APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

Post a reply


This question is a means of preventing automated form submissions by spambots.
Smilies
:D :) :ssmile: :( :o :shock: :? 8-) :lol2: :x :P :oops: :cry: :evil: :roll: :wink: :!: :?: :idea: :arrow: :| :mrgreen:
View more smilies

BBCode is ON
[img] is ON
[url] is ON
Smilies are ON

Topic review
   

Expand view Topic review: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Chris Peterson » Sat Jan 02, 2016 5:16 pm

sallyseaver wrote:I hope it does not tax your patience too much, but I'd like to try to explain more about what I think could happen with dust lanes that are heavily populated with ferromagnetic material.
But dust lanes are not heavily populated with ferromagnetic material. Indeed, they are not heavily populated with dust. Dust lanes are actually gas lanes, slightly contaminated with dust- all of which is overwhelmingly dominated by self-gravitation from hydrogen. And there is no strong magnetic field, nor a significant field gradient to generate motion. At the least, if galactic magnetic fields were resulting in the motion of iron and nickel, we'd see material gradients... which we don't.

So again, I'm unaware of any examples of bulk movement of dust in galaxies caused by magnetic fields. We only see the impact of magnetic fields in two places- locally (as around stars and small star forming regions), and over large distances in polarization effects and the like caused by particle orientation in weak fields.

You may have ideas about how you think some material should behave in galactic magnetic fields, but observation demonstrates that it doesn't, and solid theory explains why that is.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Sat Jan 02, 2016 5:01 pm

sallyseaver wrote:
Below 1043 K, the Curie temperature, ALL the magnetic domains (or magnetic moments) in ferromagnetic material align in the same direction. I figure these dust lanes are well below 1043 K.
The thermal equilibrium temperature of dust 1 AU from our Sun
should approximately the same as that of the Earth ~ 250 K.

The brightest stars are ~10,000 as luminous as the Sun
requiring a 1 AU dust temperature 10 times higher ~ 2500 K.
The Stefan–Boltzmann law states that the total energy radiated per unit surface area
of a black body across all wavelengths per unit time is directly proportional to
the fourth power of the black body's thermodynamic temperature T: Image
Therefore, dust further than ~ 6 AU from any star should be colder than 1020 K (~2500/√6)

Dust further than ~ 1 light year from any star should be colder than 10 K.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by sallyseaver » Sat Jan 02, 2016 6:55 am

I hope it does not tax your patience too much, but I'd like to try to explain more about what I think could happen with dust lanes that are heavily populated with ferromagnetic material.

So we are looking at the M96 galaxy in the APOD associated with this thread [September 21, 2015], and I put forward Centaurus A [APOD Nov 19, 2015] as another with dust lanes that are above or below the main disk of galaxy material.
Image Image
What temperature do you think the outlying dust lanes are?

Below 1043 K, the Curie temperature, ALL the magnetic domains (or magnetic moments) in ferromagnetic material align in the same direction. I figure these dust lanes are well below 1043 K.
Image
The magnetic field generated by the circular paths of charged particles around the center of the galaxy make a magnetic field like what is generated by a current ring [shown here]. The green arrows show the direction of the north-south pole alignment of the galaxy's magnetic field. Then in the presence of this strong galactic magnetic field, the poles associated with the tiny domains in the ferromagnetic material align in the opposite direction (black arrows). [Otherwise, the alignment of like poles cause a repulsive force and the system would not be in a steady state.]

The charged particles that are circling the center of the galaxy are actually in a spiral. Sort of like groves on an LP record, there are paths close to each other at different radii from the center. Thus, the galaxy's magnetic field is not as stable as the one pictured that is due to current in a wire circle of a fixed radius. The galaxy's magnetic field can have turbulence that is felt by the outer dust lanes as a wobbling of the magnetic field. Or perhaps some of the outer rings of charged particles (galactic current rings) actually twist with respect to the inner rings. And in this case, the main disc of non-magnetic material stays put according to its initial angular momentum, but the ferromagnetic material gets a small push below or above depending on the wobble of the magnetic field experienced by the dust.
Image
The European Space Agnecy's Planck Satellite has made observations regarding the galactic magnetic fields for the Milky Way, and it does show turbulence. See APOD for Jan 27, 2015 and the article it references: "Twisted, Tangled and Turbulent: Magnetic Fields in the Milky Way" http://phenomena.nationalgeographic.com ... milky-way/
Image

Here is an image of the Milky Way from the Spitzer space telescope. It's infrared, but there are opaque regions that I think are optical representations of dust. [APOD March 08,2015]

Image

Or here is another that shows dust outside of the center disk, I believe. [APOD July 24, 2014]

Image

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Chris Peterson » Fri Jan 01, 2016 5:49 am

sallyseaver wrote:
Chris Peterson wrote:I am not aware of any example of bulk dust movement in galaxies due to large-scale magnetic fields. Dust moves due to gravitational fields and due to collisions with photons and with charged particles.
Don't you think that classical physics is applicable to ferromagnetic material in a system with magnetic fields?
It's perfectly applicable. Which doesn't change my observation.
Do you contest the idea that galaxies have magnetic fields?
Not at all. Only that the fields are strong enough to have a significant impact on the position of dust (as opposed to the orientation of small particles), especially given the much greater effect of other forces.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Fri Jan 01, 2016 5:33 am


sallyseaver wrote:
Chris Peterson wrote:
I am not aware of any example of bulk dust movement in galaxies due to large-scale magnetic fields.
Don't you think that classical physics is applicable to ferromagnetic material in a system with magnetic fields?
Like iron filings, ferromagnetic material will certainly line up with magnetic fields but they will only be attracted by gradients in those magnetic fields. Large-scale galactic magnetic fields really have no gradients to speak of.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by sallyseaver » Fri Jan 01, 2016 4:23 am

Chris Peterson wrote:
sallyseaver wrote:For dv, there is another force component due to magnetism and this force component could affect the movement of dv so that it can rise above or below the disc of the rotating dv-nf elements.

I think that Spiral Galaxy M96 [APOD 2015 Sep 21] shows this and so does Centaurus A NGC 5128 [APOD 2015 Nov 19]
http://apod.nasa.gov/apod/image/1511/Ce ... ESO-LL.jpg
I am not aware of any example of bulk dust movement in galaxies due to large-scale magnetic fields. Dust moves due to gravitational fields and due to collisions with photons and with charged particles.
Don't you think that classical physics is applicable to ferromagnetic material in a system with magnetic fields? Or is your response due to not reading any peer-reviewed papers on this phenomenon?

Regarding the presence of iron in dust grains, a study of 33 planetary nebulae (granted these are not spiral galaxies), this article from the Astrophysical Journal http://iopscience.iop.org/article/10.10 ... 0-40-2-108 claims that more than 90% of [a planetary nebula's] iron atoms are condensed onto dust grains. Iron is ferromagnetic, as you know. It makes sense that iron atoms would not remain in gas form but rather gravitate towards the clumps of atoms in dust grains. And it makes sense to me that iron would present optically as dark and opaque.

Near as I can tell, when astrophysicists see wisps of brown dust above or below the main disk of the galaxy, then they assume that there has been a collision of galaxies. But I assumed that this was just because they were not in familiar with the idea that brown dust could be ferromagnetic and thus subject to magnetic forces present in any galaxy.

Do you contest the idea that galaxies have magnetic fields? Near the black hole at the center of a spiral galaxy, ions and atoms are traveling rapidly in a circular path. Most atoms (other than those of inert gases) have a slight imbalance of charge. When you get ions and atoms traveling rapidly in a circular path, they create a magnetic field (known physics). ...anyway, Art has provided solid scholar-approved evidence regarding the presence of a magnetic fieldin a spiral galaxy.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Chris Peterson » Thu Dec 31, 2015 11:51 pm

sallyseaver wrote:For dv, there is another force component due to magnetism and this force component could affect the movement of dv so that it can rise above or below the disc of the rotating dv-nf elements.

I think that Spiral Galaxy M96 [APOD 2015 Sep 21] shows this and so does Centaurus A NGC 5128 [APOD 2015 Nov 19]
http://apod.nasa.gov/apod/image/1511/Ce ... ESO-LL.jpg
I am not aware of any example of bulk dust movement in galaxies due to large-scale magnetic fields. Dust moves due to gravitational fields and due to collisions with photons and with charged particles.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by sallyseaver » Thu Dec 31, 2015 11:41 pm

I am sad that I missed out on the fascinating discussion of magnetism and dust back in September. I was refreshing my page to see if there were responses when the discussion had moved on to a second page... now, I know better. :)

Thank you very much Ann, Art and Chris for more discussion and good information.
Chris, I find it very satisfying to receive this concise telling of the relevant relationships:
Chris Peterson wrote:accretion is only spherical if the material doesn't interact like a fluid, or if the angular momentum is very low.
Ann and Art, I appreciate more dialog about the role of magnetic fields and dust. And Art, thanks so much for the great image and academic reference.
neufer wrote:
Chris Peterson wrote:
sallyseaver wrote:
IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element) with it's own magnetic properties so that it does not interact in the same way as the other orbital material?
Iron is a trace component in interstellar dust. However, dust need not be composed of ferromagnetic material to be influenced by magnetic fields.
But is dust dynamically influenced by magnetic fields
(other than simply having its dipole reoriented) :?: :arrow:
http://www.scholarpedia.org/article/Galactic_magnetic_fields wrote:
Galactic magnetic fields by Dr. Rainer Beck,
Max-Planck-Institut für Radioastronomie, Bonn, Germany

<<Galactic magnetic fields can be observed in the optical range via starlight which is polarized by interstellar dust grains in the foreground. These grains are elongated and can be aligned by magnetic fields, where the major axis becomes perpendicular to the field lines. Measurements of many stars revealed a general picture of the magnetic field in the Milky Way near the Sun. Aligned dust grains also emit polarized infrared emission, which is very useful to show magnetic fields in dust clouds in the Milky Way. In prominent spiral arms the field strength can be up to 25 μG, in regions where also cold gas and dust are concentrated.>>
I am very happy with the good information presented to-date, but I would like to further explore this. Please see what you think about the following
Image
Take a small cube of particles in a spiral galaxy, dv. In dv, we posit a high concentration of dust that has ferromagnetic properties. Now, take another small cube of particles from the same spiral galaxy, dv-nf, such that it does not contain ferromagnetic properties. For both dv and dv-nf, a classical mechanics force diagram would show the gravity vector pointing toward the center of the galaxy and the momentum vector pointing perpendicular to the gravity vector in the tangent of the directon of motion. (like where the green "v" arrow meets the "r" radius in the following picture... I'm borrowing an image rather than making my own)


For dv, there is another force component due to magnetism and this force component could affect the movement of dv so that it can rise above or below the disc of the rotating dv-nf elements.

I think that Spiral Galaxy M96 [APOD 2015 Sep 21] shows this and so does Centaurus A NGC 5128 [APOD 2015 Nov 19]
http://apod.nasa.gov/apod/image/1511/Ce ... ESO-LL.jpg

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Fri Sep 25, 2015 6:17 pm

Ann wrote:
neufer wrote:
starsurfer wrote:
I wonder what Superman's x-ray vision of the universe would be like? :lol2:
http://www.xray.mpe.mpg.de/cgi-bin/rosat/rosat-survey
I think I can see Superman flying low at lower right, cape ablaze. Unless that is the Vela pulsar.
  • It's a ROSAT test:
https://en.wikipedia.org/wiki/Klecksography#History wrote:
<<Klecksography is the Art of making images from inkblots. Justinus Kerner (18 September 1786 – 21 February 1862) invented this technique when he started accidentally dropping blots of ink onto paper due to failing eyesight. Instead of throwing them away, he found that intriguing shapes appeared if he unfolded the papers. He elaborated these shapes into intricate cartoons and used them to illustrate his poems. Kerner began a collection of klecksographs and poetry in 1857 titled Klesksographien Since the 1890s, psychologists have used it as a tool for studying the subconscious, most famously Hermann Rorschach in his Rorschach inkblot test. [Klecksograph] inkblots tend to resemble images because of apophenia, the human tendency to see patterns in nature.>>

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Ann » Fri Sep 25, 2015 4:20 pm

neufer wrote:
starsurfer wrote:
I wonder what Superman's x-ray vision of the universe would be like? :lol2:
I think I can see Superman flying low at lower right, cape ablaze.

Unless that is the Vela pulsar.

Ann

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Fri Sep 25, 2015 1:24 pm

starsurfer wrote:
I wonder what Superman's x-ray vision of the universe would be like? :lol2:

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by starsurfer » Fri Sep 25, 2015 1:12 pm

geckzilla wrote:
FullMoon wrote:What a mesmerizing galaxy. Taken by the ol' Hubble, too.
While I don't know much about this particular galaxy, I've always found the outer universe intriguing. Perhaps someday we'll be able to explore it with our own eyes.
We are exploring it with our own eyes, augmented by cameras! Without some kind of camera to aid us, our own eyes... well, I'd liken it to say we can fly about as well as a bird with our own arms as we can see the Universe with our own eyes.
I wonder what Superman's x-ray vision of the universe would be like? :lol2:

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by geckzilla » Fri Sep 25, 2015 12:38 pm

FullMoon wrote:What a mesmerizing galaxy. Taken by the ol' Hubble, too.
While I don't know much about this particular galaxy, I've always found the outer universe intriguing. Perhaps someday we'll be able to explore it with our own eyes.
We are exploring it with our own eyes, augmented by cameras! Without some kind of camera to aid us, our own eyes... well, I'd liken it to say we can fly about as well as a bird with our own arms as we can see the Universe with our own eyes.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by FullMoon » Fri Sep 25, 2015 3:11 am

What a mesmerizing galaxy. Taken by the ol' Hubble, too.
While I don't know much about this particular galaxy, I've always found the outer universe intriguing. Perhaps someday we'll be able to explore it with our own eyes.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Ann » Fri Sep 25, 2015 12:00 am

Interesting image, Art. The magnetic field of M51 appears to follow the dusty features pretty well. Could it be that large dust patches are typically more magnetized than relatively dust-free zones? Could it be that the strange dust lane of M96 really has a stronger magnetic field that its relatively dust-less yellow surroundings?

But if so, I would certainly guess that it wasn't magnetism that created that dust lane out of nothing, so to speak, but rather that an external factor such as a merger gave rise to the dust lane, and at the same time the violence of the merger created new centers of magnetism in the galaxy. Now, hundreds of millions of years after the merger, the lopsided dust lane of M96 might still carry the imprint of the magnetism that resulted from the merger.

But that would make the magnetism involved a consequence and not a cause of that dust lane.

Ann

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Thu Sep 24, 2015 3:48 pm

Chris Peterson wrote:
sallyseaver wrote:
IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element) with it's own magnetic properties so that it does not interact in the same way as the other orbital material?
Iron is a trace component in interstellar dust. However, dust need not be composed of ferromagnetic material to be influenced by magnetic fields.
But is dust dynamically influenced by magnetic fields
(other than simply having its dipole reoriented) :?: :arrow:
http://www.scholarpedia.org/article/Galactic_magnetic_fields wrote:
Galactic magnetic fields by Dr. Rainer Beck,
Max-Planck-Institut für Radioastronomie, Bonn, Germany

<<Galactic magnetic fields can be observed in the optical range via starlight which is polarized by interstellar dust grains in the foreground. These grains are elongated and can be aligned by magnetic fields, where the major axis becomes perpendicular to the field lines. Measurements of many stars revealed a general picture of the magnetic field in the Milky Way near the Sun. Aligned dust grains also emit polarized infrared emission, which is very useful to show magnetic fields in dust clouds in the Milky Way. In prominent spiral arms the field strength can be up to 25 μG, in regions where also cold gas and dust are concentrated.>>

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Chris Peterson » Thu Sep 24, 2015 1:45 pm

sallyseaver wrote:Chris, you said to be cautious about trying to infer 3D structure, but you can see the light from the middle of 96M shining through the swath of dust...
Maybe we can, maybe not. The intensity range seen in a galaxy has much greater dynamic range than our displays are capable of showing. So galaxy images are almost always processed in a way that modifies the actual intensity relationships. To really understand these kinds of images, we need to go back to the raw data.
Where does the original angular momentum come from? My understanding is that the original matter started like the big nebulae we see in other parts of the cosmos, like The Great Nebula (APOD Jan 19, 2015) or Gamma Cygni Nebula (APOD April 22, 2015) or the Carina Nebula. [from Big Bang TO stars TO the nebula material after stars die, i.e. planetary nebulae] Then if matter accretes around a denser part of the big nebula, it seems to me that the accretion would tend to be spherical. How does the angular momentum get started according to current thinking?
We don't know what galaxies formed out of, we don't really know how star formation and galaxy formation were connected, or what order they occurred in. But assuming that a galaxy formed out of something that can be thought of as a "nebula", meaning a vast region of somewhat condensed material, then the angular momentum is simply the net angular momentum of that material, which certainly would not be zero. As the huge "nebula" condensed, the rotational speed increased (because of conservation of angular momentum).

Accretion is only spherical if the material doesn't interact like a fluid, or if the angular momentum is very low. At high densities, however, that's exactly how it behaves.
IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element) with it's own magnetic properties so that it does not interact in the same way as the other orbital material?
Iron is a trace component in interstellar dust. However, dust need not be composed of ferromagnetic material to be influenced by magnetic fields.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Ann » Thu Sep 24, 2015 6:53 am

sallyseaver wrote:
And IF iron is a strong component of the brown dust clouds in our APOD picture of M96, then in cold space the microscopic domains would line up to have a macroscopic magnetic field that would influence its interaction with the other constituents of the outer ring of M96.
Oh, you are talking about magnetism!

Yes, astronomers are "upgrading" magnetism as a major player in the universe, or so I believe anyway. But personally I doubt that magnetism would normally give a galaxy a distorted shape. As for that dust lane of M96, you are of course correct that it contains iron as well as other elements. I'm sure the iron content is enough for this dust lane to "feel" the magnetic field of the galaxy.

But I don't see why this particular dust lane would be extremely rich in iron. The only thing that could make it so is if it was made of the debris of vast numbers of particularly metal-rich stars. I don't see why that would be the case, and why, say, Andromeda would not have dust lanes even richer in iron. Andromeda is larger than M96 and redder in overall color, suggesting it contains a larger population of very metal-rich stars. Also, when it comes to M96, I'm having a hard time imagining the sort of magnetic field that would have such a "lopsided" effect on the galaxy.

The universe is teeming with strangely shaped galaxies. I find it hard to believe that magnetism is acting on some parts on them and not on other parts, or that it affects some parts of the galaxies much more strongly than other parts. Why would that be?

We know that mergers give galaxies strange shapes. We also know that massive star formation in a galaxy can distort the entire galaxy. For example, galaxy NGC 1313 is distorted due to massive star formation primarily taking part in one of its arms. There is nothing strange about that. Star formation is always a localized phenomenon, never something that envelops an entire galaxy - certainly not in the nearby universe.

As for M96, I agree with Chris that a merger is by far the most likely explanation for its weird shape.

Ann

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by sallyseaver » Thu Sep 24, 2015 5:14 am

Ann wrote:
sallyseaver wrote:
Where does the original angular momentum come from? My understanding is that the original matter started like the big nebulae we see in other parts of the cosmos, like The Great Nebula (APOD Jan 19, 2015) or Gamma Cygni Nebula (APOD April 22, 2015) or the Carina Nebula.
No, the original matter did not start as a big nebula. Everything that exists in the universe was originally created in the Big Bang.
Ann, I am sorry for the misunderstanding. I know about the Big Bang theory, this is why I used the word "matter" and not the "precursors to matter." I was talking about the stage of development just prior to a galaxy forming, not from the very beginning of time. According to the current standard theory for the development of the universe, as I understand it, there have to be many stars formed and decayed before we get to the matter in a nebula which is a precursor to a galaxy. The idea is that elements heavier than hydrogen and helium had to be formed through the decay of stars. When a star dies it gives off a burst of electrons, helium nuclei (alpha particles) and a small percentage of high-z nuclei. Then through some mechanism, the output of the dying stars collect to form the a nebula. I know that nebulae are precursors to stars. I would think that a star-studded nebula would be a precursor to a galaxy.

Angular momentum is a conserved physical quantity. In the example of the skater, the skater uses force to create the initial angular momentum (as you say), then decreases the moment of inertia so that the angular speed increases. [magnitude of angular momentum = magnitude of moment-of-inertia x angular speed] The areas of the cosmos that turn into stars or galaxies are very big, we would see even a little bit of angular momentum around a common axis, like you can see the skater turning slowly at first. Also, the gases and dust are so sparse that there is a problem for getting a proper moment of inertia which is usually associated with a rigid moment-arm of some kind (e.g. skater's legs). The atomic and dust components are free to rotate in three dimensions, but to get to a big spiral, you have to get all components to orbit in such a way that they all have the same axis of rotation.

Ann wrote:
sallyseaver wrote: IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element)
Iron is not particularly abundant at all, compared with many other elements in the universe like oxygen, carbon and silicon. You can be sure that the dust in the universe is mostly made up of other elements than iron. Ann
The paper that I referred to says that Si and Mg can have similar contributions to dust grains as iron [Fe]; C and O can be even higher. Iron [Fe] is the 6th most abundant element according to current observations (which may be biased towards local observations/measurements). Admittedly this is only .11% of the total ON AVERAGE. But with heterogeneity of elements in nebulae, there can be a higher percent in localized regions. And IF iron is a strong component of the brown dust clouds in our APOD picture of M96, then in cold space the microscopic domains would line up to have a macroscopic magnetic field that would influence its interaction with the other constituents of the outer ring of M96.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Ann » Thu Sep 24, 2015 1:06 am

sallyseaver wrote:
Where does the original angular momentum come from? My understanding is that the original matter started like the big nebulae we see in other parts of the cosmos, like The Great Nebula (APOD Jan 19, 2015) or Gamma Cygni Nebula (APOD April 22, 2015) or the Carina Nebula.
No, the original matter did not start as a big nebula. Everything that exists in the universe was originally created in the Big Bang. The Big Bang was the sudden appearance and the immediate, violent expansion of the universe. From the beginning the universe was incredibly tiny, hot and dense. In the beginning it was far too hot and dense for matter and energy to be separate at all. When the universe had expanded and cooled to a certain degree, matter and energy could "decouple". That is when hydrogen first came into existence, the simplest form of ordinary matter. Helium, too, the second element, was created in the Big Bang, and also some lithium. This matter existed as a hot, dense, but expanding "soup".

The universe was certainly at least 400,000 years old, and possibly many million years old, before the first stars appeared. The first stars probably emerged out of nebulas, but the first nebulas were certainly very different from the typical nebulas of today. For one thing, the original nebulas contained no dust at all. Dust is made of elements more complex than hydrogen and helium (and lithium), but all such elements are created inside stars as rest products of their fusion of hydrogen and helium. Before the stars existed, there was no dust.

Where does the angular momentum come from? I'm not the correct person to answer that at all, but you must remember that the universe has always been teeming with energy, motion and outward expansion. Remember that the universe was always a place were outward expansion and inward-pressing gravity fought with one another. The distribution of matter and energy was always very slightly "uneven", encouraging the flow of matter away from more rarefied locations into more densely packed parts. Why should there not be angular momentum in such a dynamic place? What force could actually stop the angular momentum in the universe?

In any case, stars appears when a nebula shrinks and condenses under the influence of its own gravity. In other words, the nebula becomes smaller (or at least the part of the nebula that gives rise to the star becomes smaller). If the nebula is not perfectly "still", but contains some inherent rotation at all, this rotation will become much more pronounced as the nebula shrinks. Compared this with what figure skaters do to rotate, and to rotate faster. When they spin, they have to create their own initial rotation, but then they speed their rotation up by making themselves "smaller", by holding their arms and legs close to their "axis of rotation":
Click to play embedded YouTube video.
IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element)
Iron is not particularly abundant at all, compared with many other elements in the universe like oxygen, carbon and silicon. You can be sure that the dust in the universe is mostly made up of other elements than iron.

Ann

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by sallyseaver » Wed Sep 23, 2015 10:58 pm

Thank you Chris, Ann and Neufer. Your answsers are very helpful.
Chris Peterson wrote:
sallyseaver wrote:1. To me it looks like a big swath of dust is in a prominence above the plane of the main body of the spiral, above the main star-filled arm of the galaxy. Is this how other professional observers see it?
I'd be cautious trying to infer any 3D structure from images like this. Our visual systems did not evolve to analyze such scenes, and we can fall victim to many illusions that paint a distorted view of reality.
More regarding #1
Chris, you said to be cautious about trying to infer 3D structure, but you can see the light from the middle of 96M shining through the swath of dust, the dust that is making the image look asymmetrical, what I will call the dust prominence. If the dust prominence was in the plane of the galaxy, then I don't think the central illumination would be able to shine through it given the angle the picture was taken in.

So maybe you are saying that even though it looks like the light from the center is illuminating some of the dust rising up from the outer ring, that experienced observers are highly skeptical that this is the case, yes? Rather, the thinking is that the dust just is naturally a lighter color while lying flat in the plane of orbit?

Chris Peterson wrote:
sallyseaver wrote:2. What is the conventional explanation for why all matter in the presence of a black hole in the case of galaxies is supposed to be present as a flat spiral instead of a sphere?
Black holes have nothing to do with it. All that matters is gravitational attraction and the density of orbital material. If the density is high enough that the material can interact via electromagnetic forces, that material will flatten out (just like spinning pizza dough). If not, it won't, and will eventually settle into a spherical cloud. That's what's happening to all galaxies over time- whether or not they have a black hole at the center.
More regarding #2
Chris, your answer is very interesting and this satisfies some of my curiosity on this matter. But I have a couple follow-up questions.

a.)
Where does the original angular momentum come from? My understanding is that the original matter started like the big nebulae we see in other parts of the cosmos, like The Great Nebula (APOD Jan 19, 2015) or Gamma Cygni Nebula (APOD April 22, 2015) or the Carina Nebula. [from Big Bang TO stars TO the nebula material after stars die, i.e. planetary nebulae] Then if matter accretes around a denser part of the big nebula, it seems to me that the accretion would tend to be spherical. How does the angular momentum get started according to current thinking?

Angular momentum shows up for spiral and ring galaxies, also for the discs of material involved with star formation. The answers I have read might, in a wild stretch of imagination, produce angular momentum in one or two systems, but not the wide spread occurrence that is witnessed in the cosmos of going from no angular momentum to a system with angular momentum. What is the answer that has satisfied you?

b.)
IF there is a dust prominence in the absence of interacting with a different galaxy, then it could mean that the dust is primarily iron (an abundant element) with it's own magnetic properties so that it does not interact in the same way as the other orbital material? Would this be an acceptable explanation? This paper indicates that 90% or more of the iron in a planetary nebula is deposited in dust grains [arXiv:0812.1578v2 [astro-ph] 31 Mar 2009: "The Iron Abundance in Galactic Planetary Nebulae"]

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by neufer » Wed Sep 23, 2015 5:15 pm

Chris Peterson wrote:
neufer wrote:
  • Just to be clear...when Chris talks about "density" he means GAS "density"

    and "interact via electromagnetic forces" includes collisions of neutral gas particles:
And dust, although in most environments gas is by far the dominant player.
  • Collisions of dust with gas certainly...
    with mean free paths dependent only upon the gas density.
Dust/dust collisions would be rather rare by comparison I would think...
with mean free paths comparable to red light photon mean free paths with dust:

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by starsurfer » Wed Sep 23, 2015 4:35 pm

NGC3314 wrote:
starsurfer wrote:I always look out for background galaxies in galaxy images! I like 2MASX J00482185-2507365. It can be seen near the bottom right corner of this image of NGC 253 by CHART32.
That object showed up with obvious dust absorption in the ANGST Hubble survey of halo stars in nearby galaxies including NGC 253. ANGST principal investigator Julianne Danton chased Benne Holwerda and me down at a meeting to show us, knowing we did such occulting galaxy things, and thereby hangs a paper with detailed analysis. Such small galaxies with dust tendrils extending very far into their outskirts are rare but would explain some features of the far-IR statistics of galaxies, so one goal of projects such as the STARSMOG Hubble survey is finding more (we think we see a few more to date).

And that example has just been sitting there in many images of NGC 253 all along.
I forgot to mention that not only is it an interesting background galaxy but that it is also an overlapping pair. Another point to mention about Burbidge's Chain is that two of the galaxies might be connected together by a tidal bridge. These types of systems are quite rare and also visually striking.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Chris Peterson » Wed Sep 23, 2015 4:03 pm

neufer wrote:
  • Just to be clear...when Chris talks about "density" he means GAS "density"

    and "interact via electromagnetic forces" includes collisions of neutral gas particles:
And dust, although in most environments gas is by far the dominant player.

Re: APOD: Spiral Galaxy M96 from Hubble (2015 Sep 21)

by Ann » Wed Sep 23, 2015 3:53 pm

sallyseaver wrote:
How is NGC 3368 [M96] so different from the Andromeda Galaxy?
The Andromeda Galaxy. NASA's Wide-field Infrared Survey Explorer
I think the best answer is that there is no such thing as a "typical" spiral galaxy. Andromeda certainly isn't typical. Andromeda is a "ring galaxy" rather than a spiral galaxy, as you can see in this infrared image at left.

Like M96, Andromeda has in all probability been shaped by the mergers and collisions it has undergone. For Andromeda, (repeated) collisions with its small elliptical satellite galaxy M32 are probably responsible for creating rings like ripples in a pond. But the collisions and mergers that M96 has undergone have been different from those of Andromeda, and these two galaxies have also evolved differently.

Ann

Top