(Q18207425)

unconfirmed exoplanet

1 reference

1 reference

0.027365121 Jupiter mass

1 reference

Gliese Catalogue of Nearby Stars

catalog code

GJ 682 c

catalog

1 reference

TIC 16909043c

1 reference

time of discovery or invention

4 March 2014

1 reference

imported from Wikimedia project

English Wikipedia

June 2014

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

2 references

inferred from equatorial coordinates

constellation

Scorpius

1 reference

based on heuristic

parent astronomical body

3 references

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

object stated in reference as

GJ 682

object stated in reference as

GJ 682

argument of periapsis

320.85 degree

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

reason for deprecated rank

320 degree

item/value with less precision and/or accuracy

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

M sin i

8.7±5.8 Earth mass

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

0.027365121 Jupiter mass

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

orbital eccentricity

0.1±0.19

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

orbital period

57.32±0.48 day

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

semi-major axis of an orbit

0.176±0.03 astronomical unit

1 reference

Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics

declination component of proper motion

parallax

199.7031±0.0832 milliarcsecond

2 references

−937.912±0.124 milliarcsecond per year

2 references

right ascension component of proper motion

−706.117±0.185 milliarcsecond per year

2 references

3 references