Planet TOI-2076 c

Detailed information about planet TOI-2076 c and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

TOI-2076 c

Planet Status

Confirmed

Discovered in

2021

Update

2024-08-21

Mass

0.0145 (\pm 0.0072)

M_J 1 publication

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Mass*sin(i)

—

Semi-Major Axis

0.1411 (\begin{matrix} + 0.0015 \\ - 0.0014 \end{matrix})

AU 2 publications

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Orbital Period

21.01549 (\pm 3e-05)

day 1 publication

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Eccentricity

—

ω

—

T_peri

—

Radius

0.2989 (\pm 0.0045)

R_J 2 publications

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)
TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Inclination

88.84 (\pm 0.12)

deg 1 publication

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Detection Method

Primary Transit

Mass Meas. Method

Theoretical

Radius Meas. Method

Primary Transit

Primary transit

2458834.6615 (\pm 0.0005)

JD 1 publication

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Secondary transit

—

λ

—

Impact Parameter b

0.07 (\pm 0.05)

1 publication

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Time V_r=0

—

Velocity Semiamplitude K

1.2 (\pm 0.6)

m/s 1 publication

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Calculated temperature

734.0 (\pm 11.0)

K 1 publication

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

BD+40 2790 c, TOI-2076.03

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-2076

Distance

41.906 (\pm 0.069)

pc 1 publication

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up

Spectral type

G9/K0V

Apparent magnitude V

10.0

Mass

0.849 (\begin{matrix} + 0.027 \\ - 0.026 \end{matrix})

M_Sun 2 publications

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Age

0.3 (\pm 0.08)

Gyr 2 publications

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Effective temperature

5200.0 (\pm 100.0)

K 2 publications

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Radius

0.758 (\pm 0.014)

R_Sun 2 publications

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Metallicity [Fe/H]

-0.03 (\pm 0.06)

2 publications

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up
The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

14:29:34.0

Dec₂₀₀₀

+39:47:26.0

Alternate Names

BD+40 2790

No remarks

No link

Simbad
Most recent references (ADS)

Planet TOI-2076 c

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 3 planets

Remarks No remark

Other web pages No page

More data 2 references

Planet TOI-2076 c

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 3 planets

Remarks No remark

Other web pages No page

More data 2 references

Related publications

The GAPS Programme at TNG. LIX. A characterisation study of the ∼300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)

NEID Reveals that The Young Warm Neptune TOI-2076 b Has a Low Obliquity

Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076

TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow Up