What is the density of the Carina Nebula?

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Discussion Overview

The discussion revolves around the density of the Carina Nebula, comparing it to other astronomical densities such as those found in the intergalactic medium and interstellar medium. Participants explore the implications of these densities and seek clarification on the topic.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions the claim that the Carina Nebula has a density of a few atoms per cubic meter, suggesting it seems too low compared to known densities of the interstellar medium and planetary nebulae.
  • Another participant references a source that provides column densities consistent with NASA figures, implying that these figures may clarify the density issue.
  • A participant notes that the Carina Nebula is classified as a Giant Molecular Cloud (GMC) and cites a Wikipedia article indicating that GMCs have densities significantly greater than the average density in the solar vicinity.
  • One participant provides a scholarly reference discussing the density of interstellar matter, emphasizing that the density of the Carina Nebula should be much higher than the average density of the universe.
  • There is mention of the complexity involved in translating column density to physical density, with some uncertainty about its utility for the original poster's understanding.
  • A later reply reiterates the challenge of translating column density to density, noting that assumptions about the nebula's depth may affect the interpretation.

Areas of Agreement / Disagreement

Participants express differing views on the density of the Carina Nebula, with no consensus reached on the accuracy of the initial claim regarding its density. Multiple competing perspectives on the topic remain present.

Contextual Notes

Some participants highlight the need for specialist knowledge to translate column densities into physical densities, indicating that assumptions about the nebula's dimensions may influence the conclusions drawn.

ozipin
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In a James Webb photo thread, someone posted that the Carina Nebula has a density of a few atoms per cubic meter. This seems off to me, as this is close to the average density of the intergalactic medium of one atom per cubic meter, which is much less than the interstellar medium average density of one atom per cubic centimeter, which is much less than the average density of a planetary nebular (100-10,000 atoms per cubic centimeter). But I can't find any information on the web to help me understand this better.
 
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I believe the Carina nebula is what is called a Giant Molecular Cloud (GMC). The Wikipedia article says the following: "Whereas the average density in the solar vicinity is one particle per cubic centimetre, the average density of a GMC is a hundred to a thousand times as great." The value of one atom/cubic meter is about the average mass density of the universe as a whole, so is much too low for even the vicinity of the sun, let alone a dense nebula like Carina.

For a more scholarly reference, this paper has the following quote, "By terrestrial standards, the interstellar matter is exceedingly tenuous: in the vicinity of the Sun, its density varies from ∼ 1.5 × 10−26 g cm−3 in the hot medium to ∼ 2 × 10−20 − 2 × 10−18 g cm−3 in the densest molecular regions, with an average of about 2.7 × 10−24 g cm−3 (see next subsections). This mass density, which corresponds to approximately one hydrogen atom per cubic centimeter, is over twenty orders of magnitude smaller than in the Earth’s lower atmosphere."
 
Ibix said:
which gives column densities
Translating column density to density requires some specialist knowledge, though. I'm not sure it helps the OP by itself.
 
Bandersnatch said:
Translating column density to density requires some specialist knowledge, though. I'm not sure it helps the OP by itself.
Sure - the reddit poster translated the column densities into a density range on an assumption that the nebula was about 15ly deep from our perspective.
 

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