Ross 614
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Ross 614 is a M-type (Red) star.
At a distance of approximately 13.5 light-years, Ross 614 is one of the Sun's closest stellar neighbors. Light that we observe from Ross 614 today left the star roughly 13 years ago, making it a near neighbor in galactic terms.
Ross 614 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
At an apparent magnitude of +11.12, Ross 614 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its red hue, which corresponds to a B-V color index of +1.690.
Fiziksel Özellikler
| Spektral Sınıf | M Class M — M-type (Red) |
| Renk İndeksi (B−V) | 1,690 |
Gözlem
| Görünür Parlaklık | +11.12 |
| Mutlak Parlaklık | 13,04 |
| Mesafe | 13.5 ly |
Konum
| Sağ Açıklık | 6h 29,39m |
| Dik Açı | -2° 48,84′ |