Skip to main content

Hubble sees the changing seasons on Jupiter and Uranus

Our planet isn’t the only place in the solar system with dramatic weather changes. Other planets in the solar system also experience seasons, depending on their distance from the sun, and that affects their climates. One of the many jobs of the Hubble Space Telescope is to monitor the changing seasons on other planets, particularly the larger outer planets which aren’t so often observed. And this week, scientist have released their newest views of Jupiter and Uranus, taken by Hubble and showing seasonal changes on the two planets.

Jupiter is far from the sun, so most of its heat comes not from outside but from within. Jupiter is thought to have a very high core temperature, which may be a result of how it was formed but could also be topped up by processes inside the planet. As this heat escapes from the planet’s interior, it affects its atmosphere which contains multiple layers and has unusual features like geometric storms at its poles.

Jupiter and Uranus (not to scale).
[Jupiter: left] – The forecast for Jupiter is for stormy weather at low northern latitudes. A prominent string of alternating storms is visible, forming a ‘vortex street’ as some planetary astronomers call it.[Uranus: right] – Uranus’s north pole shows a thickened photochemical haze that looks similar to the smog over cities. Several little storms can be seen near the edge of the polar haze boundary.Note: The planets do not appear in this image to scale. NASA, ESA, STScI, A. Simon (NASA-GSFC), M. H. Wong (UC Berkeley), J. DePasquale (STScI)
In the recent Hubble image, Jupiter is experiencing storms across the part of the northern hemisphere near the equator, with a wave-like formation of cyclones and anticyclones crossing the planet. In the image you can also see the moon Io as a small orange circle, casting a black shadow toward the left of the planet.

As for Uranus, the image beautifully captures the planet’s rings and the white haze over the planet’s pole. Uranus is unusual in that it is tipped almost entirely over so it orbits on its side, unlike Earth and most other planets which orbit upright. That’s why the polar haze can be seen on the right-hand side of the planet.

The haze is thought to come from the polar cap, the appearance of which changes dramatically over the seasons. Astronomers are still learning about how this cap changes over time, and it is thought that it will get even brighter as the northern pole will be aimed toward Earth during the planet’s northern summer solstice in 2028.

If you head to the ESA Hubble website you can also see side-by-side comparisons of Jupiter in November 2022 and January 2023, and Uranus in November 2014 and November 2022, showing how the planets change in appearance over time.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Hubble spots a bright galaxy peering out from behind a dark nebula
The subject of this image taken with the NASA/ESA Hubble Space Telescope is the spiral galaxy IC 4633, located 100 million light-years away from us in the constellation Apus. IC 4633 is a galaxy rich in star-forming activity and also hosts an active galactic nucleus at its core. From our point of view, the galaxy is tilted mostly towards us, giving astronomers a fairly good view of its billions of stars.

A new image from the Hubble Space Telescope shows a galaxy partly hidden by a huge cloud of dust known as a dark nebula. The galaxy IC 4633 still shines brightly and beautifully in the main part of the image, but to the bottom right, you can see dark smudges of dust that are blocking the light from this part of the galaxy.

Taken using Hubble's Advanced Camera for Surveys (ACS) instrument, the image also incorporates data from the DECam instrument on the Víctor M. Blanco 4-meter Telescope, which is located in Chile. By bringing together data from the space-based Hubble and the ground-based DECam, astronomers can get a better look at this galaxy, located 100 million light-years away, and the dark dust partially obscuring it.

Read more
Hubble captures the dramatic jets of a baby star
FS Tau is a multi-star system made up of FS Tau A, the bright star-like object near the middle of the image, and FS Tau B (Haro 6-5B), the bright object to the far right that is partially obscured by a dark, vertical lane of dust. The young objects are surrounded by softly illuminated gas and dust of this stellar nursery. The system is only about 2.8 million years old, very young for a star system. Our Sun, by contrast, is about 4.6 billion years old.

A new image from the Hubble Space Telescope shows the drama that unfolds as a new star is born. Within a swirling cloud of dust and gas, a newly formed star is giving off powerful jets that blast away material and cut through the nearby dust of the surrounding nebula to create this stunning vista.

The image shows a system called FS Tau, located 450 light-years away in a region called Taurus-Auriga. Within this region are many stellar nurseries with new stars forming, making it a favorite target for astronomers studying star formation. But this particular system stands out for the dramatic nature of its newborn star, which has formed an epic structure called a Herbig-Haro object.

Read more
Hubble images the spooky Spider Galaxy
This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829.

This week's image from the Hubble Space Telescope shows an irregular galaxy, the spindly arms and clawed shape of which has led to it being named the Spider Galaxy. Located 30 million light-years away, the galaxy also known as UGC 5829 is an irregular galaxy that lacks the clear, orderly arms seen in spiral galaxies like the Milky Way.

This image from the NASA/ESA Hubble Space Telescope shows the irregular galaxy UGC 5829. ESA/Hubble & NASA, R. Tully, M. Messa

Read more