We just measured the mass of a rogue planet for the first time, and it is similar to Saturn’s
.KMT-2024-BLG-0792 / OGLE-2024-BLG-0516 is a recent microlensing event detected by both ground and space-based telescopes that made it possible to identify and measure the mass of a rogue planet located near the outer edge of the central bulge of our galaxy. When we observe such an event across multiple instruments, we can estimate the mass of the microlensed object because of the time delay in observing the object at different locations in space and on Earth.
This extraordinary discovery indicates that rogue planets with masses below that of Jupiter exist and may be more widespread than previously believed. We already observed directly, with the James Webb Telescope, many double Jupiter-size planets in the Orion Nebula in 2023. At first, we thought they were ejected from newly formed planetary systems, but other theories of their formation have since been proposed. They might have formed via the fragmentation of nebulae in which stars form when they collide.
Nevertheless, a large population of such planets is likely to form in star systems and be ejected during the turbulent early history of those systems. Planets form via collision with planetoids and other planets within the protoplanetary disk, and a large number of them are expected to be ejected. When a large gas giant planet is banished from a protoplanetary disk, in about 90% of cases, it loses its moons, and some can become rogue planets, as well. Let’s not forget that planets more massive than Jupiter can have moons as massive as Earth and even larger.
We now think that we previously underestimated the number of transneptunian objects in our system. There could be up to 10,000, some as large as Mars and even half the mass of Earth. We can only detect them for 1% of their orbit, which can take tens of thousands of years, and our technological civilization is too young to take advantage of the short window for their possible detection until we get better instruments that could see these objects even when they are far away. They can also be ejected sometimes and become rogue planets.
This is why the upper estimate of the number of rogue planets is as large as 100,000 for each star
. Some can have subsurface oceans heated by the tides of a moon and by radioactivity. There is even speculation that some may have liquid water on the surface if they have a specific atmospheric composition that prevents heat from escaping. This is even though they float freely in space, without a star to provide heat, and it means that they can be a fascinating destination for the search for extraterrestrial life or stopovers in our quest to reach other star systems.This also means that rogue planets can be any size, but we cannot see them yet if they are too small—they don’t produce their own light.
The question was: What is the size of a rogue planet?
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