Results 21 to 30 of about 4,877 (221)

The composition of the protosolar disk and the formation conditions for comets [PDF]

open access: yes, 2015
Conditions in the protosolar nebula have left their mark in the composition of cometary volatiles, thought to be some of the most pristine material in the solar system.
A. Dutrey   +227 more
core   +3 more sources

Carbon Speciation and Solubility in Silicate Melts

open access: yesGeophysical Monograph Series, Page 179-194., 2020

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  

+1 more source

The Volatile Composition of Comets [PDF]

open access: yesHighlights of Astronomy, 1989
ABSTRACTComets may be our best probes of the physical and chemical conditions in the outer regions of the solar nebula during that crucial period when the planets formed. The volatile composition of cometary nuclei, in particular, can be used to decide whether comets are the product of a condensation sequence similar to that invoked to explain the ...
openaire   +2 more sources

The Gateway from Centaurs to Jupiter-family Comets: Thermal and Dynamical Evolution

open access: yesThe Astrophysical Journal, 2023
It was recently proposed that there exists a “gateway” in the orbital parameter space through which Centaurs transition to Jupiter-family comets (JFCs).
Aurélie Guilbert-Lepoutre   +3 more
doaj   +1 more source

Temporal and Spatial Aspects of Gas Release During the 2010 Apparition of Comet 103P/Hartley-2 [PDF]

open access: yes, 2011
We report measurements of eight primary volatiles (H2O, HCN, CH4, C2H6, CH3OH, C2H2, H2CO, and NH3) and two product species (OH and NH2) in comet 103P/Hartley-2 using high dispersion infrared spectroscopy.
Blake, G. A.   +12 more
core   +4 more sources

Tracing the Ingredients for a Habitable Earth from Interstellar Space through Planet Formation [PDF]

open access: yes, 2015
We use the C/N ratio as a monitor of the delivery of key ingredients of life to nascent terrestrial worlds. Total elemental C and N contents, and their ratio, are examined for the interstellar medium, comets, chondritic meteorites and terrestrial planets;
Bergin, Edwin A.   +4 more
core   +2 more sources

Comet C/2004 Q2 (MACHHOLZ): Parent Volatiles, a Search for Deuterated Methane, and Constraint on the CH4 Spin Temperature [PDF]

open access: yes, 2009
High-dispersion (l/dl ~ 25,000) infrared spectra of Comet C/2004 Q2 (Machholz) were acquired on Nov. 28-29, 2004, and Jan. 19, 2005 (UT dates) with NIRSPEC at the Keck-2 telescope on Mauna Kea.
Aikawa   +43 more
core   +2 more sources

On the origin of O2 and other volatile species in comets [PDF]

open access: yesProceedings of the International Astronomical Union, 2017
AbstractMolecular oxygen, O2, was recently detected in comet 67P by the ROSINA instrument on board the Rosetta spacecraft with a surprisingly high abundance of 4% relative to H2O, making O2 the fourth most abundant in comet 67P. Other volatile species with similar volatility, such as molecular nitrogen N2, were also detected by Rosetta, but with much ...
Taquet, V.D.F.   +3 more
openaire   +4 more sources

Ice, Ice, Maybe? Investigating 46P/Wirtanen’s Inner Coma for Icy Grains

open access: yesThe Planetary Science Journal, 2023
The release of volatiles from comets is usually from direct sublimation of ices on the nucleus, but for very or hyperactive comets other sources have to be considered to account for the total production rates.
Theodore Kareta   +3 more
doaj   +1 more source

A survey of volatile species in Oort cloud comets C/2001 Q4 (NEAT) and C/2002 T7 (LINEAR) at millimeter wavelengths [PDF]

open access: yes, 2013
The line emission in the coma was measured in the comets C/2001 Q4 (NEAT) and C/2002 T7 (LINEAR), that were observed on five consecutive nights, 7-11 May 2004, at heliocentric distances of 1.0 and 0.7 AU, respectively, by means of high-resolution ...
Biver, N.   +8 more
core   +2 more sources

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