Discussion Overview
The discussion centers on the speed of the Milky Way galaxy relative to the cosmic microwave background radiation (CMBR), specifically focusing on its motion through the universe rather than its rotational speed. Participants explore various measurements and sources related to this topic.
Discussion Character
- Exploratory
- Technical explanation
- Debate/contested
Main Points Raised
- One participant inquires about the speed of the Milky Way relative to the CMBR, emphasizing that they are not interested in its rotation speed.
- Another participant cites a measurement indicating that the Solar System travels at approximately 390 km/sec relative to the CMB, and suggests that the Milky Way's speed could be around 603 km/sec relative to the CMB, although they express disagreement with the idea that the CMBR defines a preferred frame of reference.
- A different participant mentions a 2002 source that reports the speed of the Local Group as approximately 627 km/sec towards the constellation Crater, suggesting that the Milky Way's speed could be similar.
- This participant also notes that part of the observed motion could be influenced by temperature fluctuations in the CMB, but asserts that this does not significantly alter the rough estimate of about 600 km/s.
- They further clarify that the Milky Way's motion relative to the center of mass of the Local Group is small, implying that equating the Milky Way's speed with that of the Local Group is reasonable.
- Additional references to other threads and sources are provided, including a link to an Astronomy Picture of the Day that discusses the Local Group's speed, although it does not specify the Milky Way's speed directly.
Areas of Agreement / Disagreement
Participants express varying views on the exact speed of the Milky Way relative to the CMBR, with some suggesting values around 600 km/s while others cite different measurements. There is no consensus on a definitive speed or the implications of the CMBR as a reference frame.
Contextual Notes
There are limitations in the discussion regarding the accuracy of the measurements cited, the dependence on definitions of reference frames, and the potential influence of CMB temperature fluctuations on observed velocities. These factors remain unresolved.