(Q19672616)

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

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

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

High-resolution multi-band imaging for validation and characterization of small Kepler planets

Densities and eccentricities of 139 Kepler planets from transit time variations

unconfirmed exoplanet

2 references

SIMBAD

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

mass

0.016±0.02 Jupiter mass

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

Kepler object of interest

catalog code

KOI-115.01

catalog

2 references

Kepler-105b

catalog

Kepler Confirmed Names

2 references

Kepler object of interest

KOI-115b

catalog

2 references

time of discovery or invention

TIC 158625964b

1 reference

2014

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-105b&oldid=119414949

2013

1 reference

March 2014

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

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

2 references

inferred from equatorial coordinates

constellation

Lyra

1 reference

based on heuristic

parent astronomical body

Kepler-105

4 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

SIMBAD

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

object stated in reference as

Kepler-105

object stated in reference as

Kepler-105

argument of periapsis

272.16±272.16 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 eccentricity

0.47±0.47

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 inclination

85.94±3.88 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

5.41220425±0.0000006 day

1 reference

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

5.41220713±0.000002488 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

5.412 day

item/value with less precision and/or accuracy

2 references

High-resolution multi-band imaging for validation and characterization of small Kepler planets

Densities and eccentricities of 139 Kepler planets from transit time variations

5.412203±0.0000037 day

1 reference

5.4122±0.00002 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

0.0609 astronomical unit

1 reference

High-resolution multi-band imaging for validation and characterization of small Kepler planets

0.066±0.003 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

2.149±0.0257 milliarcsecond

2 references

−22.206±0.043 milliarcsecond per year

2 references

right ascension component of proper motion

−9.641±0.047 milliarcsecond per year

2 references

2.802±0.242 Earth radius

1 reference

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

2.9±0.39 Earth radius

1 reference

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

0.23 Jupiter radius

1 reference

High-resolution multi-band imaging for validation and characterization of small Kepler planets

0.492±0.269 Jupiter radius

1 reference

Densities and eccentricities of 139 Kepler planets from transit time variations

0.429±0.136 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

34,600 kilometre

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

3 references