Mass
1.05 Msun
1.05 to 1.29
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Stellar HostProfile
Gaia22dkvL
Unclassified star • 1040 pc
Records
7
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: Wu et al. 2024 • System source: Wu et al. 2024
Distance
1040 pc
890 to 1660
Planets
1
Stable across source rows
System Layout
Known planets
1 planets linked to this host
Gaia22dkvL b
Microlensing
◌
Discovery
2024
Period
—
Radius
—
Mass
187.8 M⊕
Eq. Temp
—
Gaia22dkvL b: A Microlensing Discovery
Gaia22dkvL is a host star located 3390 light-years from Earth. It has a mass of 1.05 solar masses, meaning its mass is 1.05 times that of the Sun. One planet has been found orbiting this star: Gaia22dkvL b. The star is a single-star system, so Gaia22dkvL b is the only known planet orbiting this host.
Gaia22dkvL b was discovered in 2024 using the microlensing method, which detects a planet when its gravity briefly brightens the light of a background star. The planet's reported mass is 188 Earth masses, larger than Earth's mass. No orbital period is reported for Gaia22dkvL b, so the length of its year is unknown.
Provenance
Underlying measurements and references
Evidence Summary
Rows
7
Stellar refs
1
System refs
1
Distancedisputed
Massdisputed
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | 1.15 | — | — | — | — | 1270 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.29 | — | — | — | — | 1580 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.27 | — | — | — | — | 1660 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.16 | — | — | — | — | 980 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.05 | — | — | — | — | 980 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.08 | — | — | — | — | 890 | Wu et al. 2024 | Wu et al. 2024 |
| — | 1.05 | — | — | — | — | 1040 | Wu et al. 2024 | Wu et al. 2024 |