Search Publications

Spatial distribution of impact craters on Deimos
DOI: 10.1016/j.icarus.2017.01.035 Bibcode: 2017Icar..288...69H

Hirata, Naoyuki

Deimos, one of the Martian moons, has numerous impact craters. However, it is unclear whether crater saturation has been reached on this satellite. To address this issue, we apply a statistical test known as nearest-neighbor analysis to analyze the crater distribution of Deimos. When a planetary surface such as the Moon is saturated with impact cr…

2017 Icarus
MEx 3
Direct detection of gaps in Saturn's A ring
DOI: 10.1016/j.icarus.2017.06.033 Bibcode: 2017Icar..297..110R

Esposito, Larry W.; Albers, Nicole; Brown, Zarah L. +1 more

Indirect observations spanning decades have indicated that Saturn's A ring is populated with a plethora of self-gravity wakes, small wavelike structures that arise from the gravitational attraction between ring particles. We present the direct detection of the gaps that represent the minima between the denser wakes. Through a statistical test, we …

2017 Icarus
Cassini 3
A curious ringlet that shares Prometheus' orbit but precesses like the F ring
DOI: 10.1016/j.icarus.2016.08.024 Bibcode: 2017Icar..281..322H

Hedman, M. M.; Carter, B. J.

Images obtained by the Cassini spacecraft of the region just beyond Saturn's main rings reveal a previously unreported narrow and dusty ringlet that has dynamical connections with both Saturn's small satellite Prometheus and the F ring. The radial position of this ringlet is observed to vary with time and longitude, indicating that it is eccentric…

2017 Icarus
Cassini 2
Morphology and temporal variation of the polar oval of Venus revealed by VMC/Venus express visible and UV images
DOI: 10.1016/j.icarus.2017.06.014 Bibcode: 2017Icar..295..110M

Imamura, Takeshi; Muto, Keishiro

The morphology of the dark polar oval seen at the Venus cloud top in visible and ultraviolet wavelengths has been unclear because the portion of the oval on the nightside is invisible. We analyzed in detail the variability of the whole shape of the oval by connecting VMC/Venus Express visible images taken on different days after shifting the image…

2017 Icarus
VenusExpress 2
Surface roughness of Saturn's rings and ring particles inferred from thermal phase curves
DOI: 10.1016/j.icarus.2017.05.008 Bibcode: 2017Icar..295...74M

Spilker, Linda; Morishima, Ryuji; Turner, Neal

We analyze thermal phase curves of all the main rings of Saturn (the A, B, C rings, and the Cassini division) measured by both the far-IR and mid-IR detectors of the Cassini Composite InfraRed Spectrometer (CIRS). All the rings show temperature increases toward zero phase angle, known as an opposition effect or thermal beaming. For the C ring and …

2017 Icarus
Cassini 2
Hyperactivity in 103P/Hartley 2: Chunks from the sub-surface in Type IIa jet regions
DOI: 10.1016/j.icarus.2016.12.021 Bibcode: 2017Icar..285...58B

Belton, Michael J. S.

We analyze the observed radial distribution of column densities of water-ice particulates embedded in the primary jet region (J1) of 103P's inner coma at altitudes between 439 and 1967 m (Protopapa et al., 2014, Icarus 238, 191-204) and determine the speed and acceleration of particles and their mass-flow within the filaments of the jet…

2017 Icarus
Rosetta 2
Corrigendum to "Observation of Neon at mid and high latitudes in the sunlit Lunar Exosphere: Results from CHACE aboard MIP/Chandrayaan-1", Vol. 272 (2016), pp 206-211, doi 10.1016/j.icarus.2016.02.030
DOI: 10.1016/j.icarus.2016.10.020 Bibcode: 2017Icar..284..489P

Bhardwaj, Anil; Sridharan, R.; Thampi, Smitha V. +2 more

Our paper titled "Observation of Neon at mid and high latitudes in the sunlit Lunar Exosphere: Results from CHACE aboard MIP/Chandrayaan-1" (Icarus 272 (2016) 206-211) presents the results of the observations on the distribution of neutral Neon in the mid and high lunar latitudes by the CHACE instrument aboard Moon Impact Probe (MIP) in Chandrayaa…

2017 Icarus
Chandrayaan-1 1