Striking Earth-Based Images Of Jupiter To Enhance Juno Flyby

This animation shows Jupiter as revealed by a powerful telescope and a mid-infrared filter sensitive to the giant planet’s tropospheric temperatures and cloud thickness. It combines observations made on Jan. 14, 2017, using the Subaru Telescope in Hawaii. Image Credit: NAOJ/NASA/JPL-Caltech

June 30, 2017 – Telescopes in Hawaii have obtained new images of Jupiter and its Great Red Spot, which will assist the first-ever close-up study of the Great Red Spot, planned for July 10. On that date, NASA’s Juno spacecraft will fly directly over the giant planet’s most famous feature at an altitude of only about 5,600 miles (9,000 kilometers).

Throughout the Juno mission, numerous observations of Jupiter by Earth-based telescopes have been acquired to help Juno investigate the giant planet’s atmosphere. On May 18, 2017, the Gemini North telescope and the Subaru Telescope, both on Hawaii’s Mauna Kea peak, simultaneously examined Jupiter in very high resolution at different wavelengths. These latest observations supplement others earlier this year in providing information about atmospheric dynamics at different depths at the Great Red Spot and other regions of Jupiter.

The Great Red Spot is a swirling storm, centuries old and wider than the diameter of Earth. Juno will use multiple instruments to study this feature when it flies over it about 12 minutes after the spacecraft makes the closest approach to Jupiter of its current orbit at 7:55 p.m. on July 10, MDT (9:55 p.m. on July 10, EDT; 1:55 a.m. on July 11, Universal Time).

“Observations with Earth’s most powerful telescopes enhance the spacecraft’s planned observations by providing three types of additional context,” said Juno science team member Glenn Orton of NASA’s Jet Propulsion Laboratory, Pasadena, California. “We get spatial context from seeing the whole planet. We extend and fill in our temporal context from seeing features over a span of time. And we supplement with wavelengths not available from Juno. The combination of Earth-based and spacecraft observations is a powerful one-two punch in exploring Jupiter.”

Orton collaborated with researchers at Gemini; Subaru; the University of California, Berkeley; Tohoku University, Japan; and elsewhere in planning the recent observations.

The observers used Gemini North on May 18 to examine Jupiter through special near-infrared filters. The Gemini observations focus on specific colors of light that can penetrate the upper atmosphere and clouds of Jupiter. These images are sensitive to increasing absorption by mixtures of methane and hydrogen gas in Jupiter’s atmosphere.

This composite, false-color infrared image of Jupiter reveals haze particles over a range of altitudes, as seen in reflected sunlight. It was taken using the Gemini North telescope in Hawaii on May 18, 2017, in collaboration with observations of Jupiter by NASA’s Juno mission. Image Credit: Gemini Observatory/ AURA/ NASA/ JPL-Caltech

“Back in May, Gemini zoomed in on intriguing features in and around Jupiter’s Great Red Spot: including a swirling structure on the inside of the spot, a curious hook-like cloud feature on its western side and a lengthy, fine-structured wave extending off from its eastern side,” said Orton. “Events like this show that there’s still much to learn about Jupiter’s atmosphere – the combination of Earth-based and spacecraft observations is a powerful one-two punch in exploring Jupiter.”

On the same night, researchers used Subaru’s Cooled Mid-Infrared Camera and Spectrometer (COMICS), with filters sensitive to temperatures at different layers of Jupiter’s atmosphere. These mid-infrared observations showed the Great Red Spot “had a cold and cloudy interior increasing toward its center, with a periphery that was warmer and clearer. This implied that winds were upwelling more vigorously toward its center and subsiding on the periphery,” Orton said. “A region to its northwest was unusually turbulent and chaotic, with bands that were cold and cloudy, alternating with bands that were warm and clear.”

This false-color image of Jupiter was taken on May 18, 2017, with the Subaru Telescope in Hawaii, using a mid-infrared filter centered at a wavelength of 8.8 microns. The Great Red Spot appears at the lower center of the planet as a cold region with a thick cloud layer. Image Credit: NAOJ/ NASA/ JPL-Caltech

Subaru’s mid-infrared imaging and spectroscopy with COMICS are particularly useful to Juno’s, by providing information about the temperature field and the distribution of ammonia, a condensate in Jupiter similar to water in the Earth’s atmosphere. In the full campaign of Earth-based support, the Subaru observations provide the highest spatial resolution of Jupiter’s thermal output due to the 8-meter size of its primary mirror.

The Juno spacecraft launched on a United Launch Alliance Atlas V rocket on August 5, 2011 and began orbiting Jupiter on July 4, 2016.

The spacecraft has now made five close-up passes of Jupiter’s atmosphere, the first of which was on August 27, 2016, and the latest (the sixth pass) on May 19th of this year. Each of these close passes has provided Juno’s science team with surprises.

A primary goal of the mission is to improve our understanding of Jupiter – from its atmospheric properties, to our understanding of how Jupiter and other planets in the outer Solar System formed.

NASA’s Jet Propulsion Laboratory, Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the Science Mission Directorate. Lockheed Martin Space Systems of Littleton, Colorado, built the spacecraft.