Maunakea, Hawaiʻi – For the first time in nearly three decades of observations, clouds seen on Neptune have all but vanished. Images from 1994 to 2022 of the big blue planet captured from Maunakea on Hawaiʻi Island through the lens of W. M. Keck Observatory, along with views from space via NASA’s Hubble Space Telescope show clouds are nearly gone with the exception of the south pole. The observations, which are published in the journal Icarus, further reveal a connection between Neptune’s disappearing clouds and the solar cycle – a surprising find given that Neptune is the farthest major planet from the Sun and receives only 1/900th of the sunlight we get on Earth.
A University of California (UC) Berkeley-led team of astronomers discovered the abundance of clouds normally seen at the icy giant’s mid-latitudes started to fade in 2019.
“I was surprised by how quickly clouds disappeared on Neptune,” said Imke de Pater, emeritus professor of astronomy at UC Berkeley and senior author of the study. “We essentially saw cloud activity drop within a few months.”
“Even four years later, the images we took this past June showed the clouds haven’t returned to their former levels,” said Erandi Chavez, a graduate student at Harvard University’s Center for Astrophysics who led the study when she was an undergraduate astronomy student at UC Berkeley. “This is extremely exciting and unexpected, especially since Neptune’s previous period of low cloud activity was not nearly as dramatic and prolonged.”
To monitor the evolution of Neptune’s appearance, Chavez and her team analyzed images taken from 1994 to 2022 using Keck Observatory’s second generation Near-Infrared Camera (NIRC2) paired with its adaptive optics system (since 2002), as well as observations from Lick Observatory (2018-2019) and the Hubble Space Telescope (since 1994). In recent years the Keck Observatory observations have been complemented by images taken as part of Keck Observatory’s Twilight Observing Program and by Hubble Space Telescope images taken as part of the Outer Planet Atmospheres Legacy (OPAL) program.
The data revealed an intriguing pattern between changes in Neptune’s cloud cover and the solar cycle – the period when the Sun’s magnetic field flips every 11 years, causing levels of solar radiation to fluctuate. When the Sun emits more intense ultraviolet (UV) light, specifically the strong hydrogen Lyman-alpha emission, more clouds appear on Neptune about two years later. The team further found a positive correlation between the number of clouds and the ice giant’s brightness from the sunlight reflecting off it.
“These remarkable data give us the strongest evidence yet that Neptune’s cloud cover correlates with the Sun’s cycle,” said de Pater. “Our findings support the theory that the Sun’s UV rays, when strong enough, may be triggering a photochemical reaction that produces Neptune’s clouds.”
The connection between the solar cycle and Neptune’s cloudy weather pattern is derived from 2.5 cycles of cloud activity recorded over the 29-year span of Neptunian observations. During this time, the planet’s reflectivity increased in 2002 (brightness maxima), then dimmed (brightness minima) in 2007, became bright again in 2015, then darkened in 2020 to the lowest level ever observed, which is when most of the clouds went away. The changes in Neptune’s brightness caused by the Sun appears to go up and down relatively in sync with the coming and going of clouds on the planet.
However, more work is necessary to unpack this correlation given the complexity of other factors; for example, while an increase in UV sunlight could produce more clouds and haze, it could also darken them, thereby reducing Neptune’s overall brightness. Storms on Neptune rising up from the deep atmosphere affect the cloud cover, but are not related to photochemically-produced clouds, and hence may complicate correlation studies with the solar cycle. Continued observations of Neptune are also needed to see how long the current near-absence of clouds will last.
This discovery adds to the exciting observations of the blue-hued world’s wildly active and chaotic atmosphere, which feature methane clouds that are whipped around by supersonic winds – the fastest wind speeds recorded anywhere in our solar system. One of the earliest and most striking images was captured by NASA’s Voyager 2 spacecraft during its flyby of Neptune in 1989, revealing a massive storm system named the “Great Dark Spot.” Other storms and dark spots have been spotted since, in particular a large equatorial storm in 2017 and a large dark spot at northern latitudes in 2018.
“It’s fascinating to be able to use telescopes on Earth to study the climate of a world more than 2.5 billion miles away from us,” said Carlos Alvarez, staff astronomer at Keck Observatory and co-author of the study. “Advances in technology as well as our Twilight Observing Program have enabled us to constrain Neptune’s atmospheric models, which are key to understanding the correlation between the ice giant’s climate and the solar cycle.”
The research team continues to track Neptune’s cloud activity. The recent images taken in June 2023 were obtained at the same time as when NASA’s James Webb Space Telescope (JWST) captured near- and mid-infrared images.
“We have seen more clouds in the most recent images, in particular at northern latitudes and at high altitudes, as expected from the observed increase in the solar UV flux over the past ~2 years,” said de Pater.
The combined data from JWST and Keck Observatory will enable further investigations into the physics and chemistry that leads to Neptune’s dynamic appearance, which in turn may help deepen astronomers’ understanding not only of Neptune, but also of exoplanets.
Learn more:
- “Neptune’s Disappearing Clouds Linked to the Solar Cycle” – Space Telescope Science Institute Press Release, August 17
- More images of Neptune’s disappearing clouds – Imke de Pater, Emeritus Professor of Astronomy, UC Berkeley, August 17
ABOUT NIRC2
The Near-Infrared Camera, second generation (NIRC2) works in combination with the Keck II adaptive optics system to obtain very sharp images at near-infrared wavelengths, achieving spatial resolutions comparable to or better than those achieved by the Hubble Space Telescope at optical wavelengths. NIRC2 is probably best known for helping to provide definitive proof of a central massive black hole at the center of our galaxy. Astronomers also use NIRC2 to map surface features of solar system bodies, detect planets orbiting other stars, and study detailed morphology of distant galaxies.
ABOUT ADAPTIVE OPTICS
W. M. Keck Observatory is a distinguished leader in the field of adaptive optics (AO), a breakthrough technology that removes the distortions caused by the turbulence in the Earth’s atmosphere. Keck Observatory pioneered the astronomical use of both natural guide star (NGS) and laser guide star adaptive optics (LGS AO) and current systems now deliver images three to four times sharper than the Hubble Space Telescope at near-infrared wavelengths. AO has imaged the four massive planets orbiting the star HR8799, measured the mass of the giant black hole at the center of our Milky Way Galaxy, discovered new supernovae in distant galaxies, and identified the specific stars that were their progenitors. Support for this technology was generously provided by the Gordon and Betty Moore Foundation, Mt. Cuba Astronomical Foundation, NASA, NSF, and W. M. Keck Foundation.
ABOUT W. M. KECK OBSERVATORY
The W. M. Keck Observatory telescopes are among the most scientifically productive on Earth. The two 10-meter optical/infrared telescopes atop Maunakea on the Island of Hawaii feature a suite of advanced instruments including imagers, multi-object spectrographs, high-resolution spectrographs, integral-field spectrometers, and world-leading laser guide star adaptive optics systems. Some of the data presented herein were obtained at Keck Observatory, which is a private 501(c) 3 non-profit organization operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the Native Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.