find out when this image was taken click on the icon labeled prop and look for Date-Obs: which indicates that the image was taken Aug. 11, 1953.
- Compare the image displayed in Aladin to the image shown at right. Click here (or on the image) to see a larger version and to find out when it was taken (the Date is 2007-01-02T23:03Z.) This supernova was first seen on Dec. 12, 2006, so it will not be visible in the earlier image displayed by Aladin. Do you see the supernova in the recent image? If you are unsure, click here to see another version of this image that is marked to show which star the supernova is.
- More images of this supernova can be found in Category:Supernova Images or at the Supernova 2006sr in UGC 14 webpage. Compare images taken on different dates to see if the supernova has changed brightness. The difference will be very subtle in images taken a week apart. It is more obvious after about a month.
Readings
Background information:
References
Additional helpful readings include: