Planet OGLE-2017-BLG-0560
Name |
OGLE-2017-BLG-0560 |
|
|
Planet Status |
Confirmed |
|
|
Discovered in |
2018 |
|
|
Mass |
1.9 MJ |
 |
|
Mass*sin(i) |
— |
|
|
Semi-Major Axis |
— |
|
|
Orbital Period |
— |
|
|
Eccentricity |
— |
|
|
ω |
— |
|
|
Tperi |
— |
|
|
Radius |
— |
|
|
Inclination |
— |
|
|
Update |
2018-11-21 |
|
|
Detection Method |
Microlensing |
|
|
Mass Detection Method |
— |
|
|
Radius Detection Method |
— |
|
|
Primary transit |
— |
|
|
Secondary transit |
— |
|
|
λ |
— |
|
|
Impact Parameter b |
— |
|
|
Time Vr=0 |
— |
|
|
Velocity Semiamplitude K |
— |
|
|
Calculated temperature |
— |
|
|
Measured temperature |
— |
|
|
Hottest point longitude |
— |
|
|
Geometric albedo |
— |
|
|
Surface gravity log(g/gH) |
— |
|
|
Alternate Names |
— |
|
|
System
Distance |
— |
|
|
RA2000 |
17:51:51.3 |
|
|
Dec2000 |
-30:27:31 |
|
|
Remarks
Mroz et al. 2018 : the lens masse is not unambiguously determined because the microlens parallaxe cannot be measured : if located in the Galactic disk, its mass is 1.9 MJ. If it is located in the Galactic bulge, its mass is 20 MJ.
Related publications
Two new free-floating planet candidates from microlensing
2019
MROZ P., UDALSKI A., BENNET D., RYU Y.-H., SUMI T. et al.
Astron. & Astrophys., 622, A201
paper arxiv