Search Results - "Morlok, A"
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Abundant Circumstellar Silica Dust and SiO Gas Created by a Giant Hypervelocity Collision in the ~12 Myr HD172555 System
Published in The Astrophysical journal (20-08-2009)“…The fine dust detected by infrared (IR) emission around the nearby Delta *b Pic analog star HD172555 is very peculiar. The dust mineralogy is composed…”
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HD 145263: Spectral Observations of Silica Debris Disk Formation via Extreme Space Weathering?
Published in The Astrophysical journal (01-05-2020)“…We report here time-domain infrared spectroscopy and optical photometry of the HD 145263 silica-rich circumstellar-disk system taken from 2003 through 2014. We…”
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Studying the Composition and Mineralogy of the Hermean Surface with the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) for the BepiColombo Mission: An Update
Published in Space science reviews (01-09-2020)“…Launched onboard the BepiColombo Mercury Planetary Orbiter (MPO) in October 2018, the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) is on its…”
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A SELF-CONSISTENT MODEL OF THE CIRCUMSTELLAR DEBRIS CREATED BY A GIANT HYPERVELOCITY IMPACT IN THE HD 172555 SYSTEM
Published in The Astrophysical journal (10-12-2012)“…Spectral modeling of the large infrared excess in the Spitzer IRS spectra of HD 172555 suggests that there is more than 10 super(19) kg of submicron dust in…”
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SPITZER EVIDENCE FOR A LATE-HEAVY BOMBARDMENT AND THE FORMATION OF UREILITES IN η CORVI At ∼1 Gyr
Published in The Astrophysical journal (10-03-2012)Get full text
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Cosmochemical and spectroscopic properties of Northwest Africa 7325-A consortium study
Published in Meteoritics & planetary science (01-01-2016)“…This work is part of a project to build an infrared database in order to link IR data of planetary materials (and therefore possible Mercury material) with…”
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Circumstellar Dust Created by Terrestrial Planet Formation in HD 113766
Published in The Astrophysical journal (01-02-2008)“…We present an analysis of the gas-poor circumstellar material in the HD 113766 binary system (F3/F5, 10-16 Myr), recently observed by the Spitzer Space…”
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Correction to: Studying the Composition and Mineralogy of the Hermean Surface with the Mercury Radiometer and Thermal Infrared Spectrometer (MERTIS) for the BepiColombo Mission: An Update
Published in Space science reviews (01-12-2020)“…A Correction to this paper has been published: https://doi.org/10.1007/s11214-020-00780-w…”
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Sample return of primitive matter from the outer Solar System
Published in Experimental astronomy (01-12-2022)“…The last thirty years of cosmochemistry and planetary science have shown that one major Solar System reservoir is vastly undersampled in the available suite of…”
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Spectroscopic Characterization of Impactites and a Machine Learning Approach to Determine the Oxidation State of Iron in Glass‐Bearing Materials
Published in Journal of geophysical research. Planets (01-03-2023)“…We investigated a suite of impact glass‐bearing rocks using a multi‐analytical approach including visible‐near‐infrared diffuse reflectance spectroscopy,…”
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Mid-infrared spectra of the shocked Murchison CM chondrite: Comparison with astronomical observations of dust in debris disks
Published in Icarus (New York, N.Y. 1962) (01-05-2010)“…We present laboratory mid-infrared transmission/absorption spectra obtained from matrix of the hydrated Murchison CM meteorite experimentally shocked at peak…”
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Mid-infrared spectroscopy of components in chondrites: Search for processed materials in young Solar Systems and comets
Published in Icarus (New York, N.Y. 1962) (01-03-2014)“…•We present FTIR absorption spectra for chondrules, CAIs, fine-grained matrix.•Comparison shows similarity with astronomical dust (circumstellar disks,…”
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Chondrules born in plasma? Simulation of gas-grain interaction using plasma arcs with applications to chondrule and cosmic spherule formation
Published in Meteoritics & planetary science (01-12-2012)“…– We are investigating chondrule formation by nebular shock waves, using hot plasma as an analog of the heated gas produced by a shock wave as it passes…”
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2–16 μm spectroscopy of micron-sized enstatite (Mg,Fe)2Si2O6 silicates from primitive chondritic meteorites
Published in Monthly notices of the Royal Astronomical Society (2007)“…We present mid-infrared spectra from individual enstatite silicate grains separated from primitive type 3 chondritic meteorites. The 2–16 μm transmission…”
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SPITZER EVIDENCE FOR A LATE-HEAVY BOMBARDMENT AND THE FORMATION OF UREILITES IN [eta] CORVI At ~1 Gyr
Published in The Astrophysical journal (10-03-2012)“…We have analyzed Spitzer and NASA/IRTF 2-35 mu m spectra of the warm, ~350 K circumstellar dust around the nearby MS star [eta] Corvi (F2V, 1.4 + or - 0.3…”
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Mid-infrared spectroscopy of refractory inclusions (CAIs) in CV and CO chondrites
Published in Meteoritics & planetary science (01-07-2008)“…— We present laboratory mid‐infrared absorption spectra (2.5 urn to 16.0 μm) of powdered calcium‐aluminum‐rich inclusions (CAIs) and matrix separated from the…”
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2-16 m spectroscopy of micron-sized enstatite (Mg,Fe)2Si2O6 silicates from primitive chondritic meteorites
Published in Monthly notices of the Royal Astronomical Society (11-04-2007)“…We present mid-infrared spectra from individual enstatite silicate grains separated from primitive type 3 chondritic meteorites. The 2-16 mum transmission…”
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FTIR 2-16 micron spectroscopy of micron-sized olivines from primitive meteorites
Published in Meteoritics & planetary science (01-05-2006)“…— Infrared spectra of mineral grains from primitive meteorites could be useful for comparison with astronomical infrared spectra since some of their grains…”
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FT–IR microspectroscopy of extraterrestrial dust grains: Comparison of measurement techniques
Published in Planetary and space science (01-05-2006)“…Identification of astronomical dust composition rests on comparison of Infrared (IR) spectra with standard laboratory spectra; frequently, however, a single…”
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Laboratory IR spectroscopy of soils from Apollo 14, 15, and 16: Spectral parameters and maturity
Published in Planetary and space science (15-11-2022)“…Sieved size fractions (0–25 μm, 25–63 μm, 63–125 μm, and 125–250 μm) and bulk (unsieved) material from lunar soils from Apollo 14 (14163,135 and14259,672),…”
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