Planet HD 41248 c

Detailed information about planet HD 41248 c and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

HD 41248 c

Planet Status

Controversial

Discovered in

2013

Publication Status

—

Update

2019-11-27

Mass

—

Mass*sin(i)

0.0223 (\begin{matrix} + 0.00551 \\ - 0.0111 \end{matrix})

M_J 1 publication

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

Semi-Major Axis

0.107 (\begin{matrix} + 0.005 \\ - 0.004 \end{matrix})

AU 1 publication

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

Orbital Period

13.365 (\begin{matrix} + 0.22 \\ - 0.12 \end{matrix})

day 1 publication

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

Eccentricity

0.0117 (\begin{matrix} + 0.2453 \\ - 0.0871 \end{matrix})

1 publication

Two Super-Earths Orbiting the Solar Analogue HD41248 on the edge of a 7:5 Mean Motion Resonance

Angular distance

—

ω

54.0 (\begin{matrix} + 120.0 \\ - -228.0 \end{matrix})

deg 1 publication

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

T_peri

—

Radius

—

Inclination

—

Detection Method

Radial Velocity

Mass Meas. Method

—

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

—

Velocity Semiamplitude K

1.86 (\begin{matrix} + 0.19 \\ - 0.83 \end{matrix})

m/s 1 publication

Agatha: disentangling periodic signals from correlated noise in a periodogram framework

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

25 May 2014: The planet HD 41248 c has been challenged by Santos et al. (2014).
August 2017: Feng et al (2017) say that the 26 d signal (HD 41248 c announced by Jenkins et al. 2013) is probably caused by a combination of planetary perturbation and stellar rotation while the 18.4 d signal (HD 41248 b announced by Jenkins et al. 2013) is not significant and is an alias of the 13.4 d signal.

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