(Q86843978)

Kepler object of interest

KOI-999

catalog

2 references

inferred from equatorial coordinates

Gaia DR3 2051832634677771008

1 reference

TIC 137637249

1 reference

1 reference

child astronomical body

Kepler-263 c

series ordinal

c

0 references

Kepler-263b

series ordinal

b

0 references

distance from Earth

771.069±16.588 parsec

reason for deprecated rank

item/value with less precision and/or accuracy

1 reference

745.156±12.5488 parsec

1 reference

771.069±16.5879 parsec

1 reference

771.09 parsec

1 reference

stellar rotational velocity

2.1±1 kilometre per second

1 reference

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

1.73 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

1.2969±0.0279 milliarcsecond

1 reference

1.342±0.0226 milliarcsecond

1 reference

declination component of proper motion

0.453±0.057 milliarcsecond per year

1 reference

0.44±0.031 milliarcsecond per year

1 reference

right ascension component of proper motion

5.773±0.049 milliarcsecond per year

1 reference

5.818±0.025 milliarcsecond per year

1 reference

radial velocity

−39.09±0.028539 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

−48.68±3.94 kilometre per second

1 reference

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

−39.09±0.02853 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

G8

1 reference

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

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

13.99±0.03

1 reference

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

13.53±0.03

1 reference

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

13.548±0.048

1 reference

15.40323±0.002771

1 reference

luminosity

0.334432±0.01778943 solar luminosity

1 reference

metallicity

−0.081

1 reference

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

−0.11

1 reference

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

−0.178

1 reference

reason for deprecated rank

−0.08

item/value with less precision and/or accuracy

1 reference

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

−0.222

1 reference

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

−0.07

1 reference

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

radius

0.7767811±0.0521841 solar radius

1 reference

0.79 solar radius

1 reference

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

2 references

292.46977061433 degree

1 reference

declination

37.5677921986 degree

1 reference

effective temperature

5,112 kelvin

1 reference

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

5,245 kelvin

1 reference

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

5,265 kelvin

1 reference

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

5,118 kelvin

1 reference

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

4,980.282±176.218 kelvin

1 reference

5,025 kelvin

1 reference

5,142 kelvin

1 reference

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

5,006 kelvin

1 reference

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

5,242 kelvin

1 reference

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

5,263 kelvin

1 reference

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

surface gravity

51,300 centimetre per square second

1 reference

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

37,150 centimetre per square second

1 reference

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

37,700 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

37,000 centimetre per square second

1 reference

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

32,360 centimetre per square second

1 reference

42,100 centimetre per square second

1 reference

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

50,600 centimetre per square second

1 reference

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

46,380 centimetre per square second

1 reference

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

31,600 centimetre per square second

1 reference