| 41. | It is also undergoing strong mass loss with the outer layers of the star no longer gravitationally bound.
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| 42. | It also shows H ? emission lines with P Cygni profiles, indicating mass loss through a powerful stellar wind.
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| 43. | Ordinary supergiants lack the strong H emission and broadened spectral lines that indicate rapid mass loss in the hypergiants.
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| 44. | In the TGA trace of calcium oxalate monohydrate, the first mass loss corresponds to loss of water of hydration.
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| 45. | This is about 5 times greater than the observed mass loss in Greenland but still in the same ballpark.
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| 46. | Only the very lowest metallicity population III stars will reach this stage of their life with little mass loss.
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| 47. | The mass loss from the collision will not be detectable before the radiated energy passes beyond the observers position.
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| 48. | This weight loss and mass loss would happen as the box was cooled by this process, to room temperature.
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| 49. | The second mass loss corresponds to decomposition of dehydrated calcium oxalate to calcium carbonate and carbon monoxide and carbon dioxide.
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| 50. | At such a rate of mass loss, the star probably has only another one million to three million years to live.
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