Gliese 357#Planetary system
{{Short description|Red dwarf with low starspot activity in the Hydra constellation}}
{{Starbox begin}}
{{Starbox image
| image = File:GJ 357 system.png
| caption = Artist concept of the Gliese 357 (GJ357) system.
| credit = Jack Madden
}}
{{Starbox observe
| epoch=J2000
| constell = Hydra{{cite constellation|GJ 357}}
| dec = {{DEC|-21|39|38.8776}}
}}
{{Starbox character
| type = main sequence
}}
{{Starbox astrometry
| radial_v = {{val|-35.03|0.17}}
| prop_mo_ra = {{val|138.722|0.023}}
| prop_mo_dec = {{val|-990.342|0.020}}
| parallax = 105.9789
| p_error = 0.0227
}}
{{Starbox detail
| age_myr =
}}
{{Starbox catalog
| names= {{odlist |HIP=47103 |2MASS=09360161-2139371 |TOI=562}}
}}
{{Starbox reference
| Simbad = HIP+47103
| NSTED = GJ-357
}}
{{Starbox end}}
GJ 357 (Gliese 357) is an M-type main sequence star with an unusually low star spot activity.{{citation|arxiv=2007.10262|title=A Super-Earth Orbiting an Extremely Inactive Host Star|year=2020|doi=10.1051/0004-6361/202038280|last1=Modirrousta-Galian|first1=D.|last2=Stelzer|first2=B.|last3=Magaudda|first3=E.|last4=Maldonado|first4=J.|last5=Güdel|first5=M.|last6=Sanz-Forcada|first6=J.|last7=Edwards|first7=B.|last8=Micela|first8=G.|journal=Astronomy & Astrophysics|volume=A113|page=641|s2cid=220647396}} It is located 31 light-years from the Solar System,{{Cite web|url=https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|title=TESS Discovers Habitable Zone Planet in GJ 357 System|last1=Reddy|first1=Francis|last2=Center|first2=NASA’s Goddard Space Flight|date=2019-07-31|website=SciTechDaily|language=en-US|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801162521/https://scitechdaily.com/tess-discovers-habitable-zone-planet-in-gj-357-system/|url-status=live}} in the Hydra constellation.
Planetary system
The star has three confirmed exoplanets in its orbit. {{Cite encyclopedia|url=https://exoplanet.eu/catalog/gj_357_b--7109/|title=The Extrasolar Planet Encyclopaedia — Gj 357 b|date=1995|encyclopedia=Extrasolar Planets Encyclopaedia|access-date=2019-08-01|archive-date=2023-11-07|archive-url=https://web.archive.org/web/20231107150843/https://exoplanet.eu/catalog/gj_357_b--7109/|url-status=live}} One of these, Gliese 357 d, is considered to be a "super-Earth" within the circumstellar habitable zone.Falconer, Rebecca, [https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html Newly uncovered super-Earth 31 light-years away may be habitable] {{Webarchive|url=https://web.archive.org/web/20191218061126/https://www.axios.com/super-earth-31-light-years-away-may-support-life-d1d0298d-3c82-4f99-a4af-22774fc1ed70.html |date=2019-12-18 }}, Axios, August 1, 2019{{Cite web|url=https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|title=Potentially habitable 'super-Earth' discovered just 31 light-years away|website=NBC News|date=31 July 2019|language=en|access-date=2019-08-01|archive-date=2019-07-31|archive-url=https://web.archive.org/web/20190731230808/https://www.nbcnews.com/mach/science/potentially-habitable-super-earth-discovered-just-31-light-years-away-ncna1037491|url-status=live}}{{Cite web|url=http://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world|title=NASA's TESS Helps Find Intriguing New World|last=Garner|first=Rob|date=2019-07-30|website=NASA|access-date=2019-08-01|archive-date=2019-08-01|archive-url=https://web.archive.org/web/20190801045621/https://www.nasa.gov/feature/goddard/2019/confirmation-of-toasty-tess-planet-leads-to-surprising-find-of-promising-world/|url-status=live}}
Transiting planets b and c are close to 3:7 mean-motion resonance. Presuming resonance chain extends to the outermost, cold, possibly terrestrial Gliese 357 d and the resonances are simple. Transmission spectroscopy of the planet b with JWST in 2025 found no clear evidence for atmospheric molecules, although a secondary atmosphere is considered likely to exist.{{cite arXiv|eprint=2505.24462 |last1=Taylor |first1=Jake |last2=Radica |first2=Michael |last3=Chatterjee |first3=Richard D. |last4=Hammond |first4=Mark |last5=Meier |first5=Tobias |last6=Aigrain |first6=Suzanne |last7=MacDonald |first7=Ryan J. |last8=Albert |first8=Loic |last9=Benneke |first9=Björn |last10=Coulombe |first10=Louis-Philippe |last11=Cowan |first11=Nicolas B. |last12=Dang |first12=Lisa |last13=Doyon |first13=René |last14=Flagg |first14=Laura |last15=Johnstone |first15=Doug |last16=Kaltenegger |first16=Lisa |last17=Lafrenière |first17=David |last18=Pelletier |first18=Stefan |last19=Piaulet-Ghorayeb |first19=Caroline |last20=Rowe |first20=Jason F. |last21=Roy |first21=Pierre-Alexis |title=JWST NIRISS Transmission Spectroscopy of the Super-Earth GJ 357b, a Favourable Target for Atmospheric Retention |date=2025 |class=astro-ph.EP }}
{{OrbitboxPlanet begin
}}
{{OrbitboxPlanet
| exoplanet = b
| mass_earth = {{val|1.84|0.31}}
| radius_earth = {{val|1.217|0.084|0.083}}
| semimajor = {{val|0.035|0.002}}
| period = {{val|3.93072|0.00008|0.00006}}
| eccentricity = 0.047{{±|0.059|0.047|}}
| inclination = {{val|89.12|0.37|0.31}}
}}
{{OrbitboxPlanet
| exoplanet = c
| mass_earth = {{val|3.40|0.46|p=≥}}
| radius_earth =
| semimajor = {{val|0.061|0.004}}
| period = {{val|9.1247|0.0011|0.0010}}
| eccentricity = 0.072{{±|0.053|}}
| inclination =
}}
{{OrbitboxPlanet
| exoplanet = d
| mass_earth = {{val|6.1|1.0|p=≥}}
| radius_earth =
| semimajor = {{val|0.204|0.015}}
| period = {{val|55.661|0.055}}
| eccentricity = 0.033{{±|0.057|0.033|}}
| inclination =
}}
{{Orbitbox end}}
== References ==
{{reflist|refs=
{{Cite Gaia DR3|5664814198431308288}}
{{cite journal |last1=Luque |first1=R. |last2=Pallé |first2=E. |display-authors=etal |date=August 2019 |title=Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization |journal=Astronomy & Astrophysics |volume=628 |issue= |pages=A39 |doi=10.1051/0004-6361/201935801 |arxiv=1904.12818 |bibcode=2019A&A...628A..39L|s2cid=139102184 }}
}}
{{Stars of Hydra}}
Category:Planetary systems with three confirmed planets
Category:M-type main-sequence stars