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Gliese 436 b: Revision history


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  • curprev 13:5613:56, 10 December 2021188.214.108.125 talk 20,823 bytes +51 The paper doesn't say it can be a "super-Earth" - it says the alternative possibility to an ice-rich composition is a thinner hydrogen-helium atmosphere atop a dense rocky core - but even in that possibility, it would need at least as much H2/He as Neptune has, not a "super-Earth" in the slightest. undo

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  • curprev 00:1800:18, 12 September 2021Urhixidur talk contribs 20,774 bytes +139 {{cite journal |doi=10.1051/0004-6361/201731442 |title=The CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems |last1=Trifonov |first1=Trifon |last2=Kürster |first2=Martin |last3=Zechmeister |first3=Mathias |last4=Tal-Or |first4=Lev |last5=Caballero |first5=José A. |last6=Quirrenbach |first6=Andreas |last7=Amado |first7=Pedro J. |last8=Ribas |first8=Ignasi |last9=Reiners |first9=Ansgar undo

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