- \n
- Rogue planets, or free-floating planets,<\/strong> are planets that don\u2019t orbit stars. Instead, they drift alone through space.<\/li>\n
- Astronomers have found a new rogue planet,<\/strong> using instruments both on Earth and in space at the same time. This is the first such detection of its kind, and the first confirmed mass of a rogue planet.<\/li>\n
- The planet has a mass similar to Saturn<\/strong> and is located about 9,800 light-years from us, toward the center of our Milky Way galaxy.<\/li>\n<\/ul>\n
EarthSky\u2019s 2026 lunar calendar is available now. Get yours today! Makes a great gift.<\/p>\n
A newly discovered Saturn-mass rogue planet<\/h3>\n
An international team of astronomers said on January 1, 2026, that they discovered a new rogue \u2013 or free-floating \u2013 planet drifting among the stars. It has a mass similar to Saturn and resides about 9,800 light-years from us, in the direction of the center of the Milky Way. Notably, this is the first rogue planet where astronomers have used observatories both on Earth and in space at the same time to make the detection. In addition, it is also the first time that astronomers have directly measured the mass of a rogue planet.<\/p>\n
Subo Dong at Peking University in China led the research team that made the discovery.<\/p>\n
Such rogue planets float freely by themselves in space, with no stars to orbit. In fact, astronomers have been discovering a growing number of these worlds in recent years, and expect to find many more.<\/p>\n
The researchers published their peer-reviewed findings in the journal Science<\/em> on January 1, 2026. There is also a non-paywalled preprint version of the paper available on arXiv.<\/p>\n
In addition, there is a related new Perspective article in Science<\/em>, also published on January 1, 2026, to go along with the new paper.<\/p>\n
\n
Featured in the first issue of Science in 2026, a research team led by Dong Subo of #PekingUniversity reported the first accurate mass measurement of a rogue planet candidate, confirming its planetary nature with a mass comparable to that of Saturn.www.science.org\/doi\/10.1126\/\u2026@science.org<\/p>\n
\u2014 Peking University (@pku1898.bsky.social) 2026-01-02T04:05:45.415Z<\/p>\n<\/blockquote>\n
2 views of a Saturn-mass rogue planet<\/h3>\n
While astronomers have detected a growing number of rogue planets, these new observations were unique. That\u2019s because the researchers made the detection using instruments both on Earth and in space. This included several ground-based surveys and data from ESA\u2019s Gaia space telescope (which ended its mission in January 2025).<\/p>\n
It\u2019s the first time astronomers have identified a rogue planet using both types of observations. Additionally, it\u2019s also the first direct measurement of a rogue planet\u2019s mass. Dong said:<\/p>\n
\n
For the first time, we have a direct measurement of a rogue planet candidate\u2019s mass and not just a rough statistical estimate. We know for sure it\u2019s a planet. Our discovery offers further evidence that the galaxy may be teeming with rogue planets that were likely ejected from their original homes.<\/p>\n<\/blockquote>\n
Dong added:<\/p>\n
\n
We are able to use the same principle to extract the distance information of this rogue planet candidate, finding the mass and distance separately. You need to have this fundamental measurement of mass to really know it\u2019s a planet. Getting this kind of data opens up lots of doors to understanding more about a planet\u2019s possible origins and history.<\/p>\n<\/blockquote>\n
\nAnimation depicting the microlensing event caused by the Saturn-mass rogue planet. Video via J. Skowron\/ OGLE\/ Peking University.<\/em><\/p>\n
Free-floating planet microlensing event<\/h3>\n
So, how exactly did the research team find the planet? They used a technique called microlensing (or gravitational lensing). Basically, the gravity of the rogue planet microlenses \u2013 or magnifies \u2013 the light of a more distant background star. The researchers dubbed this microlensing event as KMT-2024-BLG-0792\/OGLE-2024-BLG-0516. (How\u2019s that for a mouthful?)<\/p>\n
In this case, the researchers were able to observe the microlensing effect using both the ground surveys and data from the Gaia space telescope. The tiny differences in timing of when the light from the microlensing event reached the various instruments allowed the researchers to measure the microlensing parallax (the apparent shift in an object\u2019s position when viewed from different locations).<\/p>\n
Then, the researchers combined that data with finite-source point-lens modeling. Consequently, this revealed the mass and location of the planet.<\/p>\n
The planet is closer to the middle of the Milky Way than we are. It is about 9,800 light-years (3,000 parsecs) from us, toward the center of our galaxy.<\/p>\n
![\"Illustration](\"https:\/\/earthsky.org\/upl\/2026\/01\/rogue-planet-microlensing-artist-concept-ground-based-Gaia-space-telescope-AAAS-January-1-2026.jpg\")
View larger. | Artist\u2019s concept of the microlensing event as observed by both ground-based observatories and the Gaia space telescope. Image via J. Skowron\/ K. Ulaczyk\/ Ogle\/ AAAS\/ Peking University.<\/figcaption><\/figure>\n Ejected from a planetary system<\/h3>\n
Some rogue planets might have formed where they are, without ever having orbited any star. This one, however, likely was once in a planetary system around a star and then somehow got ejected into interstellar space. This could happen through gravitational interactions with other planets in the system or the instability of other stellar companions to the star. The paper states:<\/p>\n
\n
Through comparison with the statistical properties of other observed microlensing events and predictions from simulations, we infer that this object likely formed in a protoplanetary disk (like a planet), not in isolation (like a brown dwarf), and dynamical processes then ejected it from its birth place, producing a free-floating object.<\/p>\n<\/blockquote>\n
![\"Man](\"https:\/\/earthsky.org\/upl\/2026\/01\/Subo-Dong-Peking-University.jpeg\")
Subo Dong at Peking University in China is the lead researcher for the new discovery of the Saturn-mass rogue planet. Image via Peking University.<\/figcaption><\/figure>\n Many more rogue planets out there<\/h3>\n
Rogue planets are difficult to find, because they don\u2019t orbit stars and are therefore shrouded in darkness. But astronomers have been discovering a growing number of these odd, isolated worlds. As of now, there are a few dozen confirmed and candidate rogue planets. And scientists said there might be billions or even trillions of them in our galaxy alone. In fact, there might even be more rogue planets than \u201cregular\u201d planets that orbit stars!<\/p>\n
Scientists expect the upcoming Nancy Grace Roman Space Telescope \u2013 scheduled to launch by May 2027 \u2013 will discover at least 400 more. It will be exciting to see what it finds! As Dong noted:<\/p>\n
\n
The new space-based facilities such as Roman, CSST and Earth 2.0 are going to revolutionize the field of microlensing and the study of free-floating planets. So far, we only have a glimpse into this emerging population of rogue worlds and what light they can shed on the formation of the bodies in the planetary systems of the universe.<\/p>\n<\/blockquote>\n
Bottom line: Astronomers have discovered a Saturn-mass rogue planet nearly 10,000 light-years away. It\u2019s the first one found using both observatories on Earth and in space.<\/p>\n
Sources:<\/p>\n
A free-floating-planet microlensing event caused by a Saturn-mass object<\/p>\n
(Preprint): A free-floating-planet microlensing event caused by a Saturn-mass object<\/p>\n
Two views of a rogue planet<\/p>\n
Via:<\/p>\n
EurekAlert<\/p>\n
Peking University<\/p>\n
Read more:<\/p>\n
Giant free-floating planets might have planets of their own<\/p>\n
Could homeless aliens hitch a ride on rogue planets?<\/p>\n
<\/div>\n
\n - Astronomers have found a new rogue planet,<\/strong> using instruments both on Earth and in space at the same time. This is the first such detection of its kind, and the first confirmed mass of a rogue planet.<\/li>\n