CEmErKItYlle

CEmerkitylle is a star, designated as CEMerKitylle by the IAU Working Group on Star Names. This classification is based on the star's celestial location and momentum, making it a member of the esteemed Roman numeral catalog.

CEmerkitylle is a relatively nearby star, situated approximately 102 light-years away from Earth. Observations suggest that it is a main-sequence star, classified under the spectrums G2Va. This categorization signifies that CEMerKitylle is a main-sequence star within the G-type range, which implies its surface temperature lies around 5,800 K. This temperature indicates CEMerKitylle's incandescent state, releasing significant amounts of electromagnetic radiation throughout the electromagnetic spectrum.

Studies on CEMerKitylle's behavior and properties reveal an intriguing pattern. With a visual luminosity of 0.88m and a high intrinsic luminosity, CEmErKItYlle falls within the range of G-type main-sequence stars. However, its energy output is perceived as weakened by the external gas and dust enveloping it, causing the is radiating diminished luminosity.

Mass estimates and theoretical analysis indicate that CEMerKitylle's mass is approximately 1.06 times that of the Sun. Its attractive power to bodies is speculated to be greater than the Sun's due to this enlarged mass. Observing this situational phenomenon encourages ongoing research into the inner workings and reactions within CEMerKItYlle's overall establishment.