Gliese 682: Perbedaan antara revisi

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'''Gliese 682''' atau '''GJ 682''' adalah bintang [[katai merah]]. Ia terdaftar sebagai bintang terdekat ke-49 ke Matahari, berjarak sekitar 16 tahun cahaya dari Bumi. Meski dekat, bintang ini tergolong redup dengan magnitudo 10,95 dan oleh sebab itu, dibutuhkan teleskop untuk melihatnya. GJ 682 terletak di konstelasi [[Scorpius]], dekat dengan bintang terang [[Theta Scorpii]].<ref>{{Cite journal|last=Genova|first=F.|last2=Bonnarel|first2=F.|last3=Bartlett|first3=J. G.|last4=Dubois|first4=P.|last5=Egret|first5=D.|last6=Jasniewicz|first6=G.|last7=Lesteven|first7=S.|last8=Ochsenbein|first8=F.|last9=Wenger|first9=M.|date=1997-01-01|title=The Centre de Données Astronomiques de Strasbourg|url=http://dx.doi.org/10.1515/astro-1997-0206|journal=Open Astronomy|volume=6|issue=2|doi=10.1515/astro-1997-0206|issn=2543-6376|access-date=2020-10-28|archive-date=2023-08-06|archive-url=https://web.archive.org/web/20230806144551/https://www.degruyter.com/document/doi/10.1515/astro-1997-0206/html|dead-url=no}}</ref> Ia memiliki dua calon planet, salah satunya berada di zona layaklaik huni.<ref>{{Cite web|title=HEC: Data of Potentially Habitable Worlds - Planetary Habitability Laboratory @ UPR Arecibo|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|website=phl.upr.edu|access-date=2020-10-28|archive-date=2017-12-01|archive-url=https://web.archive.org/web/20171201032102/http://phl.upr.edu/projects/habitable-exoplanets-catalog/data|dead-url=yes}}</ref><ref>{{Cite web |url=http://www.hpcf.upr.edu/~abel/phl/tuomi/hec_orbit_GJ_682_b.png |title=Salinan arsip |access-date=2020-10-28 |archive-date=2016-03-04 |archive-url=https://web.archive.org/web/20160304042946/http://www.hpcf.upr.edu/~abel/phl/tuomi/hec_orbit_GJ_682_b.png |dead-url=no }}</ref>
== Sistem planet ==
{{OrbitboxPlanet begin
| name = Gliese 682
| table_ref = <ref name="Tuomi2014">{{Cite journal| arxiv= 1403.0430| bibcode= 2014MNRAS.441.1545T| doi = 10.1093/mnras/stu358| title = Bayesian search for low-mass planets around nearby M dwarfs - estimates for occurrence rate based on global detectability statistics| journal = [[Monthly Notices of the Royal Astronomical Society]]| volume = 441| issue = 2| pages = 1545| year = 2014| last1 = Tuomi | first1 = M.| last2 = Jones | first2 = H. R. A.| last3 = Barnes | first3 = J. R.| last4 = Anglada-Escude | first4 = G.| last5 = Jenkins | first5 = J. S.| display-authors= 1}}</ref>
| period_unit = day
}}
{{OrbitboxPlanet
| exoplanet = b
| mass_earth = >4.4
| semimajor = 0.08
| period = 17.48
| inclination =
| eccentricity = 0.08
}}
{{OrbitboxPlanet
| exoplanet = [[Gliese 682 c|c]]
| mass_earth = >8.7
| semimajor = 0.18
| period = 57.32
| inclination =
| eccentricity = 0.10
}}
{{Orbitbox end}}{{Clear}}
 
== Lihat pula ==
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== Referensi ==
{{Reflist}}
 
[[Kategori:Bintang]]
[[Kategori:Katai merah]]
 
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