HIP 21152 Overview
HIP 21152
1.59
R⦿
6596.11
K
HIP 21152 b
- Architecture
- HIP 21152
- HIP 21152
- Other Data
- Bibliography 2
- Nearby Data 3
Discovery Data
Host | Planet | Method | Year | Reference | Disposition |
---|---|---|---|---|---|
HIP 21152 | HIP 21152 b | Imaging | 2022 | Kuzuhara et al. 2022 | Confirmed Planet |
- RA
- 04h32m04.93s
- Dec
- +05d24m36.27s
- Distance
-
43.4073+0.1311-0.1303pc
- Parallax
- 23.0090000±0.0688374 mas
- Ecliptic Latitude
- -16.30314 deg
- Ecliptic Longitude
- 67.15637 deg
- Galactic Latitude
- -27.59176 deg
- Galactic Longitude
- 190.1461 deg
- Total Proper Motion
- 112.759919±0.124953 mas/yr
- Proper Motion (RA)
- 112.505000±0.125179 mas/yr
- Proper Motion (Dec)
- 7.5778900±0.0563519 mas/yr
- Photometry
-
mV6.37009±0.02300
-
mTESS5.9557±0.0060
-
mJ5.593±0.024
-
mH5.385±0.020
-
mKs5.333±0.021
-
mW15.355±0.173
-
mW25.191±0.053
-
mW35.376±0.016
-
mW45.338±0.032
-
mGaia6.2556800±0.0003405
-
mB6.778±0.024
- Tools
- IRSA Finding Chart
Source | Kuzuhara et al. 2022 | TICv8 |
---|---|---|
Teff
(K)
|
--- |
6596.110+107.649-115.208
|
L✶
(log10(L⦿))
|
--- |
0.6356535+0.0168785-0.0187667
|
Metallicity
(dex)
|
--- | 0.010±0.100 [M/H] |
ρ✶
(g/cm3)
|
--- |
0.4823185+0.1069049-0.1068121
|
M✶
(M⦿)
|
1.30±0.10 |
1.380000+0.288522-0.151927
|
R✶
(R⦿)
|
--- |
1.5918600+0.0666905-0.0559025
|
log g
(log10(cm/s2))
|
--- |
4.1741400+0.0776313-0.0963744
|
Age
(Gyr)
|
0.750±0.100 | --- |
Sp. T
|
F5 V | --- |
- Status
- Confirmed Planet
- Detected By
- Imaging
- Tools
Source | Kuzuhara et al. 2022 |
---|---|
Tp
(days)
|
2463360+5307-1419
|
Teq
(K)
|
1250±50 |
ω
(deg)
|
157+179-132
|
Mp
(M⨁)
|
8836+2670-1716
|
Mp
(MJup)
|
27.8+8.4-5.4
|
e
|
0.52±0.35 |
i
(deg)
|
104.8+15.0-6.9
|
P
(days)
|
23000+16000-7000
|
a
(au)
|
17.5+7.2-3.8
|
- Known Objects
- 1 Confirmed Planets
- 3 2MASS Point Source Catalog
- Data Files
- 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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