The “Yarkovsky-O’Keefe-Radzievskii-Paddack” (YORP) effect proposed that when sunlight strikes an asteroid’s surface, it warms the region up slightly. As the heat is radiated away, there’s a recoil effect that causes the asteroid to spin. It’s not a lot, but added up over millions of years, it can really set an asteroid spinning.
Now astronomers have found this effect in action on nearby asteroid 2000 PH5. They watched the asteroid using a variety of instruments across the Earth over the course of 4 years. During this period, they were able to measure an increase in its rotation speed. Although it takes 12 minutes to complete one rotation, that period is decreasing by 1 millisecond a year.
They calculated that over the next 35 million years, the rotation period will drop to 20 seconds, and it might end up spinning so fast that it reshapes itself or breaks apart.
Original Source: ESO News Release
Through the Artemis Program, NASA will send the first astronauts to the Moon since the…
New research suggests that our best hopes for finding existing life on Mars isn’t on…
Entanglement is perhaps one of the most confusing aspects of quantum mechanics. On its surface,…
Neutrinos are tricky little blighters that are hard to observe. The IceCube Neutrino Observatory in…
A team of astronomers have detected a surprisingly fast and bright burst of energy from…
Meet the brown dwarf: bigger than a planet, and smaller than a star. A category…