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Stellar HostProfile

MXB 1658-298

Unclassified star

Records

1

literature rows

Planets

1

system count

References

1

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: Lewin & Joss 1981 • System source: —

Mass

1.98 Msun

single adopted value

1 values • 1 distinct

Planets

1

Stable across source rows

1

System Layout

Known planets

1 planets linked to this host

MXB 1658-298 b

Eclipse Timing Variations

◌

Discovery

2017

Period

760 days

Radius

—

Mass

7532.6 M⊕

Eq. Temp

—

MXB 1658-298 b: A Circumbinary World

MXB 1658-298 is a binary star system, and the host star at its center has a reported mass of 1.98 solar masses. That star's reported mass estimate is larger than the Sun's. A single planet is known to orbit this host.

The planet is MXB 1658-298 b, a circumbinary world discovered in 2017 by the Eclipse Timing Variations method. Because it is circumbinary, it orbits both stars of the binary system rather than one star alone. Its reported mass is 7530 Earth masses, an estimate larger than Earth's and roughly 23.7 times Jupiter's mass. MXB 1658-298 b completes one orbit in 760 days.

Provenance

Underlying measurements and references

Evidence Summary

Rows

1

Stellar refs

1

System refs

0

Massstable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
—1.98—————Lewin & Joss 1981—