Skip to main content

Tiny, lonely rogue planet is smallest ever discovered

Out in the depths of space, in the huge swaths of blackness between star systems, you can find lonely, wandering rogue planets. These planets don’t orbit around a star but meander through the cosmos alone. And now, astronomers from the OGLE (Optical Gravitational Lensing Experiment) project have discovered the smallest rogue planet ever spotted.

Most rogue planets discovered so far have been several times the mass of Jupiter, but the new lonely planet is more like the size of Earth or Mars. It’s hard to spot such relatively tiny planets, so the researchers use a technique called gravitational microlensing.

Recommended Videos

This method works by looking at the light emitted by distant background stars. When an object passes between us and the background star, the light from the star is very slightly focused by the gravity of the object, making the star appear brighter for a short time. The problem is that background stars and foreground objects need to be exactly aligned for this effect to happen, which only occurs very rarely.

“If we observed only one source star, we would have to wait almost a million years to see the source being microlensed,” lead author Dr. Przemek Mroz explained in a statement. So they look at multiple source stars instead.

This allowed them to spot the tiny object which they believe to be a rogue planet, in the shortest-ever microlensing event which lasted just over 40 minutes. Typically, microlensing events caused by stars last for several days, and for exoplanets last several hours. The fact this event was so brief indicates that the object causing it, the rogue planet, is much smaller than previous detections.

An artist’s impression of a gravitational microlensing event by a free-floating exoplanet.
An artist’s impression of a gravitational microlensing event by a free-floating exoplanet. Jan Skowron / Astronomical Observatory, University of Warsaw.

“When we first spotted this event, it was clear that it must have been caused by an extremely tiny object,” co-author Dr. Radoslaw Poleski, an astronomer with the Astronomical Observatory at the University of Warsaw, said in the statement. “Indeed, models of the event indicate that the lens must have been less massive than Earth, it was probably a Mars-mass object. Moreover, the lens is likely a rogue planet.”

The research not only identified this curious rogue exoplanet but also demonstrated how microlensing can be used to spot even relatively tiny objects in space. This technique could be used to find many more of these wandering planets in the future.

The research is published in the journal 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 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
Astronomers discover how tiny dwarf galaxies form ‘fossils’
A dwarf galaxy in the throes of transitioning to an ultra-compact dwarf galaxy as it’s stripped of its outer layers of stars and gas by a nearby larger galaxy.

Galaxies come in many different shapes and sizes, including those considerably smaller than our Milky Way. These smaller galaxies, called dwarf galaxies, can have as few as 1,000 stars, compared to the several hundred billion in our galaxy. And when these dwarf galaxies age and begin to erode away, they can transform into an even smaller and more dense shape, called an ultra-compact dwarf galaxy.

The Gemini North telescope has recently been studying more than 100 of these eroding dwarf galaxies, seeing how they lose their outer stars and gas to become ultra-compact dwarf galaxies or UCDs.

Read more
James Webb captures image of the most distant star ever discovered
A massive galaxy cluster called WHL0137-08 contains the most strongly magnified galaxy known in the universe’s first billion years: the Sunrise Arc, and within that galaxy, the most distant star ever detected, nicknamed Earendel.

The James Webb Space Telescope has captured a stunning image of the most distant star ever discovered. Discovered by Hubble in 2020, the star named Earendel is located an astonishing 28 billion light-years away. While in the previous Hubble image, the star was only visible as a small blob, these new observations from Webb are detailed enough to reveal information about the star like its type and information about the galaxy in which it resides.

The Webb image shows a galaxy cluster called WHL0137-08, which is so massive that it bends spacetime and acts like a magnifying glass for the more distant galaxies behind it. Some of these distant galaxies being magnified include one called the Sunrise Arc, which hosts Earendel. The Sunrise Arc is located near the end of one of the spikes from the bright central star, at around the five o'clock position. A zoomed-in version of the image shows the Arc and Earendel within t.

Read more