K2-18: Perbedaan antara revisi
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== Referensi ==
{{Reflist|refs=
{{Reflist|refs=<ref name=arturo2017>{{cite journal |doi=10.3847/1538-4357/aa56c7 |title=Stellar and Planetary Parameters for K2's Late-type Dwarf Systems from C1 to C5 |journal=The Astrophysical Journal |volume=837 |issue=1 |pages=72 |year=2017 |last1=Martinez |first1=Arturo O. |last2=Crossfield |first2=Ian J. M. |last3=Schlieder |first3=Joshua E. |last4=Dressing |first4=Courtney D. |last5=Obermeier |first5=Christian |last6=Livingston |first6=John |last7=Ciceri |first7=Simona |last8=Peacock |first8=Sarah |last9=Beichman |first9=Charles A. |last10=Lépine |first10=Sébastien |last11=Aller |first11=Kimberly M. |last12=Chance |first12=Quadry A. |last13=Petigura |first13=Erik A. |last14=Howard |first14=Andrew W. |last15=Werner |first15=Michael W. |bibcode=2017ApJ...837...72M |arxiv=1701.00588 }}</ref>▼
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<ref name=benneke2017>{{cite journal |doi=10.3847/1538-4357/834/2/187 |title=Spitzer Observations Confirm and Rescue the Habitable-zone Super-Earth K2-18b for Future Characterization |journal=The Astrophysical Journal |volume=834 |issue=2 |pages=187 |year=2017 |last1=Benneke |first1=Björn |last2=Werner |first2=Michael |last3=Petigura |first3=Erik |last4=Knutson |first4=Heather |last5=Dressing |first5=Courtney |last6=Crossfield |first6=Ian J. M. |last7=Schlieder |first7=Joshua E. |last8=Livingston |first8=John |last9=Beichman |first9=Charles |last10=Christiansen |first10=Jessie |last11=Krick |first11=Jessica |last12=Gorjian |first12=Varoujan |last13=Howard |first13=Andrew W. |last14=Sinukoff |first14=Evan |last15=Ciardi |first15=David R. |last16=Akeson |first16=Rachel L. |bibcode=2017ApJ...834..187B |arxiv=1610.07249 }}</ref>
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