Discussion Overview
The discussion revolves around the identification of mysterious objects observed near Orion, specifically focusing on images captured using the Aladin astro software. Participants explore potential explanations for these objects, considering various optical phenomena and telescope artifacts.
Discussion Character
- Exploratory
- Technical explanation
- Conceptual clarification
- Debate/contested
Main Points Raised
- One participant suggests the objects may be internal reflections from the telescope, referring to them as "ghosts" associated with bright stars.
- Another participant confirms this view, noting that the dark region in the images corresponds to the secondary mirror and its supports.
- Several participants discuss the specific optical characteristics of the telescope, identifying it as a reflector and speculating on the type (Schmidt-Cass, Newtonian, or Dobsonian).
- Context is provided regarding the source of the images, which are from the Digitized Sky Survey, indicating they may include artifacts from the imaging process.
- There is a discussion about the relationship between the observed objects and bright stars, particularly Sirius and Rigel, as potential sources of the reflections.
- Participants inquire about the conditions under which internal reflections occur and whether similar artifacts can arise from other bright sources, such as quasars.
- One participant mentions that while any object can produce a ghost image, the visibility of such images diminishes with the object's brightness.
Areas of Agreement / Disagreement
Participants generally agree that the observed objects are likely internal reflections or "ghosts" caused by bright stars. However, there is ongoing exploration regarding the specifics of these reflections and their relationship to different types of celestial objects, indicating some unresolved aspects of the discussion.
Contextual Notes
Participants note that the optical system's imperfections lead to unintended reflections, and the visibility of ghost images is contingent on the brightness of the source. The discussion does not resolve the technical details of how these reflections are produced in various contexts.
Who May Find This Useful
Astronomy enthusiasts, astrophotographers, and individuals interested in optical phenomena in telescopes may find this discussion relevant.