Posted on 08/30/2020 1:59:23 PM PDT by MtnClimber
Explanation: How massive can a normal star be? Estimates made from distance, brightness and standard solar models had given one star in the open cluster Pismis 24 over 200 times the mass of our Sun, making it one of the most massive stars known. This star is the brightest object located just above the gas front in the featured image. Close inspection of images taken with the Hubble Space Telescope, however, have shown that Pismis 24-1 derives its brilliant luminosity not from a single star but from three at least. Component stars would still remain near 100 solar masses, making them among the more massive stars currently on record. Toward the bottom of the image, stars are still forming in the associated emission nebula NGC 6357. Appearing perhaps like a Gothic cathedral, energetic stars near the center appear to be breaking out and illuminating a spectacular cocoon.
(Excerpt) Read more at apod.nasa.gov ...
“So roughly 50 light years wide for the image at a distance of 8000 light years.”
Picture a right triangle that’s 50 units on one side and 8000 on the other.
That’s 22 seconds of arc for the “width” of the picture. Did I do that correctly?
For comparison the moon is about 1800 seconds of arc (1/2 degree).
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