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Stellar HostProfile

HD 192263

K1/2V • 19.64 pc

Records

23

literature rows

Planets

1

system count

References

24

distinct source labels

TIC: TIC 243962745HD: HD 192263HIP: HIP 99711

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: Turnbull 2015 • System source: TICv8

Temperature

4975 K

4947 to 5054

12 values • 9 distinct

Mass

0.80 Msun

0.66 to 0.82

12 values • 10 distinct

Radius

0.77 Rsun

0.70 to 0.78

8 values • 7 distinct

Age

2.56 Gyr

1 to 2.56

4 values • 3 distinct

Luminosity

-0.49 log(Lsun)

-0.55 to -0.47

5 values • 5 distinct

Distance

19.64 pc

single adopted value

23 values • 1 distinct

Spectral Type

K1/2V

Multiple classifications reported

K2 V (2), K0 (1), K0 V (1), K1/2 V (1), K1/2V (1), K2.5 V (1)

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 0.77 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

HD 192263

0.77 R☉

System Layout

Known planets

1 planets linked to this host

HD 192263 b

Radial Velocity

◌

Discovery

1999

Period

24.36 days

Radius

—

Mass

178.0 M⊕

Eq. Temp

—

HD 192263 and Its Planet

HD 192263 is a K1/2V star 64 light-years away. A trailing V marks a main-sequence dwarf, and a K-type star is cooler than the Sun. The star's reported mass estimate is 0.8 solar masses, smaller than the Sun's, and its reported radius estimate is 0.77 solar radii, also smaller than the Sun's. Its reported temperature is 4980 K, cooler than the Sun's, and its age is 2.56 billion years. One planet is known to orbit this host.

That planet, HD 192263 b, was discovered in 1999 by the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. The planet's minimum mass is 178 Earth masses, a lower bound on its true mass that is larger than Earth's, and its orbital period is 24.4 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

23

Stellar refs

23

System refs

1

Distancestable

23 values • 1 distinct

Parallaxstable

23 values • 1 distinct

Temperaturedisputed

12 values • 9 distinct

Massdisputed

12 values • 10 distinct

Radiusdisputed

8 values • 7 distinct

Agedisputed

4 values • 3 distinct

Luminositydisputed

5 values • 5 distinct

Surface Gravitydisputed

12 values • 9 distinct

Metallicitydisputed

11 values • 7 distinct

Spectral Typedisputed

7 values • 6 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
5054—————19.64Maldonado et al. 2015TICv8
—————K019.64Cannon & Pickering 1918TICv8
—————K0 V19.64Vogt et al. 2000TICv8
49960.810.732.09——19.64Dragomir et al. 2012TICv8
—0.74———K2 V19.64Paredes et al. 2021TICv8
—————K2.5 V19.64Gray et al. 2003TICv8
49950.75——-0.47—19.64Santos et al. 2003TICv8
4996—0.75—-0.50—19.64Gaia DR2TICv8
4998.10.820.78———19.64Rosenthal et al. 2021TICv8
49760.660.74———19.64Stassun et al. 2017TICv8
—————K2 V19.64Santos et al. 2000TICv8
——————19.64Valenti & Fischer 2005TICv8
49950.75————19.64Santos et al. 2003TICv8
50280.800.701-0.55—19.64Ghezzi et al. 2010TICv8
——————19.64Wright et al. 2004TICv8
49550.820.77—-0.49—19.64TICv8TICv8
49470.69————19.64Santos et al. 2004TICv8
—0.800.772.56——19.64Takeda et al. 2007TICv8
—————K1/2 V19.64Michigan Catalog, Vol. 5TICv8
49750.81————19.64Butler et al. 2006TICv8
——————19.64Nidever et al. 2002TICv8
——————19.64Nordstrom et al. 2004TICv8
49750.800.772.56-0.49K1/2V19.64Turnbull 2015TICv8