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Stellar HostProfile

BD-06 1339

K7/M0 V • 20.27 pc

Records

5

literature rows

Planets

2

system count

References

6

distinct source labels

TIC: TIC 66914642HIP: HIP 27803

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: Lo Curto et al. 2013 • System source: TICv8

Temperature

4324 K

4042 to 4324

4 values • 4 distinct

Mass

0.70 Msun

0.57 to 0.70

3 values • 3 distinct

Age

4.40 Gyr

single adopted value

1 values • 1 distinct

Luminosity

-1.02 log(Lsun)

-1.02 to -0.95

4 values • 4 distinct

Distance

20.27 pc

single adopted value

5 values • 1 distinct

Spectral Type

K7/M0 V

Multiple classifications reported

K7 (1), K7/M0 V (1), M0V (1)

Planets

2

Stable across source rows

2

System Layout

Known planets

2 planets linked to this host

BD-06 1339 b

Radial Velocity

◌

Discovery

2013

Period

3.87 days

Radius

—

Mass

8.50 M⊕

Eq. Temp

—

BD-06 1339 c

Radial Velocity

◌

Discovery

2013

Period

125.9 days

Radius

—

Mass

53 M⊕

Eq. Temp

—

BD-06 1339: A Nearby K-Type Dwarf and Its Two Known Planets

BD-06 1339 is a star 66.1 light-years from Earth. Its spectral type, K7/M0 V, places it among the cooler, redder dwarf stars. The star is 4.4 billion years old, holds 0.7 solar masses, and has a temperature of 4320 K. Its mass is smaller than the Sun's, and its temperature is cooler than the Sun's.

Two planets are known to orbit this host. Both were discovered in 2013 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.

BD-06 1339 b has a minimum mass of 8.5 Earth masses and an orbital period of 3.87 days. That minimum mass is larger than Earth's, and among the listed planets it is the smallest minimum mass and the shortest year.

BD-06 1339 c has a minimum mass of 53 Earth masses and an orbital period of 126 days. That minimum mass is larger than Earth's, and among the listed planets it is the largest minimum mass and the longest year.

A minimum mass is a lower bound on a planet's true mass, distinct from an ordinary mass estimate.

Provenance

Underlying measurements and references

Evidence Summary

Rows

5

Stellar refs

5

System refs

1

Distancestable

5 values • 1 distinct

Parallaxstable

5 values • 1 distinct

Temperaturedisputed

4 values • 4 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

3 values • 3 distinct

Agestable

1 values • 1 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

2 values • 2 distinct

Metallicitystable

1 values • 1 distinct

Spectral Typedisputed

3 values • 3 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
43240.70—4.40-1.02K7/M0 V20.27Lo Curto et al. 2013TICv8
4081.6—0.67—-0.96—20.27Gaia DR2TICv8
40420.630.69—-0.95—20.27TICv8TICv8
—————K720.27Hawley et al. 1996TICv8
40600.570.67—-0.96M0V20.27Turnbull 2015TICv8