Results 31 to 40 of about 244,858 (188)

Mercury's resonant rotation from secular orbital elements [PDF]

, 2015
We used recently produced Solar System ephemerides, which incorporate two years of ranging observations to the MESSENGER spacecraft, to extract the secular orbital elements for Mercury and associated uncertainties. As Mercury is in a stable 3:2 spin-orbit resonance these values constitute an important reference for the planet's measured rotational ...
arxiv   +1 more source

Reconciling the dawn-dusk asymmetry in Mercury's exosphere with the micrometeoroid impact directionality [PDF]

, 2017
Combining dynamical models of dust from Jupiter Family Comets and Halley-type Comets, we demonstrate that the seasonal variation of the dust/meteoroid environment at Mercury is responsible for producing the dawn-dusk asymmetry in Mercury's exosphere observed by the MESSENGER spacecraft. Our latest models, calibrated recently from ground-based and space-
arxiv   +1 more source

Total Mass of Ordinary Chondrite Matter Originally Present in the Solar System [PDF]

arXiv, 2004
Recently, I reported the discovery of a new fundamental relationship of the major elements (Fe, Mg, Si) of chondrites that admits the possibility that ordinary chondrite meteorites are derived from two components, a relatively oxidized and undifferentiated, primitive component and a somewhat differentiated, planetary component, with oxidation state ...
arxiv  

XXV.—The detection of traces of mercury salts for toxicological purposes [PDF]

, 1917
Kendall Colin Browning
openalex   +1 more source

MERCURY AND SYPHILIS. [PDF]

The Lancet
n ...
openaire   +3 more sources

SYPHILIS AND MERCURY. [PDF]

The Lancet, 1884
n ...
openaire   +2 more sources

FERRICYANIDES OF MERCURY. [PDF]

Journal of the American Chemical Society, 1906
n ...
openaire   +2 more sources

LXXII. On the absorption spectra of mercury, cadmium, and zinc vapours [PDF]

, 1915
John Cunningham McLennan, Evan Edwards
openalex   +1 more source

Forming Mercury from excited initial conditions [PDF]

arXiv
Mercury is notoriously difficult to form in solar system simulations, due to its small mass and iron-rich composition. Smooth particle hydrodynamics simulations of collisions have found that a Mercury-like body could be formed by one or multiple giant impacts, but due to the chaotic nature of collisions it is difficult to create a scenario where such ...
arxiv  

Anomalous Zeeman Effect in the Satellites of Mercury Lines [PDF]

, 1913
Hantaro Nagaoka, T. Takamine
openalex   +1 more source