Forming planetary systems that contain only minor planets
Estimates of the frequency of planetary systems in the Milky Way are observationally limited by the low-mass planet regime. Nevertheless, substantial evidence for systems with undetectably low planetary masses now exist in the form of main-sequence stars
Veras, Dimitri, Ida, Shigeru
core
Large-amplitude variability driven by giant dust storms on a planetary-mass companion. [PDF]
Tan X +19 more
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Dynamic controls on subsurface water chemistry and habitability on icy moons. [PDF]
Zhang C +8 more
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Catalytic non-energetic formation of diverse peptides on cosmic dust under extraterrestrial conditions. [PDF]
Krasnokutski SA +7 more
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Provenance and distribution of zinc in terrestrial planets. [PDF]
Martins R +4 more
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Single-photon double ionization of ozone: experiment and theory. [PDF]
Ideböhn VD +16 more
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Non-equilibrium preparation of (<i>E</i>)-phosphinimine (HPNH, X<sup>1</sup>A') - a precursor to prebiotic phosphorylating agents. [PDF]
Wang J +8 more
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Waned mantle upwelling contributes to a heavily deformed northern smooth plains on Mercury. [PDF]
Xie J, Zhan Y, Gong S, Huang C, Zhang J.
europepmc +1 more source
Shock compression of FeOOH and implications for iron-water interactions in super-earth magma oceans. [PDF]
Zhang Y +21 more
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