2011A&A...531A.106M


Query : 2011A&A...531A.106M

2011A&A...531A.106M - Astronomy and Astrophysics, volume 531A, 106-106 (2011/7-1)

Photophoretic transport of hot minerals in the solar nebula.

MOUDENS A., MOUSIS O., PETIT J.-M., WURM G., CORDIER D. and CHARNOZ S.

Abstract (from CDS):

Hot temperature minerals have been detected in a large number of comets and were also identified in the samples of Comet Wild 2 that were returned by the Stardust mission. Meanwhile, observations of the distribution of hot minerals in young stellar systems suggest that these materials were produced in the inner part of the primordial nebula and have been transported outward in the formation zone of comets. We investigate the possibility that photophoresis provides a viable mechanism to transport high-temperature materials from the inner solar system to the regions in which the comets were forming. We use a grid of time-dependent disk models of the solar nebula to quantify the distance range at which hot minerals can be transported from the inner part of the disk toward its outer regions as a function of their size (10–5 to 10–1m) and density (500 and 1000 kg/m3). These models will also yield information on the disk properties (radius of the inner gap, initial mass, and lifetime of the disk). The particles considered here are in the form of aggregates that presumably were assembled from hot mineral individual grains ranging down to submicron sizes and formed by condensation within the hottest portion of the solar nebula. Our particle-transport model includes the photophoresis, radiation pressure, and gas drag. Depending on the postulated disk parameters and the density of particles, 10–2 to 10–1m aggregates can reach heliocentric distances up to ∼35AU in the primordial nebula over very short timescales (no more than a few hundred thousand years). 10–3m particles follow the same trajectory as the larger ones but their maximum migration distance does not exceed ∼26AU and is reached at later epochs in the disks. On the other hand, 10–5 to 10–4m aggregates are continuously pushed outward during the evolution of the solar nebula. Depending on the adopted disk parameters, these particles can reach the outer edge of the nebula well before its dissipation. Our simulations suggest that irrespective of the employed solar nebula model, photophoresis is a mechanism that can explain the presence of hot temperature minerals in the formation region of comets. Comets probably had the time to trap the dust transported from the inner solar system either in their interior during accretion or in the form of shells surrounding their surface if they ended their growth before the particles reached their formation location.

Abstract Copyright:

Journal keyword(s): protoplanetary disks - comets: general - comets: individual: glutag{Viz.comet 81P|81P/Wild2} - Kuiper belt: general - Oort Cloud

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2022
#notes
1 HD 109573 PM* 12 36 01.0317461592 -39 52 10.220465388   5.786 5.774 7.25 5.81 A0V 598 1

Query : 2011A&A...531A.106M

Basic data :
HD 109573 -- High Proper Motion Star
Origin of the objects types :

(Ref) Object type as listed in the reference "Ref"
(acronym) Object type linked to the acronym according to the original reference
() Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases

Other object types:
* (HD,CD,...), IR (AKARI,IRAS,...), ** (1994CoORB,**,...), X (1AXG,2E,...), UV (FAUST,TD1,...), TT* (2014ApJ), PM* (2000A&A)
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
ICRS coord. (ep=J2000) :
12 36 01.0317461592 -39 52 10.220465388 (Optical) [ 0.0375 0.0316 90 ] A 2020yCat.1350....0G
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
FK4 coord. (ep=B1950 eq=1950) :
12 33 19.1477952701 -39 35 38.022149524 [ 0.0375 0.0316 90 ]
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
  • ra dec : right ascension and declination (unit and frame defined according to your Output Options)
    Grey values are increasing the original precision due to the computation of frame transformations
  • (wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
  • [error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
    position angle (in degrees North celestial pole to East)
  • quality : flag of quality
    • E ≥ 10"
    • D : 1-10" (and some old data)
    • C : 0.1-1"
    • B : 0.01-0.1" + 2MASS, Tyc
    • A : VLBI, Hipparcos
  • bibcode : bibcode of the coordinates reference
Gal coord. (ep=J2000) :
299.7204940836526 +22.9060661820169 [ 0.0375 0.0316 90 ]
Syntax of proper motions is : "pm-ra pm-dec [error ellipse] quality bibcode"
  • pm-ra : mu-ra*cos(dec) (expressed in the ICRS system in mas/yr)
  • pm-dec : mu-dec (expressed in the ICRS system in mas/yr)
  • [error ellipse] : error major axis and minor axis (in mas), orientation angle (in deg)
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the proper motion reference
Proper motions mas/yr :
-55.653 -23.880 [0.042 0.036 90] A 2020yCat.1350....0G
Syntax of radial velocity (or/and redshift) is : "value [error] (wavelength) quality bibcode"
  • value : radial velocity or/and redshift (Heliocentric frame) according to your Output Options
    (redshift may be not displayed if the data value is <0 and the database inside value is a radial velocity)
  • [error] : error of the corresponding value displayed before
  • (wavelength) : wavelength range of the measurement : Rad, mm, IR, Opt, UV, Xray, Gam or  '∼'(unknown)
  • quality : flag of quality ( A=best quality -> E=worst quality, {� } =unknown quality)
  • bibcode : bibcode of the value's origin
Radial velocity / Redshift / cz :
V(km/s) 7.10 [1.1] / z(~) 0.000024 [0.000004] / cz 7.10 [1.10]
   B 2006AstL...32..759G
Syntax of parallax is : 'value quality [error] bibcode'
  • value : parallax value
  • quality : flag of quality (A=best quality -> E=worst quality, {� } =unknown quality)
  • [error] : mean error
  • bibcode : bibcode of the parallax reference
Parallaxes (mas):
14.13 [0.0471] A 2020yCat.1350....0G
Spectral type is made of 3 parts: %coding is composed of 4 parts :
  • the spectral type, which is made of a temperature class, eventually a luminosity class (roman number) and/or spectral peculiarities;
  • a quality letter: A=best quality→E=worst quality, {� } =unknown quality %
  • a quality letter: A=best quality -> E=worst quality, {� } =unknown quality
  • bibcode : bibcode of the spectral type reference
Spectral type:
A0V C 1982MSS...C03....0H
Syntax of fluxes (or magnitudes) is : "filter-name (System) flux-value [error] quality MultVarFlags bibcode"
  • filter-name : U, B, V, R, I, G, J, H, K, u, g, r, i, z
  • (System) : may be AB (default is Vega)
  • flux-value : value of flux or magnitude
  • [error] : error value
  • quality : flag of quality of the flux value ( A=best quality -> E=worst quality, {� } =unknown quality)
  • MultVarFlags : Mult is zero or one char (J) for joined photometry ; Var can be zero or two chars (V[0-4])
  • bibcode : bibcode of the flux reference
Fluxes (8) :
B 5.786 [0.014] D 2000A&A...355L..27H
V 5.774 [0.009] D 2000A&A...355L..27H
R 7.25 [0.32] E 2012yCat.1322....0Z
G 5.783168 [0.002792] C 2020yCat.1350....0G
I 5.81 [~] D 2006A&A...459..511B
J 5.784 [0.019] C 2003yCat.2246....0C
H 5.794 [0.036] C 2003yCat.2246....0C
K 5.769 [0.023] C 2003yCat.2246....0C
SIMBAD within arcmin
', {sourceSize:12, color:'#30a090'})); aladin.on('objectClicked', function(object) { var objName=object.data.MAIN_ID; aladin.showPopup(object.ra,object.dec,'',''+ objName+''); });" title="Show Simbad objects"> Overlay Simbad points in this preview
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within arcsec The VizieR photometry tool allows for easy visualization of photometry points extracted around the Simbad position from photometry-enabled catalogues in VizieR.
The search radius has to be specified by the user. It is currently limited to a maximum of 30 arcsec. It depends mostly on the precision or quality of the coordinates (SIMBAD and VizieR catalogs), the resolution of the images from which the sources were extracted, source extent, and source crowding.
Suggestions are: crowded field: 0.5 to 1.5 arcsec, 3 arcsec otherwise; uncertain coordinates (SIMBAD quality E or coordinates without reference): 5 to 30 arsec (risky!).
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Some important notes on this object about identifications and objects associations.
notes:


Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 2 : 1301 Display criteria :

The link on the acronym of the identifiers give access to the information for this acronym in the dictionary of nomenclature.
Identifiers (46) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HD 109573 EXO 1233.3-3935 2MASS J12360103-3952102 UCAC4 251-056003
** HJ 4533A FAUST 3271 PPM 290347 uvby98 100109573
** FIN 1A GC 17164 PSCz Q12333-3935 WDS J12360-3952A
AKARI-IRC-V1 J1236009-395211 GEN# +1.00109573 1RXS J123559.7-395205 WISEA J123600.96-395210.9
1AXG J123602-3951 GSC 07762-01973 SAO 203621 WISE J123600.95-395210.8
CCDM J12360-3952A HD 109573A SKY# 23547 [BBW2000] FC 41
CD-39 7717 HIC 61498 TD1 16381 [DML87] 300
CPC 18 5960 HIP 61498 TWA 11 [TGN97] J123606.0-395208.3
CPD-39 5622 HR 4796 TWA 11A Gaia DR2 6147117727029871360
CSI-39 7717 21 HR 4796A TYC 7762-1973-1 Gaia DR3 6147117727029871360
2E 2788 IDS 12307-3919 A UBV 11311
2E 1233.3-3935 IRAS 12333-3935 UBV M 18391

References (598 between 1850 and 2022) (Total 598)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements


velocities : 2    diameter : 1    distance : 3    ROT : 3    Fe_H : 2    PLX : 4    PM : 5    MK : 3   

   

Observing logs


herschel : 8    IUE : 7   

   


External archives :

Archive data at HEASARC - High-Energy Astrophysics Science Archive Research Center

Data at NED - NASA/IPAC Extragalactic Database : HD 109573

Link by name to the catalogue in VizieR :

HD 109573 AKARI-IRC-V1 J1236009-395211 CCDM J12360-3952A CD-39 7717 CPD-39 5622
2E 2788 FAUST 3271 GSC 07762-01973 HD 109573A HIC 61498
HIP 61498 HR 4796 HR 4796A IRAS 12333-3935 2MASS J12360103-3952102
PPM 290347 1RXS J123559.7-395205 SAO 203621 TD1 16381 TYC 7762-1973-1
UCAC4 251-056003 uvby98 100109573 WDS J12360-3952A WISEA J123600.96-395210.9 WISE J123600.95-395210.8
[BBW2000] FC 41 [DML87] 300 Gaia DR2 6147117727029871360

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2022.10.02-01:07:18

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