Kepler-58 is a star that is in the constellation Cygnus about 3455 light-years from us. At least two planets are turning around the star.
| Kepler-58 | |||
|---|---|---|---|
| Star | |||
| Research history | |||
| Discoverer | 2MASS | ||
| opening date | 2003 | ||
| Observational data ( Epoch J2000.0 ) | |||
| Type of | Single star | ||
| Right ascension | |||
| Declination | |||
| Distance | 3455 sv. years (1060 pc ) | ||
| Visible magnitude ( V ) | 14,820 | ||
| Constellation | Swan | ||
| Specifications | |||
| Spectral class | G1V | ||
| physical characteristics | |||
| Weight | 0.95 M ☉ | ||
| Radius | 1.03 R ☉ | ||
| Temperature | 5843 K | ||
| Metallicity | [Fe / H] = - 0.12 | ||
| |||
| Information in databases | |||
| SIMBAD | data | ||
Characteristics
Kepler-58 is a sun-like star of spectral class G0 V or G1, about the size and mass of approximately equal to the Sun. For the first time in astronomical literature is mentioned in the 2MASS catalog, published in 2003 . The mass of the star is 0.95 solar, and the radius is 1.03. The surface temperature of the star is approximately 5843 Kelvin .
See also
- List of stars constellation Cygnus