Dust in Planetary Systems 2005 Proceedings

Instructions for the Proceedings Book

Project sponsored by ESA, MPG, and extra tools by PBWiki.

Overview
Chapters in the Proceedings

Will be published by ESA (publication date: mid-2006).

Harald Krüger and Amara Graps are the editors.

Deadline for manuscript submission: 31 January 2006.

Email contact: .

Papers will be reviewed. Please give one or a few suggestions of reviewers.
(This will help the editors move the reviewing process faster.)

Instructions for preparation of camera-ready manuscripts.
Please use: LaTeX style or MS Word templates.
Word Template,
LaTeX
The proceedings need Type 1, Times Roman, fonts only. To add this to LaTeX, insert the following command in the LaTeX macro:
\usepackage{times}
All of the necessary files (ASCII formatted for Macintosh) are in the zipped directory: dips2005tex.zip
or, individually:

readme.txt
esapub2005.cls (a LaTeX2e class file).
author_instructions.tex (a manual and also example file).
esa_ref.bst (a BibTeX style file for numbered references).
aa.bst (a BibTeX style file for author/date formatted references created by Astronomy and Astrophysics).
Here is the same directory, but ascii-formatted for: DOS, and for: Unix users.
You may also need the natbib style file, though it is part of most LaTeX installations these days. It may be also obtained from: http://www.ctan.org/tex-archive/macros/latex/contrib/natbib/. Also from other CTAN servers in Germany (ftp://ftp.dante.de) and UK (ftp://ftp.tex.ac.uk.)
Paper length in ESA-single-spaced-double-column format:

10 pages for invited papers
4 pages for contributed papers (oral or poster)

Please give ~10-20 index words for the index of the DIPS 2005 Proceedings Book when you submit your paper. Typical examples from the Interplanetary Dust Book (2001) and the Interstellar Dust (1989) books follow. If you do not find your index word(s) here, send it to us anyway!

(Elements) Al, Ca, C, Na, H, Ti, N, O, Cl, P, Mg, Mn, Fe, Si, S, Zn $\beta $ meteoroid $\beta $ Pic disk $\beta $ Pictoris objects 10 micron!absorption feature 10 micron band 10 micron 10 micron!silicate bump 10 micron!silicate feature 100 micron polarization 11.3 micron band 11.3/3.3 ratios 12 micron band 12 micron IRAS band 12C/13C ratio 18 micron!emission bands (silicate) 18 micron!silicate feature 2.97 micron!absorption feature 2175 A absorption band 2175 A bump 2175 feature 220 nm hump 2200 A bump 2200 A feature 25 micron IRAS band ablation absorption accelerator!electrostatic dust accelerator!plasma drag accelerator!Van de Graaff accretion accretion rate of IDP achondrite activity profile Aerobee aerocapture aerofragmentation aerogel AGB stars agglomeration aggregation AGN AIBs airglow albedo albedo!single scattering aldehydes aligned grains aligned particles alignment alignment mechanism alignment of dust grains alignment of spinning grains aliphatic CH stretch transitions alkanes alpha Sco aluminum oxide amino acids ammonia ammonia ice amorphization amorphous amorphous carbon amorphous carbon!aggregates amorphous carbon!particles amorphous grains amorphous material amorphous SiC amorphous silicate analogue material angle of incidence angular sensitivity anharmonic oscillators anhydrous mineral anomalous extinction anomalous tail anthracene antitail aphelion Apollo!17 Apollo!program aqueous alteration area time product Ariel 2 aromatic interstellar band aromatic moieties aromatic rings asteroid asteroid belt asteroidal band asteroidal dust particle asteroidal meteoroid asteroidal population astronomical silicate astronomical unit (AU) asymmetry factor $g$ asymmetry parameter atmospheric drag atmospheric entry Atmospheric Explorer C atomic absorption lines atomic clouds Babinet's principle bacillus subtilis backscattering ballistic limit ballistic limit!equation band strengths band!aromatic interstellar band!asteroidal dust band!diagnostic IR band!diffuse interstellar band!silicate band!solar system dust band!spectral 217.5 nm band!spectral 30 $\mu $m band!UIR band!unidentified infrared bandgap bare carbon grains beer can experiment bena(a)anthracene benzene Benzenoid isomers benzenoid PAH benzo(c)phenanthrene benzvalene Bergman's theorem BN-structure Boltzmann statistics Bremsat bulk density bumper shield C-C modes C-H bend modes C-H bonds C-solar abundance C-star C/O abundance ratio C10 H8 C14 H10 C18 H12 C20 H12 C2H2 C2H2+ C2H3 C3H2 C3H3+ C4H2 C6 H6 C6O canonical approximation CaO capacitor!detector capacitor!discharge carbides carbon carbon coatings carbon depletion carbon grains carbon grains (dust) carbon recycling carbon stars carbon!dust carbon!onion carbon-bearing compounds carbonaceous carbonaceous chondrite carbonaceous dust carbonaceous material carbonaceous particles carbonates carbonyl sulfide cascade Cassini mission Cassini mission Cassini, Giovanni Domenico catacondensed PAH catalyzing catastrophic collisions lifetime catastrophic disruption CCD arrays CDA CDCF ceramic microphone CH out-of-plane bending vibration CH3OH CH4 Chapman airglow mechanism charged particle absorption charged particle absorption!signature chemical evolution (of grains) chemical pathways chemical reaction rate Childrey CHON particle chondrite chondrite!group chondrite!porous chondrite!smooth chondrules chrysene CIDA CII circular polarization circumsolar dust circumstellar circumstellar chemistry Circumstellar condensates circumstellar disk circumstellar extinction circumstellar shells circumstellar system cirrus cirrus (IR) cirrus cloud classical dust model classical interstellar grain classical nucleation theory climate cycle cluster growth cluster number cluster size cluster!-cluster aggregation cluster!analysis cluster!model clusters clusters (of particles) CN CO (1-0) CO (1-0) CO J=1-0 CO-ice CO2 CO2 coagulate coagulation coal pitch coatings COBE COBE!observations CODAG coherent scattering cold cores cold dust collected dust collection experiment collision collision!cascade collision!grain collision!lifetime collision!molecule-molecule collision!particle-molecule collisional heating color excess color temperature colors coma coma!morphology comet Comet Bradfield comet dust comet dust mass distribution comet dust temperatures comet grains comet Hale-Bopp comet Halley comet Hyakatake Comet IRAS-Araki-Alcock Comet Kohoutek comet Tempel 1 comet Wild Comet Wilson comet!coma dust comet!dust comet!dust density comet!dust trail comet!Jupiter family comet!nucleus comet!star-grazing comet!sungrazing cometary (dust) cometary dust cometary dust!composition cometary dust!particle cometary dust!trail cometary meteoroid comets complete synchrone composite grains composition composition of dust condensates condensation condensation temperature conjugate gradient method constituent units in an aggregate contamination process continuum extinction (dust extinction) Contour convex hyperbola Copernicus core mantle grains core population core-mantle core-mantle grains core-mantle model core/mantle-grain cores corona corona!F corona!F, thermal emission corona!K corona!polarization coronal brightness coronal streamer coronene coronene UV properties COSIMA cosmic dust Cosmic Dust Collection Facility, CDCF cosmic ray cosmic ray heating cosmochemistry coulomb dissociation (explosion) coupled dipole approximation CRAF crater crater!age crater!depth equation cross-conjugated ketone crystalline crystalline minerals crystalline silicate cumulative distribution cumulative flux cumulative meteoroid flux cyanopolyynes cyclopropenylidene D/H ratio D2B dark cloud dark nebula Darwin Davis-Greenstein alignment Davis-Greenstein mechanism DDA DDS deceleration dehydrogenated dense cloud densities of states density of states density!bulk density!comet dust density!dust density!material {30 density!phase space density!plasma density!space density!spatial depletion depletion correlations depletions depolarization desorption desorption!ionization model desorption!rate destruction destruction (of grains) destruction of PAHs detection threshold detector!capacitor detector!dust detector!impact ionization detector!in-situ detector!microphone detector!MOS detector!multi-coincidence detector!penetration detector!pressurized-cell deuteration Deuterium deuterium enrichments Deuterium Fractionation dewar benzene diagnostic IR band diamond diamond-like structure DIB dications dichroic absorption DIDSY dielectric constant dielectric function differential ablation differential flux differential mass distribution Diffuse Band Carrier Diffuse band profiles diffuse cloud dust diffuse clouds diffuse galactic light diffuse interstellar band Diffuse Interstellar Bands (DIBs) diffuse interstellar cloud diffuse interstellar medium diffuse interstellar radiation field diffuse ISM diffuse medium dust DIRBE directional flux dirty snowball model discrete dipole approximation discrete dipole approximation, DDA discrete source disorder disordered solids dissociation dissociative shocks distribution of grain sizes distribution!cumulative distribution!differential mass distribution!flux distribution!lunar crater distribution!magnitude index distribution!mass index distribution!mass index distribution!MRN distribution!of orbits distribution!orbit distribution!out-of-ecliptic distribution!parameter distribution!radius function distribution!size distribution!size of fragments distribution!spatial distribution!textbook distribution!velocity diurnal variation Divine's interplanetary dust model Dohnanyi power law Doppler shift doppler splitting doubly adjacent H atoms Drag DUCMA Duilliers, Niccolo Fatio de dust composition dust destruction dust emissivity dust energetics (energy budget) dust formation dust fraction dust grains dust injection dust model dust model!Bird's-Nest dust model!Fluffy dust population dust temperature dust temperatures dust!-ball model dust!accelerator dust!accelerator dust!analog dust!asteroidal particle dust!belt dust!carbon dust!carbonaceous dust!charge dust!circumsolar dust!collected dust!collection dust!color dust!cometary dust!composition dust!density dust!detector dust!diameter dust!disk dust!dynamics dust!fragmentation dust!halo dust!in comet coma dust!in magnetosphere dust!in the interstellar medium dust!interplanetary dust!interstellar dust!interstellar population dust!lifecycle dust!lifetimes dust!multi-component dust!population dust!presolar grain dust!refractory dust!silhouette dust!stream dust!tail dust!trail dust!volatile dust-to-gas mass ratio dust-to-gas ratio dusty plasma E ring E ring E(B-V) E. coli bacteria Earth!gravitational focusing Earth!resonant ring Earth!shielding eccentric population eccentricity Echantillons ecliptic Edgeworth-Kuiper belt effective refractive index efficiency Einstein coefficient ejecta ejection velocity elastic scattering electromagnetic effect electronic sputtering electrostatic accelerator electrostatic distortion electrostatic dust accelerator electrostatic force electrostatic fragmentation electrostatic stress element abundances element depletions element!forced element!orbital element!osculating element!proper elemental abundances ELF/VLF meteor signal ellipsoid elongated grains elongation emissivity energy balance energy level diagram equation!ballistic limit equation!crater depth equation!hole growth equation!impact equation!Maxwell's equation!of motion equation!volume integral ERE ERE excitation source ERIS ESABASE EuReCa Timeband Capture Cell Experiment, TICCE evaporation evolution!orbit evolved stars Explorer!-16 exposure age Express-2 extended red emission extended red emission (ERE) extinction extinction bump extinction cross-sections extinction curve extinction curves (measured, laboratory) extinction law extinction!curve extinction!parameter $R$ extinction, infrared extragalactic dust extragalactic extinction Extragalactic HII Regions extreme carbon stars F-corona F-corona!thermal emission fan far infrared far infrared dust properties Far infrared emission efficiency far infrared emissivity far ultraviolet rise far-infrared dust absorption efficiency far-infrared thermal emission Far-ultraviolet extinction far-UV extinction Fe ablation trails Fe-solar abundance Fe2SiO4 feature!21 $\mu $m feature!3.4 micron feature!silicate FEB mechanism field emission field-of-view fine structure emission Finson-Probstein model fluctuating emission Fluorescence Fluorescent emission flux flux!cumulative flux!curve flux!differential flux!directional flux!distributions flux!Gr\"un flux!hazard flux!impact flux!interplanetary model flux!isotropic flux!measurement flux!particle force forced element formic acid forward-scattering Fourier analysis fractal fractal clusters fractal dimension fractal dimension fractal dust fractal grains fractionation fragment velocity fragmentation fragmentation (of PAHs) fragmentation!dust fragmentation!electrostatic fragmentation!secondary fullerene function!phase function!probability function!radius distribution function!scattering function!spectral function!volume scattering fundamental vibration FUV G Ring galactic center galactic halo Galactic sources galactic stellar population galaxies Galaxy Galileo mission gas density gas drag Gas heating Gas heating by IR emission gas phase chemistry gas temperatures gas velocity Gas-grain collisions gas-to-dust ratio gas-to-solid condensation Gegenschein GEMS generalized multiparticle Mie-solution generation of grains geometric optics Giacobinni-Zinner Giotto glassy carbon GORID GORIZONT gossamer ring gradient grain alignment grain charge grain chemical composition grain chemistry grain coaggulation grain collisions grain composition grain destruction grain elongation grain erosion grain evolution grain formation grain growth grain mantle grain mantles grain morphology Grain photoelectric heating grain populations grain processing grain production grain shapes grain size grain size distribution grain sizes grain sources grain surface chemistry grain theories grain velocities grain work function grain!alignment grain!classical interstellar grain!collision grain!core/mantle grain!generation grain!mass spectrum grain!oxide grain!presolar diamond grain!presolar dust grain!presolar graphite grain!presolar SiC grain!temperature grain-grain collision grains graphite graphite fractal grains graphite grains graphite temperature graphitic (grain) graphitic carbon graphitic structure graphitized gravitational enhancement gravitational focusing gravitational force gravitational perturbation gravitational scattering gravity ground-based photometry growth (of grains) Gr\"un flux H II H-solar abundance H2 formation H2 formation heating H2(C2)_n H20 H2CO H2S HAC HAC's Halley Halley's comet halo population harmonic oscillators HCN HC_{2N+1}N heat capacity heating efficiency heating intensity HEL Helios mission heliosphere hematite Henyey-Greenstein phase function HEOS Herbig Ae/Be stars heteromolecular homogeneous nucleation hexabenzocoronene HI clouds HI regions high altitude sounding rocket high-latitude emission high-UV radiation HII regions Hirayama family Hiten hole growth equation homomolecular homogeneous nucleation hot core hot plasma HST Hubble Space Telescope, HST Hugoniot elastic limit Huygens probe Huygens probe, Christian hydrated materials hydrated phase hydrated silicate hydrocarbon hydrocarbon grains hydrocarbon molecules Hydrocodes hydrogen hydrogenated hydrogenated amorphous carbon hydrogenated amorphous carbon (HAC) hydrogenated amorphous carbon particles hypervelocity impact ice ice absorption feature ice mantles ices icy mantles icy-conglomerate model IDE IDP IDP!accretion rate IDP!classification IDP!isotopic measurements IDP!layer silicate IDP!layer silicate IDP!olivine IDP!pyroxene IDPs image image!simulation imaging telescope impact!direction impact!equation impact!flux impact!hazard impact!ionization impact!ionization detector impact!restructuring impact!velocity in-situ detector inclination inclination dependence inclined population infrared absorption feature infrared cirrus Infrared continuum Infrared Continuum Emission infrared echo infrared emission Infrared emission bands Infrared Emission Features infrared energy distribution infrared fluorescence infrared spectra infrared spectral features Infrared spectroscopy infrared!astronomical satellite, IRAS infrared!cirrus infrared!measurement infrared!space observatory, ISO infrared!zodiacal light instrumentation intact capture interaction!electromagnetic interaction!gas-dust intercloud medium intermediate-mass YSO internal conversion interplanetary dust interplanetary dust particles interplanetary!dust interplanetary!dust particles interplanetary!electrons interplanetary!flux model interplanetary!magnetic field interstellar albedo interstellar bump interstellar cloud interstellar cloud chemistry interstellar clouds interstellar dust interstellar extinction interstellar grain mantles interstellar infrared emission features interstellar magnetic field interstellar material interstellar medium interstellar molecules Interstellar polarization interstellar radiation field interstellar shocks interstellar!depletion interstellar!dust interstellar!dust particles interstellar!dust population interstellar!extinction interstellar!polarization inversion technique ion!mass spectrometer ion!time-of-flight ion-molecule reaction ionic PAHs ionization ionization potential ionized PAHs IR bandshape IR cirrus IR continuum luminosity IR emission lines IR extinction IR fluorescence IR reflection bebula IR spectrometers IR Spectroscopy IR-cirrus IRAS IRAS bands IRAS Bands: 12, 25, 60, 100 microns IRAS catalog IRAS color-color diagrams IRAS colors IRAS data IRAS emission IRAS observations IRAS!LRS catalog IRAS!observations iron iron-nickel sulfides IRTS ISM ISM phases ISO Isotope isotopic anomalies isotopic anomaly isotopic composition isotopic fractionation isotropic flux Jacobian jet jet collimation Jupiter!dust streams Jupiter!family comet Jupiter!ring K corona K factor KAO Keplerian dynamics kerogens ketone kinematics of interplanetary dust KOSI experiment Kramers-Kronig integral relation Kuiper Airborne Observatory, KAO Kuiper belt laboratory astrophysics laboratory crater laboratory measurements lambda_max Laplace plane layer silicate IDP layer-lattice silicates LDEF LDEF!east LDEF!observations LEAM lenticular galaxies Leonid!filament Leonid!multi-instrument aircraft campaign libration point lifecycle of dust lifetime!catastrophic collisions lifetime!collisional lifetime!dust lifetime!Poynting-Robertson lifetimes light!curtain light!flash light-gas!gun limb-brightening linear polarization linearly birefringent linearly dichroic LMC LMC extinction curve LMC HI column densities Local Thermodynamic Equilibruim localization Long Duration Exposure Facility, LDEF Lorentz force Lorentz!resonance Lorentzian profile low resolution spectra low-mass YSO low-Ni group low-Zn group LRS luminescence lunar crater distribution lunar ejecta lunar microcrater M stars Mach number magnesium sulfide magnetic dissipation magnetic field magnetite magnetosphere magnitude magnitude!distribution index Mairan mantle composition mantle size mantles (grain mantles) mantles (grain) MAP map of zodiacal light Mariner 2 mass mass loss rate mass!distribution index mass!loss mass!spectrometer mass!spectrum of a single grain mass!threshold mass-losing stars massive YSO MASTER matrix effect Maxwell Garnett mixing rule Maxwell's equations MDC mean motion resonance mean UV extinction curve measurement!flux measurement!infrared measurement!isotopy of IDP melting metal carbide Metal-Oxide-Silicon metallicities metallicity metals meteor meteor meteor!jet meteor!observation meteor!shower meteor!streams meteorite meteorite inclusions meteorite!composition meteorites meteoritic dust meteoroid meteoroid!$\beta $ meteoroid!asteroidal meteoroid!cometary meteoroid!fragment meteoroid!velocity methane methanol method!conjugate gradient method!microwave analogue method!particle in a circle method!scattering order iterative MFE Mg-solar abundance Mg2+ Mg2SiO4 MgO MgS microcanonical ensemble microcanonical system micrograins micrometeorite micrometeoroid microphone microphone!detector microphone!detector microphonics microwave analogue method Mie scattering theory Mie theory Milky Way MM model!Bird's-Nest model!classical model!cluster model!desorption ionization model!Divine's interplanetary model!dust model!dust-ball model!Finson-Probstein model!fluffy model!icy-conglomerate model!interplanetary flux model!NASA orbital debris dnvironment model!plasma ionization model!rarefied flow for meteoroids model!rubble pile model!standard ISM model!volume ionization molecular absorption lines molecular abundance molecular cloud molecular clusters molecular emission molecular interactions molecular orbital molecule molecules momentum momentum!sensor mono carboxylic acids monocarboxylic acids monocations monocrystalline grains Moon impact morphology (dust) MOS detector MRN-distribution multi-coincidence dust detector multi-component dust Munich Dust Counter Murchison M\"uller matrix M\&D-SIG N-solar abundance N2 naphthalene napthacene narrow components NASA Orbital Debris Environment Model near infrared (NIR) near infrared continuum emission Near IR extinction near-surface breeze needles Neptune's rings neutral PAHs NH3 NH4+ NIR extinction nitride noctilucent cloud noise source non-equilibrium emission non-graphitic carbonaceous material non-spherical non-thermal non-thermal emission nonradiative molecular processes nonradiative transitions novae Nozomi nuclear train nucleation nucleation (heterogenous) nucleation (homogenous) nucleosynthesis nucleosynthetic process nucleus!precession nucleus!rotation O O-solar abundance O2 O2- OAO oblate speroids occultation OCN- OCS OGO OH- Olbers' paradox olivine olivine!IDP Oort Cloud optical constant optical constants (bulk) optical depth optical equivalence optical extinction optical properties optical properties!solar distance dependence optical transition orbit orbit!distribution orbit!synchronous orbital elements orbital evolution orbital perturbation organic carbon organic compounds organic grain mantle organic matter organic refractories organic refractory mantles organic residue Orgueil origin of interplanetary dust ortho-para ratio osculating elements OSO out-of-ecliptic distribution of interplanetary dust outburst oxide grain oxides packing PAH PAH chemical reactivity PAH monocation PAH anions PAH autoionization PAH cations PAH clusters PAH configuration interaction PAH crystallites PAH dications PAH doublet states PAH electron affinity PAH electronic oscillator strengths PAH first-excited state PAH formation PAH Gibbs energy PAH ground electronic state PAH ionization PAH isomers PAH molecule PAH photoelectric heating PAH reactivity PAH size PAH spectroscopy PAH stability PAH structural units PAH- absorption spectra PAHs- electronic transitions paramagnetic relaxation parameter distribution particle densities particle in a circle method particle shape particle size particle!-cluster aggregation particle!albedo particle!flux partition function PDR Pegasus mission penetration penetration!detector penetration!limit penetration!rate percolation pathway perforation perihelion persistent train perturbations perylene phase function phase lag cross-sections phase space phase!angle phase!function phase!space density photo desorption photo dissociation region photo emission Photo-Thermo-Dissociation photochemical evolution photodestruction photodissociation photodissociation regions photoelectric effect photoelectric heating photoelectric yield photoionization photolytic processing photometer photometric errors photometry photomultiplier photon absorption photophysics photoprocessing phyllosilicate MM phyrene PIA Pioneer 10 and 11 Pioneer 8 and 9 Planet-B planetary nebulae planetary shielding plasma plasma heating plasma!density plasma!drag plasma!drag accelerator plasma!ionization model plasma!tail Poisson statistics polarimetric polarimetric color polarization polarization!curve polarization!of the F corona polarization!of zodiacal light polarized emission polycrystalline grains Polycyclic Aromatic Hydrocarbon polyvinylidene fluoride population population!asteroidal population!core population!dust population!eccentric population!halo population!inclined population!interstellar dust post-AGB star power law power-law distribution power-law index Poynting Robertson!drag Poynting-Robertson!decay timescale Poynting-Robertson!drag Poynting-Robertson!lifetime preplanetary disk presolar interstellar medium presolar!corundum presolar!diamond and graphite grain presolar!dust grain presolar!SiC grain presolar!silicon nitride pressurized cell pressurized cell!detector primary condensates probability function prograde proper element PROSPERO protoplanetary nebulae protostars protostellar object protostellar sources PUMA PVDF pyrene pyroxene pyroxene!IDP pyroxenes quadrupole quantum statistical quasi-icosahedral quasiequilibrium theory quenched carbonaceous composite R CrB star r-process radar meteor radial profile radiation damage radiation pressure radiation pressure!force radiationless transitions radiative relaxation radius distribution function Raman scattering cross section random noise rarefied flow model for meteoroids Rayleigh limit Rayleigh scattering Rayleigh-Jeans approximation Rayleigh-like polarization reaction time constant reactivity red fluorescence reddening of the zodiacal light reflection nebula reflection nebula (RN) refractive index refractory absorber refractory cores refractory dust refractory grains refractory stardust relative speed repacking residue resonance resonance!Lorentz resonance!mean motion resonance!scattering domain resonance!secular resonant charge variation resonant perturbation resonant trapping retrograde ring-moons Roche zone Rosetta mission rotation axis rubble pile s-Process S2 saturated species Saturn scattered light scattering scattering!angle scattering!cross section scattering!efficiency scattering!function scattering!order iterative method Scoriaceous MM secondary electron emission secondary fragmentation secular perturbation secular precession secular resonance segregation semimajor axis serpentine shape of impact fragments shattering shepherd satellites shielding shock shock destruction shock waves shocks Si$_3$N$_4$ Si-solar abundance SiC silicate silicate band silicate core silicate grains silicate particles silicate temperature silicate!band silicate!feature silicon carbide silicon!disulfide SIMS SIMUL SiO2 SIRTF size distribution size distribution!of fragments sizes Skylab small number statistics small particle extinction small particle scattering sodium lines SOFIA SOHO sungrazing comet solar corona solar gravity solar nebula solar neighborhood solar radiation pressure solar system solar system dust band solar wind solar wind!drag solid CO absorption feature solid methanol solid-state astrophysics sonic boom soot sp2 sp2 carbon sp3 sp3 carbon space!debris space!density space!weathering spall, spallation spatial density spatial density!of interplanetary dust spatial distribution spatial structure specific heat spectra Spectra of PAHs spectral band! 217.5 nm spectral band! 30 $\mu $m spectral feature! 21 $\mu $m spectral feature! 3.4 micron spectral function spectroscopy speed speed!loss speroidal particles sphere sphere of influence spin spin!rate spin!vector spiral spokes spontaneous emission sporadic background sputtering stability standard ISM model star-forming region star-grazing comet stardust Stardust mission stardust!mineralogy statistical physics stellar dust injection stellar outflows sticking probability Stokes parameters Stokes vector streamer striae sub-millimeter emission sublimation rate submillimeter dust properties submillimeter line emission submillimeter spectrum submillimieter continuum observations sulfide sulfur Sun-grazing comet super-paramagnetic (SPM) supergiants supernova supernova (remnants) supernova condensates supernova rate supernova remnants supernova remnants (SNRs) supernova shocks supernovae supernovae (SN) supernovae ejecta superparamagnetic relaxation superparamagnetism supersaturation suprathermal rotation surface brightness surface free energy surface plasmon surface potential surface tension SXRF symmetry plane/surface synchrone synchronous orbit syndyne T-matrix solution TD-1 temperature temperature (grain temperature) temperature fluctuations temperature spiking terminal synchrone terminal velocity textbook distribution thermal thermal annealing Thermal Approximation thermal distribution function thermal emission thermal equilibrium thermal fluctuation thermal spike thermal spiking thermoionic effect thin-foil penetration TICCE timescale timescale TOF-SIMS track trail!dust trail!Fe ablation trailet train tubular structure trajectory transient heating transient recorder transiently heated transition translucent clouds triphenylene trough opacity problem turbulence U-2 UIR bands UIR bands UIR features ultraviolet ultraviolet absorption Ulysses mission unidentified infrared bands unidentified infrared bands, UIB unidentified infrared emission bands unidentified infrared features unimolecular dissociation unimolecular reaction Uranian rings Uranian system UV absorption UV absorption cross section uv absorption lines UV extinction UV extinction curve UV photolysis V-2 Van de Graaff accelerator vapor pressure variations VeGa mission Vega!excess stars Vega!excess stars Vega!phenomenon velocity velocity distribution Venus Flytrap vibrational excitation vibrational spectra vibrational states vibrational temperature visible visible extinction visible fluorescence visual extinction volatile dust volume!integral equation volume!ionization model volume!scattering function VSG's warm intercloud medium water water ice water maser emission water-ice water-ice libration mode wavelength dependence of polarization WC stars work function WR Stars X--CN x-ray XCN Xe, s-process Xe-HL anomaly Yarkovsky effect young stellar object YSO YSO!intermediate-mass YSO!low-mass YSO!massive zenithal hourly rate zodiacal background cloud zodiacal infrared emission zodiacal light zodiacal light!annual variations zodiacal light!brightness zodiacal light!color zodiacal light!infrared zodiacal light!map zodiacal light!mid- to far-infrared observations zodiacal light!near-infrared colors zodiacal light!polarimetry zodiacal light!polarization zodiacal light!polarization zodiacal light!reddening zodiacal light!spectral information zodiacal light!temporal variations
And while we have your attention, please consider visiting and contributing to our Wikipedia Cosmic Dust Pages ! To help support the public interest in Stardust, and Pluto New Horizons, we are especially interested for the comet and Kuiper belt dust experts to improve on the Wikipedia entry for Comet dust. (Ask Amara for any details and/or help.)

Last Modified by Amara Graps on 22 April 2006.