| 31. | Estimates of total mass loss for stars that reach the tip of the red-giant branch are around.
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| 32. | However, the mass loss and the burning aspects can make the consequences of the impact slightly different.
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| 33. | Suddenly, nightmare scenarios of mass loss of life have leapt from cinema screen and novel into the news.
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| 34. | The last mass loss is due to the decomposition of calcium carbonate to calcium oxide and carbon dioxide.
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| 35. | The temperature decreases slightly, but the outer layers of the star have inflated, driving even higher mass loss.
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| 36. | Stars with cores have an approximate total mass of, assuming the star has not undergone significant mass loss.
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| 37. | In contrast, measurement of mass loss on drying will detect the loss of " any " volatile substance.
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| 38. | Stellar mass loss produces a loss of angular momentum and this quickly brakes the rotation of massive stars.
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| 39. | It was an evolved star around 8, 000K showing extreme mass loss of helium and nitrogen enriched material.
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| 40. | A very wide range of possible masses can be calculated by combining the radius with hydrodynamic mass loss.
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