Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 14m 19.5623s[1] |
Declination | +41° 05′ 23.367″[1] |
Apparent magnitude (V) | 13.005±0.039[2] |
Characteristics | |
Spectral type | G0[3] |
Apparent magnitude (J) | 11.833±0.020[4] |
Apparent magnitude (H) | 11.601±0.022[4] |
Apparent magnitude (K) | 11.535±0.020[4] |
Apparent magnitude (B) | 13.620±0.029[2] |
Astrometry | |
Radial velocity (Rv) | +0.40 ± 0.10[5] km/s |
Proper motion (μ) | RA: −2.937(15) mas/yr[1] Dec.: −21.084(14) mas/yr[1] |
Parallax (π) | 1.0319 ± 0.0121 mas[1] |
Distance | 3,160 ± 40 ly (970 ± 10 pc) |
Details[5] | |
Mass | 1.347+0.072 −0.054 M☉ |
Radius | 1.843+0.048 −0.066 R☉ |
Luminosity | 4.15+0.63 −0.54 L☉ |
Surface gravity (log g) | 3.98 ± 0.10 cgs |
Temperature | 5933 ± 44 K |
Metallicity [Fe/H] | +0.11 ± 0.03 dex |
Rotational velocity (v sin i) | 4.2 ± 0.5 km/s |
Age | 3.3 ± 0.4 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Kepler-7 is a star located in the constellation Lyra in the field of view of the Kepler Mission, a NASA operation in search of Earth-like planets. It is home to the fourth of the first five planets that Kepler discovered; this planet, a Jupiter-size gas giant named Kepler-7b, is as light as styrofoam.[6] The star itself is more massive than the Sun, and is nearly twice the Sun's radius. It is also slightly metal-rich, a major factor in the formation of planetary systems. Kepler-7's planet was presented on January 4, 2010 at a meeting of the American Astronomical Society.
Gaia DR3
was invoked but never defined (see the help page).APASS DR9
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).Skrutskie2006
was invoked but never defined (see the help page).Latham2010
was invoked but never defined (see the help page).AASannouncement
was invoked but never defined (see the help page).