That icy object, an elongated body about 19 miles tall, is called 2014 MU69 or Ultima Thule, a Latin phrase that means “beyond the known world.”
CU Boulder researchers and students are playing an important role in this brush with the unknown, which took place on Jan. 1. As New Horizons zips through the outermost regions of our solar system, it will collect and analyze specks of dust using an instrument designed by students at LASP.
That’s important because even distant phenomena can tell scientists a lot about how the inner solar system formed, said Fran Bagenal, a LASP researcher and co-investigator on the New Horizons mission.
“A lot of the water that we’re made of could come from Uranus and Neptune moving out during the late stages in the formation of our solar system and kicking objects in toward Earth,” said Bagenal. “We have a terrestrial interest in thinking about what these icy bodies mean for us.”
Alan Stern, a former LASP graduate student now at the Southwest Research Institute in Boulder, is the principal investigator for New Horizons. The Johns Hopkins University Applied Physics Laboratory leads the mission’s scientific operations.
Snowman in space
The flyby is the latest in a series of firsts for New Horizons, which gained fame in 2015 for swooping past the dwarf planet Pluto.
As the spacecraft charged past Ultima Thule at about 32,000 miles per hour, one of the biggest questions facing the mission team was also among the simplest: What is it shaped like? Geometric information, Bagenal explained, might carry a lot of clues about how Ultima Thule originally formed.
“What kind of vegetable does it look like?” said Bagenal, who leads the mission’s plasma and particle science teams. “We want to know how this object has evolved and changed over time. Did it form where it is now, or did it form farther out and come inward?”
The answer, according to the first high-definition images of Ultima Thule sent back to Earth, doesn’t seem to be a vegetable at all. The icy body looks more like a peanut or a snowman and was formed by two separate spheres that became stuck together sometime in the past.
Bagenal and other LASP researchers are just as excited about what lies past that snowman, too. As New Horizons reaches the edges of the Kuiper Belt, a region of space that is rich in icy bodies, it will collect critical data about how Earth’s solar system interacts with the galaxy outside.
One way it will do that is through dust, said LASP scientist Mihály Horányi who leads scientific research using the spacecraft’s Student Dust Counter.
The instrument gets its name because it was designed and built by undergraduate and graduate students at LASP in the early 2000s as part of a NASA educational program. The device, which is about the size of a cake pan, detects the small particles that stream past New Horizons, recording their masses.
The instrument has detected thousands of such particles in its voyage to Pluto and beyond. And Horányi is curious to see how far those streams of dust extend.
“Is there an edge to it?” he said.
Horányi added that the success of LASP’s Student Dust Counter has paved the way for CU Boulder to build more complex dust-detecting instruments on upcoming space missions. They include Europa Clipper and the Interstellar Mapping and Acceleration Probe (IMAP).
“We know that dust carries so much information—as they are the little building blocks of our solar system,” said Horányi, also a professor in the CU Boulder Department of Physics. “It’s one of the highlights of my entire career that we put something on this spacecraft that is performing so well and makes great scientific contributions.”
For her part, Bagenal was just excited to be in the room as the first images come streaming in from Ultima Thule. “This flyby is going to be more about enjoying the exploration and curiosity for its own sake,” she said.