(Q21037703)

The occurrence rate of small planets around small stars

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

Densities and eccentricities of 139 Kepler planets from transit time variations

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

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

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

Characterizing the cool Kepler objects of interests. New effective temperatures, metallicities, masses, and radii of low-mass Kepler planet-candidate host stars

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

unconfirmed exoplanet

2 references

SIMBAD

Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)

mass

0.077±0.062 Jupiter mass

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

catalog code

Kepler-83d

Kepler Confirmed Names

3 references

KOI-898.02

Kepler object of interest

3 references

KOI-898d

Kepler object of interest

2 references

Kepler-83 Ad

Kepler Confirmed Names

2 references

time of discovery or invention

TIC 123416515d

1 reference

March 2014

1 reference

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

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

2 references

inferred from equatorial coordinates

constellation

Lyra

1 reference

based on heuristic

parent astronomical body

4 references

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

object stated in reference as

Kepler-83

object stated in reference as

2MASS J18485580+4339562

orbital inclination

88.87 degree

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

reason for deprecated rank

orbital period

5.17 day

item/value with less precision and/or accuracy

2 references

The occurrence rate of small planets around small stars

Densities and eccentricities of 139 Kepler planets from transit time variations

5.1698149493±0.0000099587 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

5.169809946±0.00000975 day

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

5.16981333±0.0000229 day

1 reference

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

5.16990995±0.00011 day

1 reference

Characterizing the cool Kepler objects of interests. New effective temperatures, metallicities, masses, and radii of low-mass Kepler planet-candidate host stars

5.16979783±0.00000249 day

1 reference

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

5.169796±0.000016 day

1 reference

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

5.169804269±0.000009036 day

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

semi-major axis of an orbit

0.051 astronomical unit

1 reference

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

0.04773±0.00186 astronomical unit

1 reference

Characterizing the cool Kepler objects of interests. New effective temperatures, metallicities, masses, and radii of low-mass Kepler planet-candidate host stars

0.0467 astronomical unit

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

declination component of proper motion

parallax

2.4691±0.0319 milliarcsecond

2 references

−13.641±0.059 milliarcsecond per year

2 references

right ascension component of proper motion

1.91±0.057 milliarcsecond per year

2 references

1.96±0.18 Earth radius

1 reference

The occurrence rate of small planets around small stars

1.95±0.12 Earth radius

1 reference

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

0.19±0.013 Jupiter radius

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

2.004±0.076 Earth radius

1 reference

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

1.78±0.24 Earth radius

1 reference

The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity

1.88±1.84 Earth radius

1 reference

Characterizing the cool Kepler objects of interests. New effective temperatures, metallicities, masses, and radii of low-mass Kepler planet-candidate host stars

2.133±0.148 Earth radius

1 reference

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

0.173±0.012 Jupiter radius

1 reference

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

0.1481±0.0134 Jupiter radius

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

diameter

27,200±1,890 kilometre

1 reference

Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right?

3 references