Neptune long-lived atmospheric features in 2013-2015 from small (28-cm) to large (10-m) telescopes

TL;DR

This study documents the long-term observation and analysis of Neptune's atmospheric features from small to large telescopes, revealing persistent cloud systems and their oscillatory motions over several years.

Contribution

It provides a comprehensive multi-scale observational analysis of Neptune's atmospheric features, combining data from small telescopes, large observatories, and amateur astronomers.

Findings

Detection of long-lived bright atmospheric features on Neptune from 2013 to 2015.

Identification of a bright cloud system with a 90-day oscillation in longitude.

Observation of a dark spot associated with the bright cloud in 2015.

Abstract

Since 2013, observations of Neptune with small telescopes have resulted in several detections of long-lived bright atmospheric features that have also been observed by large telescopes such as Keck II or Hubble. The combination of both types of images allows the study of the long term evolution of major cloud systems in the planet. In 2013 and 2014 two bright features were present on the planet at southern mid latitudes. These may have merged in late 2014, possibly leading to the formation of a single bright feature observed during 2015 at the same latitude. This cloud system was first observed in January 2015 and nearly continuously from July to December 2015 in observations with telescopes in the 2 to 10 meter class and in images from amateur astronomers. These images show the bright spot as a compact feature at 40.1 deg South planetographic latitude well resolved from a nearby bright zonal band that extended from 42 deg South to 20 deg South. Tracking its motion from July to November 2015 suggests a longitudinal oscillation of 16 deg in amplitude with a 90 day period, typical of dark spots on Neptune and similar to the Great Red Spot oscillation in Jupiter. The limited time covered by high-resolution observations only covers one full oscillation and other interpretations of the changing motions could be possible. HST images in September 2015 show the presence of a dark spot at short wavelengths in the southern flank of the bright cloud observed throughout 2015.