Discussion Overview
The discussion revolves around estimates of the number of galaxies in the observable universe, particularly in relation to observations made by the Herschel Space Observatory. Participants explore the implications of these observations and compare them to other significant astronomical surveys, such as the Hubble Ultra Deep Field.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant mentions an article by Steve Eales that suggests imaging the entire celestial sphere with Herschel could imply around 23 million galaxies, prompting a question about the actual estimated total number of galaxies.
- Another participant cites estimates of approximately 10^11 galaxies in the observable universe, noting that Herschel primarily observes relatively nearby galaxies, which may account for the lower number suggested by the first participant.
- The Hubble Ultra Deep Field is referenced as a benchmark for galaxy counts, with about 10,000 galaxies observed in a very small portion of the sky, indicating a much larger total when extrapolated.
- A participant expresses admiration for the Herschel image, highlighting its significance in showing galaxies whose light has traveled a significant portion of the universe's age.
- There is a request for a link to the specific Herschel image, with suggestions for where to find it.
- Another participant discusses the density of galaxies observed by Herschel, noting it represents only a fraction of the total density and reflects on why the night sky is not as bright as expected, attributing this to the processing of raw data and the effects of cosmic expansion.
- The same participant speculates about the role of the Virial Theorem in understanding the dynamics of galaxy distributions and their gravitational interactions.
Areas of Agreement / Disagreement
Participants express varying estimates of the number of galaxies, with some agreeing on the rough figure of 10^11 while others propose different interpretations based on Herschel's observations. The discussion remains unresolved regarding the implications of these observations and the reasons behind the perceived brightness of the night sky.
Contextual Notes
There are limitations in the discussion regarding the assumptions made about galaxy density and the effects of cosmic expansion on observed brightness. The calculations and interpretations of data from Herschel and Hubble are not fully resolved.