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Stellar HostProfile

HD 93963 A

G0 V • 82.34 pc

Records

6

literature rows

Planets

2

system count

References

6

distinct source labels

TIC: TIC 368435330HD: HD 93963 A

Approximate color

from effective temperature

Canonical Summary

Adopted host values from all rows

Numeric fields use the median of non-null measurements. Disagreement stays visible through ranges, counts, and provenance.

Temperature

5922 K

5908 to 5987

6 values • 3 distinct

Mass

1.09 Msun

1.08 to 1.11

4 values • 4 distinct

Radius

1.05 Rsun

1.03 to 1.05

6 values • 5 distinct

Age

1.35 Gyr

1.30 to 1.40

2 values • 2 distinct

Luminosity

0.08 log(Lsun)

0.07 to 0.10

4 values • 4 distinct

Distance

82.34 pc

single adopted value

6 values • 1 distinct

Spectral Type

G0 V

Consistent across records

G0 V (1)

Planets

2

Stable across source rows

2

Scale Comparison

Radius against the Sun

Current adopted radius: 1.05 R☉ • circles scaled linearly by radius

Sun

1.0 R☉ baseline

HD 93963 A

1.05 R☉

System Layout

Known planets

2 planets linked to this host

Discovery

2022

Period

3.65 days

Radius

3.23 R⊕

Mass

19.20 M⊕

Eq. Temp

1344 K

Discovery

2022

Period

1.04 days

Radius

1.47 R⊕

Mass

2.80 M⊕

Eq. Temp

1842.2 K

Provenance

Underlying measurements and references

Evidence Summary

Rows

6

Stellar refs

5

System refs

1

Distancestable

6 values • 1 distinct

Parallaxstable

6 values • 1 distinct

Temperaturedisputed

6 values • 3 distinct

Massdisputed

4 values • 4 distinct

Radiusdisputed

6 values • 5 distinct

Agedisputed

2 values • 2 distinct

Luminositydisputed

4 values • 4 distinct

Surface Gravitydisputed

6 values • 5 distinct

Metallicitydisputed

3 values • 2 distinct

Spectral Typestable

1 values • 1 distinct

ST TEFFST MASSST RADST AGEST LUMST SPECTYPESY DISTStellar RefSystem Ref
59081.081.031.300.0782.34MacDougall et al. 2023TICv8
59871.091.030.0882.34Brinkman et al. 2025TICv8
59221.081.050.0982.34TICv8TICv8
59221.0582.34ExoFOPTICv8
59221.0582.34ExoFOPTICv8
59871.111.041.400.10G0 V82.34Serrano et al. 2022TICv8