by Ann » Sun Mar 17, 2013 5:53 am
Ah yes, very interesting. V838 Mon is a reminder of how bright stars can get and how red they can get in the process.
In order for a star to get so bright and so red, its outer envelope has to expand tremendously, yet remain luminous the whole time. Personally I can't help wondering if the fusion processes going on inside it must work faster during this enormous outer expansion. Or were we watching the effects of some kind of gravitational core contraction?
There has been a lot of speculation as to the cause of V838 Mon's exceptional behavior. One hypothesis has been that the star suddenly "ate" one of its planets.
I think it has been proven that V838 Mon started out as a bright blue star before it had its tremendous outburst. Personally I doubt that a less massive star, for example the Sun, could imitate V838 Mon's behavior under any circumstances.
For all of that, I hope the Sun will refrain from flaring up like mad because it suddenly snacked on Mercury, for example!
Ann
Ah yes, very interesting. V838 Mon is a reminder of how bright stars can get and how red they can get in the process.
In order for a star to get so bright and so red, its outer envelope has to expand tremendously, yet remain luminous the whole time. Personally I can't help wondering if the fusion processes going on inside it must work faster during this enormous outer expansion. Or were we watching the effects of some kind of gravitational core contraction?
There has been a lot of speculation as to the cause of V838 Mon's exceptional behavior. One hypothesis has been that the star suddenly "ate" one of its planets.
I think it has been proven that V838 Mon started out as a bright blue star before it had its tremendous outburst. Personally I doubt that a less massive star, for example the Sun, could imitate V838 Mon's behavior under any circumstances.
For all of that, I hope the Sun will refrain from flaring up like mad because it suddenly snacked on Mercury, for example!
Ann