(Q82188606)

SIMBAD

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

5 references

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

1 reference

1.75 Jupiter mass

1 reference

time of discovery or invention

catalog code

HD 47366b

catalog

Henry Draper Catalogue

1 reference

TIC 443578538b

1 reference

March 2016

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

2 references

inferred from equatorial coordinates

constellation

Canis Major

1 reference

based on heuristic

parent astronomical body

HD 47366

3 references

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

object stated in reference as

HD 47366

SIMBAD

object stated in reference as

HD 47366

argument of periapsis

6.08±24.16 degree

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

−152.1±299.7 degree

1 reference

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

100±100 degree

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

M sin i

1.75±0.2 Jupiter mass

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

2.3±0.18 Jupiter mass

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

2.082±0.113 Jupiter mass

1 reference

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

orbital eccentricity

0.089±0.079

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

0.06±0.04

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

0.071±0.046

1 reference

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

orbital period

359.15±2.34 day

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

359.15±2.34 day

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

363.3±2.5 day

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

360.08±0.72 day

1 reference

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

semi-major axis of an orbit

1.28±0.06 astronomical unit

1 reference

Re-analyzing the Dynamical Stability of the HD 47366 Planetary System

1.214±0.03 astronomical unit

1 reference

A pair of giant planets around the evolved intermediate-mass star HD 47366: multiple circular orbits or a mutually retrograde configuration

1.207±0.002 astronomical unit

1 reference

Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars

declination component of proper motion

parallax

11.8263±0.0636 milliarcsecond

2 references

−125.718±0.082 milliarcsecond per year

2 references

right ascension component of proper motion

9.834±0.081 milliarcsecond per year

2 references

3 references