Results 1 to 10 of about 129,106 (151)

Astrometric results of observations of mutual occultations and eclipses of the Uranian satellites in 2007 [PDF]

open access: yesAstronomy and Astrophysics, 2013
Context. The photometry of mutual occultations and eclipses of natural planetary satellites can be used to infer very accurate astrometric data.
Paolo Tanga, B C Bhatt, Ricard Casas
exaly   +3 more sources

Chaotic dust dynamics and implications for the hemispherical color asymmetries of the Uranian satellites

open access: yesIcarus, 2013
a b s t r a c t Dust grains generated by the Uranian irregular satellites will undergo chaotic large-amplitude eccentricity oscillations under the simultaneous action of radiation forces and the highly misaligned quadrupole potentials of the oblate ...
Douglas Hamilton   +2 more
exaly   +1 more source
Some of the next articles are maybe not open access.

Sounding the Icy Shell of Uranian Satellites with Radar

2023
R. Orosei   +9 more
openaire   +1 more source

CCD astrometric observations of Uranian satellites: 1995-1998 [PDF]

open access: yesAstronomy and Astrophysics, 1999
Astrometric positions of the ve largest Uranian satellites from 750 CCD frames taken at the oppositions of 1995 through 1998 are presented. The im- ages were obtained over 35 nights. Observed positions are compared with the calculated positions from GUST86.
C. H. Veiga, R. Vieira Martins
exaly   +3 more sources

Observations of Five Major Uranian Satellites during 2013–2020 Based on Gaia DR3

open access: yesAstrophysical Journal, Supplement Series
A total of 10,339 positions of the five major Uranian satellites (Ariel, Umbriel, Titania, Oberon and Miranda) were collected at the Yunnan Observatories from 2013 to 2020 with the 1.0 m astrometric reflector.
Kai Tang, Huiyan Zhang
exaly   +3 more sources

Astrometry of five major Uranian satellites in 1995–1997 [PDF]

open access: yesAstronomy and Astrophysics, 2002
At the oppositions of 1995-1997, a total of 122 CCD frames were taken on the 1.56 m astrometric telescope at the Sheshan station, yielding 864 positions of the major Uranian satellites. The calibration of the images was carried out using a least-squares iterative program by fitting to the well-known orbits of the brighter moons of Uranus, based on the ...
Katerina Hadjifotinou   +2 more
exaly   +3 more sources

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