Kepler-32 (Q4042147)

rotating variable star

1 reference

1 reference

eruptive variable star

1 reference

imported from Wikimedia project

image

Kepler-32.jpg
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media legend

Сравнительные размеры Солнца и Kepler-32. (Russian)

1 reference

Russian Wikipedia

Wikimedia import URL

https://ru.wikipedia.org/?oldid=120722376

mass

0.58 solar mass

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

Kepler object of interest

catalog code

2MASS J19512217+4634273

1 reference

KOI-952

2 references

Gaia DR2 2080287892525359872

1 reference

Kepler-32

Kepler Confirmed Names

2 references

Fourth USNO CCD Astrograph Catalog

UCAC4 683-075607

catalog

1 reference

inferred from equatorial coordinates

Gaia DR3 2080287892525359872

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TIC 273590427

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KIC 9787239

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1 reference

child astronomical body

Kepler-32c

series ordinal

c

0 references

Kepler-32b

series ordinal

b

0 references

Kepler-32f

series ordinal

f

1 reference

e

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d

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inferred from

Kepler-32d

distance from Earth

326.851±3.44 parsec

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322.997±2.8794 parsec

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326.851±3.4399 parsec

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326.85 parsec

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parallax

3.0595±0.0322 milliarcsecond

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3.096±0.0276 milliarcsecond

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declination component of proper motion

19.646±0.068 milliarcsecond per year

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19.586±0.032 milliarcsecond per year

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right ascension component of proper motion

−13.618±0.058 milliarcsecond per year

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−13.762±0.031 milliarcsecond per year

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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

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

spectral class

M1V

2 references

Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts

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

M1 V

1 reference

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

13.616±0.023

1 reference

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

12.901±0.024

1 reference

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

12.757±0.024

1 reference

16.0

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15.795283±0.002786

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

15.563±0.48

1 reference

luminosity

0.06988551±0.00175538 solar luminosity

1 reference

metallicity

0.00

3 references

SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

−0.02

2 references

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

Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts

−0.15

1 reference

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

−0.5

1 reference

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

radius

0.59739065±0.09162735 solar radius

1 reference

0.53 solar radius

1 reference

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

diameter

736,000±48,700 kilometre

1 reference

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

2 references

297.84239345946 degree

1 reference

declination

46.57427516205001 degree

1 reference

effective temperature

4,061 kelvin

1 reference

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

3,731 kelvin

1 reference

Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts

3,801 kelvin

1 reference

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

4,223 kelvin

1 reference

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

reason for deprecated rank

3,900 kelvin

item/value with less precision and/or accuracy

2 references

SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs

Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models

3,911 kelvin

1 reference

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

3,839.67±333.3403 kelvin

1 reference

3,938 kelvin

1 reference

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

surface gravity

44,000 centimetre per square second

2 references

SWEET-Cat: A catalogue of parameters for Stars With ExoplanETs

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

54,100 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

55,000 centimetre per square second

1 reference

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

1,480 centimetre per square second

1 reference

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