Intense aqueous alteration on C-type asteroids: Perspectives from giant fine-grained micrometeorites [PDF]
Abstract This study explores the petrology of five giant (>400 μm) hydrated fine-grained micrometeorites from the Transantarctic Mountain (TAM) micrometeorite collection. For the first time, the extent and mechanisms of aqueous alteration in unmelted cosmic dust are evaluated and quantified.
M.D. Suttle +5 more
openaire +2 more sources
Grain Size Effects on UV–MIR (0.2–14 μm) Spectra of Carbonaceous Chondrite Groups
Carbonaceous chondrites are among the most important meteorite types and have played a vital role in deciphering the origin and evolution of our solar system.
David C. Cantillo +9 more
doaj +1 more source
Detection of the Yarkovsky effect for C-type asteroids in the Veritas family [PDF]
20 pages, 19 figures, 1 table.
Carruba, V. +2 more
openaire +4 more sources
JBILET WINSELWAN; A STEP TOWARD UNDERSTANDING THE COMPOSITION OF C-TYPE ASTEROIDS [PDF]
AbstractJbilet Winselwan is one of the largest CM carbonaceous chondrites available for study. Its light, major, and trace elemental compositions are within the range of other CM chondrites. Chondrules are surrounded by dusty rims and set within a matrix of phyllosilicates, oxides, and sulfides.
Michael J. Cato, Amy L. Fagan
openaire +4 more sources
Taxonomic Classification of Asteroids Using the KMTNet Multiband Photometry Data Set
We report the multiband photometry of asteroids observed over 14 nights from 2015 December to 2017 December using the Korea Microlensing Telescope Network telescopes with the taxonomic classification of those objects. The data set contains the photometry
Sangho Choi +5 more
doaj +1 more source
Optimization of Future Multifilter Surveys Toward Asteroid Characterization
The aim of this paper is to find a set of photometric passbands that will give optimal results for spectrophotometric classification of asteroids into taxonomic types and classes.
Hanna Klimczak +6 more
doaj +1 more source
Characteristics and large bulk density of the C-type main-belt triple asteroid (93) Minerva [PDF]
From a set of adaptive optics (AO) observations collected with the W.M. Keck telescope between August and September 2009, we derived the orbital parameters of the most recently discovered satellites of the large C-type asteroid (93) Minerva. The satellites of Minerva, which are approximately 3 and 4 km in diameter, orbit very close to the primary $\sim$
Marchis, F. +13 more
openaire +5 more sources
Environmental Impact of Silicic Magmatism in Large Igneous Province Events
Exploring the links between Large Igneous Provinces and dramatic environmental impact
An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
Scott E. Bryan
wiley +1 more source
Carbon Speciation and Solubility in Silicate Melts
This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.
Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions
Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
Natalia Solomatova +2 more
wiley +2 more sources
Low thermal conductivity boulder with high porosity identified on C-type asteroid (162173) Ryugu [PDF]
C-type asteroids are among the most pristine objects in the Solar System, but little is known about their interior structure and surface properties. Telescopic thermal infrared observations have so far been interpreted in terms of a regolith-covered surface with low thermal conductivity and particle sizes in the centimetre range.
Grott, Matthias +36 more
openaire +3 more sources

