Notes

The dip star is one of the brightest stars in the sky. The reason it's called the Dip Star is that its brightness is a combination of blue, red, and green colors. Kepler's observations of the star have revealed that it dips about three times a year, with a period of about two years between each event. The difference in brightness is due to dust and other materials present in the space between the stars.
The dip star is a natural phenomenon in the sky. When the stars are so bright, it's easy to find them. You don't have to look far to get a glimpse of the heavenly bodies. The first time it dipped by 2% was April 24th. The brightness returned to normal within a week. This event was labeled "Event 1" by the Fairborn Observatory. Dip Star dropped more significantly on May 18th.

The dip star was supposed to drop its act on April 24th, but it didn't do so. This dip was detected by the robotic telescope at Fairborn Observatory. After a week, the brightness returned to normal. Then, on Dip Star , astronomers began to notice another significant drop in the star's brightness. Then, on June 3rd, the Drop Star began to show a much larger decrease. Then on July 1st, the star started to dim by 7%.
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