Skip to main content

Exoplanet catalog details over 100 worlds beyond our solar system

TOI-1798, a system that is home to two planets. The inner planet is a strange Super-Earth so close to its star, one year on this alien world lasts only half an Earth day.
TOI-1798 is a system that is home to two planets. The inner planet is a strange Super-Earth so close to its star that one year on this alien world lasts only half an Earth day. W. M. Keck Observatory/Adam Makarenko

A new catalog of exoplanets from two telescopes shows the incredible variety of planets that exist beyond our solar system. The catalog, using data from NASA’s TESS (Transiting Exoplanet Survey Satellite) space telescope and the ground-based W. M. Keck Observatory, shows 126 planets, along with the radius, mass, density and temperature of each.

“Relatively few of the previously known exoplanets have a measurement of both the mass and the radius. The combination of these measurements tell us what the planets could be made of and how they formed,” explained Stephen Kane, University of California, Riverside astrophysicist and principal investigator of the TESS-Keck Survey, in a statement. “With this information, we can begin to answer questions about where our solar system fits in to the grand tapestry of other planetary systems.”

Artist conception of 126 planets in the latest TESS-Keck Survey catalog is based on data including planet radius, mass, density, and temperature. Question marks represent planets requiring more data for full characterization.
An artist’s concept of 126 planets in the latest TESS-Keck Survey catalog is based on data including planet radius, mass, density, and temperature. Question marks represent planets requiring more data for full characterization. W. M. Keck Observatory/Adam Makarenko

Among the exoplanets in the catalog are worlds like TOI-1798 c, shown at the top of this page, which orbits extremely close to its star and is bombarded by intense radiation as a result.

Recommended Videos

“TOI-1798 c orbits its star so quickly that one year on this planet lasts less than half a day on Earth. Because of their proximity to their host stars, planets like this one are also ultra hot — receiving more than 3,000 times the radiation that Earth receives from the sun,” said one of the catalog researchers, Alex Polanski of the University of Kansas.

Please enable Javascript to view this content

Exoplanets like this one are unlikely to have any atmosphere as the intense radiation from their host stars would strip it away. But other worlds are more potentially hospitable, such as those orbiting small, cool stars called red dwarfs.

One big open question in exoplanet research is how typical our solar system is. The most commonly discovered exoplanets are gas giants, because their large size makes them easier to spot from extreme distances. But we don’t know how common Earth-sized worlds are because these are harder to identify in distant star systems due to their smaller size.

There is also a class of planet called sub-Neptunes which appear to be common elsewhere. “Planets smaller than Neptune, but larger than Earth are the most prevalent worlds in our galaxy, yet they are absent from our own solar system. Each time a new one is discovered, we are reminded of how diverse our universe is, and that our existence in the cosmos may be more unique than we can understand,” said Daria Pidhorodetska, also of UC Riverside.

Catalogs like this one help to show our place in the universe and the variety of planets out there. “Are we unusual? The jury is still out on that one, but our new mass catalog represents a major step toward answering that question,” Kane said.

The research is published in The Astrophysical Journal Letters.

Georgina Torbet
Georgina has been the space writer at Digital Trends space writer for six years, covering human space exploration, planetary…
James Webb observes extremely hot exoplanet with 5,000 mph winds
This artist’s concept shows what the hot gas-giant exoplanet WASP-43 b could look like. WASP-43 b is a Jupiter-sized planet circling a star roughly 280 light-years away, in the constellation Sextans. The planet orbits at a distance of about 1.3 million miles (0.014 astronomical units, or AU), completing one circuit in about 19.5 hours. Because it is so close to its star, WASP-43 b is probably tidally locked: its rotation rate and orbital period are the same, such that one side faces the star at all times.

Astronomers using the James Webb Space Telescope have modeled the weather on a distant exoplanet, revealing winds whipping around the planet at speeds of 5,000 miles per hour.

Researchers looked at exoplanet WASP-43 b, located 280 light-years away. It is a type of exoplanet called a hot Jupiter that is a similar size and mass to Jupiter, but orbits much closer to its star at just 1.3 million miles away, far closer than Mercury is to the sun. It is so close to its star that gravity holds it in place, with one side always facing the star and the other always facing out into space, so that one side (called the dayside) is burning hot and the other side (called the nightside) is much cooler. This temperature difference creates epic winds that whip around the planet's equator.

Read more
First indications of a rare, rainbow ‘glory effect’ on hellish exoplanet
For the first time, potential signs of the rainbow-like ‘glory effect’ have been detected on a planet outside our Solar System. Glory are colourful concentric rings of light that occur only under peculiar conditions. Data from ESA’s sensitive Characterising ExOplanet Satellite, Cheops, along with several other ESA and NASA missions, suggest this delicate phenomenon is beaming straight at Earth from the hellish atmosphere of ultra-hot gas giant WASP-76b, 637 light-years away.

Just from looking at our own solar system, we can see that planets come in a wide variety of colors -- from the dusty red of Mars to the bright blues of Uranus and Neptune. Planets like Jupiter have beautiful bands of color caused by variations in the atmosphere, while it's hard to even see the surface of Venus because its atmosphere is so thick. But there are other variations in color which planets can display, like a stunning rainbow-hued set of circular rings called a glory.

Glories are observed on Earth, and have been seen just once on another planet, Venus. But now, researchers believe they may have identified a glory on a planet outside our solar system for the first time. The extreme exoplanet WASP-76b could be host to the first known extrasolar glory, observed by the European Space Agency (ESA)'s Characterising ExOplanet Satellite (Cheops).

Read more
James Webb photographs two potential exoplanets orbiting white dwarfs
Illustration of a cloudy exoplanet and a disk of debris orbiting a white dwarf star.

Even though scientists have now discovered more than 5,000 exoplanets, or planets outside our solar system, it's a rare thing that any telescope can take an image of one of these planets. That's because they are so small and dim compared to the stars that they orbit around that it's easier to detect their presence based on their effects on the star rather than them being detected directly.

However, thanks to its exceptional sensitivity, the James Webb Space Telescope was recently able to image two potential exoplanets orbiting around small, cold cores of dead stars called white dwarfs directly.

Read more