Timeline for Old star vs New star
Current License: CC BY-SA 4.0
11 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| S Jul 14, 2018 at 18:08 | history | suggested | Chappo Hasn't Forgotten | CC BY-SA 4.0 |
Improved expression, in particular to address the confusion in one of the comments.
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| Jul 13, 2018 at 14:05 | comment | added | Kornpob Bhirombhakdi | A star loses its total mass when evolves from many channels. Fusion combine light elements to heavier ones, implying that the total mass decreases. Stars also have stellar wind, or eruption, which expels some mass. In a binary system, a star can lose mass if its companion pulls the gas envelope. Or, it can gain the mass by accretion. | |
| Jul 11, 2018 at 6:11 | comment | added | James K | Is "mean" the "average"? Please edit to say either "Does that mean that the mass of the old sun...." or "Is the average mass of the particles of the old sun". | |
| Jul 10, 2018 at 11:58 | review | Suggested edits | |||
| S Jul 14, 2018 at 18:08 | |||||
| Jul 10, 2018 at 7:06 | review | Close votes | |||
| Jul 15, 2018 at 23:30 | |||||
| Jul 10, 2018 at 4:00 | history | edited | HDE 226868♦ | CC BY-SA 4.0 |
Fission -> fusion.
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| Jul 9, 2018 at 22:40 | comment | added | ProfRob | Not clear what you mean by "mean mass"? | |
| Jul 9, 2018 at 20:14 | answer | added | HDE 226868♦ | timeline score: 8 | |
| Jul 9, 2018 at 19:35 | answer | added | Steve Linton | timeline score: 4 | |
| Jul 9, 2018 at 19:32 | comment | added | Steve Linton | I think you mean "fusion" not "fission" | |
| Jul 9, 2018 at 19:24 | history | asked | Haris Ansari | CC BY-SA 4.0 |