(Q27961912)

Kepler-283

catalog

Kepler Confirmed Names

2 references

inferred from equatorial coordinates

Gaia DR3 2128811951996688768

1 reference

TIC 270695184

1 reference

1 reference

child astronomical body

Kepler-283b

series ordinal

b

0 references

Kepler-283c

series ordinal

c

0 references

distance from Earth

474.338±7.965 parsec

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

489.38±8.5739 parsec

1 reference

474.338±7.9648 parsec

1 reference

474.33±7.96 parsec

1 reference

parallax

2.1082±0.0354 milliarcsecond

1 reference

2.0434±0.0358 milliarcsecond

1 reference

declination component of proper motion

−16.43±0.07 milliarcsecond per year

1 reference

−16.15±0.047 milliarcsecond per year

1 reference

right ascension component of proper motion

3.188±0.071 milliarcsecond per year

1 reference

2.923±0.043 milliarcsecond per year

1 reference

type of variable star

rotating variable star

4 references

Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars

Rotation and differential rotation of active Kepler stars

Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators

Photometric amplitude distribution of stellar rotation of KOIs--Indication for spin-orbit alignment of cool stars and high obliquity for hot stars

spectral class

K7V

1 reference

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

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.927±0.022

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.263±0.023

1 reference

VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)

13.14±0.03

1 reference

15.865565±0.002833

1 reference

luminosity

0.104782544±0.004109979 solar luminosity

1 reference

metallicity

−0.21

1 reference

Testing the metal of late-type Kepler planet hosts with iron-clad methods

reason for deprecated rank

−0.20

item/value with less precision and/or accuracy

1 reference

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

−0.26

1 reference

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

radius

0.58203715±0.03792705 solar radius

1 reference

0.57±0.02 solar radius

1 reference

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

diameter

871,000±48,700 kilometre

1 reference

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

2 references

293.61372248403 degree

1 reference

declination

47.83900752255 degree

1 reference

reason for deprecated rank

effective temperature

4,351 kelvin

item/value with less precision and/or accuracy

1 reference

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

4,141 kelvin

1 reference

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

4,327 kelvin

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

4,157 kelvin

1 reference

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data

4,304.505±147.495 kelvin

1 reference

4,351±100 kelvin

1 reference

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

surface gravity

52,600 centimetre per square second

1 reference

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

51,300 centimetre per square second

1 reference

A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42

30,000 centimetre per square second

1 reference

Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data