Portal:Radiation astronomy/Lesson/13

First superluminal source in Indus edit

 
This is an Aladin at SIMBAD image of ICRF J230343.5-680737, a Seyfert 1 galaxy in the constellation Indus. Credit: Aladin at SIMBAD.

The first superluminal source in Indus is unknown.

The field of superluminal astronomy is the result of observations and theories about superluminal sources detected in the sky above.

The first astronomical superluminal source discovered may have been the Sun.

But, superluminal rays from the Sun are intermingled with other radiation so that the Sun may appear as other than a primary source for superluminal rays.

The early use of sounding rockets and balloons to carry superluminal detectors high enough may have detected superluminal rays from the Sun as early as the 1940s.

This is a lesson in map reading, coordinate matching, and searching. It is also a project in the history of superluminal astronomy looking for the first astronomical superluminal source discovered in the constellation of Indus.

Nearly all the background you need to participate and learn by doing you've probably already been introduced to at a secondary level and perhaps even a primary education level.

Some of the material and information is at the college or university level, and as you progress in finding superluminal sources, you'll run into concepts and experimental tests that are an actual search.