Planet MOA-2013-BLG-605L b

Detailed information about planet MOA-2013-BLG-605L b and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

MOA-2013-BLG-605L b

Planet Status

Confirmed

Discovered in

2015

Update

2015-12-02

Mass

0.066 (\begin{matrix} + 0.02 \\ - 0.02 \end{matrix})

M_J 1 publication

The First Neptune Analog or Super-Earth with a Neptune-like Orbit: MOA-2013-BLG-605Lb

Mass*sin(i)

—

Semi-Major Axis

4.2 (\pm 0.9)

AU 1 publication

The First Neptune Analog or Super-Earth with a Neptune-like Orbit: MOA-2013-BLG-605Lb

Orbital Period

—

Eccentricity

—

ω

—

T_peri

—

Radius

—

Inclination

—

Detection Method

Microlensing

Mass Meas. Method

Microlensing

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

—

Calculated temperature

—

Measured temperature

—

Hottest point longitude

—

Geometric albedo

—

Surface gravity log(g/g_H)

—

Alternate Names

—

Data Source	Type	Result Value	Result Figure	Notes	Reference

Molecule	Data Source	Type	Result Value	Result Figure	Notes	Reference

02 Dec 2015: The microlensing light curve solution is degenerate and has 3 solutions. The two other solutions for the planet mass and star-planet projected distance at the time of observation are 7.9 +1.8/-1.2 and 3.2 +0.5/-0.3 M_Earth and 2.1 +0.4/-0.2 and 0.94 +0.12/-0.09 AU respectively (Sumi et al. 2015).

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Star

Name

MOA-2013-BLG-605L

Distance

3600.0 (\begin{matrix} + 600.0 \\ - 800.0 \end{matrix})

pc 1 publication

The First Neptune Analog or Super-Earth with a Neptune-like Orbit: MOA-2013-BLG-605Lb

Spectral type

—

Apparent magnitude V

—

Mass

0.19 (\pm 0.06)

M_Sun 1 publication

The First Neptune Analog or Super-Earth with a Neptune-like Orbit: MOA-2013-BLG-605Lb

Age

—

Effective temperature

—

Radius

—

Metallicity [Fe/H]

—

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

17:58:43.0

Dec₂₀₀₀

-29:23:54.0

Alternate Names

—

02 Dec 2015: The microlensing light curve solution is degenerate and has 3 solutions. The two other solutions for the distance and stellar mass are 1.8 +04/-0.2 kpc,0.85 +/0.13/-0.08 kpc, 0.068 +0.019/-0.011 M_Sun and 0.025 +0.005/-0.004 M_Sun respectively (Sumi et al. 2015).

No link