Discussion Overview
The discussion revolves around the characteristics and composition of superclusters, specifically focusing on the number of galaxies within them. Participants explore the definition of superclusters, the specific case of the Laniakea supercluster, and the implications of varying estimates of galaxy counts.
Discussion Character
- Exploratory, Technical explanation, Debate/contested
Main Points Raised
- One participant questions the average number of galaxies in a supercluster, noting that Laniakea has 47,000 galaxies and asks if this is considered large or small.
- Another participant cites Wikipedia, suggesting that if there are approximately 2 trillion galaxies in the observable universe and around 10 million superclusters, then an average supercluster might contain at least 200,000 galaxies.
- There is mention of conflicting information regarding the number of galaxies in Laniakea, with estimates ranging from 100,000 to 150,000 galaxies, leading to a discussion about the normalcy of Laniakea's size.
- A participant highlights the complexity of counting galaxies, referencing the Milky Way's history of consuming other galaxies and noting the discovery of Antlia 2, suggesting that galaxy counts in superclusters may be incomplete due to observational limitations.
- Another participant reiterates the conflicting information about the number of galaxies in the local supercluster, emphasizing the need for clarity.
- Discussion includes the hierarchical structure of superclusters, with the Virgo Cluster being part of the Virgo Supercluster, which is in turn part of Laniakea, and how galaxies are grouped by their motion rather than their spatial location.
Areas of Agreement / Disagreement
Participants express uncertainty regarding the exact number of galaxies in superclusters, with multiple competing views on the estimates for Laniakea and the implications of these figures. The discussion remains unresolved with no consensus on the average number of galaxies in superclusters.
Contextual Notes
Participants note limitations in the accuracy of galaxy counts due to observational challenges, such as the "zone of avoidance" caused by dust in the Milky Way, which may obscure parts of Laniakea.