Helene's surface properties from a photometric multi-wavelength analysis

Icarus Elsevier 392 (2022) 115376

Authors:

E Royer, A Hendrix, J Elliott, L Esposito, C Howett, L Spilker

Abstract:

On January 31, 2011, the remote-sensing instruments onboard the Cassini spacecraft (UVIS (Ultraviolet Imaging Spectrograph; ISS (Imaging Science Subsystem); VIMS (Visual and Infrared Mapping Spectrometer) and CIRS (Composite Infrared Spectrometer)) observed Helene, Dione's leading Lagrangian moon. We report here on the photometric characteristics of Helene between 0.11 μm and 5.2 μm. We find that Helene's spectrum is dominated by the signature of water-ice and we retrieve a grain size of 3.4 μm in the ultraviolet. At all wavelengths, Helene shows signs of being a relatively fresh surface less affected by space weathering effects than other observed surfaces in the Saturn system. We present the first phase curve of Helene at 0.61 μm and place our ultraviolet and near-IR results in a wider spectral context toward a better understanding of Helene's surface evolution. Previous studies suggested that either a recent impact on Helene or an asymmetric flux of E-ring particles could explain the satellite high surface brightness (Hedman et al., 2020). Results from this study favor the impactor hypothesis to explain Helene's photometric behavior.

Inclusion of early-career researchers in space missions

Nature Astronomy Springer Nature 6:12 (2022) 1339-1341

Authors:

B Fernando, IJ Daubar, JCE Irving, CL Johnson, AG Marusiak, MM Baker, S Stanley

Characteristics of de Gerlache crater, site of girlands and slope exposed ice in a lunar polar depression

Icarus Elsevier 388 (2022) 115231

Authors:

A Kereszturi, R Tomka, PA Gläser, BD Pal, V Steinmann, T Warren

The Winchcombe meteorite, a unique and pristine witness from the outer solar system

Science Advances American Association for the Advancement of Science 8:46 (2022) eabq3925

Authors:

Ashley J King, Luke Daly, James Rowe, James Bryson, Rowan Curtis, Tristram Warren, Neil Bowles, Sanjana Sridhar

Abstract:

Direct links between carbonaceous chondrites and their parent bodies in the solar system are rare. The Winchcombe meteorite is the most accurately recorded carbonaceous chondrite fall. Its pre-atmospheric orbit and cosmic-ray exposure age confirm that it arrived on Earth shortly after ejection from a primitive asteroid. Recovered only hours after falling, the composition of the Winchcombe meteorite is largely unmodified by the terrestrial environment. It contains abundant hydrated silicates formed during fluid-rock reactions, and carbon- and nitrogen-bearing organic matter including soluble protein amino acids. The near-pristine hydrogen isotopic composition of the Winchcombe meteorite is comparable to the terrestrial hydrosphere, providing further evidence that volatile-rich carbonaceous asteroids played an important role in the origin of Earth’s water.

Largest recent impact craters on Mars: Orbital imaging and surface seismic co-investigation

Science American Association for the Advancement of Science (AAAS) 378:6618 (2022) 412-417

Authors:

LV Posiolova, P Lognonné, WB Banerdt, J Clinton, GS Collins, T Kawamura, S Ceylan, IJ Daubar, B Fernando, M Froment, D Giardini, MC Malin, K Miljković, SC Stähler, Z Xu, ME Banks, É Beucler, BA Cantor, C Charalambous, N Dahmen, P Davis, M Drilleau, CM Dundas, C Durán, F Euchner, RF Garcia, M Golombek, A Horleston, C Keegan, A Khan, D Kim, C Larmat, R Lorenz, L Margerin, S Menina, M Panning, C Pardo, C Perrin, WT Pike, M Plasman, A Rajšić, L Rolland, E Rougier, G Speth, A Spiga, A Stott, D Susko, NA Teanby, A Valeh, A Werynski, N Wójcicka, G Zenhäusern