Emek and Luna prepared a space telescope to study one of three faint stars. The database listed their distances as 72,000,000,000,000 kilometers for Star A, 95,000,000,000,000 kilometers for Star B, and 81,000,000,000,000 kilometers for Star C. Their sensors measured incoming light levels of 0.0000048, 0.0000021, and 0.0000036 units. Emek rewrote the distances as 7.2 x 10^13, 9.5 x 10^13, and 8.1 x 10^13 kilometers. Luna expressed the light levels as 4.8 x 10^-6, 2.1 x 10^-6, and 3.6 x 10^-6. Their research required a star at least 8.0 x 10^13 kilometers away with a light level of at least 3.0 x 10^-6. Star A was too close, while Star B was too faint. Star C met both conditions. Emek aimed the telescope at Star C, and Luna confirmed a clear signal. Their careful comparisons had identified the only suitable target.




