Spatio-temporal Variation of Bright Ephemeral Features on Titan’s North Pole

• Published in: The Planetary Science Journal
• Main Authors: Dhingra, Rajani, Barnes, Jason, Heslar, Michael, Brown, Robert, Buratti, Bonnie, Sotin, Christophe, Soderblom, Jason, Rodriguez, Sebastien, Mouélic, Stéphane Le, Nicholson, Philip, Baines, Kevin, Clark, Roger, Jaumann, Ralf
• Other Authors: Institut de Physique du Globe de Paris (IPGP (UMR_7154)), Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 2020
• Subjects: [SDU]Sciences of the Universe [physics]; North Pole
• Online Access: https://insu.hal.science/insu-03578758; https://insu.hal.science/insu-03578758/document; https://insu.hal.science/insu-03578758/file/Dhingra_2020_Planet._Sci._J._1_31.pdf; https://doi.org/10.3847/PSJ/ab9c2b

International audience Abstract We identify and document the instances of bright ephemeral features (BEF)—bright areas that appear, disappear, and shift from flyby to flyby on Titan’s north pole, using the Cassini Visual and Infrared Mapping Spectrometer data set, thereby developing a sense of their spatial distribution and temporal frequency. We find that BEFs have differing geographic location and spatial extents. However, they have similar observation geometries and orders of surface area coverage and are mostly accompanied by specular reflections. We find the BEFs to represent either broad specular reflection off of a recently wetted surface on the north pole of Titan or a near-surface fog—both owing to probable recent rainfalls. Our surface model constrains the surface roughness to be of 9°–15° indicating the approximate vertical relief of the region to be that of cobbles. We also find that within less than two Titan days the BEF (if on the surface) might infiltrate into the subsurface. We hypothesize the parts of BEFs that extend into the maria to be precipitation fog.