(Q28502766)

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

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

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

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 Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

unconfirmed exoplanet

1 reference

Kepler-130c

Kepler Confirmed Names

3 references

SIMBAD

Kepler object of interest

KOI-282.01

catalog

3 references

SIMBAD

Kepler object of interest

KOI-282c

catalog

2 references

Kepler-130 Ac

catalog

Kepler Confirmed Names

2 references

imported from Wikimedia project

TIC 121603794c

1 reference

discoverer or inventor

Kepler

1 reference

Spanish Wikipedia

time of discovery or invention

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

3 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-130

object stated in reference as

Kepler-130

argument of periapsis

0±10.89 degree

2 references

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

orbital eccentricity

0±0.07

2 references

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

0.08±0.15

1 reference

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

reason for deprecated rank

0

item/value with less precision and/or accuracy

1 reference

The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

orbital inclination

89.34±0.66 degree

1 reference

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

orbital period

27.508686±0.000037 day

1 reference

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

27.50862867±0.00000078 day

1 reference

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

27.5086932361±0.0000142265 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

27.50867519±0.00002053 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

27.50867519 day

item/value with less precision and/or accuracy

1 reference

The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

27.50868±0.00007 day

1 reference

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

semi-major axis of an orbit

0.1738919771 astronomical unit

1 reference

The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

0.178±0.005 astronomical unit

1 reference

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

declination component of proper motion

parallax

3.1292±0.0231 milliarcsecond

2 references

−28.375±0.042 milliarcsecond per year

2 references

right ascension component of proper motion

−13.074±0.039 milliarcsecond per year

2 references

683.0 kelvin

sourcing circumstances

mean

1 reference

Extrasolar Planets Encyclopaedia exoplanet ID

Kepler-130 c

radius

2.811±0.084 Earth radius

1 reference

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

2.95±0.1 Earth radius

1 reference

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

3.002±0.216 Earth radius

1 reference

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

2.877±0.072 Earth radius

1 reference

The Kepler Giant Planet Search. I: A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory

0.259±0.022 Jupiter radius

1 reference

Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates

diameter

36,300±1,120 kilometre

1 reference

A statistical reconstruction of the planet population around Kepler solar-type stars

43,500±1,280 kilometre

1 reference

Fundamental properties of Kepler planet-candidate host stars using asteroseismology

4 references