Skip to main content

James Webb to join observations of asteroid that could strike Earth in 2032

Artist's impression of an asteroid. This image is not intended to reflect the characteristics of any specific known asteroid.
Artist's impression of an asteroid. This image is not intended to reflect the characteristics of any specific known asteroid. ESA-Science Office

If you’ve been following the story of an asteroid that could hit Earth in 2032, there’s bad news and good news. The bad news is that the likelihood of the asteroid striking the Earth has now risen slightly, but the good news is that astronomers are using tools like the James Webb Space Telescope to track it in more detail.

The probability that Asteroid 2024 YR4 will impact Earth on December 22, 2032 has now risen to 2.3%, according to NASA. The asteroid is being observed by ground-bases telescopes that are part of the International Asteroid Warning Network, which will be following the it for as long as it continues to be visible — which should be through April this year. After that, it will be too faint to observe until 2028.

Recommended Videos

These observations are important for astronomers to accurately pin down the orbit of the asteroid, which will allow them to say with more certainty if the object threatens Earth. Because of the uncertainties involved in spotting an incoming asteroid, it is not uncommon for the probability of an Earth impact to drop to very low or no risk as more observations are made.

Please enable Javascript to view this content

As alarming as a possibly incoming asteroid sounds, experts are clear that there’s no need to panic. “As more observations of the asteroid’s orbit are obtained, its impact probability will become better known,” NASA writes. “It is possible that asteroid 2024 YR4 will be ruled out as an impact hazard, as has happened with many other objects that have previously appeared on NASA’s asteroid risk list, maintained by NASA’s Center for Near-Earth Object Studies. It is also possible its impact probability will continue to rise.”

However, another factor to consider about this asteroid is its size. The first rough estimate put its size at between 40 and 90 meters long, but further observations have not helped to refine this number more precisely.

“It is very important that we improve our size estimate for 2024 YR4: the hazard represented by a 40 m asteroid is very different from that of a 90 m asteroid,” the European Space Agency (ESA) writes. That’s why the James Webb Space Telescope will be observing the asteroid using its infrared instruments.

“Webb is able to study the infrared light (heat) that 2024 YR4 emits, rather than the visible light it reflects. Infrared observations can offer a much better estimate of an asteroid’s size,” ESA explains, pointing to a recently published paper showing how Webb’s infrared capabilities can be used to measure asteroid sizes.

Webb’s MIRI and NIRCam instruments will observe the asteroid in early March, as that is the first time that the asteroid will be visible to the telescope, with another round of observations in May.

Normally observing time on a space telescope is booked up years in advance, but there is a small amount of observing time set aside each year for discoveries made which need critical observations right away. Planetary defense experts proposed using some of this “Director’s Discretionary Time” to observe the asteroid, including taking the final measurements of it until it returns closer to Earth in 2028.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
Stunning view of the Sombrero Galaxy captured by James Webb
The NASA/ESA/CSA James Webb Space Telescope recently imaged the Sombrero galaxy with its MIRI (Mid-Infrared Instrument), resolving the clumpy nature of the dust along the galaxy’s outer ring. The mid-infrared light highlights the gas and dust that are part of star formation taking place among the Sombrero galaxy’s outer disk. The rings of the Sombrero galaxy produce less than one solar mass of stars per year, in comparison to the Milky Way’s roughly two solar masses a year. It’s not a particular hotbed of star formation. The Sombrero galaxy is around 30 million light-years from Earth in the constellation Virgo.

A new image from the James Webb Space Telescope shows a stunning and fashionable sight: the Sombrero Galaxy, named for its resemblance to the traditional Mexican hat. With its wide, flat shape reminiscent of the hat's wide brim, the galaxy, also known as Messier 104, has outer rings that are clearly visible for the first time.

The Sombrero Galaxy is located 30 million light-years away, in the constellation of Virgo, and it has been previously imaged by the Hubble Space Telescope. But while in the Hubble image, the galaxy appears as an opaque, pale disk, in the new Webb image you can see an outer blue disk, with a small bright core right at the center.

Read more
Creepy cosmic eyes stare out from space in Webb and Hubble image
The gruesome palette of these galaxies is owed to a mix of mid-infrared light from the NASA/ESA/CSA James Webb Space Telescope, and visible and ultraviolet light from the NASA/ESA Hubble Space Telescope. The pair grazed one another millions of years ago. The smaller spiral on the left, catalogued as IC 2163, passed behind NGC 2207, the larger spiral galaxy at right. Both have increased star formation rates. Combined, they are estimated to form the equivalent of two dozen new stars that are the size of the Sun annually. Our Milky Way galaxy forms the equivalent of two or three new Sun-like stars per year. Both galaxies have hosted seven known supernovae, each of which may have cleared space in their arms, rearranging gas and dust that later cooled, and allowed many new stars to form. (Find these areas by looking for the bluest regions).

These sinister eyes gazing out from the depths of space star in a new Halloween-themed image, using data from both the Hubble Space Telescope and the James Webb Space Telescope. It shows a pair of galaxies, IC 2163 on the left and NGC 2207 on the right, which are creeping closer together and interacting to form a creepy-looking face.

The two galaxies aren't colliding directly into one another, as one is passing in front of the other, but they have passed close enough to light scrape by each other and leave indications. If you look closely at the galaxy on the left, you can see how its spiral arms have been pulled out into an elongated shape, likely because of its close pass to the gravity of the other nearby galaxy. The lines of bright red around the "eyes" are created by shock fronts, with material from each galaxy slamming together.

Read more
James Webb discovers a new type of exoplanet: an exotic ‘steam world’
An artist’s conception of the “steam world” GJ 9827 d, shown in the foreground in blue.

Our solar system has a wide variety of planet types, from tiny rocky Mercury to huge puffy gas giant Jupiter to distant ice giant Uranus. But beyond our own system, there are even more types of exoplanet out there, including water worlds covered in ocean and where life could potentially thrive. Now, researchers using the James Webb Space Telescope have identified a new and exotic type of planet called a steam world, which has an atmosphere almost entirely composed of water vapor.

The planet, called GJ 9827 d, was examined by the Hubble Space Telescope earlier this year and had researchers so intrigued that they wanted to go back for a closer look using Webb. They found that the planet, which is around twice the size of Earth, had a very different atmosphere from the typical hydrogen and helium that is usually seen. Instead, it was full of hot steam.

Read more