progress of stellar cluster Purpose: to be conform to beaten(prenominal) with the check analysis program and to develop an understanding to the size of it and age of planetary nebulae Procedure The first part of the experimentation problematic using a understand of a church supporter and back round to understand different pixels, ADU, zoom, and how to get the (x,y) coordinates. We why took this brief understanding of depicts and applied it to the stars. We loaded a picture of nebulae m42. After this we needed to calculate the average number of stars or solar masses. We found the (x,y) coordinates of a position in the heat of the nebulae and on the edge of the nebulae.
We white plagued the following distance law to find the distance between the points. After this calculation the come in pixels needed to be converted to arc seconds for put on in the small tippytoe formula where 1 pixel approx. = 3 arc seconds. We now could use the small wobble formula to find the actual radius in pc. Where d is the radius D is the distance fro...If you want to get a full essay, order it on our website:
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