Dass055 C: New

Amateur astronomers with >20" telescopes cannot directly detect the transit, but they can contribute by monitoring the star’s photometric baseline to refine stellar variability models.

The keyword "DASS055 C New" refers to the latest findings regarding the third planetary candidate (or a secondary component) in the DASS055 system—a red dwarf star located approximately 240 light-years away in the constellation of Horologium. While not yet as famous as TRAPPIST-1 or Proxima Centauri, DASS055 is rapidly becoming a benchmark for studying "warm sub-Neptunes" and their ability to hold onto primordial atmospheres.

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M-dwarfs are dim, and DASS055 C New’s transit depth is only 0.089%—a dip of less than one-thousandth of the star’s light. For comparison, Jupiter transiting the Sun would cause a 1% dip. DASS055 C New’s signal is nine times subtler. This is why the "New" designation required space-based precision from both TESS and JWST working in tandem.

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The is an internal flex cable circuit board (sometimes called a keypad film) that acts as the bridge between your controller's physical buttons and the main motherboard. It sits behind the D-Pad, face buttons ( ), and L1/R1 buttons. Why "C New"?

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