←Back to Stellar Hosts
Stellar HostProfile

BD+20 2457

K2 II • 1539.7 pc

Records

5

literature rows

Planets

2

system count

References

6

distinct source labels

TIC: TIC 95359428

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: Niedzielski et al. 2009 • System source: TICv8

Temperature

4137 K

4137 to 4329.9

5 values • 4 distinct

Mass

2.80 Msun

1.06 to 10.83

3 values • 3 distinct

Radius

49 Rsun

43.02 to 71.02

4 values • 4 distinct

Luminosity

3.17 log(Lsun)

2.77 to 3.17

2 values • 2 distinct

Distance

1539.7 pc

single adopted value

5 values • 1 distinct

Spectral Type

K2 II

Consistent across records

K2 II (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 49 R☉ (circles scaled linearly by radius)

Sun

1.0 R☉ baseline

BD+20 2457

49 R☉

System Layout

Known planets

2 planets linked to this host

BD+20 2457 b

Radial Velocity

◌

Discovery

2009

Period

379.6 days

Radius

—

Mass

6807.6 M⊕

Eq. Temp

—

BD+20 2457 c

Radial Velocity

◌

Discovery

2009

Period

622.0 days

Radius

—

Mass

3963.2 M⊕

Eq. Temp

—

BD+20 2457: A Distant Star With Two Massive Planets

BD+20 2457 is a star located 5020 light-years away. Its spectral type, K2 II, indicates a cool, bright star, and its measured properties are extreme: a mass of 2.8 solar masses, a radius of 49 solar radii, and a temperature of 4140 K. The star is larger than the Sun in both mass and radius, but cooler than the Sun. Two planets orbit this host.

Both planets were discovered in 2009 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion. BD+20 2457 b has a minimum mass of 6810 Earth masses, meaning its true mass is at least that value, and an orbital period of 380 days. This makes it the shortest-period planet among the listed worlds and the most massive by minimum mass, with a minimum mass roughly 21.4 times Jupiter's mass. BD+20 2457 c has a minimum mass of 3960 Earth masses and an orbital period of 622 days, giving it the longest period among the listed planets and the smallest minimum mass. Its minimum mass is roughly 12.5 times Jupiter's mass. Both planets' minimum masses are larger than Earth's.

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

5 values • 4 distinct

Massdisputed

3 values • 3 distinct

Radiusdisputed

4 values • 4 distinct

Luminositydisputed

2 values • 2 distinct

Surface Gravitydisputed

3 values • 2 distinct

Metallicitydisputed

4 values • 3 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
4329.9—43.02—2.77—1539.7Gaia DR2TICv8
425910.8371.02———1539.7Stassun et al. 2017TICv8
41372.8049—3.17K2 II1539.7Niedzielski et al. 2009TICv8
4182.0—46.05———1539.7TICv8TICv8
42591.06————1539.7Mortier et al. 2013TICv8