The nucleus of a comet discovered in 2014 is the largest ever spotted.
The “dirty snowball” at the center of comet C/2014 UN271 is about 120 kilometers across, researchers report in the April 10 Astrophysical Journal Letters. That makes this comet — also known as Bernardinelli-Bernstein, after its discoverers — about twice as wide as Rhode Island, says David Jewitt, an astronomer at UCLA.
Though the comet is big — and vastly larger than Halley’s comet, which measures a little more than 11 kilometers across — it will never be visible to the naked eye from Earth because it’s too far away, Jewitt says (SN: 12/14/15). The object is now about 3 billion kilometers from Earth. At its closest approach in 2031, the comet will come no closer to the sun than 1.6 billion kilometers, about the same distance as Saturn. Jewitt and colleagues sized up the comet with the help of new images from the Hubble Space Telescope, combined with images taken by another team at far-infrared wavelengths. The analysis also revealed that the comet’s nucleus reflects only about 3 percent of the light that strikes it. That makes the object “blacker than coal,” Jewitt says.
Comet Bernardinelli-Bernstein takes about 3 million years to circle the sun in a highly elliptical orbit. At its farthest, the comet may reach about half a light-year from the sun — about one-eighth of the distance to the next nearest star.
The comet is likely “just the tip of the iceberg” as far as undiscovered comets of this size go, Jewitt says. And for every comet this size, he suggests, there could be tens of thousands of smaller objects circling the sun undetected.
Two mysterious galaxies, devoid of dark matter, could have a smashing origin story.
About 8 billion years ago, researchers propose, two dwarf galaxies slammed into one another. That cosmic crash caused the gas within those two galaxies to split up and form multiple new dwarf galaxies, including the two dark matter–free ones.
A newfound row of dwarf galaxies, more than 6 million light-years long, could have formed in the aftermath of the hypothesized crash, researchers report in the May 19 Nature. If correct, the finding could help solve the mystery of how such unusual dark matter–free galaxies form, and reveal new details about the nature of dark matter.
But other scientists are skeptical that there’s enough evidence to support this backstory. “If this is true, I think it would be really exciting. I just don’t think the bar has been met,” says astronomer Michelle Collins of the University of Surrey in Guildford, England.
In 2018, Yale University astronomer Pieter van Dokkum and colleagues reported a dwarf galaxy with no dark matter (SN: 3/28/18). The invisible, mysterious substance is typically detectable in galaxies via its gravitational effects on stars. When a second dark matter–free dwarf galaxy was found in the vicinity in 2019, it raised an obvious question: How did the two oddball galaxies form? Dark matter is generally thought to form the foundation of all galaxies, gravitationally attracting the gas that eventually forms stars. So some process must have separated the dark matter from the galaxies’ gas.
Scientists have previously seen dark matter and normal matter separate on a very large scale in the Bullet Cluster, which formed when two clusters of galaxies rammed into one another (SN: 8/23/06). Other researchers had proposed that something similar might happen with colliding dwarf galaxies, what van Dokkum and colleagues call “bullet dwarfs.”
In such a collision, the dwarf galaxies’ ethereal dark matter would continue on unperturbed, because the dark matter doesn’t interact with other matter. But the gas from the two galaxies would slam together, eventually forming multiple clumps that would each become its own galaxy, free of dark matter.
Now, van Dokkum and colleagues say that the bullet dwarf idea explains the two previously reported dark matter–free galaxies — and several other galaxies nearby. The two galaxies are moving away from each other as if they had come from the same spot, the researchers say. What’s more, the two galaxies are part of a chain of 11 galaxies aligned in a row, a structure that could have formed in the aftermath of a bullet dwarf collision. “It’s super satisfying to finally have an explanation for these weird objects,” van Dokkum says.
But, Collins says, “there could be much more done to make it convincing.” For example, she says, the scientists didn’t measure the distances of all the galaxies from Earth. That means some of the galaxies could be much farther away than others, and it could be a coincidence that the galaxies appear to be lined up from our viewpoint.
And the researchers haven’t yet measured the velocities of all the galaxies in the trail or determined whether those galaxies are also missing their dark matter, which would help confirm whether the scenario is correct.
Other scientists are more optimistic. “The origin story is very plausible in my opinion,” says astrophysicist Eun-jin Shin of Seoul National University in South Korea. Shin cowrote a perspective article on the discovery with astrophysicist Ji-hoon Kim, also of Seoul National University, that was also published in Nature.
Computer simulations performed by Shin, Kim and others have shown that bullet dwarfs can produce such dark matter–free galaxies. If confirmed, the bullet dwarf idea could help pin down dark matter’s properties, in particular whether dark matter interacts with itself (SN: 4/5/18).
Van Dokkum and colleagues are planning additional measurements that could confirm or refute the case. But so far, he says, “It has, to me, the ring of truth.”
