Final Answer:
The evidence indicating that the energy source powering quasars is small in size lies in their rapid variability and the immense luminosity observed. This variability occurs on timescales as short as hours or days, suggesting a compact region emitting the energy. Additionally, the high luminosity emanating from a relatively confined area supports the notion of a compact energy source within quasars.
Step-by-step explanation:
The rapid variability of quasars' luminosity provides crucial evidence for a compact energy source. Observations have recorded fluctuations in brightness occurring within incredibly short periods, sometimes mere hours apart. This rapid variability suggests that the source emitting this immense energy is physically small. To quantify this, consider the distance light can travel in the observed timescale compared to the physical size of the emitting region. Calculations show that the observed changes in luminosity can only originate from a source considerably smaller than our solar system.
Moreover, the luminosity emitted by quasars is astoundingly high, equivalent to the energy output of billions of stars. However, this enormous energy output emerges from a relatively confined area. By estimating the size of the emitting region using the luminosity and the maximum speed achievable in that space, calculations reveal a compact energy source. The dimensions derived from these calculations align with the incredibly short timescales of variability observed, further supporting the theory of a small-sized energy source within quasars.
In essence, the evidence supporting a small-sized energy source in quasars stems from their rapid luminosity fluctuations and the immense energy emitted from a relatively confined space. Both observations and calculations strongly suggest that the powerful energy driving quasars originates from a compact region, significantly smaller than conventional astronomical scales.