Kepler-32c (Q6393171)

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

Characterizing the cool KOIs. IV. Kepler-32 as a prototype for the formation of compact planetary systems throughout the galaxy

The occurrence rate of small planets around small stars

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

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

Densities and eccentricities of 139 Kepler planets from transit time variations

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

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

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

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

0.5 Jupiter mass

2 references

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

0.024±0.016 Jupiter mass

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

Kepler object of interest

catalog code

KOI-952.02

catalog

3 references

Kepler object of interest

Kepler-32c

1 reference

KOI-952c

2 references

reason for deprecated rank

TIC 273590427c

1 reference

Kepler-32c

Kepler Confirmed Names

item/value with less precision and/or accuracy

2 references

imported from Wikimedia project

discoverer or inventor

Kepler Space Telescope

1 reference

English Wikipedia

time of discovery or invention

2013

1 reference

imported from Wikimedia project

English Wikipedia

2011

1 reference

May 2012

1 reference

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

2 references

inferred from equatorial coordinates

constellation

Cygnus

1 reference

based on heuristic

parent astronomical body

3 references

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

object stated in reference as

Kepler-32

object stated in reference as

2MASS J19512217+4634273

orbital period

8.7522±0.0003 day

2 references

Characterizing the cool KOIs. IV. Kepler-32 as a prototype for the formation of compact planetary systems throughout the galaxy

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

8.75208025±0.0000209 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

reason for deprecated rank

8.752 day

item/value with less precision and/or accuracy

2 references

Densities and eccentricities of 139 Kepler planets from transit time variations

The occurrence rate of small planets around small stars

8.75245953±0.00015 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

8.75210645±0.00001454 day

1 reference

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

8.75208271±0.00000304 day

1 reference

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

semi-major axis of an orbit

0.09 astronomical unit

1 reference

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

0.06699±0.00268 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

0.067±0.001 astronomical unit

1 reference

Characterizing the cool KOIs. IV. Kepler-32 as a prototype for the formation of compact planetary systems throughout the galaxy

declination component of proper motion

parallax

3.0595±0.0322 milliarcsecond

2 references

19.646±0.068 milliarcsecond per year

2 references

right ascension component of proper motion

−13.618±0.058 milliarcsecond per year

2 references

1.98±0.34 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

0.18±0.01 Jupiter radius

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

2.08±0.65 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

2.37±0.26 Earth radius

1 reference

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

1.94±0.26 Earth radius

1 reference

The occurrence rate of small planets around small stars

2±0.2 Earth radius

2 references

Characterizing the cool KOIs. IV. Kepler-32 as a prototype for the formation of compact planetary systems throughout the galaxy

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

2.021±0.108 Earth radius

1 reference

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

2.112±0.078 Earth radius

1 reference

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

0.178±0.018 Jupiter radius

1 reference

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

diameter

25,800±1,380 kilometre

1 reference

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

3 references