Planet 2M0045+16
Name |
2M0045+16 |
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|
Planet Status |
Confirmed |
|
|
Discovered in |
2019 |
|
|
Mass |
25.0 (± 4.6) MJ |
 |
|
Mass*sin(i) |
— |
|
|
Semi-Major Axis |
— |
|
|
Orbital Period |
— |
|
|
Eccentricity |
— |
|
|
ω |
— |
|
|
Tperi |
— |
|
|
Radius |
— |
|
|
Inclination |
— |
|
|
Update |
2019-06-07 |
|
|
Detection Method |
Imaging |
|
|
Mass Detection Method |
Spectrum |
|
|
Radius Detection Method |
— |
|
|
Primary transit |
— |
|
|
Secondary transit |
— |
|
|
λ |
— |
|
|
Impact Parameter b |
— |
|
|
Time Vr=0 |
— |
|
|
Velocity Semiamplitude K |
— |
|
|
Calculated temperature |
— |
|
|
Measured temperature |
— |
|
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Hottest point longitude |
— |
|
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Geometric albedo |
— |
|
|
Surface gravity log(g/gH) |
— |
|
|
Alternate Names |
— |
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System
Distance |
15.4 (± 0.05) pc |
|
|
RA2000 |
00:45:21.4 |
|
|
Dec2000 |
+16:34:45 |
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|
Remarks
Riedel et al. 2019 : 2M0045+16 is a member of 50 Myr old Argus association. Its spectral type is L2β.
Related publications
Radial Velocities, Space Motions, and Nearby Young Moving Group Memberships of Eleven Candidate Young Brown Dwarfs
2019
RIEDEL A., DITOMASSO V., RICE E., ALAM M., ABRAHAMS E. et al.
Astron. J., 157, 247
paper