Don’t miss Jupiter’s ‘unravelling’ Great Red Spot

13 June update: click here for new Great Red Spot images.

Dramatic changes in the appearance of Jupiter’s Great Red Spot (GRS) in less than three Earth days are revealed in this looping animation. The GRS made seven circuits of the planet in the interval between these two images captured by Australian amateur astronomer Anthony Wesley on 25 and 28 May (AEST dates). Interactions with Jupiter’s South Equatorial Belt (SEB) appear to be peeling material from the GRS on a roughly weekly basis. These filaments, some of which are 10,000 kilometres long or more, form a temporary bridge between the GRS and the SEB. Image credits: Anthony Wesley, AN animation: Ade Ashford.
The Great Red Spot (GRS) is the solar system’s largest known storm, an Earth-sized anticyclone boasting wind speeds approaching 400 kilometres per hour that has raged in the atmosphere of Jupiter for at least two centuries. But recent observations from Earth and space suggest that this iconic Jovian feature is undergoing enormous changes that could herald its demise. With Jupiter currently at its closest to Earth for 2019, there’s no better time to look for these dramatic changes yourself.

History of observation
While it’s possible that the GRS is the same storm discovered by Italian astronomer Giovanni Cassini in 1665, the first definite observations of the Great Red Spot date back to drawings made by German astronomer Samuel Heinrich Schwabe in 1831. The storm’s striking colour in 1878 led American astronomer Carr W. Pritchett to coin the name we use today, and the feature has been observed continuously since.

What is the GRS?
The Great Red Spot is an anticyclone weather feature that rotates counter-clockwise with a period of about six Earth days. Other Jovian cloud layers intermittently cover it leading to changes in colour, but generally, the GRS cloud tops are colder and extend 8 kilometres above their surroundings. The storm’s longevity is partly because Jupiter has no land masses or solid surface to cause it to lose energy due to friction.

Changing size
In the glory days of the Great Red Spot in the 19th century, the feature was a large oval some 48,000 kilometres (30,000 miles) long, but it was only half that length by the time the Voyager spacecraft visited Jupiter 40 years ago. The storm has become more rounded in recent years, but its decline continues; it’s presently under 16,000 kilometres long.

Why is the GRS red?
The reason for the storm’s signature hue is unknown, but theories suggest that compounds of phosphorus and sulfur or the Sun’s ultraviolet light acting on ammonium hydrosulfide and acetylene in Jupiter’s outer atmosphere could create organic compounds called tholins that would account for the red colour.

What’s now happening to the GRS?
The Great Red Spot lies south of Jupiter’s South Equatorial Belt (SEB), constrained to a latitude close to 22 degrees south of the planet’s equator by easterly jet streams to the north and a westerly jet to the south. Recently, observers have witnessed interactions with Jupiter’s SEB that appear to be peeling material from the GRS on a roughly weekly basis. These filaments, some of which are 10,000 kilometres long or more, form a temporary bridge between the GRS and the SEB.

Image credit: Anthony Wesley, AN graphic: Ade Ashford.
Recent pictures captured by two renowned amateur astroimagers, Anthony Wesley in Australia and Christopher Go in the Philippines, reveal that the Great Red Spot now sports a curved dark bridge between Jupiter’s South Equatorial Belt and the Great Red Spot. But these events have not just been seen from Earth. NASA’s Juno spacecraft currently orbiting Jupiter hopes to take a closer look at the GRS when it passes over the feature in late July 2019, but mission scientists have witnessed structures described as flakes or blades detaching from the GRS with increasing frequency since 2017.
Jupiter’s Great Red Spot almost circled the planet twice in the 19.6 hours separating these two images captured by Christopher Go in the Philippines. Compare GRS developments in this looping animation with that of Anthony Wesley’s four to five Earth days earlier at the top of the page. The black dot to the upper right of the GRS in the 1 June image is Galilean moon Io’s shadow. Image credits: Christopher Go, AN animation: Ade Ashford.
A little more than two Jupiter rotations separate these images from Christopher Go and Anthony Wesley on 12 and 13 June in this looping animation. Note how the Great Red Spot has regained a rounded appearance – at least for now. Image credits: Christopher Go, Anthony Wesley; AN animation: Ade Ashford.
When to see the Great Red Spot
Since Jupiter is a gaseous body, it rotates faster at the equator compared to the poles. At the southerly Jovian latitude of the Great Red Spot, cloud features make one rotation about the planet every 9h 56m, on average. However, the GRS is free to drift in Jovian longitude, so observations are used to refine predictions of when the feature is best placed to see from Earth.

The Great Red Spot is easiest to view (tip: a blue filter in your telescope’s eyepiece helps) when it crosses the imaginary line joining Jupiter’s north and south poles. At such times we say that the GRS is ‘in transit’, though the storm is observable for up to an hour or so either side of the transit time.

The table above lists transits of Jupiter’s Great Red Spot (GRS) visible from Western Europe and the British Isles, with those best seen from the UK highlighted in grey. All events are given in British Summer Time (BST), so subtract one hour to convert to Universal Time/GMT. Computation and data preparation: Ade Ashford/Guide.

GRS predictions for other dates, times and global locations are also available through our interactive online Almanac. To see the Jupiter events for any given day, ensure that the ‘Add phenomena of Jupiter?’ checkbox is ticked. All Galilean moon phenomena and Great Red Spot predictions are in Universal Time (UT). For help using the Almanac, see this article.

For general information on observing Jupiter and its Galilean moons for the 2019 opposition, see this article.