In the far reaches of our Solar System, beyond Pluto, astronomers have uncovered a potential new dwarf planet named 2017 OF201. This rocky body spans about 700 kilometers (or 435 miles) across, making it sizable enough to fit into the dwarf planet category. What’s fascinating is its orbit, which casts doubt on the existence of a mysterious Planet Nine in our solar neighborhood.
Sihao Cheng, an astrophysicist from the Institute for Advanced Study, explains, "The object’s aphelion—its farthest point from the Sun—exceeds 1,600 times the Earth’s distance from the Sun. Its perihelion, where it approaches the Sun, is 44.5 times that distance. This is similar to Pluto’s path."
Finding such distant objects, known as trans-Neptunian objects (TNOs), isn’t easy. These bodies orbit beyond Neptune, usually around 30 astronomical units from the Sun. They’re often small and very cold, reflecting little light. Recent advancements in powerful telescopes have improved our ability to search the Kuiper Belt and beyond. The most distant one detected so far, named FarFarOut, is about 400 kilometers across and located 132 astronomical units away.
Cheng and his team found 2017 OF201 by sifting through data from the Dark Energy Camera Legacy Survey and the Canada France Hawaii Telescope. Their analysis tracked the object over 19 observations from 2011 to 2018, allowing them to accurately map its orbit.
2017 OF201 was initially spotted at a distance of 90.5 astronomical units, which is more than double Pluto’s 40 astronomical units. This dwarf planet’s orbit is highly elliptical, taking it as close as 44 astronomical units and as far out as 1,600 astronomical units—into the inner Oort Cloud that envelopes our Solar System.
The origins of its unusual orbit, which takes 25,000 years to complete, remain a mystery. It might have experienced a significant gravitational event or evolved through a series of interactions over time.
Interestingly, 2017 OF201’s path doesn’t align with the patterns of other known TNOs, which led some astronomers to believe in a lurking Planet Nine. Cheng’s team conducted simulations with and without this hypothetical planet. They found that, without Planet Nine, 2017 OF201 maintains a stable orbit. However, the presence of such a planet would likely disturb its trajectory, potentially ejecting it from the Solar System within 100 million years.
This discovery provides strong evidence against Planet Nine’s existence. It also suggests there could be many more objects like 2017 OF201 waiting to be discovered. Cheng notes, "Since 2017 OF201 is detectable only 1% of the time it’s near us, there could be a hundred similar objects just too far away for us to spot right now."
Despite our technological advancements in telescopes, the mysteries of our Solar System remain vast. The International Astronomical Union has officially recognized 2017 OF201, and the research detailing its findings is accessible on arXiv. There’s still a lot to learn about the distant worlds that share our solar neighborhood, and discoveries like this remind us of the wonders yet to be explored.
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