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Stellar HostProfile

HD 190360

G6 IV • 16.01 pc

Records

35

literature rows

Planets

3

system count

References

24

distinct source labels

HD: HD 190360HIP: HIP 98767TIC: TIC 105999792

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: Naef et al. 2003 • System source: TICv8

Temperature

5590 K

5537.7 to 5590

11 values • 9 distinct

Mass

0.96 Msun

0.96 to 1

13 values • 8 distinct

Radius

1.13 Rsun

1.13 to 1.20

8 values • 7 distinct

Age

6.70 Gyr

6.70 to 15

6 values • 5 distinct

Luminosity

0.05 log(Lsun)

0.05 to 0.08

4 values • 4 distinct

Distance

16.01 pc

single adopted value

35 values • 1 distinct

Spectral Type

G6 IV

Multiple classifications reported

G7 IV-V (3), G6 IV (2), G (1), G V (1), G6IV+... (1), K0 (1)

Planets

3

Stable across source rows

3

Scale Comparison

Radius against the Sun

Current adopted radius: 1.13 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 190360

1.13 R☉

System Layout

Known planets

3 planets linked to this host

HD 190360 b

Radial Velocity

◌

Discovery

2003

Period

2887.5 days

Radius

—

Mass

537 M⊕

Eq. Temp

—

HD 190360 c

Radial Velocity

◌

Discovery

2005

Period

17.12 days

Radius

—

Mass

26.20 M⊕

Eq. Temp

—

HD 190360 d

Radial Velocity

◌

Discovery

2026

Period

88.69 days

Radius

—

Mass

11.90 M⊕

Eq. Temp

—

HD 190360 and Its Three Known Planets

HD 190360 is a star of spectral type G6 IV located 52.2 light-years away, and three planets have been reported orbiting it. The star's age is 6.7 billion years, its mass is 0.96 solar masses, its radius is 1.13 solar radii, and its temperature is 5590 K. Its mass estimate is smaller than the Sun's, its radius is larger than the Sun's, and its temperature is cooler than the Sun's.

HD 190360 b was discovered in 2003 by the radial velocity method, which detects the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. Its mass is 537 Earth masses and its orbital period is 2890 days. Among the listed planets, it has the largest reported mass and the longest year.

HD 190360 c was discovered in 2005, also by radial velocity. Its mass is 26.2 Earth masses and its orbital period is 17.1 days. Among the listed planets, it has the second-smallest reported mass and the shortest year.

HD 190360 d was discovered in 2026 by radial velocity. Its mass is 11.9 Earth masses and its orbital period is 88.7 days. Among the listed planets, it has the smallest reported mass and the second-shortest year.

Provenance

Underlying measurements and references

Evidence Summary

Rows

35

Stellar refs

23

System refs

1

Distancestable

35 values • 1 distinct

Parallaxstable

35 values • 1 distinct

Temperaturedisputed

11 values • 9 distinct

Massdisputed

13 values • 8 distinct

Radiusdisputed

8 values • 7 distinct

Agedisputed

6 values • 5 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

9 values • 7 distinct

Metallicitydisputed

9 values • 6 distinct

Spectral Typedisputed

9 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
55840.96————16.01Santos et al. 2004TICv8
——————16.01Valenti & Fischer 2005TICv8
5537.70.991.17———16.01Rosenthal et al. 2021TICv8
55510.96—8.50—G6 IV16.01Vogt et al. 2005TICv8
——————16.01Duncan et al. 1991TICv8
———15——16.01Sanz-Forcada et al. 2010TICv8
5566.5—1.17—0.07—16.01Gaia DR2TICv8
—0.98————16.01Bryan et al. 2016TICv8
——————16.01Duncan et al. 1991TICv8
—0.981.1513.40——16.01Takeda et al. 2007TICv8
55601.00———G7 IV-V16.01Giovinazzi et al. 2025TICv8
—————G7 IV-V16.01Gray et al. 2006TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
55520.981.1513.400.08G6IV+...16.01Turnbull 2015TICv8
5563—————16.01Harada et al. 2025TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
55900.961.136.700.05G6 IV16.01Naef et al. 2003TICv8
——————16.01Vogt et al. 2005TICv8
——————16.01Nidever et al. 2002TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Wright et al. 2004TICv8
—————G7 IV-V16.01Gray et al. 2003TICv8
55490.981.17—0.07—16.01TICv8TICv8
——————16.01Duncan et al. 1991TICv8
——————16.01Duncan et al. 1991TICv8
—0.991.2011.30—G16.01Giovinazzi et al. 2025TICv8
55900.96————16.01Santos et al. 2003TICv8
—1———G V16.01Feng et al. 2021TICv8
55520.991.14———16.01Stassun et al. 2017TICv8
—————K016.01Cannon & Pickering 1918TICv8