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Stellar HostProfile

PSR J2322-2650

Unclassified star • 230 pc

Records

1

literature rows

Planets

1

system count

References

2

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: Spiewak et al. 2018 • System source: Spiewak et al. 2018

Mass

1.40 Msun

single adopted value

1 values • 1 distinct

Distance

230 pc

single adopted value

1 values • 1 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

PSR J2322-2650 b

Pulsar Timing

◌

Discovery

2017

Period

0.32 days

Radius

—

Mass

252.6 M⊕

Eq. Temp

—

PSR J2322-2650 b: A Planet Orbiting a Pulsar

PSR J2322-2650 is a pulsar, the small dense remnant of a massive star, located 750 light-years away. Its reported mass estimate is 1.4 solar masses, larger than the Sun's. One planet orbits this host.

PSR J2322-2650 b was discovered in 2017 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. The planet's minimum mass is 253 Earth masses, larger than Earth's, and its orbital period is 0.323 days. A minimum mass is a lower bound on a planet's true mass, differing from an ordinary mass estimate.

Provenance

Underlying measurements and references

Evidence Summary

Rows

1

Stellar refs

1

System refs

1

Distancestable

1 values • 1 distinct

Parallaxstable

1 values • 1 distinct

Massstable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.40————230Spiewak et al. 2018Spiewak et al. 2018