Skip to main content

Astronomers discover three exoplanets in final data from Kepler Space Telescope

The Kepler Space Telescope was retired in 2018 after a nine-year mission that saw it discover an incredible 2,600 confirmed exoplanets, kicking off the modern era of exoplanet research. But now there are three more exoplanets to add to the mission’s total, even after the telescope has been dark for the last five years. Astronomers were recently able to use data from the very last observations of Kepler to discover three more planets.

Two of the three exoplanets have been confirmed — K2-416 b and K2-417 b — with a third planet, EPIC 246251988 b, remaining an exoplanet candidate. (To be upgraded from exoplanet candidate to confirmed exoplanet, an initial observation has to be verified through observations by two other telescopes.) The planets range from 2.6 times the size of Earth to 4 times the size of Earth, making them small in comparison to most discovered exoplanets.

An artist's concept of the Kepler spacecraft.
An artist’s concept of the Kepler spacecraft. NASA/Ames/JPL-Caltech

The planets themselves might not be the most exciting of discoveries, according to the researchers, but what is special about them is the way that they were discovered.

”These are fairly average planets in the grand scheme of Kepler observations,” said lead researcher Elyse Incha of the University of Wisconsin-Madison in a statement. “But they’re exciting because Kepler observed them during its last few days of operations. It showcases just how good Kepler was at planet hunting, even at the end of its life.”

The observations were made during the telescope’s last weeks of observations before it was retired on October 30, 2018. As the spacecraft ran out of fuel, it could no longer point in the correct direction and its data became blurry. But the researchers were able to use the last good data to find transits — when the light from a star drops slightly due to a planet passing in front of it.

Even though the mission is now long over, the telescope leaves behind a legacy of publicly available data that it collected over its nearly decade-long observations. It has been succeeded by other planet-hunting telescopes like TESS, NASA’s Transiting Exoplanet Survey Satellite, which was launched in 2018 and continues to discover new exoplanets.

“In many ways, Kepler passed the planet-hunting torch to TESS,” said TESS project scientist Knicole Colón, who also worked on Kepler. “Kepler’s dataset continues to be a treasure trove for astronomers, and TESS helps give us new insights into its discoveries.”

The exoplanet research is published in the journal Monthly Notices of the Royal Astronomical Society.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
James Webb telescope gets a view of the ‘white whale’ of exoplanet research
This artist’s concept depicts the planet GJ 1214 b, a “mini-Neptune” with what is likely a steamy, hazy atmosphere. A new study based on observations by NASA’s Webb telescope provides insight into this type of planet, the most common in the galaxy.

Studying other planets is difficult not only because they are so far away, but also because they can have properties that make taking readings much harder. Here in our solar system, we only have scant information about the surface of Venus because its thick atmosphere makes it hard to view. Being 50 light-years away, the planet GJ 1214 b has proved similarly tricky, defying 15 years of attempted observations due to its hazy nature.

But now, the James Webb Space Telescope has been able to peer into the planet's atmosphere for the first time, revealing the secrets of this mysterious place. It's known as a mini-Neptune because it has a thick atmosphere and layers of ice like Neptune. Only around three times the diameter of the Earth, the planet likely has lots of water, but it is located in the atmosphere, not on the surface, due to its high surface temperature.

Read more
Hubble observes weird star system with three off-kilter, planet-forming disks
This illustration is based on Hubble Space Telescope images of gas and dust discs encircling the young star TW Hydrae. We have an oblique view of three concentric rings of dust and gas. At the centre is the bright white glow of the central star. The reddish-coloured rings are inclined to each other and are therefore casting dark shadows across the outermost ring.

Planets form from large disks of dust and gas that collect around their host stars. Billions of years ago, our solar system would have looked like a single point of bright light coming from the sun, with a disk of matter swirling around it that eventually clumped into planets. To learn about how our solar system formed, it's helpful to look at other systems that are currently going through this process -- such as TW Hydrae, a system located 200 light-years away and turned face-on toward us, making it the perfect place to observe planetary formation.

But there's something odd about the TW Hydrae system. In 2017, astronomers first noticed a strange shadow that was visible on the disk of dust and gas surrounding the star. While such shadows are typically from a planet formed within the disk, in this case the shadow's shape and movement suggested it was actually from a second disk, located within the first disk and tilted at a different angle. Now, astronomers think they have spotted evidence of a third disk, with all three stacked up and creating a complex pattern of shadows.

Read more
Astronomers watch a preview of the destruction of the Earth
Astronomers using the Gemini South telescope in Chile, operated by NSF’s NOIRLab, have observed the first compelling evidence of a dying Sun-like star engulfing an exoplanet. The “smoking gun” of this event was seen in a long and low-energy outburst from the star — the telltale signature of a planet skimming along a star’s surface. This never-before-seen process may herald the ultimate fate of Earth when our own Sun nears the end of its life in about five billion years.

Astronomers recently caught the grisly sight of an exoplanet being devoured by its star, in a preview of what will eventually happen to the Earth. The sun-like star is located within our galaxy, around 12,000 light-years away, and has puffed up into an end-of-life state called a red giant. As it grows, it expands outward, which is how it was able to swallow the Jupiter-sized planet that had been in orbit around it.

The researchers were able to spot the event because of the distinctive brightening pattern of the star, which is similar to what we can expect will eventually happen to our sun. “We are seeing the future of the Earth,” said lead author of the research, Kishalay De of the Massachusetts Institute of Technology (MIT), in a statement. “If some other civilization was observing us from 10,000 light-years away while the sun was engulfing the Earth, they would see the sun suddenly brighten as it ejects some material, then form dust around it, before settling back to what it was.”

Read more