Gemini Gets Lucky and Takes a Deep Dive Into Jupit

Credit: Credit: International Gemini Observatory/NOIRLab/NSF/AURA, M.H. Wong (UC Berkeley) and team Acknowledgments: Mahdi Zamani

This video shows one lucky imaging set of observations on Jupiter, taken 8 April 2019, as a timelapse on each pointing of the mosaic (left) used to construct the final full view of Jupiter (right). The power of lucky imaging is clearly shown: some frames are sharp and detailed, while others seem blurred or even unfocused because of changes in Earth’s atmosphere above the telescope. By combining only the sharpest images in each pointing, astronomers can dramatically reduce the adverse effects of Earth’s atmosphere on the quality of the images. Also note that the features on Jupiter noticeably move as each set of images is taken. Astronomers correct for that movement before stitching the clearest images together into a sharp view of the full planet.

Newswise — Three years of imaging observations using the international Gemini Observatory, a program of NSF’s NOIRLab, have probed deep into Jupiter’s cloud tops. The ultra-sharp Gemini infrared images complement optical and ultraviolet observations by Hubble and radio observations by the Juno spacecraft to reveal new secrets about the giant planet.

“The Gemini data were critical because they allowed us to probe deeply into Jupiter’s clouds on a regular schedule,” said Michael Wong of UC Berkeley, who led the research team. “We used a very powerful technique called lucky imaging,” adds Wong. With lucky imaging, a large number of very short exposure images are obtained and only the sharpest images, when the Earth’s atmosphere is briefly stable, are used. The result in this case is some of the sharpest infrared images of Jupiter ever obtained from the ground. According to Wong, “These images rival the view from space.”

Gemini North’s Near Infrared Imager (NIRI) allows astronomers to peer deep into Jupiter’s mighty storms, since the longer wavelength infrared light can pass through the thin haze but is obscured by thicker clouds high in Jupiter’s atmosphere. This creates a “jack-o-lantern”-like effect in the images where the warm, deep layers of Jupiter’s atmosphere glow through gaps in the planet’s thick cloud cover.

The detailed, multiwavelength imaging of Jupiter by Gemini and Hubble has, over the past three years, proven crucial to contextualizing the observations by the Juno orbiter, and to understanding Jupiter’s wind patterns, atmospheric waves, and cyclones. The two telescopes, together with Juno, can observe Jupiter’s atmosphere as a system of winds, gases, heat, and weather phenomena, providing coverage and insight much like the network of weather satellites meteorologists use to observe Earth.

Mapping giant lightning storms

On each of its close passes over Jupiter’s clouds, Juno detected radio signals created by powerful lightning flashes called sferics (short for atmospherics) and whistlers (so-called because of the whistle-like tone they cause on radio receivers). Whenever possible, Gemini and Hubble focused on Jupiter and obtained high-resolution, wide-area maps of the giant planet to augment the Juno observations.

Juno’s instruments could determine the latitude and longitude coordinates of clusters of sferic and whistler signals. With Gemini and Hubble images at multiple wavelengths, researchers now can probe the cloud structure at these locations. By combining these three pieces of information the research team found that the lightning strikes, and some of the largest storm systems that create them, are formed in and around large convective cells over deep clouds of water ice and liquid.

“Scientists track lightning because it is a marker of convection, the turbulent mixing process that transports Jupiter's internal heat up to the visible cloud tops,” explained Wong. The largest concentration of lightning seen by Juno came from a swirling storm called a “filamentary cyclone.” Imaging from Gemini and Hubble shows details in the cyclone, revealing it to be a twisted collection of tall convective clouds with deep gaps offering glimpses to the water clouds far below.

“Ongoing studies of lightning sources will help us understand how convection on Jupiter is different from or similar to convection in the Earth's atmosphere,” Wong commented.

Glowing features in the Great Red Spot

While scanning the gas giant for gaps in cloud cover, Gemini spotted a telltale glow in the Great Red Spot, indicating a clear view down to deep, warmer atmospheric layers.

“Similar features have been seen in the Great Red Spot before,” said team member Glenn Orton of JPL, “but visible-light observation couldn’t distinguish between darker cloud material, and thinner cloud cover over Jupiter’s warm interior, so their nature remained a mystery.”

Now with the data from Gemini, this mystery is solved. Where visible light images from Hubble show a dark semicircle in the Great Red Spot, images taken by Gemini using infrared light reveal a bright arc lighting up the region. This infrared glow, from Jupiter’s internal heat, would have been blocked by thicker clouds, but can pass through Jupiter’s hazy atmosphere unobscured. By seeing these features as bright infrared hotspots, Gemini confirms that they are gaps in the clouds.

“NIRI at Gemini North is the most effective way for the US and the international Gemini partnership investigators to get detailed maps of Jupiter at this wavelength,” explained Wong. Gemini achieved a 500-kilometer (300-mile) resolution on Jupiter. “At this resolution, the telescope could resolve the two headlights of a car in Miami, seen from New York City,” said Andrew Stephens, the Gemini astronomer who led the observations.[1]

“These coordinated observations prove once again that ground-breaking astronomy is made possible by combining the capabilities of the Gemini telescopes with complimentary ground- and space-based facilities,” said Martin Still, an astronomy program director at the National Science Foundation, which is Gemini’s US funding agency. “The international Gemini Partnership provides open access to a powerful combination of large telescopes’ collecting area, flexible scheduling, and a broad selection of interchangeable instruments.”

Notes

[1] This corresponds to an angular resolution of the Gemini infrared lucky imaging observations down to 0.13 arc-seconds.

More information

The results were published in the April 2020 issue of The Astrophysical Journal Supplement Series.

Because of their value for ongoing and future research, Wong is making the processed Gemini and Hubble data available to other researchers through the Mikulski Archives for Space Telescopes (MAST) at the Space Telescope Science Institute in Baltimore, Maryland.

The publication team was composed of: Michael H. Wong (University of California, Berkeley), Amy A. Simon (NASA Goddard Space Flight Center), Joshua W. Tollefson and Imke de Pater (University of California, Berkeley), Megan N. Barnett (University of Chicago), Andrew I. Hsu (University of California, Berkeley), Andrew W. Stephens (Gemini Observatory North), Glenn S. Orton (Jet Propulsion Laboratory, California Institute of Technology), Scott W. Fleming (Space Telescope Science Institute), Charles Goullaud (University of California, Berkeley), William Januszewski and Anthony Roman (Space Telescope Science Institute), Gordon L. Bjoraker (NASA Goddard Space Flight Center), Sushil K. Atreya (University of Michigan), Alberto Adriani (Istituto di Astrofisica e Planetologia Spaziali), and Leigh N. Fletcher (University of Leicester).

NSF’s National Optical-Infrared Astronomy Research Laboratory (NOIRLab), the US center for ground-based optical-infrared astronomy, operates the international Gemini Observatory (a facility of NSF, NRC–Canada, ANID–Chile, MCTIC–Brazil, MINCyT–Argentina, and KASI–Republic of Korea), Kitt Peak National Observatory (KPNO), Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and the Vera C. Rubin Observatory. It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona. The astronomical community is honored to have the opportunity to conduct astronomical research on Iolkam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawaiʻi, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence that these sites have to the Tohono O’odham Nation, to the Native Hawaiian community, and to the local communities in Chile, respectively.