KOI-2650 (Q77687239)

mass

0.53 solar mass

1 reference

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

Kepler object of interest

catalog code

Gaia DR2 2126465903421535744

1 reference

2MASS J19340266+4508117

1 reference

KIC 8890150

1 reference

KOI-2650

2 references

Kepler-395

catalog

Kepler Confirmed Names

2 references

Fourth USNO CCD Astrograph Catalog

UCAC4 676-072214

catalog

1 reference

inferred from equatorial coordinates

Gaia DR3 2126465903421535744

1 reference

TIC 270520765

1 reference

1 reference

child astronomical body

Kepler-395c

series ordinal

c

0 references

Kepler-395b

series ordinal

b

0 references

distance from Earth

426.348±8.216 parsec

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

410.442±5.3234 parsec

1 reference

426.348±8.2161 parsec

1 reference

426.34±8.22 parsec

1 reference

stellar rotational velocity

4.894 kilometre per second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

parallax

2.3455±0.0452 milliarcsecond

1 reference

2.4364±0.0316 milliarcsecond

1 reference

declination component of proper motion

7.013±0.068 milliarcsecond per year

1 reference

6.928±0.039 milliarcsecond per year

1 reference

right ascension component of proper motion

12.963±0.079 milliarcsecond per year

1 reference

12.991±0.039 milliarcsecond per year

1 reference

radial velocity

−19.868999±0.021435 kilometre per second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

−19.868999±0.02143 kilometre per second

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

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

M1V

1 reference

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

M0.7

1 reference

Temperatures and Metallicities of M Dwarfs in the APOGEE Survey

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

13.818±0.023

1 reference

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

13.131±0.027

1 reference

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

12.948±0.03

1 reference

15.942506±0.002793

1 reference

luminosity

0.09977403±0.00429213 solar luminosity

1 reference

metallicity

−0.08

1 reference

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

reason for deprecated rank

−0.16

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

0.01

1 reference

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

−0.163

1 reference

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

0.186

1 reference

0.04

1 reference

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

0.26

1 reference

Temperatures and Metallicities of M Dwarfs in the APOGEE Survey

0.048

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

radius

0.69188225±0.05282861 solar radius

1 reference

0.56±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

789,000±47,300 kilometre

1 reference

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

2 references

293.5111096370599 degree

1 reference

declination

45.13659536423 degree

1 reference

reason for deprecated rank

effective temperature

4,262 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

3,915 kelvin

1 reference

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

3,765 kelvin

1 reference

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

4,050 kelvin

1 reference

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

3,900±158 kelvin

1 reference

4,027 kelvin

1 reference

4,157 kelvin

1 reference

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

3,960 kelvin

1 reference

Temperatures and Metallicities of M Dwarfs in the APOGEE Survey

4,154 kelvin

1 reference

APOGEE Data and Spectral Analysis from SDSS Data Release 16: Seven Years of Observations Including First Results from APOGEE-South

4,262±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

53,600 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

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

36,400 centimetre per square second

1 reference

47,000 centimetre per square second

1 reference

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

43,690 centimetre per square second

1 reference