Confirmed Exoplanet Discovered 2023

TOI-2018 b

A sub-neptune orbiting the k-type orange TOI-2018, located approximately 91.3 light-years from Earth.

Key parameters at a glance

  • A radius of 2.27 Earth radii
  • A mass of 9.20 Earth masses
  • Surface gravity around 1.79 g
  • An orbital period of 7.436 days
  • Equilibrium temperature 576 K (303 °C)
  • Distance from Earth 91.31 light-years
  • Earth Similarity Index 0.476
  • Travel time at Voyager 1 speed 1,610,240 years
  • Almost certainly tidally locked to its host star given the close orbit

TOI-2018 b Planet Profile

Physical Specs

Radius
2.27 R⊕
Radius (Jupiter)
0.202 R♃
Mass
9.20 M⊕
Mass (Jupiter)
0.029 M♃
Density
4.33 g/cm³
Surface Gravity
1.79 g (Earth)

Classification

Planet Type

Sub-Neptune

ESI Score 0.476
HZ Position Inner
Controversial No

Discovery

Year 2023
Method Transit
Facility Transiting Exoplanet Survey Satellite (TESS)
Telescope 0.1 m TESS Telescope

Size rank in cohort

Rank by radius

#1568of 1978

top 79.2%

This planet

2.27R⊕

Sub-Neptune median

2.71R⊕

Nearest-size peers

Metric Earth TOI-2018 b Jupiter
Radius (R⊕)1.002.2711.21
Mass (M⊕)1.009.20317.83
Density (g/cm³)5.514.331.33
Surface Gravity (g)1.001.792.53
Insolation (S⊕)1.0026.080.037

Alternative Mass Estimates

Method Value Interpretation
Best measured mass 9.200 M⊕ Direct mass measurement (not derived).

Star Catalogue Identifiers

HIP

HIP 74981

TIC

TIC 357501308

Gaia DR2

Gaia DR2 1272123859439770368

Gaia DR3

Gaia DR3 1272123859439770368

System

TOI-2018

Percentile among Sub-Neptune cohort

Radius 2.268 R⊕ · percentile 21 / cohort 1978
Mass 9.200 M⊕ · percentile 67 / cohort 1978
Orbital period 7.44 d · percentile 24 / cohort 1946
Distance 28.00 pc · percentile 7 / cohort 1975
ESI 0.476 · percentile 67 / cohort 1978

Orbit & Habitability

Orbital Dynamics

Period
7.436 days
Semi-major axis
AU
Eccentricity
0.000
Inclination
88.52 °

Year Length

A year here lasts approximately 7.44 Earth days (2.0% of a terrestrial year) on a nearly circular orbit.

Transit Fingerprint

Depth

0.131 %

Duration

2.360 h

Impact parameter b

0.546

Rp / R★

0.033500

Transit midpoint (BJD)

2,458,958.2580

Photometric dip

Transit produces a flux drop of 1,311 ppm lasting ≈ 2.36 h.

Extended Orbital Architecture

Planet / star radius ratio

0.033500

Semi-major axis / stellar radius

21.120

Impact parameter (b)

0.546

RV semi-amplitude (K)

4.400 m/s

Transit mid-time (BJD)

2,458,958.2580

Eq. Temperature

576K

(303 °C)

Insolation (S⊕)

26.08

Earth = 1.00

Earth Similarity (ESI)

0.476

0 = alien, 1 = Earth-identical

Inside the inner HZ boundary (too hot for liquid water) — the surface is too hot to retain surface water. Close-orbiting tidally-locked around a cool host.

Detection Signatures

Transit photometry

A transit dip has been observed from at least one telescope.

Radial velocity

Stellar wobble has been measured spectroscopically.

Discovery Paper

Primary reference

Dai et al. 2023

Instrument

TESS CCD Array

Publication

2023-06

Observation locale

Space

Host System: TOI-2018

Spectral Class

K-type orange

Effective Temperature

4,174 K — cooler than the Sun (5,778 K)

Estimated Age

Stellar Radius

0.620 R☉

Stellar Mass

0.570 M☉

Metallicity [Fe/H]

-0.58

Extended Stellar Properties

Surface gravity (log g)

4.620 dex

Stellar density

3.229 g/cm³

Rotational v·sin i

2.00 km/s

Rotation period

23.50 days

Activity index (log R'HK)

-4.750

Metallicity ratio

[Fe/H]

Distance
28.00 parsec
Light-years 91.31 ly
V-band magnitude
10.25 mag
Voyager-speed travel 1,610,240 yr

Multi-band Host Photometry — 12 bands

7.115.815.79U11.43B10.25V9.72Gaia8.96TESS11.04Sloan g13.37Sloan r9.29Sloan i10.05Sloan z7.84J7.26H7.10K

Astrometric Data

Parallax

35.691 mas

Total Proper Motion

419.917 mas/yr

PM Right Ascension

-141.10 mas/yr

PM Declination

395.50 mas/yr

Galactic Cartesian (pc)

x = -0.563 · y = -0.667 · z = 0.488

Equatorial (J2000)

RA 229.83744° · Dec 29.20788°

Galactic ℓ, b

45.426° · 57.468°

Ecliptic λ, β

216.584° · 45.484°

HTM-20 index

-1327903545

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