Re: APOD: The Mysterious Rings of Supernova 1987A (2012 Feb
Posted: Mon Feb 27, 2012 9:42 pm
APOD and General Astronomy Discussion Forum
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You probably have the basic general idea correct.Interested Observer wrote:Does anyone else, besides me, think the rings are bubbles of superheated gas which are escaping along the field lines of the star's magnetic poles? Sort of like an aurora but in reverse.
It seems to me that the poles of a star going supernova would be the first place from which the explosion would escape, given that the field would provide the least resistance at the poles. The lack of resistance might also mean the bubbles travel faster than the shock wave emanating along the plane of the ecliptic.
Also, the study of bursting bubbles has shown they become rings of smaller bubbles as they expand.
To me, these two concepts seem to adequately explain what has been observed. It doesn't seem so mysterious to me but, I'd appreciate any feedback, in case there's something I've missed.
It is perhaps confusing to introduce planetary nebulas here. The object in this APOD is not a planetary nebula, and its structure probably comes about by very different mechanisms.neufer wrote:You probably have the basic general idea correct.
However, it is very long road from having a correct basic general idea
to explaining the bewildering variety of observed Planetary Nebula.
Almost certainly, the structure seen in supernova remnants derives from asymmetries in the parent star or star system, which includes the fact that there is an axis of rotation, and a magnetic axis. The magnetic field is probably important in influencing the initial direction some material is ejected in. That said, I think that the magnetic field falls off rapidly, and is probably not a major factor in influencing subsequent structure.Interested Observer wrote:Does anyone else, besides me, think the rings are bubbles of superheated gas which are escaping along the field lines of the star's magnetic poles?
I'm guessing that it is strongly connected to planetary nebula except that it is a "planetary nebula" made visible by a supernova/neutron star rather than a by UV radiation from a white dwarf.Chris Peterson wrote:It is perhaps confusing to introduce planetary nebulas here. The object in this APOD is not a planetary nebula, and its structure probably comes about by very different mechanisms.neufer wrote:
You probably have the basic general idea correct.
However, it is very long road from having a correct basic general idea
to explaining the bewildering variety of observed Planetary Nebula.
I don't doubt that there are at least some similar mechanisms involved in producing the range of structures observed around both planetary nebulas and supernovas. But that doesn't change the fact that there is no planetary nebula here. Planetary nebulas are the result of a series of gentle expulsions of material from a lower mass star over a long period. The material in a supernova remnant is ejected violently and suddenly. High mass stars don't produce planetary nebulas.neufer wrote:I'm guessing that it is strongly connected to planetary nebula except that it is a "planetary nebula" made visible by a supernova/neutron star rather than a by UV radiation from a white dwarf.
High mass stars don't produce the white dwarfs necessary to fully illuminate planetary nebulas.Chris Peterson wrote:I don't doubt that there are at least some similar mechanisms involved in producing the range of structures observed around both planetary nebulas and supernovas. But that doesn't change the fact that there is no planetary nebula here. Planetary nebulas are the result of a series of gentle expulsions of material from a lower mass star over a long period. The material in a supernova remnant is ejected violently and suddenly. High mass stars don't produce planetary nebulas.neufer wrote:
I'm guessing that [the rings are] strongly connected to planetary nebula except that it is a "planetary nebula"
made visible by a supernova/neutron star rather than a by UV radiation from a white dwarf.
Exactly. Nor do they produce planetary nebulas to be illuminated.neufer wrote:High mass stars don't produce the white dwarfs necessary to fully illuminate planetary nebulas.
Semantics (again).Chris Peterson wrote:Exactly. Nor do they produce planetary nebulas to be illuminated.neufer wrote:
High mass stars don't produce the white dwarfs necessary to fully illuminate planetary nebulas.
Sorry, I'm really trying to understand the point you're trying to make, and I can't. I don't follow how you are connecting planetary nebulas to this APOD.neufer wrote:Semantics (again).Exactly. Nor do they produce planetary nebulas to be illuminated.High mass stars don't produce the white dwarfs necessary to fully illuminate planetary nebulas.
I believe that is a first for me.Chris Peterson wrote:
Sorry, I'm really trying to understand the point you're trying to make, and I can't.
If nothing else:Chris Peterson wrote:
I don't follow how you are connecting planetary nebulas to this APOD.
Planetary nebulas are produced by successive waves of shells shed by low to middle mass stars at the end of their lives, which are then illuminated by the core of that star once it is exposed.
SN 1987A was a Type II (core collapse) supernova. The progenitor is now a neutron star or black hole, and is not illuminating the supernova remnant. Thus, this APOD is unrelated to planetary nebulas in two ways: a supernova, by definition, can't produce a planetary nebula, and a planetary nebula requires a central illumination source, which is not present in 1987A.
Perhaps you could help me to understand how discussing planetary nebulas makes anything about 1987A easier to understand.
The fastest gaseous parts of the 1987 supernova explosion rammed into slow debris from 20,000 years ago.Interested Observer wrote:
This hypothesis seems to explain the observed phenomena, hence my head-scratching at the use of the word "mysterious". To my mind, the real mystery is: why has the equatorial ring started glowing? Any thoughts?
I think that the actual situation is extremely complex, and can't be broken down into any simple scenario like this. AFAIK the research that has been done on structure in supernovas has largely involved the use of supercomputers and finite-element analysis. Models show these lobed structures emerging as the result of an extremely complex interplay between many parameters. You can't point at any single thing to explain it.Interested Observer wrote:The hypothesis I was suggesting is that, during the "rebound" phase of the core collapse, matter escapes more easily from the magnetic poles of the star than from its equator...
Interested Observer wrote:
Is it believed that the rings formed prior to the star going supernova? That is truly mysterious.
Probably based upon Doppler measurements of radial speed.Interested Observer wrote:
How did the number "20,000 years ago" come about?
Is that based on computer modelling?
Interested Observer wrote:
Just as an aside, how's this for some symmetry? The large lobed structures observed as supernovae remnants look very similar to one type of electron orbital(dz2). Weird.