(Q85833766)

Kepler-119

catalog

Kepler Confirmed Names

2 references

inferred from equatorial coordinates

Gaia DR3 2077236713401973888

1 reference

TIC 271964647

1 reference

1 reference

child astronomical body

Kepler-119b

series ordinal

b

0 references

Kepler-119c

series ordinal

c

0 references

distance from Earth

716.23±12.67 parsec

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

706.265±7.3824 parsec

1 reference

716.23±12.6707 parsec

1 reference

716.23±12.65 parsec

1 reference

parallax

1.3962±0.0247 milliarcsecond

1 reference

1.4159±0.0148 milliarcsecond

1 reference

declination component of proper motion

−17.194±0.04 milliarcsecond per year

1 reference

−17.181±0.017 milliarcsecond per year

1 reference

right ascension component of proper motion

−7.15±0.035 milliarcsecond per year

1 reference

−7.127±0.016 milliarcsecond per year

1 reference

radial velocity

−24.24±0.75 kilometre per second

1 reference

−20.98±1.39 kilometre per second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

type of variable star

rotating variable star

1 reference

Photometric amplitude distribution of stellar rotation of KOIs--Indication for spin-orbit alignment of cool stars and high obliquity for hot stars

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.997±0.023

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.636±0.024

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

12.58±0.021

1 reference

14.18924±0.002763

1 reference

luminosity

0.83005047±0.03744953 solar luminosity

1 reference

reason for deprecated rank

metallicity

−0.08

item/value with less precision and/or accuracy

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

−0.083

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

0.149

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

0.129

1 reference

0.4

1 reference

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

radius

1.0612607±0.006846 solar radius

1 reference

0.84±0.32 solar radius

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

2 references

295.94642713485 degree

1 reference

declination

42.65890632226 degree

1 reference

reason for deprecated rank

effective temperature

5,595 kelvin

item/value with less precision and/or accuracy

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

5,570 kelvin

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

5,388 kelvin

1 reference

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

5,348±17.3335 kelvin

1 reference

5,651 kelvin

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

5,498 kelvin

1 reference

4,875 kelvin

1 reference

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

5,595±200 kelvin

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

surface gravity

36,900 centimetre per square second

1 reference

Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems

38,000 centimetre per square second

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

74,000 centimetre per square second

1 reference

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

22,230 centimetre per square second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

24,000 centimetre per square second

1 reference

3,160 centimetre per square second

1 reference