Voyager I, now in space for over 35 years, is just approaching the very edge of our solar system. Astronomers have expected some very particular things to happen once it crosses over into interstellar space. Only, those things aren’t happening at all, and nobody can say why for sure.
The first Voyager sped out of the solar system in 1980 and it has since been edging closer and closer to interstellar space. The probe is currently out more than 120 times the distance between the Earth and the sun.
Scientists initially thought that Voyager’s transition into this new realm, where effects from the rest of the galaxy become more pronounced, would be gradual and unexciting. But it’s proven to be far more complicated than anything researchers had imagined…
…it’s almost as if Voyager thought it was going outside but instead found itself standing in the foyer of the sun’s home with an open door that allows wind to blow in from the galaxy. Not only were scientists not expecting this foyer to exist, they have no idea how long the probe will stay inside of it. Stone speculated that the probe could travel some months or years before it reaches interstellar space.
For the curious reader, 120 times the distance between the Earth and the sun is approximately 18.5 billion kilometers, or 11.5 billion miles. It’s hard to imagine such a distance, so think of it this way: The speed of light is 299,792,458 meters per second. If you could travel that quickly, it would take more than 34 hours to go from the sun to Voyager I’s current position and back.
Or think of it in miles per hour: 300,000,000 meters per second is around 671 million miles per hour. You could get to Jupiter in about 40 minutes at that speed. Voyager I was launched on 5 September 1977, but its closest approach to Jupiter didn’t happen until 1979. It would take roughly a year to reach the Oort cloud.
It takes sunlight eight full minutes to reach the Earth.
Once you start to fix the distance in your head, Voyager I’s position becomes all the more amazing.
A team of researchers has discovered evidence that an extrasolar planet may be forming quite far from its star — about twice the distance Pluto is from our Sun. The planet lies inside a dusty, gaseous disk around a small red dwarf TW Hydrae, which is only about 55% of the mass of the Sun. The discovery adds to the ever-increasing variety of planetary systems in the Milky Way.
Planet formation far away from a small parent star is at odds with the conventional planet-making dogma. Under the most accepted scenario, planets form over tens of millions of years from the slow accretion of dust, rocks, and gas. That happens most easily close to the central star, where orbital timescales are short. Even under a disk instability scenario, in which planets can collapse quickly from the disk, it’s not clear such a low mass planet could form.
Carnegie astrophysicist Alan Boss, who works on disk instability models, said “If the mass of this suspected planet is as low as it seems to be, this presents a real puzzle. Theory would say that it cannot exist!”
But apparently it does exist. I’m excited by this kind of news because it demonstrates the versatility of planet formation in the universe. The more possible planets, the more places life could exist. And like lots of other people, I want to believe we’re not alone.