Kepler-32 e (Q18613719)

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

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

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

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

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

The occurrence rate of small planets around small stars

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

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)

catalog code

KOI-952e

catalog

Kepler object of interest

2 references

Kepler-32e

catalog

Kepler Confirmed Names

2 references

Kepler object of interest

KOI-952.04

catalog

2 references

imported from Wikimedia project

TIC 273590427e

1 reference

discoverer or inventor

Kepler Space Telescope

1 reference

Spanish Wikipedia

time of discovery or invention

2013

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

imported from Wikimedia project

Spanish Wikipedia

Wikimedia import URL

https://es.wikipedia.org/w/index.php?title=Kepler-32e&oldid=119410495

2012

1 reference

February 2013

1 reference

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

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

2 references

inferred from equatorial coordinates

constellation

Cygnus

1 reference

based on heuristic

parent astronomical body

3 references

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

object stated in reference as

Kepler-32

object stated in reference as

2MASS J19512217+4634273

orbital period

2.896±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

2.8960227414±0.0000092811 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

2.896029±0.000063 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

2.89601166±0.00000934 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

2.896013787±0.000004215 day

1 reference

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

reason for deprecated rank

2.896 day

item/value with less precision and/or accuracy

1 reference

The occurrence rate of small planets around small stars

semi-major axis of an orbit

0.033 astronomical unit

1 reference

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

0.03205±0.00128 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

0.0323±0.0005 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

0.134±0.009 Jupiter 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

1.501±0.098 Earth radius

1 reference

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

1.04±0.15 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

1.43±0.19 Earth radius

1 reference

The occurrence rate of small planets around small stars

1.09±0.14 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

1.42±0.07 Earth radius

1 reference

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

reason for deprecated rank

1.5±0.1 Earth radius

item/value with less precision and/or accuracy

1 reference

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

1.418±0.061 Earth radius

1 reference

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

diameter

19,100±1,250 kilometre

1 reference

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

3 references