(Q28855532)

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

A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems

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

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

unconfirmed exoplanet

2 references

SIMBAD

Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data

mass

12.5±3.2 Earth mass

1 reference

A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems

Kepler object of interest

catalog code

KOI-279.02

catalog

3 references

Kepler-450c

catalog

Kepler Confirmed Names

3 references

Kepler object of interest

KOI-279c

catalog

2 references

imported from Wikimedia project

TIC 27534138c

1 reference

discoverer or inventor

Kepler

1 reference

Spanish Wikipedia

time of discovery or invention

August 2015

1 reference

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

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

2 references

inferred from equatorial coordinates

constellation

Cygnus

1 reference

based on heuristic

parent astronomical body

KOI-279

4 references

Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data

SIMBAD

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

object stated in reference as

Kepler-450

object stated in reference as

Kepler-450

orbital eccentricity

0.02±0.17

1 reference

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

orbital period

15.41312391±0.00000371 day

1 reference

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

15.4131395±0.0000029 day

1 reference

A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems

15.41308581±0.00002984 day

1 reference

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

15.4131373094±0.0000219078 day

1 reference

Transit Timing Variations and linear ephemerides of confirmed Kepler transiting exoplanets

15.413135±0.000085 day

1 reference

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

declination component of proper motion

parallax

2.1645±0.0245 milliarcsecond

2 references

6.655±0.052 milliarcsecond per year

2 references

right ascension component of proper motion

4.172±0.048 milliarcsecond per year

2 references

2.62±0.14 Earth radius

1 reference

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

2.5958±0.0017 Earth radius

1 reference

A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems

2.55±0.16 Earth radius

1 reference

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

2.68±0.13 Earth radius

1 reference

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

0.234 Jupiter radius

1 reference

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

diameter

34,700±7,650 kilometre

1 reference

Fundamental properties of Kepler planet-candidate host stars using asteroseismology

3 references