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Stellar HostProfile

PSR B1257+12

Unclassified star • 600 pc

Records

2

literature rows

Planets

3

system count

References

3

distinct source labels

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: Konacki and Wolszczan 2003 • System source: Konacki and Wolszczan 2003

Mass

1.40 Msun

single adopted value

1 values • 1 distinct

Age

3 Gyr

0.80 to 3

2 values • 2 distinct

Distance

600 pc

single adopted value

2 values • 1 distinct

Planets

3

Stable across source rows

3

System Layout

Known planets

3 planets linked to this host

PSR B1257+12 b

Pulsar Timing

◌

Discovery

1994

Period

25.26 days

Radius

—

Mass

0.02 M⊕

Eq. Temp

—

PSR B1257+12 c

Pulsar Timing

◌

Discovery

1992

Period

66.54 days

Radius

—

Mass

4.30 M⊕

Eq. Temp

—

PSR B1257+12 d

Pulsar Timing

◌

Discovery

1992

Period

98.21 days

Radius

—

Mass

3.90 M⊕

Eq. Temp

—

PSR B1257+12: A Pulsar With Three Planets

PSR B1257+12 is a pulsar, the small dense remnant of a massive star, located 1,960 light-years away. The star has an age of 3 billion years and a mass of 1.4 solar masses, larger than the Sun's. Three planets are known to orbit it.

PSR B1257+12 b, PSR B1257+12 c, and PSR B1257+12 d were all found by pulsar timing, which detects planets by measuring the clock-like radio pulses of a pulsar; tiny shifts in the pulse schedule reveal orbiting planets. PSR B1257+12 b was announced in 1994, while PSR B1257+12 c and PSR B1257+12 d were both announced in 1992.

PSR B1257+12 b has a mass of 0.02 Earth masses, smaller than Earth's, and an orbital period of 25.3 days, the shortest year among the listed planets. PSR B1257+12 c has a mass of 4.3 Earth masses, larger than Earth's, and an orbital period of 66.5 days, the second-shortest year among the listed planets. PSR B1257+12 d has a mass of 3.9 Earth masses, larger than Earth's, and an orbital period of 98.2 days, the longest year among the listed planets.

Provenance

Underlying measurements and references

Evidence Summary

Rows

2

Stellar refs

2

System refs

1

Distancestable

2 values • 1 distinct

Massstable

1 values • 1 distinct

Agedisputed

2 values • 2 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.40—3——600Konacki and Wolszczan 2003Konacki and Wolszczan 2003
———0.80——600Wolszczan et al. 1992Konacki and Wolszczan 2003