Mass
0.45 Msun
single adopted value
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Stellar HostProfile
V2376 Ori
M
Records
1
literature rows
Planets
1
system count
References
2
distinct source labels
TIC: TIC 427394299
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: Vila et al. 2025 • System source: TICv8
Age
7.00e-3 Gyr
single adopted value
Spectral Type
M
Consistent across records
Planets
1
Stable across source rows
System Layout
Known planets
1 planets linked to this host
V2376 Ori b
Imaging
◌
Discovery
2025
Period
—
Radius
87.21 R⊕
Mass
6356.6 M⊕
Eq. Temp
2100 K
V2376 Ori b: A Young Red Dwarf's Giant Planet
V2376 Ori is a small, cool red dwarf with spectral type M, and its age class is very young, with a reported age of 0.007 billion years. The star's reported mass estimate is 0.45 solar masses, smaller than the Sun's. One planet is known to orbit this host: V2376 Ori b, a Jupiter-like world discovered by imaging in 2025.
V2376 Ori b is substantial even by giant-planet standards. Its reported mass estimate is 6360 Earth masses, larger than Earth's and roughly 20 times Jupiter's mass, and its reported radius estimate is 87.2 Earth radii, larger than Earth's. Because a Jupiter-like classification reflects a radius exceeding 4 times Earth's, the size class and the reported radius agree. The planet's mean density is 0.0528 g/cm³, 0.00958 times Earth's.
No orbital period is reported for V2376 Ori b.
Provenance
Underlying measurements and references
Evidence Summary
Rows
1
Stellar refs
1
System refs
1
Massstable
Agestable
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| — | 0.45 | — | 7.00e-3 | — | M | — | Vila et al. 2025 | TICv8 |