Results 91 to 100 of about 33,171 (317)
Since the Voyager fly-bys of Uranus and Neptune, improved gravity field data have been derived from long-term observations of the planets' satellite motions, and modified shape and solid-body rotation periods were suggested. A faster rotation period (-40
Anderson+47 more
core +1 more source
The Centenary of the Discovery of Uranus [PDF]
n ...
openaire +2 more sources
The rotation rate of Uranus is investigated by measuring the tilts of reflected Fraunhofer lines observed through a slit spectrograph. The data obtained are corrected for the effect of astronomical seeing, and the data-reduction procedures are outlined in detail.
R. M. Goody, R. A. Brown
openaire +2 more sources
Thermal evolution of Uranus and Neptune [PDF]
The brightness of Neptune is often found to be in accordance with an adiabatic interior, while the low luminosity of Uranus challenges this assumption.
L. Scheibe, N. Nettelmann, R. Redmer
semanticscholar +1 more source
Podczas badań przeprowadzonych w latach 2004–2005 oceniono wpływ terminu sadzenia rozsady na plonowanie 3 odmian cykorii sałatowej. Rozsadę sadzono 20 kwietnia, 5 i 20 maja, 5 czerwca, 15 lipca i 3 sierpnia w rozstawie 30 × 30 cm (‘Indigo’, ‘Leonardo’) i
Ewa Rożek
doaj
RESEARCHES OF LONG-TERM VARIATIONS IN URANUS AND NEPTUNE SPECTRA
The results of long-term spectral observations of Solar System giant planets Uranus and Neptune are presented here. Data were obtaining in period 2002-2012 at the peak Terskol Observatory (Northern Caucasus, Russia) using 2-meter Ritchey-Chretien ...
Yu. Kuznyetsova+5 more
doaj +1 more source
Interior Models of Uranus and Neptune
'Empirical' models (pressure vs. density) of Uranus and Neptune interiors constrained by the gravitational coefficients J_2, J_4, the planetary radii and masses, and Voyager solid-body rotation periods are presented.
Gerald Schubert+13 more
core +1 more source
Abstract The Solar, Anomalous, and Magnetospheric Explorer (SAMPEX) mission launched in July 1992 was the first NASA “Small Explorer” project. It had the goal to show how space missions could be developed much more rapidly than had become the situation in the 1980s and 1990s.
D. N. Baker, G. M. Mason
wiley +1 more source
Observations of Uranus at High Phase Angle as Seen by New Horizons
We present flux measurements of Uranus observed at phase angles of 43.°9, 44.°0, and 52.°4 by the Multispectral Visible Imaging Camera on the New Horizons spacecraft during 2023, 2010, and 2019, respectively.
Samantha N. Hasler+16 more
doaj +1 more source
The ζ ring is the innermost component of the Uranian ring system. It is of scientific interest because its morphology changed significantly between the Voyager 2 encounter in 1986 and subsequent Earth-based observations around 2007.
M. M. Hedman+5 more
doaj +1 more source