Temperature
5991 K
5985.4 to 5991
←Back to Stellar Hosts
Stellar HostProfile
HIP 94235
G V • 58.51 pc
Records
3
literature rows
Planets
1
system count
References
4
distinct source labels
HIP: HIP 94235TIC: TIC 464646604
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: Zhou et al. 2022 • System source: TICv8
Mass
1.09 Msun
1.09 to 1.10
Radius
1.08 Rsun
1.08 to 1.09
Age
0.12 Gyr
single adopted value
Distance
58.51 pc
single adopted value
Spectral Type
G V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 1.08 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
HIP 94235
1.08 R☉
System Layout
Known planets
1 planets linked to this host
HIP 94235 b
Transit
◌
Discovery
2022
Period
7.71 days
Radius
3 R⊕
Mass
379 M⊕
Eq. Temp
1060 K
HIP 94235: A Sun-Like Star and Its Neptune-Like Planet
HIP 94235 is a G V star 191 light-years away, with one known planet. The star's spectral type places it among the Sun-like G-type dwarfs. Its reported mass estimate is larger than the Sun's, at 1.09 solar masses, and its radius is 1.08 solar radii. The star's reported temperature of 5990 K is hotter than the Sun's, and its age is 0.118 billion years.
The single planet, HIP 94235 b, was discovered in 2022 by the transit method and is Neptune-like, a size class that reaches 4 times Earth's radius. Its reported radius estimate is 3 Earth radii, larger than Earth's. Its mass is a reported upper limit of 379 Earth masses. HIP 94235 b orbits every 7.71 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
3
Stellar refs
3
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositystable
Surface Gravitydisputed
Metallicitystable
Spectral Typestable