Search Publications

Comet 41P/Tuttle-Giacobini-Kresak, 45P/Honda-Mrkos-Pajdusakova, and 46P/Wirtanen: Water Production Activity over 21 yr with SOHO/SWAN
DOI: 10.3847/PSJ/abb026 Bibcode: 2020PSJ.....1...72C

Bertaux, J. -L.; Combi, M. R.; Quémerais, E. +3 more

In 2017, 2018, and 2019, comets 46P/Wirtanen, 45P/Honda-Mrkos-Pajdusakova, and 41P/Tuttle-Giacobini-Kresak all had perihelion passages. Their hydrogen comae were observed by the Solar Wind ANisotropies (SWAN) all-sky hydrogen Lyα camera on the SOlar and Heliospheric Observer (SOHO) satellite: comet 46P for the fourth time and comets 45P and 41P fo…

2020 The Planetary Science Journal
SOHO 28
Experimental Investigation of Oxidation of Pyroxene and Basalt: Implications for Spectroscopic Analyses of the Surface of Venus and the Ages of Lava Flows
DOI: 10.3847/PSJ/ab8faf Bibcode: 2020PSJ.....1...21C

Filiberto, J.; Cutler, K. S.; Treiman, A. H. +1 more

Alteration of basalt on the surface of Venus should be dominated by nanophase hematite and sulfate coatings, but the timescale of oxidation and how that affects spectroscopic measurements has not been extensively studied. The oxidation rate and the effect on reflectance spectroscopy are needed to constrain the age of lava flows with high emissivit…

2020 The Planetary Science Journal
VenusExpress 20
Stellar Occultation by the Resonant Trans-Neptunian Object (523764) 2014 WC510 Reveals a Close Binary TNO
DOI: 10.3847/PSJ/abb23d Bibcode: 2020PSJ.....1...48L

Buie, Marc W.; Wasserman, Lawrence H.; Leiva, Rodrigo +22 more

We report on the stellar occultation by (523764) 2014 WC510 observed on 2018 December 1 UT. This occultation campaign was part of the Research and Education Collaborative Occultation Network (RECON), a network of small telescopes spread over 2000 km in western USA and Canada. Light curves from six stations revealed three groups of two o…

2020 The Planetary Science Journal
Gaia 14
Detection of a Satellite of the Trojan Asteroid (3548) Eurybates—A Lucy Mission Target
DOI: 10.3847/PSJ/abac54 Bibcode: 2020PSJ.....1...44N

Marchi, S.; Weaver, H. A.; Buie, M. W. +8 more

We describe the discovery of a satellite of the Trojan asteroid (3548) Eurybates in images obtained with the Hubble Space Telescope. The satellite was detected on three separate epochs, two in 2018 September and one in 2020 January. The satellite has a brightness in all three epochs consistent with an effective diameter of d2 = 1.2 ± 0.…

2020 The Planetary Science Journal
eHST 14
Possible Evidence of p-modes in Cassini Measurements of Saturn's Gravity Field
DOI: 10.3847/PSJ/ab9f21 Bibcode: 2020PSJ.....1...27M

Iess, Luciano; Durante, Daniele; Markham, Steve +1 more

We analyze the range-rate residual data from Cassini's gravity experiment that cannot be explained with a static, zonally symmetric gravity field. We reproduce the data using a simple forward model of gravity perturbations from normal modes. To do this, we stack data from multiple flybys to improve sensitivity. We find a partially degenerate set o…

2020 The Planetary Science Journal
Cassini 13
Saturn's Atmospheric Helium Abundance from Cassini Composite Infrared Spectrometer Data
DOI: 10.3847/PSJ/ab9cb6 Bibcode: 2020PSJ.....1...30A

Achterberg, Richard K.; Flasar, F. Michael

We use thermal infrared data from the Composite Infrared Spectrometer, which was on board the Cassini orbiter, to retrieve the helium abundance in Saturn's visible atmosphere. We find that the data is most consistent with a helium-to-hydrogen mole ratio in the range between 0.04 and 0.075, near the lower end of previous measurements, and implying …

2020 The Planetary Science Journal
Cassini 10
HST UV Observations of Asteroid (16) Psyche
DOI: 10.3847/PSJ/abb67e Bibcode: 2020PSJ.....1...53B

Roth, Lorenz; Feaga, Lori M.; Becker, Tracy M. +7 more

The Main Belt Asteroid (16) Psyche is the target object of the NASA Discovery Mission Psyche. We observed the asteroid at ultraviolet (UV) wavelengths (170-310 nm) using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope during two separate observations. We report that the spectrum is very red in the UV, with a blue upturn shor…

2020 The Planetary Science Journal
eHST 8
Recurrent Cometary Activity in Near-Earth Object (3552) Don Quixote
DOI: 10.3847/PSJ/ab8ae5 Bibcode: 2020PSJ.....1...12M

Smith, Howard A.; Hora, Joseph L.; Agarwal, Jessica +12 more

We report on observations of activity in near-Earth object (3552) Don Quixote using the Spitzer Space Telescope and ground-based telescopes around its 2018 perihelion passage. Spitzer observations obtained six months before perihelion show extended emission around the target's nucleus that is most likely caused by molecular band emission from eith…

2020 The Planetary Science Journal
Gaia 7
Tidal Currents Detected in Kraken Mare Straits from Cassini VIMS Sun Glitter Observations
DOI: 10.3847/PSJ/aba191 Bibcode: 2020PSJ.....1...35H

Sotin, Christophe; Barnes, Jason W.; Soderblom, Jason M. +3 more

We present Cassini Visual and Infrared Mapping Spectrometer (VIMS) observations of sun glitter—wave-induced reflections from a liquid surface offset from a specular point—on Kraken Mare. sun glitter reveals rough sea surfaces around Kraken Mare, namely the coasts and narrow straits. The sun glitter observations indicate wave activity driven by the…

2020 The Planetary Science Journal
Cassini 1
Changes in a Dusty Ringlet in the Cassini Division after 2010
DOI: 10.3847/PSJ/abacc7 Bibcode: 2020PSJ.....1...43H

Bridges, Bill; Hedman, Mathew

A dusty ringlet designated R/2006 S3, also known as the "Charming Ringlet," is located around 119,940 km from the center of Saturn within the Laplace Gap in the Cassini Division. Prior to 2010, the ringlet had a simple radial profile and a predictable eccentric shape with two components, one forced by solar radiation pressure and the other freely …

2020 The Planetary Science Journal
Cassini 1