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Stellar HostProfile

XO-3

Unclassified star • 213.1 pc

Records

13

literature rows

Planets

1

system count

References

14

distinct source labels

TIC: TIC 8400842

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: Rusznak et al. 2025 • System source: TICv8

Temperature

6970 K

6429 to 6970

10 values • 6 distinct

Mass

1.45 Msun

0.58 to 1.45

9 values • 5 distinct

Radius

1.52 Rsun

1.38 to 2.13

10 values • 9 distinct

Age

0.97 Gyr

0.97 to 3

3 values • 3 distinct

Luminosity

0.69 log(Lsun)

0.47 to 0.71

4 values • 4 distinct

Distance

213.1 pc

single adopted value

13 values • 1 distinct

Planets

1

Stable across source rows

1

Scale Comparison

Radius against the Sun

Current adopted radius: 1.52 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

XO-3

1.52 R☉

System Layout

Known planets

1 planets linked to this host

XO-3 b

Transit

◌

Discovery

2007

Period

3.19 days

Radius

14.80 R⊕

Mass

4217.6 M⊕

Eq. Temp

1890 K

XO-3 b: A Giant Planet Around a Hot Star

XO-3 is a single star system 695 light-years away, and it hosts one known planet. The host star is an F5 V main-sequence dwarf with an age of 0.97 billion years, a mass of 1.45 solar masses, a radius of 1.52 solar radii, and a temperature of 6970 K. Its mass and radius estimates are larger than the Sun's, and its temperature is hotter than the Sun's as well.

The planet, XO-3 b, was discovered in 2007 by the transit method, in which a planet passes in front of its star from our viewpoint and causes a small dip in observed brightness. It is classified as Jupiter-like, meaning its radius exceeds four times Earth's. XO-3 b has a mass of 4220 Earth masses, roughly 13.3 times Jupiter's mass, and it orbits its star every 3.19 days.

XO-3 b's radius is 14.8 Earth radii, larger than Earth's. Its mean density is 7.17 g/cm³, 1.3 times Earth's.

Provenance

Underlying measurements and references

Evidence Summary

Rows

13

Stellar refs

13

System refs

1

Distancestable

13 values • 1 distinct

Parallaxstable

13 values • 1 distinct

Temperaturedisputed

10 values • 6 distinct

Massdisputed

9 values • 5 distinct

Radiusdisputed

10 values • 9 distinct

Agedisputed

3 values • 3 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

7 values • 6 distinct

Metallicitydisputed

8 values • 6 distinct

Spectral Typedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
67811.411.49———213.1Tsantaki et al. 2014TICv8
——————213.1Garai et al. 2017TICv8
66731.411.69—0.71—213.1TICv8TICv8
6885.3—1.45—0.63—213.1Gaia DR2TICv8
69701.451.520.970.69—213.1Rusznak et al. 2025TICv8
—————F5 V213.1Johns-Krull et al. 2007TICv8
64301.211.382.82——213.1Bonomo et al. 2017TICv8
64290.581.54———213.1Stassun et al. 2017TICv8
64291.412.13——F5V213.1Johns-Krull et al. 2008TICv8
64291.211.413——213.1Southworth 2010TICv8
64291.211.38—0.47—213.1Winn et al. 2008TICv8
—1.21————213.1Knutson et al. 2014TICv8
6673—1.69———213.1ExoFOPTICv8