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Stellar HostProfile

Pr0211

Unclassified star • 182.7 pc

Records

4

literature rows

Planets

2

system count

References

5

distinct source labels

TIC: TIC 175291727

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: Malavolta et al. 2016 • System source: TICv8

Temperature

5300 K

5088.6 to 5326

4 values • 4 distinct

Mass

0.94 Msun

0.88 to 0.95

3 values • 3 distinct

Radius

0.83 Rsun

0.83 to 0.87

4 values • 4 distinct

Age

0.58 Gyr

single adopted value

1 values • 1 distinct

Distance

182.7 pc

single adopted value

4 values • 1 distinct

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 0.83 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

Pr0211

0.83 R☉

System Layout

Known planets

2 planets linked to this host

Pr0211 b

Radial Velocity

◌

Discovery

2012

Period

2.15 days

Radius

—

Mass

597.5 M⊕

Eq. Temp

—

Pr0211 c

Radial Velocity

◌

Discovery

2016

Period

4850 days

Radius

—

Mass

2475.9 M⊕

Eq. Temp

—

Pr0211: A Two-Planet System Nearly 596 Light-Years Away

Pr0211 is a star 596 light-years from Earth with two planets. The host star is 0.578 billion years old and has a mass of 0.935 solar masses, a radius of 0.827 solar radii, and a temperature of 5300 K. Its mass and radius are smaller than the Sun's, and its temperature is cooler than the Sun's.

The planets orbit a star whose gravity they tug on, and both were found by the radial velocity method, which detects the wobble a planet induces in its star's motion. Pr0211 b was discovered in 2012 and has a minimum mass of 598 Earth masses, roughly 1.88 times Jupiter's mass, with an orbital period of 2.15 days. Pr0211 c was discovered in 2016, has a minimum mass of 2480 Earth masses - roughly 7.79 times Jupiter's mass and larger than Earth's - and takes 4850 days to complete one orbit. Among the listed planets, Pr0211 b has the shortest orbital period and the smallest minimum mass, while Pr0211 c has the longest orbital period and the largest minimum mass.

Provenance

Underlying measurements and references

Evidence Summary

Rows

4

Stellar refs

4

System refs

1

Distancestable

4 values • 1 distinct

Parallaxstable

4 values • 1 distinct

Temperaturedisputed

4 values • 4 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

4 values • 4 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitystable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
53260.950.87———182.7Quinn et al. 2012TICv8
5088.6—0.87—-0.34—182.7Gaia DR2TICv8
51680.880.85—-0.33—182.7TICv8TICv8
53000.940.830.58——182.7Malavolta et al. 2016TICv8