Skip to main content

Kepler finds 104 exoplanets in the largest single haul of confirmed planets

exoplanet haul transits2 on starfield editable 02 20x30
The Kepler spacecraft telescope. NASA
The largest ever haul of exoplanets has been announced by an international team of scientists using images gathered by NASA’s Kepler space telescope. A total of 104 planets out of 197 original candidates have been confirmed, with four of those offering promise as potentially rocky, habitable worlds. The astronomers, led by a team at the University of Arizona, published their findings this week in Astrophysical Journal Supplement Series.

Oddly enough, the finding was facilitated by technical trouble with the telescope, which trails Earth’s orbit, peering into space in search of Earth-sized exoplanets near habitable zones.

Depiction of the confirmed exoplanets in their respective fields, with an artist's rendition of Kepler and a rocky planet to the right.
Depiction of the confirmed exoplanets in their respective fields, with an artist’s rendition of Kepler and a rocky planet to the right. NASA

“Kepler’s malfunction necessitated a change in mission strategy, from a long-term survey of a small patch of sky to a set of shorter-duration observations of a much wider fraction of the sky,” the paper’s lead author, Ian Crossfield, told Digital Trends. “This new K2 observing strategy means that we find planets with shorter ‘years,’ but the planets we find tend to orbit stars closer to the Earth.” These target stars are relatively bright, enabling more refined study and understanding of their systems.

The four promising exoplanets orbit K2-72, a cool, red, dwarf star 181 light years from Earth that’s about half the size of our sun. The planets themselves are between 20 and 50 percent larger than Earth.

“From studying other planetary systems, we know that these sizes mean that the odds are good that all four of these planets are rocky,” Crossfield said. “Although some of these planets receive roughly the same amount of starlight from their star as Earth does from the Sun, we know nothing about these planets’ atmospheres … and so can’t be sure which of these might be as temperate as the Earth, or which might be inhospitable, infernal greenhouse planets like Venus.”

In order to confirm that the data did indeed depict planets, scientists collected high-resolution images of target stars using an array of telescope around the world. Optical spectroscopy data allowed the astronomers to determine the stars’ properties and infer the properties of the planets in their orbit.

Exciting in its own right, the finding also paves the way for NASA’s future exoplanet hunting missions, including the Transiting Exoplanet Survey Satellite that is set to launch in December 2017 and the James Webb Space Telescope that is scheduled to begin operations in October 2018.

Editors' Recommendations

Dyllan Furness
Dyllan Furness is a freelance writer from Florida. He covers strange science and emerging tech for Digital Trends, focusing…
James Webb finds that rocky planets could form in extreme radiation environment
This is an artist’s impression of a young star surrounded by a protoplanetary disk in which planets are forming.

It takes a particular confluence of conditions for rocky planets like Earth to form, as not all stars in the universe are conducive to planet formation. Stars give off ultraviolet light, and the hotter the star burns, the more UV light it gives off. This radiation can be so significant that it prevents planets from forming from nearby dust and gas. However, the James Webb Space Telescope recently investigated a disk around a star that seems like it could be forming rocky planets, even though nearby massive stars are pumping out huge amounts of radiation.

The disk of material around the star, called a protoplanetary disk, is located in the Lobster Nebula, one of the most extreme environments in our galaxy. This region hosts massive stars that give off so much radiation that they can eat through a disk in as little as a million years, dispersing the material needed for planets to form. But the recently observed disk, named XUE 1, seems to be an exception.

Read more
How astronomers used James Webb to detect methane in the atmosphere of an exoplanet
An artists rendering of a blue and white exoplanet known as WASP-80 b, set on a star-studded black background. Alternating horizontal layers of cloudy white, grey and blue cover the planets surface. To the right of the planet, a rendering of the chemical methane is depicted with four hydrogen atoms bonded to a central carbon atom, representing methane within the exoplanet's atmosphere. An artist’s rendering of the warm exoplanet WASP-80 b whose color may appear bluish to human eyes due to the lack of high-altitude clouds and the presence of atmospheric methane identified by NASA’s James Webb Space Telescope, similar to the planets Uranus and Neptune in our own solar system.

One of the amazing abilities of the James Webb Space Telescope is not just detecting the presence of far-off planets, but also being able to peer into their atmospheres to see what they are composed of. With previous telescopes, this was extremely difficult to do because they lacked the powerful instruments needed for this kind of analysis, but scientists using Webb recently announced they had made a rare detection of methane in an exoplanet atmosphere.

Scientists studied the planet WASP-80 b using Webb's NIRCam instrument, which is best known as a camera but also has a slitless spectroscopy mode which allows it to split incoming light into different wavelengths. By looking at which wavelengths are missing because they have been absorbed by the target, researchers can tell what an object -- in this case, a planetary atmosphere -- is composed of.

Read more
James Webb investigates a super puffy exoplanet where it rains sand
Artistic concept of the exoplanet WASP-107b and its parent star. Even though the rather cool host star emits a relatively small fraction of high-energy photons, they can reach deep into the planet’s fluffy atmosphere.

Exoplanets come in many forms, from dense, rocky planets like Earth and Mars to gas giants like Jupiter and Saturn. But some planets discovered outside our solar system are even less dense than gas giants and are a type known informally as super-puff or cotton candy planets. One of the least dense exoplanets known, WASP-107b, was recently investigated using the James Webb Space Telescope (JWST) and the planet's weather seems to be as strange as its puffiness.

The planet is more atmosphere than core, with a fluffy atmosphere in which Webb spotted water vapor and sulfur dioxide. Strangest of all, Webb also saw silicate sand clouds, suggesting that it would rain sand between the upper and lower layers of the atmosphere. The planet is almost as big as Jupiter but has a tiny mass similar to that of Neptune.

Read more