←Back to Stellar Hosts
Stellar HostProfile

TOI-4504

K1 V • 342.6 pc

Records

4

literature rows

Planets

3

system count

References

4

distinct source labels

TIC: TIC 349972412

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: Vítková et al. 2025 • System source: TICv8

Temperature

5315 K

5271 to 5315

4 values • 2 distinct

Mass

0.89 Msun

0.89 to 0.90

2 values • 2 distinct

Radius

0.92 Rsun

0.92 to 0.96

4 values • 2 distinct

Age

10 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-0.21 log(Lsun)

-0.21 to -0.19

2 values • 2 distinct

Distance

342.6 pc

single adopted value

4 values • 1 distinct

Spectral Type

K1 V

Consistent across records

K1 V (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 0.92 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-4504

0.92 R☉

System Layout

Known planets

3 planets linked to this host

TOI-4504 b

Transit

◌

Discovery

2024

Period

2.43 days

Radius

2.69 R⊕

Mass

—

Eq. Temp

—

TOI-4504 c

Transit

◌

Discovery

2024

Period

82.97 days

Radius

11.10 R⊕

Mass

1197.3 M⊕

Eq. Temp

—

TOI-4504 d

Transit Timing Variations

◌

Discovery

2024

Period

40.56 days

Radius

—

Mass

450.2 M⊕

Eq. Temp

—

TOI-4504 and Its Three Planets

TOI-4504 is a K1 V star located 1120 light-years away. Its spectral type marks it as a main-sequence dwarf, and it is cooler and less massive and smaller than the Sun, with a reported temperature of 5320 K, a mass of 0.89 solar masses, and a radius of 0.92 solar radii. It is also older than the Sun, with an age of 10 billion years. Three planets orbit this star.

TOI-4504 b is a Neptune-like planet discovered by transit in 2024. Its radius is 2.65 Earth radii, larger than Earth's, and its mass is reported as an upper limit of 140 Earth masses. Its orbital period of 2.43 days is the shortest among the listed planets.

TOI-4504 c is a Jupiter-like planet found by transit in 2024. It has a radius of 11.2 Earth radii, larger than Earth's, and a mass of 821 Earth masses, larger than Earth's and roughly 2.58 times Jupiter's mass. Its mean density is 3.25 g/cm³, 0.589 times Earth's. Its orbital period is 82.8 days, the longest among the listed planets.

TOI-4504 d is a Jupiter-like planet detected through transit timing variations in 2024. Its radius of 11.3 Earth radii is larger than Earth's and the largest among the listed planets, and its mass of 643 Earth masses is larger than Earth's and roughly 2.02 times Jupiter's mass. Its mean density is 2.48 g/cm³, 0.45 times Earth's. Its orbital period is 41.3 days, the second-shortest among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

3

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 2 distinct

Massdisputed

2 values • 2 distinct

Radiusdisputed

4 values • 2 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

4 values • 3 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
53150.890.9210-0.21K1 V342.6Vítková et al. 2025TICv8
52710.900.96—-0.19—342.6TICv8TICv8
5271—0.96———342.6ExoFOPTICv8
5271—0.96———342.6ExoFOPTICv8