We Know Less About CDM Than We Did Before

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Discussion Overview

The discussion revolves around the complexities of dark matter distribution in dwarf galaxies, particularly in light of recent studies that suggest a lack of clarity in understanding these systems. Participants explore the implications of star movement in dwarf galaxies compared to spiral galaxies and the role of dark matter in these dynamics.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants reference a study indicating that understanding of dark matter has decreased, highlighting the unusual movement of stars in dwarf galaxies, which swarm rather than follow circular orbits.
  • One participant expresses confusion regarding the analogy of stars swarming like bees and seeks clarification on this behavior.
  • Another participant criticizes the use of analogies in scientific explanations, asserting that stars in dwarf galaxies have elliptical orbits that are not aligned in a single plane, contrasting them with spiral galaxies.
  • A participant questions the assumption that dark matter would clump at the center of dwarf galaxies, suggesting that without a significant rotational aspect, dark matter might be more uniformly distributed.
  • Some participants challenge the notion that dwarf galaxies lack a center of mass, asserting that they do possess one and questioning the influence of supermassive black holes on galaxy rotation.

Areas of Agreement / Disagreement

Participants express differing views on the movement of stars in dwarf galaxies and the implications for dark matter distribution. There is no consensus on the role of center of mass or the influence of supermassive black holes in these systems.

Contextual Notes

Participants note the limitations of analogies used in scientific discourse and the potential for misinterpretation. The discussion reflects varying levels of understanding regarding the dynamics of dwarf galaxies and dark matter.

Dotini
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http://www.sciencedaily.com/releases/2011/10/111017124344.htm

"After completing this study, we know less about dark matter than we did before," said lead author Matt Walker, a Hubble Fellow at the Harvard-Smithsonian Center for Astrophysics.

"Stars in a dwarf galaxy swarm like bees in a beehive instead of moving in nice, circular orbits like a spiral galaxy," explained Peñarrubia. "That makes it much more challenging to determine the distribution of dark matter."


Respectfully submitted,
Steve
 
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Dotini said:
http://www.sciencedaily.com/releases/2011/10/111017124344.htm
"Stars in a dwarf galaxy swarm like bees in a beehive instead of moving in nice, circular orbits like a spiral galaxy," explained Peñarrubia.

I find it bemusing that stars would swarm like bees in a hive instead of orbiting. Can anyone explain this, please?

Respectfully,
Steve
 
Ugh, I hate it when scientists use bad analogies. He doesn't mean that the stars move around randomly. The stars have elliptical orbits but they're not aligned in a plane like in spiral galaxies. The orbital planes of the stars' orbits are randomly aligned. Similar to a globular cluster.
 
Without the rotational aspect that spiral galaxies have (presumably created by Super-massive black holes in the center), why would one assume that the dark matter would clump at the center? The rotation creates a center of mass in the galaxy where I would presume the dark matter would start to accumulate, bringing together the normal matter, then distributing it from there.

Wouldn't you assume that in a dwarf galaxy, basically without a center of mass, the dark matter be more uniformly placed?
 
Dr_Morbius said:
Ugh, I hate it when scientists use bad analogies. He doesn't mean that the stars move around randomly. The stars have elliptical orbits but they're not aligned in a plane like in spiral galaxies. The orbital planes of the stars' orbits are randomly aligned. Similar to a globular cluster.

Here's yet another scientist who uses the same exact bad analogy:

"If you watched a time-lapse movie of our galaxy, you would see the swarm of dwarf galaxies buzzing around it like bees around a beehive," said astronomer Anna Frebel of the Harvard-Smithsonian Center for Astrophysics, who led the study that found the old star. "Over time, those galaxies smashed together and mingled their stars to make one large galaxy ? the Milky Way."
http://www.space.com/7996-milky-cannibal-ancient-star-confirms.html

Slightly off-topic, are the movements of bees random, or are they purposeful or according to some "program"?

Respectfully submitted,
Steve
 
Last edited:
Kronos5253 said:
Without the rotational aspect that spiral galaxies have (presumably created by Super-massive black holes in the center), why would one assume that the dark matter would clump at the center? The rotation creates a center of mass in the galaxy where I would presume the dark matter would start to accumulate, bringing together the normal matter, then distributing it from there.

Wouldn't you assume that in a dwarf galaxy, basically without a center of mass, the dark matter be more uniformly placed?

I still kind of want an answer for this. I'm curious.
 
Why wouldn't a a dwarf galaxy have a center of mass? It absolutely must and does have one. I also don't know how much the black hole really affects the entire galaxy. I don't think it has much to do with the rotation in a spiral galaxy.
 

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