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Kepler-84(Q4042001)

From Wikidata

star in the constellation Cygnus

Language	Label	Description	Also known as
default for all languages	Kepler-84
English	Kepler-84	star in the constellation Cygnus

Statements

1 reference

rotating variable star

1 reference

1 reference

eruptive variable star

1 reference

KOI-1589

Kepler object of interest

2 references

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

KIC 5301750

Kepler Input Catalog

1 reference

2MASS J19530049+4029458

1 reference

Gaia DR2 2073776859551124992

Gaia Data Release 2

1 reference

Kepler-84

Kepler Confirmed Names

1 reference

UCAC4 653-081879

Fourth USNO CCD Astrograph Catalog

1 reference

Gaia DR3 2073776859551124992

Gaia Data Release 3

1 reference

TIC 170646917

TESS Input Catalog

1 reference

SPOCS 3460

Spectroscopic Properties of Cool Stars

1 reference

Kepler-84A

Kepler Confirmed Names

1 reference

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

1 reference

based on heuristic

inferred from equatorial coordinates

child astronomical body

b

1 reference

c

1 reference

d

1 reference

e

1 reference

f

1 reference

distance from Earth

1,053.44±156.54parsec

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

stated in source according to

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

stellar rotational velocity

4.5±1kilometre per second

1 reference

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

stated in source according to

3.7±0.6kilometre per second

1 reference

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

stated in source according to

0.6929±0.7043milliarcsecond

1 reference

Gaia Data Release 2

stated in source according to

declination component of proper motion

−2.872±1.233milliarcsecond per year

1 reference

Gaia Data Release 2

stated in source according to

right ascension component of proper motion

−0.15±1.266milliarcsecond per year

1 reference

Gaia Data Release 2

stated in source according to

radial velocity

12.7kilometre per second

1 reference

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

stated in source according to

type of variable star

rotating variable star

3 references

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

stated in source according to

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

stated in source according to

Inferring probabilistic stellar rotation periods using Gaussian processes

stated in source according to

F9/G0V

1 reference

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

apparent magnitude

13.583±0.021

astronomical filter

1 reference

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

stated in source according to

13.234±0.024

astronomical filter

1 reference

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

stated in source according to

13.193±0.026

astronomical filter

1 reference

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

stated in source according to

15.032

astronomical filter

1 reference

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

14.95041±0.0094

astronomical filter

1 reference

Gaia Early Data Release 3

stated in source according to

14.804±0.08

astronomical filter

1 reference

Fourth USNO CCD Astrograph Catalog

stated in source according to

−0.18

1 reference

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

stated in source according to

−0.05

2 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

stated in source according to

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

stated in source according to

−0.111

1 reference

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

stated in source according to

−0.06

1 reference

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

stated in source according to

0.987±0.072solar mass

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

stated in source according to

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

1.131±0.176solar radius

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

stated in source according to

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

1,990,000kilometre

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

stated in source according to

2 references

Gaia Data Release 2

right ascension

298.25202160968040degree

1 reference

Gaia Data Release 2

stated in source according to

40.49609659382195degree

1 reference

Gaia Data Release 2

stated in source according to

effective temperature

6,026kelvin

1 reference

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

stated in source according to

6,013kelvin

1 reference

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

stated in source according to

5,866kelvin

1 reference

Spectroscopy of faint Kepler mission exoplanet candidate host stars

stated in source according to

6,031kelvin

1 reference

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

stated in source according to

5,755kelvin

1 reference

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

stated in source according to

5,361±229.325kelvin

1 reference

Gaia Data Release 2

6,053kelvin

1 reference

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

stated in source according to

6,066kelvin

1 reference

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

stated in source according to

5,867kelvin

1 reference

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

stated in source according to

6,036±132kelvin

1 reference

Planetary Candidates Observed by Kepler. VIII. A Fully Automated Catalog with Measured Completeness and Reliability Based on Data Release 25

stated in source according to

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

surface gravity

26,300centimetre per square second

2 references

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

stated in source according to

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

stated in source according to

21,040centimetre 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

stated in source according to

13,500centimetre per square second

2 references

Spectroscopy of faint Kepler mission exoplanet candidate host stars

stated in source according to

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

stated in source according to

36,600centimetre per square second

1 reference

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

stated in source according to

42,000centimetre per square second

1 reference

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

stated in source according to

35,000centimetre per square second

1 reference

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

stated in source according to

age estimated by a dating method

4.9gigaannum

1 reference

imported from Wikimedia project

English Wikipedia

Wikimedia import URL

https://en.wikipedia.org/w/index.php?title=Kepler-84&oldid=1077687776

3.98±1.91gigaannum

1 reference

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

stated in source according to

Extrasolar Planets Encyclopaedia

Extrasolar Planets Encyclopaedia exoplanet ID

kepler_84_b--1398

Identifiers

2073776859551124992

0 references

Google Knowledge Graph ID

0 references

NASA Exoplanet Archive ID

0 references

0 references

Sitelinks

Wikipedia(6 entries)

Wikibooks(0 entries)

Wikinews(0 entries)

Wikiquote(0 entries)

Wikisource(0 entries)

Wikiversity(0 entries)

Wikivoyage(0 entries)

Wiktionary(0 entries)

Multilingual sites(0 entries)

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