HATS-16 Overview
HATS-16
1.24
R⦿
5738.00
K
HATS-16 b
1.300
RJup
HATS-16 Architecture & Discovery Information
| Name | Orbital Separation | Planet Size | Method | Year | Reference | Disposition |
|---|---|---|---|---|---|---|
| HATS-16 | ||||||
| HATS-16 b | 2.69 d | 14.57 R⨁ | Transit | 2016 | Ciceri et al. 2016 | Confirmed Planet |
- RA
- 23h54m14.12s
- Dec
- -30d00m46.94s
- Distance
-
757.044+13.735-13.262pc
- Parallax
- 1.2921000±0.0233744 mas
- Ecliptic Latitude
- -26.76032 deg
- Ecliptic Longitude
- 345.80187 deg
- Galactic Latitude
- -77.12348 deg
- Galactic Longitude
- 16.62766 deg
- Total Proper Motion
- 20.4258335±0.0475491 mas/yr
- Proper Motion (RA)
- 20.3207000±0.0476784 mas/yr
- Proper Motion (Dec)
- -2.0697400±0.0327705 mas/yr
- Photometry
-
mV13.957±0.103
-
mTESS13.2576±0.0065
-
mJ12.652±0.024
-
mH12.335±0.025
-
mKs12.280±0.021
-
mW112.252±0.023
-
mW212.268±0.023
-
mW312.367±0.435
-
mW48.924
-
mGaia13.686400±0.000611
-
mB14.395±0.027
-
mg14.086±0.020
-
mi13.496±0.030
-
mr13.645±0.010
| Source | TICv8 | Gaia DR2 | Ciceri et al. 2016 | ExoFOP | ||
|---|---|---|---|---|---|---|
|
Teff
(K)
|
5863.0±123.0 |
5841.0+59.0-35.0
|
5738±79 | 5738 | ||
|
L✶
(log10(L⦿))
|
0.1729562 |
0.17309649+0.01990833-0.02086500
|
0.173+0.077-0.094
|
--- | ||
|
Metallicity
(dex)
|
--- | --- | -0.100±0.050 [Fe/H] | --- | ||
|
γ
(km/s)
|
--- | --- | 31.594±0.023 | --- | ||
|
v sin i
(km/s)
|
--- | --- | 6.17±0.22 | --- | ||
|
Age
(Gyr)
|
--- | --- | 9.50±1.80 | --- | ||
|
ρ✶
(g/cm3)
|
0.9032306 | --- |
0.72+0.26-0.13
|
--- | ||
|
M✶
(M⦿)
|
1.06 | --- | 0.9700±0.0350 | --- | ||
|
R✶
(R⦿)
|
1.18274 |
1.1918634+0.0144130-0.0237181
|
1.238+0.097-0.127
|
1.1827399730682373 | ||
|
log g
(log10(cm/s2))
|
4.31759 | --- | 4.239±0.079 | 4.23836 | ||
|
Sp. T
|
--- | --- | G3 V | --- | ||
|
Prot
(days)
|
--- | --- | 12.350±0.024 | --- |
- Status
- Confirmed Planet
- Detected By
- Radial Velocity, Transit
| Source | Ciceri et al. 2016 | Patel & Espinoza 2022 | Ivshina & Winn 2022 | ExoFOP | ||
|---|---|---|---|---|---|---|
|
a/R✶
|
6.50+0.70-0.43
|
7.26+1.22-0.87
|
--- | --- | ||
|
b
|
0.732+0.043-0.091
|
0.610+0.120-0.310
|
--- | --- | ||
|
P
(days)
|
2.686502±0.000011 |
2.6865009+0.0000103-0.0000097
|
2.6865049±0.0000042 | 2.6865063856827396±0.0000029802710000 | ||
|
Rp/R✶
|
0.1075±0.0037 |
0.1046+0.0051-0.0063
|
--- | --- | ||
|
TC
(days)
|
2456824.79069±0.00076
(BJD)
|
2459097.57525+0.00100-0.00097
(BJD)
|
2458356.10012±0.00098
(BJD-TDB)
|
2458356.10011600±0.00062408
(BJD)
|
||
|
Teq
(K)
|
1592+61-82
|
--- | --- | 1432.368383466273 | ||
|
Mp
(M⨁)
|
1039±60 | --- | --- | --- | ||
|
Mp
(MJup)
|
3.27±0.19 | --- | --- | --- | ||
|
e
|
<0.00 | --- | --- | --- | ||
|
i
(deg)
|
83.53+1.37-0.86
|
--- | --- | --- | ||
|
ρ
(g/cm3)
|
1.86+0.94-0.48
|
--- | --- | --- | ||
|
Rp
(R⨁)
|
14.6±1.7 | --- | --- | 14.047660228910724±0.286728700000000 | ||
|
Rp
(RJup)
|
1.30±0.15 | --- | --- | 1.2532504609371595±0.0255802652956660 | ||
|
K
(m/s)
|
485±25 | --- | --- | --- | ||
|
a
(au)
|
0.03744±0.00045 | --- | --- | --- | ||
|
T14
(hours)
|
2.621±0.077 | --- | --- | 2.6567230728849522±0.0751722500000000 | ||
|
S
(S⨁)
|
--- | --- | --- | 994.8094610766811 | ||
|
δ
(%)
|
--- | --- | --- | 1.21353375306309±0.03148761000000 |
Nearby Data
(within 30 arcseconds)
Browse Nearby Data
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- Known Objects
- 1 Confirmed Planets
- 2 2MASS Point Source Catalog
- Data Files
- 2 KELT Time Series
- 1 SuperWASP Time Series
- 1 Associated Literature Data
-
Empirical Limb-darkening Coefficients and Transit Parameters of Known Exoplanets from TESS
Patel & Espinoza 2022 Reference Overview -
TESS Transit Timing of Hundreds of Hot Jupiters
Ivshina & Winn 2022 Reference Overview -
The Revised TESS Input Catalog and Candidate Target List
TICv8 Reference Overview -
Gaia Data Release 2
Gaia DR2 Reference Overview -
ExoFOP TOI Table
ExoFOP -
HATS-15b and HATS-16b: Two Massive Planets Transiting Old G Dwarf Stars
Ciceri et al. 2016 Reference Overview -
All WISE Data Release
Cutri et al. 2014 Reference Overview -
2MASS All-Sky Catalog of Point Sources
2MASS Point Source Catalog Reference Overview
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