(Q19660205)

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

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

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

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

unconfirmed exoplanet

2 references

SIMBAD

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

mass

0.01196 Jupiter mass

1 reference

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

3.8 Earth mass

1 reference

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

7.7 Earth mass

1 reference

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

catalog code

Kepler-107d

catalog

Kepler Confirmed Names

3 references

Kepler object of interest

KOI-117.04

catalog

3 references

Kepler object of interest

KOI-117d

catalog

2 references

time of discovery or invention

TIC 27988327d

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

Cygnus

1 reference

based on heuristic

parent astronomical body

4 references

An abundance of small exoplanets around stars with a wide range of metallicities

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-107

object stated in reference as

Kepler-107

orbital eccentricity

0.0

reason for deprecated rank

item/value with less precision and/or accuracy

3 references

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

0.14±0.25

1 reference

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

0.11

1 reference

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

orbital inclination

87.55±0.64 degree

2 references

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

orbital period

7.95839±0.00012 day

2 references

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

7.9579290104±0.0000724137 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

7.95825±0.00011 day

1 reference

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

7.958203±0.000104 day

1 reference

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

7.95830216±0.00005983 day

1 reference

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

semi-major axis of an orbit

0.08377±0.00065 astronomical unit

2 references

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

0.082 astronomical unit

1 reference

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

declination component of proper motion

parallax

1.8725±0.0202 milliarcsecond

2 references

0.321±0.043 milliarcsecond per year

2 references

right ascension component of proper motion

−9.48±0.036 milliarcsecond per year

2 references

1,173.0 kelvin

sourcing circumstances

mean

1 reference

Extrasolar Planets Encyclopaedia exoplanet ID

Kepler-107 d

radius

0.86±0.06 Earth radius

2 references

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

Cold Jupiters and improved masses in 38 Kepler and K2 small-planet systems from 3661 high-precision HARPS-N radial velocities. No excess of cold Jupiters in small-planet systems

1.064±0.062 Earth radius

1 reference

Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities

0.095±0.005 Jupiter radius

1 reference

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

1.102±0.195 Earth radius

1 reference

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

1.09±0.06 Earth radius

1 reference

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

0.077 Jupiter radius

1 reference

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

diameter

16,400±918 kilometre

1 reference

Fundamental properties of Kepler planet-candidate host stars using asteroseismology

3 references