exoclock

WASP-130b (HIGH)

Discovered by: Hellier et al. 2017

The Star
Simbad
GAIA
2MASS
CD-41 7923
DR2 6112606840179716096
J13322543-4228309
RA 13:32:25.4360 DEC -42:28:30.964
Parallax
5.777 mas
P.M. RA
6.111 mas/y
P.M. DEC
-1.238 mas/y
MagV
11.1
MagR*
10.736
MagI*
10.304
MagJ
9.896
MagH
9.547
MagK
9.461
MagG
10.972
MagGBP
11.367
MagGRP
10.446
*Calculated from GAIA magnitudes.

Ephemeris - Verified True
Kokori et al. 2022
Mid-time
2457937.62925 ± 0.00022 BJDTDB
Period
11.5509711 ± 2.1e-06 days

Transit Parameters
Hellier et al. 2017
Rp/Rs
0.0957 ± 0.0007
a/Rs
22.66 +0.03 -0.03
i
88.66 +0.12 -0.12 deg
e
-
ω
- deg
DepthR*
11.32 mmag
Duration*
3.74 hours
*Calculated from the other parameters, using PyLightcurve.
**Adjusted based on the space observations.

Limb Darkening Parameters
Hellier et al. 2017
Teff
5625.0 +90.0 -90.0 K
Log(g)
4.49 +0.02 -0.02 cm/s2
Fe/H
0.26 +0.1 -0.1 dex
ExoClock Status
Observing Priority HIGH
Minimum aperture 5.0"
Total Observations (Recent) 9 (2)
O-C -6.69 ± 2.52 minutes
ExoClock Observations (Recent) 4 (2)
Space Observations (Recent) 4 (0)
ETD Observations (Recent) 0 (0)
Literature Mid-times (Recent) 1 (0)
Kepler Rp/Rs -
TESS Rp/Rs 0.09748 ± 0.00054

WASP-130b


ExoClock Observations

Planet
Observation Date
Observer
Observatory
Telescope
Camera / Filter / Exp [s]
O-C
minutes
WASP-130b (HIGH)
2024-05-02
THIAGO PRADO
Home
askar
294MC Pro /ZWO 533 MC / Clear / 45.0
-11.67 ± 3.89
WASP-130b (HIGH)
2023-06-02
Jean-Pascal Vignes
Deep Sky Chile
Planewave CDK400
QHYCCD 600M / rpr / 30.0
-3.09 ± 3.31
WASP-130b (HIGH)
2021-07-09
Yves Jongen
Deep Sky Chile
Plane Wave CDK 17"
Moravian 4G / R / 60.0
-3.57 ± 1.58
WASP-130b (HIGH)
2021-03-27
Yves Jongen
Deep Sky Chile
Plane Wave CDK 17"
Moravian 4G / R / 120.0
-0.78 ± 1.44

Space Observations

Planet
Observation Date
Mission O-C
minutes
WASP-130b (HIGH)
2021-04-19
TESS0.46 ± 0.81
WASP-130b (HIGH)
2021-04-07
TESS1.25 ± 0.79
WASP-130b (HIGH)
2019-05-15
TESS0.15 ± 0.81
WASP-130b (HIGH)
2019-05-04
TESS-0.73 ± 0.72

Literature Mid-times

Planet
Observation Date
Reference O-C
minutes
2014-09-20 Hellier et al. 2017 0.04 ± 0.36
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