Planet QS Vir (AB)b

Detailed information about planet QS Vir (AB)b and its parameters.

Planet parameters Publications Observability Predictor

Planet

Name

QS Vir (AB)b

Planet Status

Candidate

Discovered in

2009

Update

2024-08-03

Mass

57.71 (\begin{matrix} + 6.29 \\ - 17.71 \end{matrix})

M_J

Mass*sin(i)

57.71 (\begin{matrix} + 6.29 \\ - 17.71 \end{matrix})

M_J 1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

Semi-Major Axis

7.06 AU 1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

Orbital Period

6091.85 (\begin{matrix} + 171.55 \\ - 153.3 \end{matrix})

day 1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

Eccentricity

0.91 (\begin{matrix} + 0.07 \\ - 0.17 \end{matrix})

1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

ω

215.95 deg 1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

T_peri

—

Radius

—

Inclination

—

Detection Method

Timing

Mass Meas. Method

Timing

Radius Meas. Method

—

Primary transit

—

Secondary transit

—

λ

—

Impact Parameter b

—

Time V_r=0

53849.16 JD 1 publication

Unveiling hidden companions in post-common-envelope binaries: A robust strategy and uncertainty exploration

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

24 May 2010: Planetary companion incompatible with new data (Parsons et al. 2010).
Jul 2022: Alternative orbital solution considers a brown dwarf third body in highly eccentric orbit and possibly a fourth unseen (substellar?) object too.
Jan 2024: The presence of third body appears confirmed whereas it cannot be excluded for the hypothetical fourth body in the outer regions of the QS Vir system. However current available observations are insufficient to confidently confirm or rule out the presence of such an additional body.

No link

Star

Name

QS Vir (AB)

Distance

48.0 (\pm 5.0)

pc 1 publication

The DA+dMe eclipsing binary EC13471-1258: its cup runneth over ... just

Spectral type

DA+M3.5V

Apparent magnitude V

14.4

Mass

0.78 (\pm 0.04)

M_Sun 1 publication

The DA+dMe eclipsing binary EC13471-1258: its cup runneth over ... just

Age

—

Effective temperature

14220.0 (\pm 350.0)

K 1 publication

The DA+dMe eclipsing binary EC13471-1258: its cup runneth over ... just

Radius

0.011 (\pm 0.01)

R_Sun 1 publication

The DA+dMe eclipsing binary EC13471-1258: its cup runneth over ... just

Metallicity [Fe/H]

—

Detected Disc

—

Magnetic Field

—

RA₂₀₀₀

13:49:52.0

Dec₂₀₀₀

-13:13:38.0

Alternate Names

EC 13471-1258

QS Vir is an eclipsing binary of cataclysmic variable type (P = 0.15069444 d, i = 75.5 ± 2°). Secondary star is a red dwarf (spT M3.5-M4V, m_B = 0.43 ± 0 .04 M_Sol, r_B = 0.42 ± 0.02 R_Sol, T_B = 3100 ± 75 K). Combined luminosity at quiescent state is 0.0104 L_Sol (0.004 + 0.01 L_Sol).