Timeline for Radiation from binary star systems and how that would affect a planet orbiting both stars
Current License: CC BY-SA 3.0
8 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Jun 26, 2017 at 23:21 | answer | added | Logan R. Kearsley | timeline score: 2 | |
| Jun 6, 2017 at 19:22 | answer | added | anon | timeline score: 4 | |
| Jun 6, 2017 at 16:21 | comment | added | HDE 226868♦ | Adrienne - Ah, I see. Thank you. I was wrong about the separation. @steverino .5 solar masses is actually pretty normal for a white dwarf. | |
| Jun 6, 2017 at 14:50 | comment | added | steverino | .5 solar masses is way too small for a white dwarf. Your numbers need some rework | |
| Jun 6, 2017 at 13:52 | comment | added | Adrienne | The Roche Lobes of these two stars would be hugely smaller than that of their orbital seperation and as such shouldn't see major acretion. At that distance it should be occasional small ones. | |
| Jun 6, 2017 at 13:47 | comment | added | HDE 226868♦ | You're essentially describing a cataclysmic variable system, albeit one with low activity. You should probably be concerned about large outbursts. | |
| Jun 6, 2017 at 12:08 | history | edited | Frostfyre | CC BY-SA 3.0 |
Edited for spelling, grammar, and clarity
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| Jun 6, 2017 at 10:22 | history | asked | Adrienne | CC BY-SA 3.0 |