Skip to main content

Neptune’s temperatures are fluctuating, and no one knows why

Something strange is happening on Neptune. Researchers have studied 17 years of data from the planet, collected using telescopes including the European Southern Observatory’s Very Large Telescope, NASA’s Spitzer Space Telescope, the Gemini South and North telescopes, the Subaru Telescope, and the Keck Telescope. And they’ve found surprising swings in the planet’s temperatures which they can’t explain.

This composite shows thermal images of Neptune taken between 2006 and 2020. The first three images (2006, 2009, 2018) were taken with the VISIR instrument on ESO’s Very Large Telescope while the 2020 image was captured by the COMICS instrument on the Subaru Telescope (VISIR wasn’t in operation in mid-late 2020 because of the pandemic). After the planet’s gradual cooling, the south pole appears to have become dramatically warmer in the past few years, as shown by a bright spot at the bottom of Neptune in the images from 2018 and 2020.
This composite shows thermal images of Neptune taken between 2006 and 2020. The first three images (2006, 2009, 2018) were taken with the VISIR instrument on ESO’s Very Large Telescope while the 2020 image was captured by the COMICS instrument on the Subaru Telescope (VISIR wasn’t in operation in mid-late 2020 because of the pandemic). After the planet’s gradual cooling, the south pole appears to have become dramatically warmer in the past few years, as shown by a bright spot at the bottom of Neptune in the images from 2018 and 2020. ESO/M. Roman, NAOJ/Subaru/COMICS

Neptune does have seasons, as it rotates and moves around the sun. However, its seasons are much slower than those on Earth, lasting around 40 years. In the southern hemisphere, it has been summer since 2005, so researchers were surprised by the apparent significant variation in temperatures they saw.

“Our data cover less than half of a Neptune season, so no one was expecting to see large and rapid changes,” said co-author Glenn Orton, senior research scientist at NASA’s Jet Propulsion Laboratory, in a statement.

In a series of observations taken between 2003 and 2018, the global average temperature of the planet dropped by eight degrees Celsius (46 degrees Fahrenheit), and then around the planet’s southern pole, the temperatures rose quickly by 11 degrees Celsius (52 degrees Fahrenheit) between 2018 and 2020. While Neptune is known to host vortices, or areas of atmospheric turbulence, including one at the planet’s southern pole which affects temperatures there, that isn’t enough to explain how temperatures rose so fast. And the overall global cooling is strange too.

“This change was unexpected,” said lead author of the study, Michael Roman of the University of Leicester, U.K. “Since we have been observing Neptune during its early southern summer, we expected temperatures to be slowly growing warmer, not colder.”

The astronomers were puzzled by their findings and have no clear answer as to what could have caused them. Some of the theories suggested by the European Southern Observatory are that the temperatures changes could be due to something happening in the chemistry of the planet’s atmosphere, or due to a weather phenomenon, or even perhaps due to some kind of effects from the sun.

To learn more, astronomers will need to take more readings of Neptune using powerful upcoming telescopes like the Extremely Large Telescope or the James Webb Space Telescope.

“I think Neptune is itself very intriguing to many of us because we still know so little about it,” says Roman. “This all points towards a more complicated picture of Neptune’s atmosphere and how it changes with time.”

The research is published today in The Planetary Science Journal.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Merged galaxy gives a glimpse at the future of the Milky Way
The galaxy NGC 7727 was born from the merger of two galaxies that started around a billion years ago. The cosmic dance of the two galaxies has resulted in the spectacular wispy shape of NGC 7727. At the heart of the galaxy, two supermassive black holes are spiralling closer to each other, expected to merge within 250 million years, the blink of an eye in astronomical time. This image of NGC 7727 was captured by the FOcal Reducer and low dispersion Spectrograph 2 (FORS2) instrument at ESO’s Very Large Telescope (VLT).

At the heart of almost every galaxy lies an enormous black hole. These monsters are so massive that they get a classification of their own: supermassive black holes, with masses millions or even billions of times the mass of our sun. And when two galaxies collide, their supermassive black holes get closer and closer until these beasts eventually merge as well.

This almost incomprehensible process is on display in an image recently shared by the European Southern Observatory (ESO), showing an almost-merged galaxy that contains the closest pair of supermassive black holes ever discovered at just 1,600 light years apart. Galaxy NGC 7727 started off as two galaxies, which began merging around a billion years ago, and within the next few hundred million years, the two supermassive black holes are set to collide, creating an even bigger black hole in the process.

Read more
See elements as colors in this galaxy where stars are being born
This week, we feature an image of the spiral galaxy NGC 4303, also known as Messier 61, which is one of the largest galactic members of the Virgo Cluster. Being a so-called starburst galaxy, it has an unusually high amount of stars being born, and has been used by astronomers as a laboratory to better understand the fascinating phenomena of star formation.

From Hubble to the James Webb Space Telescope, when you think of the tools that capture images of space some of the first examples that come to mind are likely to be space-based telescopes. These telescopes have the advantage of being above the water vapor in Earth's atmosphere which can distort readings, and allows them to look out at the universe in great detail. But there are advantages of ground-based telescopes as well, such as being able to build much larger structures and to more easily upgrade these telescopes with new instruments.

One such ground-based telescope is the European Southern Observatory (ESO)'s Very Large Telescope. As the name suggests it is indeed very large, being made up of four separate telescopes each of which has an 8.2-meter (27 feet) primary mirror and which work together to look out at space in the visible light and infrared wavelengths. On the telescope named Yepun sits an instrument called MUSE, or the Multi-Unit Spectroscopic Explorer (MUSE), which uses a technology called adaptive optics to collect high-resolution data about areas of space.

Read more
Just one instrument mode left and the James Webb Telescope will be ready for science
MIRI Flight Instrument Undergoing Alignment Testing

The countdown is on for the release of the first science images from the James Webb Space Telescope, scheduled for July 12. But before full science operations begin, each of Webb's four instruments has to be calibrated and checked in its various modes to ensure it's ready to collect data. This week, the Mid-Infrared instrument (MIRI) has completed its checks and NASA has announced that it is ready for science.

Unlike Webb's other three instruments which operate in the near-infrared range, MIRI operates in the mid-infrared which means it has some peculiarities. It was the last instrument to reach its operating temperature because its silicon detectors have to be so cold to work -- at a temperature of less than 7 degrees Kelvin. In order to control its temperature exactly, the MIRI instrument has both a heater and a cooler. MIRI reached its operating temperature in April this year, and since then  it ha been through an extensive calibration process and engineers have confirmed that its imaging, its low- and medium-resolution spectroscopy, and finally its coronagraphic imaging modes are all ready to go.

Read more