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taylordnz
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if you have a three solar mass star then it eneters into supernovae, how much mass is lost into space?
Most 3Ms stars would (without a companion) puff off outer layers during the giant phases and not go supernova at all.taylordnz said:if you have a three solar mass star then it eneters into supernovae, how much mass is lost into space?
You may be thinking of the 3.2 Ms upper limit for a neutron star or any stellar remnant above which that mass must collapse to a black hole.taylordnz said:a three solar mass star is the lowest limit for supernovae, for my research paper i need stats on how much matter is lost at any possible way?
I think that average IQ is inversely proportional to the number of 50 cent, BS phrases posted in the quote above. Therefore, since that number is so very high, the IQ of the poster must be dragging right at about 3.2, which is also the maximum limiting mass of a neutron star and ~ equal to the IQ of a snail. However, if the relationship is not a straight-line function, then the number of 1.44 (Chandra's limit) might be closer to actual.Pinkline Jones said:Perhaps it is pertinent for us all to consider the latitudinal coordinates purely from the fragmented distribution of secondary prismatic deflections - interdependent of the physical location - in that they are in proximity to the centre line on the equator. The 3.2 Ms upper limit is certainly close to the upper limit of a neutron star and also alludes to the average I.Q. of the people who attend Run DMC concerts or Anthony Robbins seminars.
I am very interested in opinions as to whether the mass of the supernova is inversely proportional to the acceleration of a bucket of lobster innards - in a clockwise direction across the upper stratosphere of a parallel universe.
DR PINKLINE JONES
Australia's Leading Social Critic
A post supernovae star is a star that has undergone a supernova explosion, which is a catastrophic event that occurs when a massive star reaches the end of its life and collapses in on itself, releasing an enormous amount of energy and leaving behind a compact remnant.
The mass of a post supernovae star is calculated by measuring the mass of the compact remnant left behind after the supernova explosion. This can be done through various methods such as studying the orbital motion of the remnant in a binary system or analyzing the radiation emitted by the remnant.
The calculated mass of a post supernovae star can be influenced by several factors, including the mass of the original star before the supernova explosion, the amount of mass lost during the explosion, and any interactions with other stars or stellar remnants in its vicinity.
Yes, the mass of a post supernovae star can change over time due to various factors such as accretion of material from a companion star, interactions with other stars or stellar remnants, and the emission of mass through stellar winds.
The mass of a post supernovae star is important for understanding stellar evolution because it provides valuable information about the initial mass of the star before the supernova explosion and the processes that occur during and after the explosion. This information can help scientists better understand the life cycle of stars and the formation of different types of stellar remnants such as neutron stars and black holes.