Planet TOI-1467 b

Detailed information about planet TOI-1467 b and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

TOI-1467 b

Planet Status

Confirmed

Discovered in

2021

Update

2024-06-11

Mass

0.028 (\begin{matrix} + 0.0 \\ - 0.028 \end{matrix})

M_J 2 publications

The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey Targets
VaTEST III: Validation of 8 Potential Super-Earths from TESS Data

Mass*sin(i)

—

Semi-Major Axis

0.0495 (\pm 0.0009)

AU 2 publications

The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey Targets
VaTEST III: Validation of 8 Potential Super-Earths from TESS Data

Orbital Period

5.97199 (\pm 0.00083)

day 3 publications

The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey Targets
VaTEST III: Validation of 8 Potential Super-Earths from TESS Data
The TESS-Keck Survey: Science Goals and Target Selection

Eccentricity

— 1 publication

The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey Targets

ω

—

T_peri

—

Radius

0.1633 (\pm 0.0143)

R_J 2 publications

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data
The TESS-Keck Survey: Science Goals and Target Selection

Inclination

89.0 (\begin{matrix} + 0.73 \\ - 0.44 \end{matrix})

deg 1 publication

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data

Detection Method

Primary Transit

Mass Meas. Method

Radial Velocity

Radius Meas. Method

Primary Transit

Primary transit

2458766.985 (\pm 0.003)

JD 2 publications

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data
The TESS-Keck Survey: Science Goals and Target Selection

Secondary transit

—

λ

—

Impact Parameter b

0.48 (\pm 0.2)

1 publication

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data

Time V_r=0

—

Velocity Semiamplitude K

1.8 (\begin{matrix} + 0.0 \\ - 1.8 \end{matrix})

m/s

Calculated temperature

526.0 K 2 publications

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data
The TESS-Keck Survey: Science Goals and Target Selection

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

No remarks

No link

Star

Name

TOI-1467

Distance

34.44 (\pm 0.05)

pc 1 publication

The Revised TESS Input Catalog and Candidate Target List

Spectral type

—

Apparent magnitude V

12.3

Mass

0.49 (\pm 0.02)

M_Sun 1 publication

The Revised TESS Input Catalog and Candidate Target List

Age

—

Effective temperature

3834.0 (\pm 57.0)

K 1 publication

The Revised TESS Input Catalog and Candidate Target List

Radius

0.49 (\pm 0.01)

R_Sun 1 publication

The Revised TESS Input Catalog and Candidate Target List

Metallicity [Fe/H]

—

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

01:16:28.0

Dec₂₀₀₀

+49:13:59.0

Alternate Names

—

No remarks

No link

Simbad
Most recent references (ADS)

Planet TOI-1467 b

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 1 planet

Remarks No remark

Other web pages No page

More data 2 references

Planet TOI-1467 b

Planet

Basic informations 28 parameters

Atmospheric parameters : Temperatures 0 temperatures

Atmospheric parameters : Molecules 0 molecules

Remarks No remark

Other web pages No page

Star

Basic informations 13 parameters

Planetary system 1 planet

Remarks No remark

Other web pages No page

More data 2 references

Related publications

The TESS-Keck Survey XX: 15 New TESS Planets and a Uniform RV Analysis of all Survey Targets

VaTEST III: Validation of 8 Potential Super-Earths from TESS Data

The TESS-Keck Survey: Science Goals and Target Selection

The Revised TESS Input Catalog and Candidate Target List