Planet KMT-2019-BLG-0842 b
Name |
KMT-2019-BLG-0842 b |
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Planet Status |
Confirmed |
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Discovered in |
2019 |
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Mass |
10.28 ( -5.28 +5.84 ) MJ |
 |
|
Mass*sin(i) |
— |
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Semi-Major Axis |
3.31 ( -1.47 +1.38 ) AU |
 |
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Orbital Period |
— |
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Eccentricity |
— |
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ω |
— |
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Tperi |
— |
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Radius |
— |
|
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Inclination |
— |
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Update |
2019-12-10 |
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Detection Method |
Microlensing |
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Mass Detection Method |
Microlensing |
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Radius Detection Method |
— |
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Primary transit |
— |
|
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Secondary transit |
— |
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λ |
— |
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Impact Parameter b |
— |
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Time Vr=0 |
— |
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Velocity Semiamplitude K |
— |
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Calculated temperature |
— |
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Measured temperature |
— |
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Hottest point longitude |
— |
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Geometric albedo |
— |
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Surface gravity log(g/gH) |
— |
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Alternate Names |
— |
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Star
Name |
KMT-2019-BLG-0842 |
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|
Distance |
3320.0 ( -1390.0 +1220.0 ) pc |
 |
|
Spectral type |
— |
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Apparent magnitude V |
— |
|
|
Mass |
0.76 ( -0.39 +0.42 ) MSun |
 |
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Age |
— |
|
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Effective temperature |
— |
|
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Radius |
— |
|
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Metallicity [Fe/H] |
— |
|
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Detected Disc |
— |
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Magnetic Field |
— |
|
|
RA2000 |
17:53:50.0 |
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Dec2000 |
-29:52:39 |
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Alternate Names |
|
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Planetary system |
1 planet
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Related publications
Systematic KMTNet Planetary Anomaly Search. IV. Complete Statistical Sample of 2019 Prime-Field Microlensing Planets
2022
ZANG W., YANG H., HAN Ch., LEE Ch.-U., UDALSKY A. et al.
MNRAS, 515, 928
paper arxiv
KMT-2019-BLG-0842Lb: A Cold Planet Below the Uranus/Sun Mass Ratio
2019
JUNG Y., UDALSKI A., ZANG W., BOND I., YEE J. et al.
Astron. J., 160, 255
paper arxiv