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The Bathymetry of Moray Sinus at Titan's Kraken Mare
DOI: 10.1029/2020JE006558 Bibcode: 2020JGRE..12506558P

Lunine, J. I.; Hayes, A. G.; Le Gall, A. +4 more

Moray Sinus is an estuary located at the northern end of Titan's Kraken Mare. The Cassini RADAR altimeter acquired three segments over this mare during the T104 flyby of Titan, on August 21, 2014. Herein, we present a detailed analysis of the received echoes. Some of these waveforms exhibit a reflection from the seafloor, from up to 85-18+28 m of …

2020 Journal of Geophysical Research (Planets)
Cassini 16
Small Impact Crater Populations on Saturn's Moon Tethys and Implications for Source Impactors in the System
DOI: 10.1029/2020JE006400 Bibcode: 2020JGRE..12506400F

Ferguson, S. N.; Rhoden, A. R.; Kirchoff, M. R.

Current estimates place the ages of the inner Saturnian satellites (Mimas, Enceladus, Tethys, Dione, and Rhea) between 4.5 Gyr and 100 Myr. These estimates are based on impact crater measurements and dynamical simulations, both of which have uncertainties. Models of satellite evolution are inherently simplified and rely on uncertain or unknown par…

2020 Journal of Geophysical Research (Planets)
Cassini 15
Updated Equipotential Shapes of Jupiter and Saturn Using Juno and Cassini Grand Finale Gravity Science Measurements
DOI: 10.1029/2019JE006354 Bibcode: 2020JGRE..12506354B

Helled, Ravit; Folkner, William M.; Parisi, Marzia +2 more

A commonly used shape model for the giant plants of Jupiter and Saturn is an oblate ellipsoid, a simplified model of the equipotential shape. The ellipsoidal shape models were originally derived from radio occultation data and gravity data after the Voyager flybys in 1979. Through precise Doppler tracking of NASA's Juno and Cassini spacecraft tele…

2020 Journal of Geophysical Research (Planets)
Cassini 10
Compositional Measurements of Saturn's Upper Atmosphere and Rings from Cassini INMS
DOI: 10.1029/2020JE006427 Bibcode: 2020JGRE..12506427S

Yelle, R. V.; Hörst, S. M.; Koskinen, T. T. +4 more

The Cassini spacecraft's last orbits directly sampled Saturn's thermosphere and revealed a much more chemically complex environment than previously believed. Observations from the Ion and Neutral Mass Spectrometer (INMS) aboard Cassini provided compositional measurements of this region and found an influx of material raining into Saturn's upper at…

2020 Journal of Geophysical Research (Planets)
Cassini 7
Relative Crater Scaling Between the Major Moons of Saturn: Implications for Planetocentric Cratering and the Surface Age of Titan
DOI: 10.1029/2020JE006392 Bibcode: 2020JGRE..12506392B

Bell, Samuel W.

The chronology of the moons of Saturn, especially Titan, has been limited by a lack of strong constraints on the cratering rate, low number statistics for small-N counts of large-diameter craters, and uncertainty about whether impactors are mostly heliocentric impactors orbiting the Sun or planetocentric impactors orbiting Saturn itself. Here, I p…

2020 Journal of Geophysical Research (Planets)
Cassini 7
Nondetection of Radio Emissions From Titan Lightning by Cassini RPWS
DOI: 10.1029/2020JE006496 Bibcode: 2020JGRE..12506496F

Gurnett, D. A.; Kurth, W. S.; Fischer, G. +1 more

The Saturn-orbiting Cassini spacecraft completed 126 close Titan flybys from 2004 until 2017. During almost all of them the Cassini Radio and Plasma Wave Science (RPWS) instrument was turned on to search for radio emissions attributed to Titan lightning. Here we report about their nondetection after close inspection of all Titan flybys throughout …

2020 Journal of Geophysical Research (Planets)
Cassini 3