Search Results - "Joswiak, D."
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Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples
Published in Science (American Association for the Advancement of Science) (24-02-2023)“…Samples of the carbonaceous asteroid Ryugu were brought to Earth by the Hayabusa2 spacecraft. We analyzed 17 Ryugu samples measuring 1 to 8 millimeters. Carbon…”
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Carbonaceous aerosols recorded in a southeastern Tibetan glacier: analysis of temporal variations and model estimates of sources and radiative forcing
Published in Atmospheric chemistry and physics (02-02-2015)“…High temporal resolution measurements of black carbon (BC) and organic carbon (OC) covering the time period of 1956–2006 in an ice core over the southeastern…”
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Refractory materials in comet samples
Published in Meteoritics & planetary science (01-08-2017)“…Transmission electron microscope examination of more than 250 fragments, >1 μm from comet Wild 2 and a giant cluster interplanetary dust particle (GCP) of…”
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Temperature lapse rate in complex mountain terrain on the southern slope of the central Himalayas
Published in Theoretical and applied climatology (01-08-2013)“…This study presents the first results of monthly, seasonal and annual characteristics of temperature lapse rate on the southern slope of the central Himalayas,…”
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Compositional evidence for chondrule origins of low‐Ca pyroxenes in comet Wild 2 and a giant cluster IDP
Published in Meteoritics & planetary science (01-07-2024)“…A literature compilation of 1136 low‐Ca pyroxene compositions from chondrules from 12 primitive type 2–3 carbonaceous, ordinary and enstatite chondrite groups…”
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Fine‐grained material associated with a large sulfide returned from Comet 81P/Wild 2
Published in Meteoritics & planetary science (01-05-2019)“…In a consortium analysis of a large particle captured from the coma of comet 81P/Wild 2 by the Stardust spacecraft, we report the discovery of a field of…”
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Diversity of the initial rocky planetary building materials at the edge of the solar system
Published in Meteoritics & planetary science (01-03-2017)“…Asteroids and comets are surviving members of the vast planetesimal population that was distributed across the early solar system. They appear to be a diverse…”
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A refractory inclusion returned by Stardust from comet 81P/Wild 2
Published in Meteoritics & planetary science (01-11-2008)“…— Among the samples returned from comet 81P/Wild 2 by the Stardust spacecraft is a suite of particles from one impact track (Track 25) that are Ca‐, Al‐rich…”
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The future of Stardust science
Published in Meteoritics & planetary science (01-09-2017)“…Recent observations indicate that >99% of the small bodies in the solar system reside in its outer reaches—in the Kuiper Belt and Oort Cloud. Kuiper Belt…”
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Constraints on the Formation Age of Cometary Material from the NASA Stardust Mission
Published in Science (American Association for the Advancement of Science) (23-04-2010)“…We measured the ²⁶Al-²⁶Mg isotope systematics of a approximately 5-micrometer refractory particle, Coki, returned from comet 81P/Wild 2 in order to relate the…”
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Possible in situ formation of meteoritic nanodiamonds in the early Solar System
Published in Nature (London) (11-07-2002)“…Grains of dust that pre-date the Sun provide insights into their formation around other stars and into the early evolution of the Solar System. Nanodiamonds…”
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Terminal particle from Stardust track 130: Probable Al-rich chondrule fragment from comet Wild 2
Published in Geochimica et cosmochimica acta (01-11-2014)“…A 4×6μm terminal particle from Stardust track 130, named Bidi, is composed of a refractory assemblage of Fo97 olivine, Al- and Ti-bearing clinopyroxene and…”
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Kosmochloric Ca-rich pyroxenes and FeO-rich olivines (Kool grains) and associated phases in Stardust tracks and chondritic porous interplanetary dust particles: Possible precursors to FeO-rich type II chondrules in ordinary chondrites
Published in Meteoritics & planetary science (01-10-2009)“…— Terminal particles and mineral fragments from comet 81P/Wild 2 were studied in 16 aerogel tracks by transmission and secondary electron microscopy. In eight…”
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Comparison of the composition of the Tempel 1 ejecta to the dust in Comet C/Hale–Bopp 1995 O1 and YSO HD 100546
Published in Icarus (New York, N.Y. 1962) (01-03-2007)“…Spitzer Infrared Spectrograph observations of the Deep Impact experiment in July 2005 have created a new paradigm for understanding the infrared spectroscopy…”
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Carbon investigation of two Stardust particles: A TEM, NanoSIMS, and XANES study
Published in Meteoritics & planetary science (01-02-2008)“…— In this work we present the results of a systematic search for cometary organics in 14 Stardust particles (particles from comet 81P/Wild 2, captured by…”
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Comparison of the composition of the Tempel 1 ejecta to the dust in Comet C/Hale–Bopp 1995 O1 and YSO HD 100546
Published in Icarus (New York, N.Y. 1962) (2007)“…Spitzer Infrared Spectrograph observations of the Deep Impact experiment in July 2005 have created a new paradigm for understanding the infrared spectroscopy…”
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A 70-yr record of oxygen-18 variability in an ice core from the Tanggula Mountains, central Tibetan Plateau
Published in Climate of the past (08-04-2010)“…A 33 m ice core was retrieved from the Tanggula Mts, central Tibetan Plateau at 5743 m a.s.l. in August 2005. Annual average δ18O values were determined for…”
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A nuclear microprobe study of the distribution and concentration of carbon and nitrogen in Murchison and Tagish Lake meteorites, Antarctic micrometeorites, and IDPs: Implications for astrobiology
Published in Meteoritics & planetary science (01-11-2003)“…— Using a nuclear microprobe, we measured the carbon and nitrogen concentrations and distributions in several interplanetary dust particles (IDPs) and…”
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Oxygen isotope measurements of individual unmelted Antarctic micrometeorites
Published in Geochimica et cosmochimica acta (01-08-2006)“…We present oxygen isotope measurements of 28 unmelted Antarctic micrometeorites measuring 150–250 μm (long axis) collected in the South Pole water well. The…”
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THE ORIGIN OF THE 3.4 μm FEATURE IN WILD 2 COMETARY PARTICLES AND IN ULTRACARBONACEOUS INTERPLANETARY DUST PARTICLES
Published in The Astrophysical journal (10-03-2013)Get full text
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