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Title: The 1.95-2.50 μm Spectrum of J6 Himalia
Authors: Geballe, Thomas R.; Ore, C. M. Dalle; Cruikshank, Dale P.;
Owen, T. C.
Journal: Icarus, Volume 159, Issue 2, p. 542-544. (Icarus
Homepage)
Publication Date: 10/2002
Origin: ELSEVIER
Abstract Copyright: (c) 2002 Elsevier Science (USA)
Bibliographic Code: 2002Icar..159..542G
Abstract
The reflectance spectrum of Jupiter's sixth satellite, Himalia, is
featureless in the wavelength region 1.95-2.50 μm as seen at a
spectral resolution of 0.005 μm, with no absorptions deeper than a
few percent. From model calculations we establish an upper limit of 10%
by weight of H2O (30-μm grains) mixed intimately in the
soil of Himalia, or alternatively 0.3% of the surface covered by
exposures of H2O ice spatially segregated from the darker
soil. For CH4 and CO2 ices the upper limits in
spatially segregated models are both 0.3%.
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Abstract
Title: Mutual phenomena involving J5 Amalthea in 2002-2003
Authors: Vachier, F.; Arlot, J. E.; Thuillot, W.
Affiliation: AA(Institut de mécanique céleste et de calcul des
éphémerides, IMCCE-Observatoire de Paris
vachier@bdl.fr), AB(Institut de mécanique céleste et
de calcul des éphémerides, IMCCE-Observatoire de Paris
arlot@bdl.fr), AC(Institut de mécanique céleste et de
calcul des éphémerides, IMCCE-Observatoire de Paris
thuillot@bdl.fr)
Journal: Astronomy and Astrophysics, v.394, p.L19-L21 (2002)
(A&A Homepage)
Publication Date: 10/2002
Origin: A&A
A&A Keywords: Amalthea, mutual events, dynamical modeling
Abstract Copyright: (c) 2002: Astronomy & Astrophysics
Bibliographic Code: 2002A&A...394L..19V
Abstract
Every six years mutual eclipses and occultations occur among the Jovian system
of satellites. Very accurate astrometric measurements and several physical characteristics
of the surfaces can be infered from their observation. This paper is provide predictions
of this type of events involving the fifth satellite J5 Amalthea, spanning from
November 2002 to June 2003 and to urge astronomers to observe them. Only the predictions
of the eclipses of Amalthea by Io are presented, when the distance between Amalthea-Io
and Amalthea-Jutpiter is large enough for photometric purposes. A full list of
phenomena is available on the server http://www.imcce.fr/Phemu03/phemu03_eng.html
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Title: Mutual Occultations and Eclipses of Galilean
Satellites of Jupiter in 2002-2003
Authors: Emel'yanov, N. V.
Affiliation: Sternberg Astronomical Institute, Universitetskii
pr. 13, Moscow, 119899 Russia. Institute of
Celestial Mechanics and Calculation of Ephemerides,
IMCEE-Observatory of Paris, 77 Avenue
Denfert-Rocherean, Paris, F-75014, France
Journal: Solar System Research, v. 36, Issue 4, p. 353-354
(2002).
Publication Date: 07/2002
Origin: KLUWER
Abstract Copyright: (c) 2002 Kluwer Academic Publishers
Bibliographic Code: 2002SoSyR..36..353E
Abstract
Information on the approach of a new epoch of mutual occultations and eclipses
in the system of Galilean satellites of Jupiter is presented. The importance
of observations of such phenomena is highly emphasized.
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Title: Astrometry from CCD photometry of mutual events of
Jovian satellites from VBO during 1997
Authors: Vasundhara, R.
Affiliation: Indian Institute of Astrophysics, Bangalore 560034,
India
Journal: Astronomy and Astrophysics, v.389, p.325-333 (2002)
(A&A Homepage)
Publication Date: 07/2002
Origin: A&A
A&A Keywords: eclipses, astrometry, ephemerides, occultations,
planets and satellites: general
Abstract Copyright: (c) 2002: Astronomy & Astrophysics
Bibliographic Code: 2002A&A...389..325V
Abstract
Astrometric results of CCD observations of the mutual events of the Galilean
satellites of Jupiter from the Vainu Bappu Observatory are presented. The
shifts in the photo-centers on the disks of Io and Europa due to albedo variations
inferred from the available mosaics of Galileo imagery are determined. The
estimated shifts from ~90 km East to ~50 km West on Io and from ~50 km East
to ~30 km West for Europa during one orbital period are comparable to the
accuracies provided by the present-day ephemerides. In a given mutual event
series, the mutual events involving a given satellite pair dominate in number
and occur nearly at the same orbital longitude within +/-20 degr ; all the
events are therefore delayed or all of them advanced depending on the direction
of the shift of the photo-center. The implications of including these cumulative
and sustained longitude residuals on the constructed ephemerides are discussed.
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Abstract
Title: Astrometric CCD observations of the inner Jovian
satellites in 1999-2000
Authors: Kulyk, I.; Jockers, K.; Karpov, N.; Sergeev, A.
Affiliation: AA( Main Astronomical Observatory of Ukrainian
National Academy of Sciences 03680, Golosiiv,
Kyiv-127, Ukraine; Isaac Newton Institute, Kiev
Branch Casilla 8-9,Correo 9, Santiago, Chile),
AB(Max-Planck-Institute for Aeronomy 37191
Katlenburg-Lindau, Germany), AC(International Center
for Astronomical and Medico-Ecological Studies
03680, Golosiiv, Kyiv-127, Ukraine),
AD(International Center for Astronomical and
Medico-Ecological Studies 03680, Golosiiv, Kyiv-127,
Ukraine)
Journal: Astronomy and Astrophysics, v.383, p.724-728 (2002)
(A&A Homepage)
Publication Date: 02/2002
Origin: A&A
A&A Keywords: PLANETS AND SATELLITES: INDIVIDUAL: JOVIAN INNER
SATELLITES, ASTROMETRY
Abstract Copyright: (c) 2002: Astronomy & Astrophysics
Bibliographic Code: 2002A&A...383..724K
Abstract
This paper presents the results of observations of the inner Jovian satellites
Thebe, Amalthea, Adrastea and Metis made in October-November 1999 and in November
2000. We provide Delta alpha and Delta delta of Thebe and Amalthea with respect
to the Galilean satellites, while the positions of Adrastea and Metis are
referred to either the Galilean moons or to Thebe or to Amalthea. All observed
positions are compared with theoretical ones. Residual statistics show an
inner accuracy of our observations in the range from about 0.1 to 0.9 arcsec.
The dependence of the differences of the observed and calculated positions
on the orbital longitude is presented for our observations of Adrastea and
Metis.
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Abstract
Title: Predictions of the mutual events of the Galilean
Satellites of Jupiter occurring in 2002-2003
Authors: Arlot, J.-E.
Affiliation: Institut de mécanique céleste et de calcul des
éphémérides - Observatoire de Paris, UMR 8028 du
CNRS, 77 avenue Denfert-Rochereau, 75014 Paris,
France
Journal: Astronomy and Astrophysics, v.383, p.719-723 (2002)
(A&A Homepage)
Publication Date: 02/2002
Origin: A&A
A&A Keywords: PLANETS AND SATELLITES: GENERAL, PLANETS AND
SATELLITES: INDIVIDUAL: JUPITER
Abstract Copyright: (c) 2002: Astronomy & Astrophysics
Bibliographic Code: 2002A&A...383..719A
Abstract
Mutual occultations and eclipses of the Galilean satellites of Jupiter will
occur in 2002-2003. This paper provides predictions of these events as well
as information useful for their observations. Such events are uncommon, since
they occur only every 6 years when the Earth and the Sun pass through the
common orbital plane of the Galilean satellites. Therefore, we encourage professional
and amateur astronomers to join the networks of observers in order to get
as many observations as possible. Data on the predictions of the events are
available on the web server of the IMCCE (www.bdl.fr).