2020A&A...639A..83T


Query : 2020A&A...639A..83T

2020A&A...639A..83T - Astronomy and Astrophysics, volume 639A83-83 (2020/7-1)

Global photometric properties of (162173) Ryugu.

TATSUMI E., DOMINGUE D., SCHRODER S., YOKOTA Y., KURODA D., ISHIGURO M., HASEGAWA S., HIROI T., HONDA R., HEMMI R., LE CORRE L., SAKATANI N., MOROTA T., YAMADA M., KAMEDA S., KOYAMA T., SUZUKI H., CHO Y., YOSHIOKA K., MATSUOKA M., HONDA C., HAYAKAWA M., HIRATA N., HIRATA N., YAMAMOTO Y., VILAS F., TAKATO N., YOSHIKAWA M., ABE M. and SUGITA S.

Abstract (from CDS):


Context. The Hayabusa2 spacecraft launched by Japan Aerospace Exploration Agency has been conducting observations of the asteroid (162173) Ryugu since June 2018. The Telescopic Optical Navigation Camera (ONC-T) onboard Hayabusa2 has obtained thousands of images under a variety of illumination and viewing conditions.
Aims. Our objective is to examine and validate the camera calibration, derive a photometric correction for creating global albedo maps, and to interpret the photometric modeling results to characterize the surface of Ryugu.
Methods. We observed (162173) Ryugu with the Gemini-South telescope, and combined these measurements with other published ground-based observations of the asteroid. The ground-based observations were compared with the data obtained by ONC-T in order to validate the radiometric calibration mutually. We used a combination of the Hapke disk-integrated and disk-resolved model equations to simultaneously analyze the combined ground- and spacecraft-based data.
Results. The average spectrum of Ryugu was classified as Cb-type following the SMASSII taxonomy and C/F-type following the Tholen taxonomy based on spacecraft observations. We derived Hapke model parameters for all seven color filters, which allowed us to photometrically correct images to within an error of <10% for ∼80% of the image pixels used in the modeling effort. Using this model, we derived a geometric albedo of 4.0±0.5% (v band) for Ryugu. The average reflectance factor at the standard illumination condition was 1.87±0.14% in the v band. Moreover we measured a phase reddening of (2.0±0.7)x10–3µm–1deg–1 for Ryugu, similar to that observed for the asteroid (101955) Bennu.
Conclusions. The global color map showed that the general trend was for darker regions to also be redder regions, however there were some distinct exceptions to this trend. For example, Otohime Saxum was bright and red while Kibidango crater was dark and blue. The darkness and flatness of Ryugu's reflectance might be caused by a high abundance of organic materials.

Abstract Copyright: © ESO 2020

Journal keyword(s): techniques: photometric - minor planets, asteroids: individual: Ryugu - space vehicles - methods: observational

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 142801 * 15 56 55.4364195480 -12 58 10.013939184   10.60 9.97     G2V 18 0

Query : 2020A&A...639A..83T

Basic data :
HD 142801 -- Star
Other object types:
otypes_help
* (HD,BD,...), NIR (2MASS)
ICRS coord. (ep=J2000) :
15 56 55.4364195480 -12 58 10.013939184 (Optical) [ 0.0143 0.0098 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
15 54 08.5998237912 -12 49 30.685455382 [ 0.0143 0.0098 90 ]
Gal coord. (ep=J2000) :
357.2598171336256 +29.7404238658338 [ 0.0143 0.0098 90 ]
Proper motions mas/yr :
-11.036 -26.890 [0.018 0.012 90] A 2020yCat.1350....0G
Radial velocity / Redshift / cz :
V(km/s) -65.21 [0.29] / z(spectroscopic) -0.000217 [0.000001] / cz -65.20 [0.29]
   (Opt) A 2018yCat.1345....0G
Parallaxes (mas):
8.5516 [0.0157] A 2020yCat.1350....0G
Spectral type:
G2V C 1988MSS...C04....0H
Fluxes (6) :
B 10.60 [0.04] D 2000A&A...355L..27H
V 9.97 [0.03] D 2000A&A...355L..27H
G 9.819585 [0.002764] C 2020yCat.1350....0G
J 8.769 [0.021] C 2003yCat.2246....0C
H 8.489 [0.029] C 2003yCat.2246....0C
K 8.412 [0.024] C 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 2 : 1803 Display criteria :

Identifiers (13) :
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HD 142801 HIP 78107 TIC 410543620 Gaia DR3 6264377206163200896
BD-12 4374 2MASS J15565543-1258099 TYC 5618-1037-1
GSC 05618-01037 PPM 230986 YZC 11 5531
HIC 78107 SAO 159596 Gaia DR2 6264377206162295552

References (18 between 1850 and 2026) (Total 18)
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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Velocities : 1    Distance : 2    Plx : 4    PM : 4    SpT : 2   

   


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HD 142801 BD-12 4374 GSC 05618-01037 HIC 78107 HIP 78107
2MASS J15565543-1258099 PPM 230986 SAO 159596 TYC 5618-1037-1 YZC 11 5531
Gaia DR2 6264377206162295552 Gaia DR3 6264377206163200896

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