Kepler-102 (Q16852002)

high proper-motion star

1 reference

1 reference

eruptive variable star

1 reference

mass

0.81±0.09 solar mass

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

Spectroscopic Properties of Cool Stars

KIC 10187017

1 reference

2MASS J18455585+4712289

1 reference

SPOCS 2983

1 reference

Gaia DR2 2119583201145735808

1 reference

Gaia DR1 2119583196848841472

1 reference

Kepler-102

Kepler Confirmed Names

2 references

Kepler object of interest

KOI-82

catalog

2 references

Fourth USNO CCD Astrograph Catalog

UCAC4 687-064315

catalog

1 reference

inferred from equatorial coordinates

Gaia DR3 2119583201145735808

1 reference

TIC 123357864

1 reference

TYC 3544-1383-1

1 reference

1 reference

child astronomical body

Kepler-102 b

b

0 references

Kepler-102c

c

0 references

Kepler-102d

d

0 references

Kepler-102e

e

0 references

Kepler-102f

f

0 references

distance from Earth

108.134±0.22 parsec

1 reference

108.088±0.1192 parsec

1 reference

108.134±0.2198 parsec

1 reference

108.088±0.1191 parsec

1 reference

stellar rotational velocity

1.7±0.5 kilometre per second

1 reference

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

0.7±1 kilometre per second

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

9.44 kilometre per second

1 reference

1.9±0.5 kilometre per second

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

parallax

9.2478±0.0188 milliarcsecond

1 reference

9.62±0.34 milliarcsecond

1 reference

Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties

9.2517±0.0102 milliarcsecond

1 reference

declination component of proper motion

−43.142±0.036 milliarcsecond per year

1 reference

−43.267±0.013 milliarcsecond per year

1 reference

right ascension component of proper motion

−41.143±0.04 milliarcsecond per year

1 reference

−41.044±0.013 milliarcsecond per year

1 reference

radial velocity

−27.67±0.61 kilometre per second

1 reference

−16.3±17.5 kilometre per second

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

−5.9±19.9 kilometre per second

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

−28.51±0.37 kilometre per second

1 reference

Gaia Data Release 3

−34.88±3.41 kilometre per second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

−34.89±4.17 kilometre per second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

−31.8 kilometre per second

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

type of variable star

rotating variable star

4 references

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

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

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

Inferring probabilistic stellar rotation periods using Gaussian processes

spectral class

K3V

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

K3

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

The Tycho-2 catalogue of the 2.5 million brightest stars

12.58±0.24

1 reference

The Tycho-2 catalogue of the 2.5 million brightest stars

12.07±0.19

1 reference

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

9.984±0.023

1 reference

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

9.446±0.018

1 reference

11.474475±0.002762

1 reference

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

9.351±0.011

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

11.17±0.01

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

11.425±0.01

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

12.298±0.01

1 reference

VizieR Online Data Catalog: UCAC4 Catalogue (Zacharias+, 2012)

11.51±0.03

1 reference

luminosity

0.26082382±0.00101173 solar luminosity

1 reference

metallicity

0.109

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

0.08

2 references

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

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

0.07

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

0.04

2 references

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

0.12

1 reference

Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars

0.29

1 reference

A super-solar metallicity for stars with hot rocky exoplanets

0.18±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

0.1

1 reference

0.11

1 reference

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

−0.02

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

0.13

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

radius

0.74708015±0.02656505 solar radius

1 reference

0.76±0.07 solar 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

2 references

281.48273327128 degree

1 reference

declination

47.20801257195001 degree

1 reference

effective temperature

4,909 kelvin

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

4,908 kelvin

2 references

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

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

4,903 kelvin

1 reference

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

4,974 kelvin

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

5,035 kelvin

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

4,816 kelvin

1 reference

Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars

4,812 kelvin

1 reference

Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars

4,810 kelvin

1 reference

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

4,727 kelvin

1 reference

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

4,772.32±87.18 kelvin

1 reference

4,916 kelvin

1 reference

4,870 kelvin

1 reference

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

4,785 kelvin

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

4,839 kelvin

1 reference

4,849 kelvin

1 reference

A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap

4,811 kelvin

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

4,906 kelvin

1 reference

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

4,909±41 kelvin

1 reference

surface gravity

9,100 centimetre per square second

1 reference

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

32,000 centimetre per square second

2 references

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

A Spectroscopic Analysis of the California-Kepler Survey Sample. I. Stellar Parameters, Planetary Radii, and a Slope in the Radius Gap

43,700 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

40,700 centimetre per square second

1 reference

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

19,000 centimetre per square second

1 reference

Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars

34,000 centimetre per square second

1 reference

Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars

42,000 centimetre per square second

2 references

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets

40,500 centimetre per square second

1 reference

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets

44,000 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

41,900 centimetre per square second

1 reference

The California-Kepler Survey. I. High-resolution Spectroscopy of 1305 Stars Hosting Kepler Transiting Planets

47,500 centimetre per square second

1 reference

49,400 centimetre per square second

1 reference

Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys

24,000 centimetre per square second

1 reference

36,000 centimetre per square second

1 reference

Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest

49,000 centimetre per square second

1 reference

The Kepler Follow-up Observation Program. II. Stellar Parameters from Medium- and High-resolution Spectroscopy

40,000 centimetre per square second

1 reference

Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra.

age estimated by a dating method

1.41 gigaannum

1 reference

Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets