2011A&A...533A..98D


Query : 2011A&A...533A..98D

2011A&A...533A..98D - Astronomy and Astrophysics, volume 533A98-98 (2011/9-1)

Organic materials in planetary and protoplanetary systems: nature or nurture?.

DALLE ORE C.M., FULCHIGNONI M., CRUIKSHANK D.P., BARUCCI M.A., BRUNETTO R., CAMPINS H., DE BERGH C., DEBES J.H., DOTTO E., EMERY J.P., GRUNDY W.M., JONES A.P., MENNELLA V., ORTHOUS-DAUNAY F.R., OWEN T., PASCUCCI I., PENDLETON Y.J., PINILLA-ALONSO N., QUIRICO E. and STRAZZULLA G.

Abstract (from CDS):

The objective of this work is to summarize the discussion of a workshop aimed at investigating the properties, origins, and evolution of the materials that are responsible for the red coloration of the small objects in the outer parts of the solar system. Because of limitations or inconsistencies in the observations and, until recently, the limited availability of laboratory data, there are still many questions on the subject. Our goal is to approach two of the main questions in a systematic way: - Is coloring an original signature of materials that are presolar in origin (``nature'') or stems from post-formational chemical alteration, orweathering (``nurture'')? - What is the chemical signature of the material that causes spectra to be sloped towards the red in the visible? We examine evidence available both from the laboratory and from observations sampling different parts of the solar system and circumstellar regions (disks). We present a compilation of brief summaries gathered during the workshop and describe the evidence towards a primordial vs. evolutionary origin for the material that reddens the small objects in the outer parts of our, as well as in other, planetary systems. We proceed by first summarizing laboratory results followed by observational data collected at various distances from the Sun. While laboratory experiments show clear evidence of irradiation effects, particularly from ion bombardment, the first obstacle often resides in the ability to unequivocally identify the organic material in the observations. The lack of extended spectral data of good quality and resolution is at the base of this problem. Furthermore, that both mechanisms, weathering and presolar, act on the icy materials in a spectroscopically indistinguishable way makes our goal of defining the impact of each mechanism challenging. Through a review of some of the workshop presentations and discussions, encompassing laboratory experiments as well as observational data, we infer that both ``nature'' and ``nurture'' are instrumental in the coloration of small objects in the outer parts

Abstract Copyright: ∼

Journal keyword(s): planets and satellites: composition - comets: general - circumstellar matter - Kuiper belt: general - dust, extinction

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 - 2026
#notes
1 HD 109573 TT* 12 36 01.0317461592 -39 52 10.220465388   5.786 5.774   5.81 A0V 684 1

Query : 2011A&A...533A..98D

Basic data :
HD 109573 -- T Tauri Star
Other object types:
otypes_help
* (2023A&A,HD,...), X (1AXG,2E,...), ** (**,CCDM,...), UV (FAUST,TD1,...), MIR (AKARI,WISEA,...), IR (IRAS,PSCz,...), TT* (2014ApJ), PM* (2000A&A), Pu* (2020MNRAS), NIR (2MASS)
ICRS coord. (ep=J2000) :
12 36 01.0317461592 -39 52 10.220465388 (Optical) [ 0.0375 0.0316 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
12 33 19.1477959401 -39 35 38.022146209 [ 0.0375 0.0316 90 ]
Gal coord. (ep=J2000) :
299.7204940836526 +22.9060661820169 [ 0.0375 0.0316 90 ]
Proper motions mas/yr :
-55.653 -23.880 [0.042 0.036 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) 10.95 [0.59] / z(spectroscopic) 0.000037 [0.000002] / cz 10.95 [0.59]
   (Opt) A 2022yCat.1355....0G
Parallaxes (mas):
14.1300 [0.0471] A 2020yCat.1350....0G
Spectral type:
A0V C 1982MSS...C03....0H
Fluxes (7) :
B 5.786 [0.014] D 2000A&A...355L..27H
V 5.774 [0.009] D 2000A&A...355L..27H
G 5.783168 [0.002792] C 2022yCat.1355....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
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 3 : 3390 Display criteria :

Identifiers (46) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HD 109573 FAUST 3271 PPM 290347 UCAC4 251-056003
** FIN 1A GC 17164 PSCz Q12333-3935 uvby98 100109573
AKARI-IRC-V1 J1236009-395211 GEN# +1.00109573 1RXS J123559.7-395205 WDS J12360-3952A
1AXG J123602-3951 GSC 07762-01973 SAO 203621 WISEA J123600.96-395210.9
CCDM J12360-3952A HD 109573A SKY# 23547 WISE J123600.95-395210.8
CD-39 7717 HIC 61498 TD1 16381 [BBW2000] FC 41
CPC 18 5960 HIP 61498 TIC 144221009 [DML87] 300
CPD-39 5622 HR 4796 TWA 11 [TGN97] J123606.0-395208.3
CSI-39 7717 21 HR 4796A TWA 11A Gaia DR3 6147117727029871360
2E 2788 IDS 12307-3919 A TYC 7762-1973-1 Gaia DR2 6147117727029871360
2E 1233.3-3935 IRAS 12333-3935 UBV 11311
EXO 1233.3-3935 2MASS J12360103-3952102 UBV M 18391

References (684 between 1850 and 2026) (Total 684)
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 Description of Measurements

Velocities : 4    Diameter : 1    Distance : 4    Rot : 6    Fe/H : 3    Plx : 5    PM : 5    SpT : 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 DR3 6147117727029871360 Gaia DR2 6147117727029871360

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