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Stellar HostProfile

TOI-1670

F7 V • 168.1 pc

Records

6

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 441739020

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: Tran et al. 2022 • System source: TICv8

Temperature

6170 K

6170 to 6453

6 values • 4 distinct

Mass

1.21 Msun

1.21 to 1.26

3 values • 3 distinct

Radius

1.32 Rsun

1.31 to 1.32

6 values • 4 distinct

Age

2.53 Gyr

2.30 to 2.53

2 values • 2 distinct

Distance

168.1 pc

single adopted value

6 values • 1 distinct

Spectral Type

F7 V

Consistent across records

F7 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.32 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

TOI-1670

1.32 R☉

System Layout

Known planets

2 planets linked to this host

TOI-1670 b

Transit

◌

Discovery

2022

Period

10.98 days

Radius

2.06 R⊕

Mass

41.32 M⊕

Eq. Temp

1062 K

TOI-1670 c

Transit

◌

Discovery

2022

Period

40.75 days

Radius

11.06 R⊕

Mass

200.2 M⊕

Eq. Temp

684 K

TOI-1670: A Distant Star With Two Known Worlds

TOI-1670 is a star located 548 light-years away with two known planets. It is an F7 V star, a main-sequence dwarf hotter than the Sun, with a reported temperature of 6170 K. Its mass is 1.21 solar masses, its radius is 1.32 solar radii, and its age is 2.53 billion years. The star's mass and radius estimates are both larger than the Sun's, and its temperature is hotter as well.

The two planets orbit this star and were both discovered by the transit method in 2022. TOI-1670 b is classified as a Super-Earth, with a radius of 2.06 Earth radii, larger than Earth's. Its mass is reported as an upper limit of 41.31769291 Earth masses, and its orbital period is 11 days. Among the listed planets, it has the shortest year and the smallest radius.

TOI-1670 c is a Jupiter-like planet with a radius of 11.1 Earth radii, also larger than Earth's. Its mass is 200 Earth masses, larger than Earth's, and its mean density is 0.815 g/cm³, 0.148 times Earth's. Its orbital period is 40.7 days. Among the listed planets, TOI-1670 c has the longest year and the largest radius.

Provenance

Underlying measurements and references

Evidence Summary

Rows

6

Stellar refs

4

System refs

1

Distancestable

6 values • 1 distinct

Parallaxstable

6 values • 1 distinct

Temperaturedisputed

6 values • 4 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

6 values • 4 distinct

Agedisputed

2 values • 2 distinct

Luminositystable

1 values • 1 distinct

Surface Gravitydisputed

6 values • 3 distinct

Metallicitydisputed

2 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
63301.221.312.30——168.1Lubin et al. 2023TICv8
6453—1.31———168.1ExoFOPTICv8
6453—1.31———168.1ExoFOPTICv8
63451.261.31—0.40—168.1TICv8TICv8
61701.211.322.53—F7 V168.1Tran et al. 2022TICv8
6453—1.31———168.1ExoFOPTICv8