2014A&A...568A..79D


Query : 2014A&A...568A..79D

2014A&A...568A..79D - Astronomy and Astrophysics, volume 568A79-79 (2014/8-1)

Photometric and spectroscopic evidence for a dense ring system around Centaur Chariklo.

DUFFARD R., PINILLA-ALONSO N., ORTIZ J.L., ALVAREZ-CANDAL A., SICARDY B., SANTOS-SANZ P., MORALES N., COLAZO C., FERNANDEZ-VALENZUELA E. and BRAGA-RIBAS F.

Abstract (from CDS):

A stellar occultation observed on 3rd June 2013 revealed the presence of two dense and narrow rings separated by a small gap around the Centaur object (10199) Chariklo. The composition of these rings is not known. We suspect that water ice is present in the rings, as is the case for Saturn and other rings around the giant planets. In this work, we aim to determine if the variability in the absolute magnitude of Chariklo and the temporal variation of the spectral ice feature, even when it disappeared in 2007, can be explained by an icy ring system whose aspect angle changes with time. We explained the variations on the absolute magnitude of Chariklo and its ring by modeling the light reflected by a system as the one described above. Using X-shooter at VLT, we obtained a new reflectance spectra. We compared this new set of data with the ones available in the literature. We showed how the water ice feature is visible in 2013 in accordance with the ring configuration, which had an opening angle of nearly 34° in 2013. Finally, we also used models of light scattering to fit the visible and near-infrared spectra that shows different characteristics to obtain information on the composition of Chariklo and its rings. We showed that absolute photometry of Chariklo from the literature and new photometric data that we obtained in 2013 can be explained by a ring of particles whose opening angle changes as a function of time. We used the two possible pole solutions for the ring system and found that only one of them, α=151.30 ±0.5, δ=41.48±0.2° (λ=137.9±0.5, β=27.7±0.2°), provides the right variation of the aspect angle with time to explain the photometry, whereas the other possible pole solution fails to explain the photometry. From spectral modeling, we derived the composition of the Chariklo surface and that of the rings using the result on the pole solution. Chariklo surface is composed with about 60% of amorphous carbon, 30% of silicates and 10% of organics; no water ice was found on the surface. The ring, on the other hand, contains 20% of water ice, 40-70% of silicates, and 10-30% of tholins and small quantities of amorphous carbon.

Abstract Copyright: ∼

Journal keyword(s): Kuiper belt objects: individual: glutag{Viz.MP 10199|Chariklo} - planets and satellites: rings

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 144585 PM* 16 07 03.3696573456 -14 04 16.671141984 7.22 6.98 6.32     G2V 211 0

Query : 2014A&A...568A..79D

Basic data :
HD 144585 -- High Proper Motion Star
Other object types:
otypes_help
* (2015A&A,BD,...), PM* (2016ApJ,LTT,...), ** (**,WDS), UV (TD1), NIR (2MASS), MIR (WISEA), IR (IRAS)
ICRS coord. (ep=J2000) :
16 07 03.3696573456 -14 04 16.671141984 (Optical) [ 0.0251 0.0225 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
16 04 15.8575239164 -13 56 17.603050276 [ 0.0251 0.0225 90 ]
Gal coord. (ep=J2000) :
358.1819811414951 +27.1670361177885 [ 0.0251 0.0225 90 ]
Proper motions mas/yr :
-261.591 9.683 [0.035 0.030 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -14.055 [0.0003] / z(spectroscopic) -0.000047 [0.000000] / cz -14.05 [0.00]
   (Opt) A 2018A&A...616A...7S
Parallaxes (mas):
36.2249 [0.027] A 2020yCat.1350....0G
Spectral type:
G2V C 1989ApJS...71..245K
Fluxes (7) :
U 7.22 [~] C 2002yCat.2237....0D
B 6.98 [~] C 2002yCat.2237....0D
V 6.32 [~] C 2002yCat.2237....0D
G 6.160456 [0.002769] C 2020yCat.1350....0G
J 5.181 [0.043] C 2003yCat.2246....0C
H 4.970 [0.034] C 2003yCat.2246....0C
K 4.800 [0.024] C 2003yCat.2246....0C
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Identifiers (31) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

LTT 6427 HIP 78955 SKY# 29087 WDS J16071-1404A
** NSN 153A HR 5996 SPOCS 684 WEB 13345
BD-13 4342 IRAS 16042-1356 TD1 18873 WISEA J160703.19-140416.5
GC 21653 2MASS J16070340-1404166 TIC 410994457 YZC 11 5583
GCRV 65950 NLTT 41992 TYC 5624-1433-1 Gaia DR3 4341501106288171008
GEN# +1.00144585 PPM 231226 UBV 13643 Gaia DR1 4341501101988663680
HD 144585 RAVE J160703.4-140417 UBV M 21163 Gaia DR2 4341501106288171008
HIC 78955 SAO 159706 uvby98 100144585

References (211 between 1850 and 2026) (Total 211)
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 : 13    Distance : 4    Rot : 9    Fe/H : 50    Plx : 6    PM : 6    SpT : 5   

   


External archives :

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

Data at NED - NASA/IPAC Extragalactic Database : HD 144585

Link by name to the catalogue in VizieR :

BD-13 4342 HD 144585 HIC 78955 HIP 78955 HR 5996
IRAS 16042-1356 2MASS J16070340-1404166 NLTT 41992 PPM 231226 RAVE J160703.4-140417
SAO 159706 TD1 18873 TYC 5624-1433-1 uvby98 100144585 WDS J16071-1404A
WISEA J160703.19-140416.5 YZC 11 5583 Gaia DR3 4341501106288171008 Gaia DR1 4341501101988663680 Gaia DR2 4341501106288171008

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