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.