Black holes, often illustrated as cosmic vacuums, are regions in space where the gravitational pull is so strong that nothing, not even light, can escape from them. This characteristic makes them invisible and challenging to study. However, quasars, or actively feeding black holes, offer a glimpse into the enigmatic behaviors of these dark entities by ejecting enormous amounts of radiation as they consume matter from their surroundings. It is this radiation that allows scientists to detect and study them from the comfort of our home planet.

The quasar J0529-4351, sitting at a redshift of 3.9, is an object of wonder, primarily due to its staggering mass of 17 billion solar masses and its unprecedented growth rate of one solar mass per day. The significance of this discovery cannot be overstated. It represents not only an impressive addition to our galactic compendium but also a key to understanding the mechanics of cosmic feeding and growth. To put this into perspective, our Sun is about 330,000 times the mass of Earth, making this quasar over 5.6 trillion times the mass of our planet.

Observations made by a dedicated team using the Very Large Telescope in Chile's Atacama Desert have shed light on this colossal entity. These observations, published in Nature Astronomy, detail how the quasar's strong gravitational field pulls gas, dust, and other space debris towards it, facilitating its rapid growth. Such an astronomical growth rate is indicative of the massive amounts of matter available in its vicinity, allowing the black hole to accrete efficiently and continuously.

The illumination from quasars like J0529-4351 is not just a spectacle; it serves as a beacon tracing back to the early universe. The light from this particular quasar is over 12 billion years old, a relic from a time when the universe was still in its formative years. This connection to the primordial cosmos provides invaluable insights into the formation and evolution of early galactic structures, potentially reshaping our understanding of the universe's history.

Further research and observations have unveiled that approximately 65% of galaxies housing quasars at their centers exhibit evidence of past interactions or mergers with other galaxies. This statistic opens up a new frontier in understanding galactic evolution, suggesting that these colossal cosmic collisions might trigger the awakening or formation of quasars. Such a realization underscores the dynamic and often violent nature of galaxies, constantly shaping and being shaped by their surroundings.

In conclusion, the discovery of the quasar J0529-4351 stands as a testament to the relentless pursuit of knowledge by the astronomical community. It challenges preconceived notions about the limits of cosmic growth and illuminates the intricate dynamics that govern our universe. As we continue to probe the depths of space, each discovery brings us closer to answering the fundamental questions of our existence and the nature of the cosmos.