HD 124330 Overview
HD 124330
1.30
R⦿
5873.00
K
HD 124330 b
- Architecture
- HD 124330
- HD 124330
- Other Data
- Bibliography 2
- Nearby Data 4
Discovery Data
Host | Planet | Method | Year | Reference | Disposition |
---|---|---|---|---|---|
HD 124330 | HD 124330 b | Radial Velocity | 2021 | Dalal et al. 2021 | Confirmed Planet |
- RA
- 14h11m16.97s
- Dec
- +54d24m32.30s
- Distance
-
60.1977+0.1025-0.1022pc
- Parallax
- 16.5830000±0.0280328 mas
- Ecliptic Latitude
- 60.64128 deg
- Ecliptic Longitude
- 176.0175 deg
- Galactic Latitude
- 59.05418 deg
- Galactic Longitude
- 100.20285 deg
- Total Proper Motion
- 152.2965432±0.0491708 mas/yr
- Proper Motion (RA)
- -147.5000000±0.0495928 mas/yr
- Proper Motion (Dec)
- -37.9208000±0.0422743 mas/yr
- Photometry
-
mV7.88±0.03
-
mTESS7.292±0.006
-
mJ6.712±0.021
-
mH6.459±0.018
-
mKs6.389±0.018
-
mW16.327±0.088
-
mW26.332±0.031
-
mW36.402±0.015
-
mW46.326±0.047
-
mGaia7.716740±0.000324
-
mB8.540±0.024
Source | Dalal et al. 2021 | TICv8 |
---|---|---|
Teff
(K)
|
5873±19 |
6138.000+106.709-145.901
|
Metallicity
(dex)
|
0.22±0.01 [Fe/H] | --- |
γ
(km/s)
|
-30.687±0.001 | --- |
v sin i
(km/s)
|
3.2±1.0 | --- |
M✶
(M⦿)
|
1.150±0.079 |
1.160000+0.189731-0.124504
|
log g
(log10(cm/s2))
|
4.24±0.04 |
4.2716600+0.0994955-0.0652394
|
Sp. T
|
G4 IV | --- |
L✶
(log10(L⦿))
|
--- |
0.33766388+0.01498202-0.01403808
|
ρ✶
(g/cm3)
|
--- |
0.7367696+0.2012894-0.1341902
|
R✶
(R⦿)
|
--- |
1.3044600+0.0730995-0.0473427
|
- Status
- Confirmed Planet
- Detected By
- Radial Velocity
- Tools
Source | Dalal et al. 2021 |
---|---|
ω
(deg)
|
18.28±10.44 |
Mp sin i
(M⨁)
|
238±19 |
Mp sin i
(MJup)
|
0.75±0.06 |
e
|
0.34±0.05 |
i
(deg)
|
>0.8084 |
P
(days)
|
270.66±1.21 |
K
(m/s)
|
22.85±1.23 |
a
(au)
|
0.86±0.04 |
- Known Objects
- 1 Confirmed Planets
- 1 2MASS Point Source Catalog
- Data Files
- 1 SuperWASP Time Series
- 1 Associated Literature Data
- System
- Star
- Confirmed
- Candidate
- False Positive Planet
- Controversial
- False Positive
- Aliases
- Data Access
- Transit Prediction Service
- Time Series
- Kepler | K2
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