ดาวกัปไตน์

ดาวกัปไตน์ is a M-type (Red) star.

At a distance of approximately 12.8 light-years, ดาวกัปไตน์ is one of the Sun's closest stellar neighbors. Light that we observe from ดาวกัปไตน์ today left the star roughly 12 years ago, making it a near neighbor in galactic terms.

ดาวกัปไตน์ is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.

ดาวกัปไตน์ has an apparent magnitude of +8.86, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its red hue, which corresponds to a B-V color index of +1.543.