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Stellar HostProfile

TOI-1736

Unclassified star • 88.95 pc

Records

5

literature rows

Planets

2

system count

References

6

distinct source labels

TIC: TIC 408618999

Approximate color

from effective temperature

Canonical Summary

Adopted host values from one source row

Values come from the row with the most populated summary measurements. Missing values stay missing. Ranges and counts describe all source rows.

Stellar source: MacDougall et al. 2023 • System source: TICv8

Temperature

5636 K

5636 to 5807

5 values • 4 distinct

Mass

1.04 Msun

1 to 1.08

4 values • 4 distinct

Radius

1.43 Rsun

1.15 to 1.43

5 values • 5 distinct

Age

9.20 Gyr

4.90 to 9.20

3 values • 3 distinct

Luminosity

0.27 log(Lsun)

0.25 to 0.27

3 values • 3 distinct

Distance

88.95 pc

single adopted value

5 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.43 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1736

1.43 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1736 b

Transit

◌

Discovery

2023

Period

7.07 days

Radius

3.18 R⊕

Mass

12.30 M⊕

Eq. Temp

1099.8 K

TOI-1736 c

Radial Velocity

◌

Discovery

2023

Period

571.2 days

Radius

—

Mass

2441 M⊕

Eq. Temp

—

TOI-1736: A Distant Star with Two Known Worlds

TOI-1736 is a star located 290 light-years from Earth, and two planets have been detected in orbit around it. The host star is 9.2 billion years old and contains 1.04 solar masses of material. Its radius is 1.43 solar radii, so it is larger than the Sun, and its temperature of 5640 K makes it cooler than the Sun.

The first planet, TOI-1736 b, was discovered in 2023 by the transit method, which detects the small dip in a star's brightness when a planet passes in front of it. Classified as Neptune-like, this planet has a radius of 3.18 Earth radii, larger than Earth's, and a mass of 12.3 Earth masses, also greater than Earth's. Its mean density is 2.1 g/cm³, 0.382 times Earth's. TOI-1736 b completes one orbit in 7.07 days, the shortest year among the listed planets.

TOI-1736 c was also announced in 2023, but it was found through the radial velocity method, which measures the wobble a planet's gravity induces in its star. This planet has a minimum mass of 2440 Earth masses, meaning its true mass is at least that value, and this lower bound is larger than Earth's. In fact, the minimum mass is roughly 7.68 times Jupiter's mass. TOI-1736 c takes 571 days to complete one orbit, the longest year among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

5 values • 4 distinct

Massdisputed

4 values • 4 distinct

Radiusdisputed

5 values • 5 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

3 values • 3 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitydisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
56701.061.388.60——88.95Akana Murphy et al. 2023TICv8
565611.41—0.26—88.95TICv8TICv8
58071.081.154.900.25—88.95Martioli et al. 2023TICv8
56361.041.439.200.27—88.95MacDougall et al. 2023TICv8
5656—1.41———88.95ExoFOPTICv8