A shift in Jupiter's equatorial haze distribution imaged with the Multi-Conjugate Adaptive Optics Demonstrator at the VLT
Michael H. Wong (1), Franck Marchis (1, 2), Enrico Marchetti (3),, Paola Amico (3), Sebastien Tordo (3), Herve Bouy (4), Imke de Pater (1) ((1), UC Berkeley, (2) SETI Institute, (3) ESO, (4) IAC)

TL;DR
This study used advanced adaptive optics imaging to observe Jupiter's equatorial haze, revealing significant distribution changes potentially linked to atmospheric dynamics and cloud activity.
Contribution
First high-resolution adaptive optics images of Jupiter's equatorial haze showing a shift in distribution and insights into haze formation and transport mechanisms.
Findings
Haze distribution shifted from 5°N to the equator since 2005.
Haze reflectivity varies with particle size and cloud source changes.
Haze variation is influenced by particle size, cloud sources, diffusion, and transport.
Abstract
Jupiter was imaged during the Science Demonstration of the MCAO Demonstrator (MAD) at the European Southern Observatory's UT3 Very Large Telescope unit. Io and Europa were used as natural guide stars on either side of Jupiter, separated from each other by about 1.6 arcmin from 23:41 to 01:32 UT (2008 Aug 16/17). The corrected angular resolution was 0.090 arcsec across the entire field of view, as measured on background stars. The observations at 2.02, 2.14, and 2.16 micrometers were sensitive to portions of the Jovian spectrum with strong methane absorption. The data probe the upper troposphere, which is populated with a fine (~0.5 micrometer) haze. Two haze sources have been proposed: lofting of fine cloud particles into the stable upper troposphere, and condensation of hydrazine produced via ammonia photochemistry. The upper tropospheric haze is enhanced over Jupiter's equatorial…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
