WebGravitational scattering of planetesimals towards the white dwarf requires the presence of more massive bodies(6), yet no planet has so far been detected at a white dwarf. Here we report optical spectroscopy of a hot (about 27,750 kelvin) white dwarf, WD J091405.30+191412.25, that is accreting from a circumstellargaseous disk composed of … Web1 May 2024 · An emerging hypothesis is that evaporation of molten or partially molten rocky planetesimals, planetary embryos, and/or proto-planets 1 caused losses of moderately volatile elements (e.g., Zn and K) and “common” or moderately refractory elements (e.g., Mg and Si, with condensation temperatures >~1300 K and <~1580 K, Lodders, 2003) during …
The evolution of the Earth surface sulfur reservoir
Web13 Sep 2014 · Their aim is to constrain the nature of volatile element depletion and so potentially to reveal how and when such depletion occurred and whether it relates to … Web3 Mar 2024 · Here, we address the problem of planetesimal volatile loss by focusing on carbon and sulfur, two siderophile volatile elements that give important clues to the … perto ccid driver download
Elemental sulfur reduction in the deep-sea vent thermophile ...
WebThe presence of sulfur mass-independent fractionation (S-MIF) in sediments more than 2.45 × 10(9) years old is thought to be evidence for an early anoxic atmosphere. Photolysis of … Web1 Oct 1987 · The sublimation flux for sulfur samples at room temperature was found to vary with the following parameters: (a) sample melt temperature, (b) sublimation period (time), (c) open-space constraint (presence or absence of the cover (plate), and (d) background chamber pressure. Web7 Apr 2024 · Understanding whether sulfur exists and how it affects these atmospheres can help scientists determine whether sulfur gases could be used as a source for life to … pertobe road warrnambool