HAT-P-7 b (Q1328150)

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7

HAT-P-7: a retrograde or polar orbit, and a third body

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

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

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planets

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

TESS Transit Timing of Hundreds of Hot Jupiters

ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

HAT‐P‐7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field

ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations

unconfirmed exoplanet

2 references

SIMBAD

Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)

1 reference

Exoplanet Comparison HAT-P-7 b.png
1,040 × 480; 136 KB

1 reference

https://en.wikipedia.org/w/index.php?title=HAT-P-7b&oldid=910153953

English Wikipedia

Wikimedia import URL

mass

1.799±0.04 Jupiter mass

1 reference

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

1.682±0.021 Jupiter mass

1 reference

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

1.84±0.53 Jupiter mass

1 reference

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

1.776±0.077 Jupiter mass

1 reference

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

1.781±0.081 Jupiter mass

1 reference

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

1.697±0.027 Jupiter mass

1 reference

Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planets

1.776±0.077 Jupiter mass

1 reference

HAT-P-7: a retrograde or polar orbit, and a third body

1.806±0.036 Jupiter mass

1 reference

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

1.79±0.034 Jupiter mass

1 reference

Properties of extrasolar planets and their host stars: A case study of HAT-P-7

Kepler object of interest

catalog code

KOI-2.01

catalog

2 references

HAT-P-7b

1 reference

Kepler-2b

1 reference

BD+47 2846b

1 reference

TOI-1265.01

TESS Object of Interest

2 references

Kepler object of interest

KOI-2b

catalog

1 reference

reason for deprecated rank

TOI-1265b

catalog

TESS Object of Interest

1 reference

TIC 424865156b

1 reference

Kepler-2b

Kepler Confirmed Names

item/value with less precision and/or accuracy

2 references

discoverer or inventor

Kepler Space Telescope

1 reference

time of discovery or invention

Portuguese Wikipedia

6 March 2008

1 reference

English Wikipedia

June 2008

1 reference

HAT‐P‐7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field

site of astronomical discovery

0 references

2 references

HAT‐P‐7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field

inferred from equatorial coordinates

constellation

Cygnus

1 reference

based on heuristic

parent astronomical body

3 references

HAT‐P‐7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field

object stated in reference as

HAT-P-7

object stated in reference as

HAT-P-7

argument of periapsis

165±93 degree

2 references

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations

204±89 degree

1 reference

Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planets

reason for deprecated rank

orbital eccentricity

0.0

item/value with less precision and/or accuracy

5 references

HAT‐P‐7b: An Extremely Hot Massive Planet Transiting a Bright Star in the Kepler Field

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

0.0016±0.0034

2 references

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations

0.0055±0.007

1 reference

Friends of hot Jupiters. I. A radial velocity search for massive, long-period companions to close-in gas giant planets

0.039

1 reference

HAT-P-7: a retrograde or polar orbit, and a third body

0.004

1 reference

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

orbital inclination

83.4±0.12 degree

1 reference

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

82.2±1.2 degree

2 references

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations

reason for deprecated rank

83.11±0.03 degree

item/value with less precision and/or accuracy

1 reference

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

83.111±0.03 degree

1 reference

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

83.143±0.023 degree

1 reference

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

80.8±2.8 degree

1 reference

HAT-P-7: a retrograde or polar orbit, and a third body

83.151±0.033 degree

1 reference

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

83.5±0.5 degree

1 reference

Exoplanet System Kepler-2 with comparisons to Kepler-1 and 13

orbital period

2.204735365±0.000000038 day

1 reference

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

2.2047304±0.0000024 day

2 references

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

HAT-P-7: a retrograde or polar orbit, and a third body

2.2047372±0.0000011 day

1 reference

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

2.20473657±0.00000019 day

1 reference

TESS Transit Timing of Hundreds of Hot Jupiters

2.2047354±0.00000002 day

1 reference

Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set

2.20474±0.000017 day

1 reference

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

2.204737±0.000017 day

2 references

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

2.2047354±0.0000001 day

1 reference

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

2.2047363±0.0000007 day

1 reference

ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides

2.204736003±0.000000049 day

1 reference

ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations

2.20473825±0.00000046 day

1 reference

Spin-orbit angles of Kepler-13Ab and HAT-P-7b from gravity-darkened transit light curves

semi-major axis of an orbit

0.03805±0.00036 astronomical unit

1 reference

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

0.03676±0.00019 astronomical unit

1 reference

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

0.0377±0.0005 astronomical unit

1 reference

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

0.0355±0.0045 astronomical unit

1 reference

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

0.032±0.0033 astronomical unit

1 reference

HAT-P-7: a retrograde or polar orbit, and a third body

0.03813±0.00036 astronomical unit

1 reference

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

0.039±0.0005 astronomical unit

1 reference

Tools for discovering and characterizing extrasolar planets

angular distance

0.000118 arcsecond

1 reference

Extrasolar Planets Encyclopaedia exoplanet ID

HAT-P-7 b

parallax

2.9031±0.0206 milliarcsecond

2 references

declination component of proper motion

8.91±0.037 milliarcsecond per year

2 references

right ascension component of proper motion

−18.281±0.038 milliarcsecond per year

2 references

2,121.0 kelvin

sourcing circumstances

mean

1 reference

Extrasolar Planets Encyclopaedia exoplanet ID

HAT-P-7 b

radius

16.05±0.35 Earth radius

1 reference

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

1.465±0.016 Jupiter radius

1 reference

Homogeneous studies of transiting extrasolar planets -- IV. Thirty systems with space-based light curves

1.491±0.061 Jupiter radius

1 reference

3.6 AND 4.5μmSPITZERPHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

1.51±0.21 Jupiter radius

1 reference

Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

16.416±0.699 Earth radius

1 reference

Revised Radii of Kepler Stars and Planets Using Gaia Data Release 2

1.342±0.068 Jupiter radius

1 reference

Kepler's optical secondary eclipse of HAT-P-7b and probable detection of planet-induced stellar gravity darkening

1.419±0.178 Jupiter radius

1 reference

Changing phases of alien worlds: probing atmospheres of Kepler planets with high-precision photometry

1.363±0.195 Jupiter radius

1 reference

HAT-P-7: a retrograde or polar orbit, and a third body

1.51±0.02 Jupiter radius

1 reference

The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets

1.51±0.01 Jupiter radius

1 reference

Properties of extrasolar planets and their host stars: A case study of HAT-P-7

diameter

209,000±1,910 kilometre

1 reference

Fundamental properties of Kepler planet-candidate host stars using asteroseismology

3 references

right ascension

292.24730755480870 degree

2 references

47.96950451412388 degree

2 references

HAT-P-7 b

1 reference