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Moreover, the system's close separation and eclipsing nature make it an excellent target for future studies with the upcoming James Webb Space Telescope and other next-generation instruments. Such missions will allow scientists to investigate the system's stellar evolution history in greater detail, shedding light on topics such as: y118 alina
The secondary component, Y118 Alina B, is significantly smaller, with a mass about 0.2 times that of our sun. Its spectral type is DQ, indicating the presence of trace elements such as barium, strontium, and calcium in its atmosphere. Y118 Alina B's surface temperature is estimated to be around 15,000 Kelvin (27,000° F), making it cooler than its companion. Here is a feature proposal tailored to that