HIP 39017 Overview
HIP 39017
1.52
R⦿
7201.00
K
HIP 39017 b
- Architecture
- HIP 39017
- HIP 39017
- Other Data
- Bibliography 2
- Nearby Data 3
Discovery Data
| Host | Planet | Method | Year | Reference | Disposition |
|---|---|---|---|---|---|
| HIP 39017 | HIP 39017 b | Imaging | 2024 | Tobin et al. 2024 | Confirmed Planet |
- RA
- 07h59m03.98s
- Dec
- -04d19m57.36s
- Distance
-
66.3217+0.2047-0.2035pc
- Parallax
- 15.0493000±0.0460595 mas
- Ecliptic Latitude
- -24.4323 deg
- Ecliptic Longitude
- 122.93477 deg
- Galactic Latitude
- 12.92289 deg
- Galactic Longitude
- 224.74088 deg
- Total Proper Motion
- 52.1902863±0.0531753 mas/yr
- Proper Motion (RA)
- 30.1022000±0.0711883 mas/yr
- Proper Motion (Dec)
- -42.6343000±0.0413625 mas/yr
- Photometry
-
mV6.96076±0.02300
-
mTESS6.6877±0.0061
-
mJ6.361±0.026
-
mH6.263±0.044
-
mKs6.227±0.026
-
mW16.192±0.082
-
mW26.076±0.026
-
mW36.222±0.015
-
mW46.058±0.048
-
mGaia6.904580±0.001071
-
mB7.255±0.025
| Source | Tobin et al. 2024 | TICv8 |
|---|---|---|
|
Teff
(K)
|
--- |
7201.000+142.405-111.618
|
|
L✶
(log10(L⦿))
|
--- |
0.7478793+0.0206789-0.0107203
|
|
ρ✶
(g/cm3)
|
--- |
0.6465040+0.1697699-0.1088059
|
|
M✶
(M⦿)
|
1.52+0.28-0.26
|
1.610000+0.334047-0.214753
|
|
R✶
(R⦿)
|
--- |
1.5198700+0.0406367-0.0743382
|
|
log g
(log10(cm/s2))
|
--- |
4.2812800+0.0940913-0.0723440
|
|
Metallicity
(dex)
|
-0.26±0.13 [Fe/H] | --- |
|
Age
(Gyr)
|
0.115 | --- |
|
Sp. T
|
A9/F0 | --- |
- Status
- Confirmed Planet
- Detected By
- Imaging
- Tools
| Source | Tobin et al. 2024 |
|---|---|
|
Tp
(days)
|
2469682+14648-3741
|
|
ω
(deg)
|
174+131-115
|
|
Mp
(M⨁)
|
7501+2892-2352
|
|
Mp
(MJup)
|
23.6+9.1-7.4
|
|
e
|
0.55+0.35-0.39
|
|
i
(deg)
|
84.0+14.0-20.0
|
|
P
(days)
|
31000+19000-9500
|
|
a
(au)
|
22.1±8.0 |
- Known Objects
- 1 Confirmed Planets
- 2 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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