Temperature
5725 K
5438.3 to 5725
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Stellar HostProfile
NGC 2682 YBP 1514
G5 V • 914.2 pc
Records
5
literature rows
Planets
1
system count
References
6
distinct source labels
TIC: TIC 437034879
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: Brucalassi et al. 2014 • System source: TICv8
Mass
0.96 Msun
0.96 to 0.99
Radius
0.89 Rsun
0.89 to 1.10
Age
4.15 Gyr
single adopted value
Distance
914.2 pc
single adopted value
Spectral Type
G5 V
Consistent across records
Planets
1
Stable across source rows
Scale Comparison
Radius against the Sun
Current adopted radius: 0.89 R☉ (circles scaled linearly by radius)
Sun
1.0 R☉ baseline
NGC 2682 YBP 1514
0.89 R☉
System Layout
Known planets
1 planets linked to this host
NGC 2682 YBP 1514 b
Radial Velocity
◌
Discovery
2014
Period
5.12 days
Radius
—
Mass
127.1 M⊕
Eq. Temp
—
A Distant Sun-Like Star and Its Close-Orbiting Planet
NGC 2682 YBP 1514 is a G-type main-sequence star located 2980 light-years away. Its spectral type is G5 V, and it is 4.15 billion years old. The star's reported mass is 0.96 solar masses, its radius is 0.89 solar radii, and its temperature is 5730 K. Its mass and radius are both smaller than the Sun's, and its temperature is cooler than the Sun's.
One planet orbits this star. NGC 2682 YBP 1514 b was discovered in 2014 using the radial velocity method, which measures the wobble a planet's gravity induces in its star's motion; repeated wobbles reveal the planet and its orbital period. The planet has a minimum mass of 127 Earth masses, meaning its true mass is at least this value, and its minimum mass is larger than Earth's. It completes an orbit every 5.12 days.
Provenance
Underlying measurements and references
Evidence Summary
Rows
5
Stellar refs
5
System refs
1
Distancestable
Parallaxstable
Temperaturedisputed
Massdisputed
Radiusdisputed
Agestable
Luminositydisputed
Surface Gravitydisputed
Metallicitydisputed
Spectral Typestable
| ST TEFF | ST MASS | ST RAD | ST AGE | ST LUM | ST SPECTYPE | SY DIST | Stellar Ref | System Ref |
|---|---|---|---|---|---|---|---|---|
| 5438.3 | — | 1.10 | — | -0.02 | — | 914.2 | Gaia DR2 | TICv8 |
| 5725 | 0.96 | 0.89 | 4.15 | — | G5 V | 914.2 | Brucalassi et al. 2014 | TICv8 |
| 5725 | 0.96 | — | — | — | G5 V | 914.2 | Brucalassi et al. 2017 | TICv8 |
| 5725 | 0.96 | — | — | — | G5 V | 914.2 | Brucalassi et al. 2016 | TICv8 |
| 5605.8 | 0.99 | 1.07 | — | 0.01 | — | 914.2 | TICv8 | TICv8 |