2008A&A...489..777L


Query : 2008A&A...489..777L

2008A&A...489..777L - Astronomy and Astrophysics, volume 489777-785 (2008/10-2)

Spitzer Space Telescope observations of the nucleus of comet 67P/Churyumov-Gerasimenko.

LAMY P.L., TOTH I., GROUSSIN O., JORDA L., KELLEY M.S. and STANSBERRY J.A.

Abstract (from CDS):

Comet 67P/Churyumov-Gerasimenko is the target of the Rosetta mission, and an early characterization of its nucleus is required to assist in preparing the orbital strategy of the spacecraft, the delivery of the Philae surface module and the science operations. We detected the nucleus using the Hubble Space Telescope in March 2003, but had to assume an albedo to derive its size from its observed magnitudes. It is important to derive an additional constraint for independently determining both the comet size and albedo. We implemented the well-known ``radiometric method'', which combines visible and infrared photometry. Sixteen thermal images of 67P/C-G were obtained by the Multiband Imaging Photometer (MIPS) 24 µm channel of the Spitzer Space Telescope (SST) on 25 February 2004: the observations spanned a time interval of ∼12.5h, which sampled the rotational light curve of its nucleus. The comet was then outbound at a heliocentric distance of 4.48AU, at a distance of 4.04AU from SST, and at a solar phase angle of 12.1°. The nucleus conspicuously appeared as a bright point source superimposed on a dust trail; it was necessary to apply the point-spread function fitting technique using an adequate model of the trail to correctly determine the thermal flux from the nucleus. The data were analyzed using a standard thermal model that incorporated the thermal inertia. Our preferred solution with a low thermal inertia has overall dimensions measured along the principal axis of 4.40-5.20km, 4.16-4.30km, and 3.40-3.50km, corresponding to an effective radius of a sphere with the same volume in the range of 1.93-2.03km. Larger values of thermal inertia produce larger sizes but the effective radius cannot exceed ∼2.3km. The albedo is in the range 0.039-0.043, remarkably consistent with the canonical value of 0.04 for cometary nuclei. The success of the landing of the Philae surface module remains critically dependent upon the bulk density of the nucleus: it would be safe if close to 0.35g/cm3, but a larger value, for instance 0.5g/cm3, would present some risks.

Abstract Copyright: ∼

Journal keyword(s): comets: general - comets: individual: glutag{Viz.comet 67P | 67P/Churyumov-Gerasimenko} - techniques: image processing

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 159330 * 17 30 43.5747719616 +57 52 36.566848992 9.210 7.640 6.210     K2III 44 0

Query : 2008A&A...489..777L

Basic data :
HD 159330 -- Star
Other object types:
otypes_help
* (HD,AG,...), NIR (2MASS), IR (IRAS)
ICRS coord. (ep=J2000) :
17 30 43.5747719616 +57 52 36.566848992 (Optical) [ 0.0263 0.0228 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
17 29 55.2948182604 +57 54 46.585460503 [ 0.0263 0.0228 90 ]
Gal coord. (ep=J2000) :
086.2524011960962 +33.3268687907119 [ 0.0263 0.0228 90 ]
Proper motions mas/yr :
13.303 -13.779 [0.036 0.032 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -12.71 [0.14] / z(spectroscopic) -0.000042 [0.000000] / cz -12.71 [0.14]
   (Opt) A 2018yCat.1345....0G
Parallaxes (mas):
3.5857 [0.0255] A 2020yCat.1350....0G
Spectral type:
K2III C 2007PASP..119..994E
Fluxes (7) :
U 9.210 [0.010] C 1991A&AS...89..415O
B 7.640 [0.007] C 1991A&AS...89..415O
V 6.210 [0.009] C 1991A&AS...89..415O
G 5.739629 [0.002804] C 2020yCat.1350....0G
J 3.755 [0.208] D 2003yCat.2246....0C
H 3.035 [0.158] D 2003yCat.2246....0C
K 2.787 [0.206] D 2003yCat.2246....0C
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Identifiers (22) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

HD 159330 GCRV 10134 2MASS J17304356+5752365 WEB 14461
AG+57 1117 GSC 03896-01507 PPM 36024 YZ 57 9321
AGKR 15628 HIC 85692 SAO 30434 Gaia DR2 1434412634690504192
BD+57 1774 HIP 85692 SKY# 31602 Gaia DR3 1434412634690504192
DO 35801 HR 6540 TIC 356111584
GC 23758 IRAS 17299+5754 TYC 3896-1507-1

References (44 between 1850 and 2026) (Total 44)
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 : 10    Distance : 2    Rot : 1    Fe/H : 5    Plx : 4    PM : 7    SpT : 1   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : HD 159330

Link by name to the catalogue in VizieR :

HD 159330 AG+57 1117 BD+57 1774 DO 35801 GSC 03896-01507
HIC 85692 HIP 85692 HR 6540 IRAS 17299+5754 2MASS J17304356+5752365
PPM 36024 SAO 30434 TYC 3896-1507-1 Gaia DR2 1434412634690504192 Gaia DR3 1434412634690504192

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