What is the density of the Carina Nebula?

  • Context: Undergrad 
  • Thread starter Thread starter ozipin
  • Start date Start date
  • Tags Tags
    Density Nebula
Click For Summary
SUMMARY

The Carina Nebula has a density significantly higher than the previously mentioned few atoms per cubic meter, which is close to the average density of the intergalactic medium. The average density of a Giant Molecular Cloud (GMC) like the Carina Nebula is estimated to be between 100 to 1,000 atoms per cubic centimeter, compared to the interstellar medium's average of one atom per cubic centimeter. Scholarly references indicate that the density in the vicinity of the Sun is approximately 1.5 × 10-26 g cm-3 in the hot medium, with denser regions reaching up to 2 × 10-20 - 2 × 10-18 g cm-3. Accurate translation of column density to actual density requires specialized knowledge.

PREREQUISITES
  • Understanding of Giant Molecular Clouds (GMCs)
  • Familiarity with interstellar medium density measurements
  • Knowledge of column density and its implications
  • Basic grasp of astrophysical mass density units (g cm-3)
NEXT STEPS
  • Research the properties and characteristics of Giant Molecular Clouds (GMCs)
  • Study the differences between intergalactic and interstellar medium densities
  • Learn about methods for translating column density to physical density
  • Explore scholarly articles on interstellar matter density variations
USEFUL FOR

Astronomy enthusiasts, astrophysicists, and students studying interstellar matter and nebulae will benefit from this discussion.

ozipin
Messages
1
Reaction score
1
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.
 
  • Informative
Likes   Reactions: Delta2
Astronomy news on Phys.org
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.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 6 ·
Replies
6
Views
2K
Replies
5
Views
2K
  • · Replies 6 ·
Replies
6
Views
4K
  • · Replies 29 ·
Replies
29
Views
1K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 20 ·
Replies
20
Views
4K
  • · Replies 7 ·
Replies
7
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 5 ·
Replies
5
Views
4K