The high-frequency electromagnetic radiation beam detected by the scouting device left behind by Chen Ming was not something particularly rare in the universe.
After all, stellar activity inherently means that a large amount of radiation is emitted by the star.
Such a high-frequency electromagnetic radiation beam could only be counted as one of the many natural phenomena that a star would exhibit.
There was nothing inherently noteworthy about it.
However.
The high-frequency electromagnetic radiation beam Chen Ming was observing at this moment was not just an ordinary high-frequency electromagnetic radiation beam; its existence was accompanied by a special pattern.
That was, the time interval between two bursts of high-frequency electromagnetic radiation from the star was shortening at the same fixed interval, and it was estimated that three hours later the interval between two emissions of the radiation beam would be completely reduced to zero.
