(Q132124)

Two new "very hot Jupiters" among the OGLE transiting candidates

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

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 radius and mass of the transiting exoplanet OGLE-TR-132b

Improved Parameters for Extrasolar Transiting Planets

The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry$^{, }$

unconfirmed exoplanet

1 reference

imported from Wikimedia project

SIMBAD

image

Exoplanet Comparison OGLE-TR-132 b.png
1,040 × 480; 161 KB

1 reference

English Wikipedia

Wikimedia import URL

https://en.wikipedia.org/w/index.php?title=OGLE-TR-132b&oldid=889339653

mass

1.17±0.15 Jupiter mass

1 reference

Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets

1.01±0.31 Jupiter mass

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

2.7±3.4 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

1.19±0.13 Jupiter mass

1 reference

Accurate radius and mass of the transiting exoplanet OGLE-TR-132b

1.18±0.14 Jupiter mass

1 reference

Improved Parameters for Extrasolar Transiting Planets

1.14±0.12 Jupiter mass

1 reference

The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry$^{, }$

1.17±0.14 Jupiter mass

1 reference

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

time of discovery or invention

TIC 465144510b

1 reference

14 April 2004

1 reference

imported from Wikimedia project

English Wikipedia

July 2004

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

Two new "very hot Jupiters" among the OGLE transiting candidates

2 references

inferred from equatorial coordinates

constellation

Carina

1 reference

based on heuristic

parent astronomical body

3 references

Two new "very hot Jupiters" among the OGLE transiting candidates

object stated in reference as

OGLE-TR-132

object stated in reference as

OGLE-TR-132

orbital eccentricity

0.0

1 reference

0.6

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

83.83±0.96 degree

1 reference

Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets

84±6 degree

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

83.3±2.4 degree

1 reference

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

83.4±2.9 degree

2 references

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

Improved Parameters for Extrasolar Transiting Planets

orbital period

1.689868±0.000003 day

2 references

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry$^{, }$

1.68986531±0.00000064 day

2 references

Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets

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

1.68965 day

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

1.689857±0.000006 day

1 reference

Accurate radius and mass of the transiting exoplanet OGLE-TR-132b

reason for deprecated rank

1.689868 day

item/value with less precision and/or accuracy

2 references

Improved Parameters for Extrasolar Transiting Planets

The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry$^{, }$

semi-major axis of an orbit

0.0306±0.0008 astronomical unit

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

0.03026±0.00102 astronomical unit

1 reference

Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets

0.03029±0.00065 astronomical unit

1 reference

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

0.03036±0.00055 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

0.03035±0.00057 astronomical unit

1 reference

Improved Parameters for Extrasolar Transiting Planets

declination component of proper motion

parallax

0.4735±0.0544 milliarcsecond

2 references

3.164±0.083 milliarcsecond per year

2 references

right ascension component of proper motion

−5.547±0.087 milliarcsecond per year

2 references

1.229±0.076 Jupiter radius

1 reference

Homogeneous studies of transiting extrasolar planets - V. New results for 38 planets

1.15±0.8 Jupiter radius

1 reference

Two new "very hot Jupiters" among the OGLE transiting candidates

1.25±0.16 Jupiter radius

1 reference

Homogeneous studies of transiting extrasolar planets - III. Additional planets and stellar models

1.2±0.15 Jupiter radius

2 references

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

Improved Parameters for Extrasolar Transiting Planets

1.43±0.1 Jupiter radius

1 reference

Accurate radius and mass of the transiting exoplanet OGLE-TR-132b

1.18±0.07 Jupiter radius

1 reference

The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry$^{, }$

3 references