LHS 1140 b
Sign in to saveAlso known as NAME G 268-38b, TOI-256.01, TIC 92226327b, LHS 1140b
extrasolar planet
In the Vinony graph
Within Vinony's link graph, LHS 1140 b is referenced by 462 other articles, and connects out to Tau Ceti, method of detecting extrasolar planets and day.
It is catalogued under topics including Cetus, Exoplanets discovered in 2017 and Extraterrestrial water.
Its subject is documented across 19 Wikipedia language editions.
Astronomical data · SIMBAD
- Object type
- Pl
- Distance
- 49 light-years
- Coordinates
- RA 11.2472° · Dec -15.2715°
View on SIMBAD →
via SIMBAD · CDS Strasbourg
Exoplanet data
- Host star
- LHS 1140
- Discovered
- 2017
- Discovered by
- MEarth Project
- Orbital period
- 24.74 days
- Radius
- 1.73 × Earth
- Mass
- 5.60 × Earth
- Equilibrium temp
- 226 K
- Distance
- 14.99 pc
via NASA Exoplanet Archive
Wikidata facts
- Instance of
- star
- Constellation
- Cetus
- Parent body
- LHS 1140
- Radius
- 0.15407
- Mass
- 0.02196
- Orbital period
- 24.736
- Image
- Artist’s impression of the super-Earth exoplanet LHS 1140b.jpg
Show 14 more facts
- time of discovery or invention
- 2017-04-00
- right ascension
- 11.24721458043250
- declination
- -15.27153975691278
- epoch
- J2000.0
- catalog code
- TIC 92226327b
- orbital inclination
- 89.912
- discovery method
- transit method
- semi-major axis of an orbit
- 0.0946
- orbital eccentricity
- 0.043
- M sin i
- 6.09
- right ascension component of proper motion
- 317.585
- declination component of proper motion
- -596.617
- parallax
- 66.6996
- Commons category
- LHS 1140 b
Sources (1)
via Wikidata · CC0